The purpose of this blog is the creation of an open, international, independent and free forum, where every UFO-researcher can publish the results of his/her research. The languagues, used for this blog, are Dutch, English and French.You can find the articles of a collegue by selecting his category. Each author stays resposable for the continue of his articles. As blogmaster I have the right to refuse an addition or an article, when it attacks other collegues or UFO-groupes.
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Deze blog is opgedragen aan mijn overleden echtgenote Lucienne.
In 2012 verloor ze haar moedige strijd tegen kanker!
In 2011 startte ik deze blog, omdat ik niet mocht stoppen met mijn UFO-onderzoek.
BEDANKT!!!
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UFO'S of UAP'S, ASTRONOMIE, RUIMTEVAART, ARCHEOLOGIE, OUDHEIDKUNDE, SF-SNUFJES EN ANDERE ESOTERISCHE WETENSCHAPPEN - DE ALLERLAATSTE NIEUWTJES
UFO's of UAP'S in België en de rest van de wereld In België had je vooral BUFON of het Belgisch UFO-Netwerk, dat zich met UFO's bezighoudt. BEZOEK DUS ZEKER VOOR ALLE OBJECTIEVE INFORMATIE , enkel nog beschikbaar via Facebook en deze blog.
Verder heb je ook het Belgisch-Ufo-meldpunt en Caelestia, die prachtig, doch ZEER kritisch werk leveren, ja soms zelfs héél sceptisch...
Voor Nederland kan je de mooie site www.ufowijzer.nl bezoeken van Paul Harmans. Een mooie site met veel informatie en artikels.
MUFON of het Mutual UFO Network Inc is een Amerikaanse UFO-vereniging met afdelingen in alle USA-staten en diverse landen.
MUFON's mission is the analytical and scientific investigation of the UFO- Phenomenon for the benefit of humanity...
Je kan ook hun site bekijken onder www.mufon.com.
Ze geven een maandelijks tijdschrift uit, namelijk The MUFON UFO-Journal.
Since 02/01/2020 is Pieter ex-president (=voorzitter) of BUFON, but also ex-National Director MUFON / Flanders and the Netherlands. We work together with the French MUFON Reseau MUFON/EUROP.
ER IS EEN NIEUWE GROEPERING DIE ZICH BUFON NOEMT, MAAR DIE HEBBEN NIETS MET ONZE GROEP TE MAKEN. DEZE COLLEGA'S GEBRUIKEN DE NAAM BUFON VOOR HUN SITE... Ik wens hen veel succes met de verdere uitbouw van hun groep. Zij kunnen de naam BUFON wel geregistreerd hebben, maar het rijke verleden van BUFON kunnen ze niet wegnemen...
21-04-2022
Astronomers Discover Micronovae: A New Kind of Thermonuclear Stellar Explosion
Astronomers Discover Micronovae: A New Kind of Thermonuclear Stellar Explosion
ByEUROPEAN SOUTHERN OBSERVATORY (ESO)
A team of astronomers, with the help of the European Southern Observatory’s Very Large Telescope (ESO’s VLT), have observed a new type of stellar explosion — a micronova. These outbursts happen on the surface of certain stars, and can each burn through around 3.5 billion Great Pyramids of Giza of stellar material in only a few hours.
“We have discovered and identified for the first time what we are calling a micronova,” explains Simone Scaringi, an astronomer at Durham University in the UK who led the study on these explosions published today in Nature. “The phenomenon challenges our understanding of how thermonuclear explosions in stars occur. We thought we knew this, but this discovery proposes a totally new way to achieve them,” he adds.
Astronomers have discovered a new type of explosion occurring on white dwarf stars in two-star systems. This video summarizes the discovery.
Micronovae are extremely powerful events, but are small on astronomical scales; they are much less energetic than the stellar explosions known as novae, which astronomers have known about for centuries. Both types of explosions occur on white dwarfs, dead stars with a mass about that of our Sun, but as small as Earth.
A white dwarf in a two-star system can steal material, mostly hydrogen, from its companion star if they are close enough together. As this gas falls onto the very hot surface of the white dwarf star, it triggers the hydrogen atoms to fuse into helium explosively. In novae, these thermonuclear explosions occur over the entire stellar surface. “Such detonations make the entire surface of the white dwarf burn and shine brightly for several weeks,” explains co-author Nathalie Degenaar, an astronomer at the University of Amsterdam, the Netherlands.
This artist’s impression shows a two-star system where micronovae may occur. The blue disc swirling around the bright white dwarf in the centre of the image is made up of material, mostly hydrogen, stolen from its companion star. Towards the centre of the disc, the white dwarf uses its strong magnetic fields to funnel the hydrogen towards its poles. As the material falls on the hot surface of the star, it triggers a micronova explosion, contained by the magnetic fields at one of the white dwarf’s poles.
Credit: ESO/M. Kornmesser, L. Calçada
Micronovae are similar explosions that are smaller in scale and faster, lasting just several hours. They occur on some white dwarfs with strong magnetic fields, which funnel material towards the star’s magnetic poles. “For the first time, we have now seen that hydrogen fusion can also happen in a localized way. The hydrogen fuel can be contained at the base of the magnetic poles of some white dwarfs, so that fusion only happens at these magnetic poles,” says Paul Groot, an astronomer at Radboud University in the Netherlands and co-author of the study.
“This leads to micro-fusion bombs going off, which have about one millionth of the strength of a nova explosion, hence the name micronova,” Groot continues. Although ‘micro’ may imply these events are small, do not be mistaken: just one of these outbursts can burn through about 20,000,000 trillion kg, or about 3.5 billion Great Pyramids of Giza, of material.[1]
This artist’s impression shows a two-star system, with a white dwarf (in the foreground) and a companion star (in the background), where micronovae may occur. The white dwarf steals materials from its companion, which is funneled towards its poles. As the material falls on the hot surface of the white dwarf, it triggers a micronova explosion, contained at one of the star’s poles.
Credit: Mark Garlick
These new micronovae challenge astronomers’ understanding of stellar explosions and may be more abundant than previously thought. “It just goes to show how dynamic the Universe is. These events may actually be quite common, but because they are so fast they are difficult to catch in action,” Scaringi explains.
The team first came across these mysterious micro-explosions when analyzing data from NASA’s Transiting Exoplanet Survey Satellite (TESS). “Looking through astronomical data collected by NASA’s TESS, we discovered something unusual: a bright flash of optical light lasting for a few hours. Searching further, we found several similar signals,” says Degenaar.
This video shows an animation of a micronova explosion. The blue disc swirling around the bright white dwarf in the center of the image is made up of material, mostly hydrogen, stolen from its companion star. Towards the center of the disc, the white dwarf uses its strong magnetic fields to funnel the hydrogen towards its poles. As the material falls on the hot surface of the star, it triggers a micronova explosion, contained by the magnetic fields at one of the white dwarf’s poles.
Credit: ESO/L. Calçada, M. Kornmesser
The team observed three micronovae with TESS: two were from known white dwarfs, but the third required further observations with the X-shooter instrument on ESO’s VLT to confirm its white dwarf status.
“With help from ESO’s Very Large Telescope, we found that all these optical flashes were produced by white dwarfs,” says Degenaar. “This observation was crucial in interpreting our result and for the discovery of micronovae,” Scaringi adds.
This artist’s animation shows a two-star system where one of the components is a normal star and the other is a white dwarf, which appears surrounded by a disc of gas and dust. A white dwarf in a two-star system can steal material, mostly hydrogen, from its companion star if they are close enough together.
Credit: ESO/M. Kornmesser
The discovery of micronovae adds to the repertoire of known stellar explosions. The team now want to capture more of these elusive events, requiring large scale surveys and quick follow-up measurements. “Rapid response from telescopes such as the VLT or ESO’s New Technology Telescope and the suite of available instruments will allow us to unravel in more detail what these mysterious micronovae are,” Scaringi concludes.
Reference: “Localized thermonuclear bursts from accreting magnetic white dwarfs” by S. Scaringi, P. J. Groot, C. Knigge, A. J. Bird, E. Breedt, D. A. H. Buckley, Y. Cavecchi, N. D. Degenaar, D. de Martino, C. Done, M. Fratta, K. Iłkiewicz, E. Koerding, J.-P. Lasota, C. Littlefield, C. F. Manara, M. O’Brien, P. Szkody and F. X. Timmes, 20 April 2022, Nature. DOI: 10.1038/s41586-022-04495-6
Notes
We use trillion to mean a million million (1,000,000,000,000 or 1012) and billion to mean a thousand million (1,000,000,000 or 109). The weight of the Great Pyramid of Giza in Cairo, Egypt (also known as the Pyramid of Khufu or Pyramid of Cheops) is about 5,900,000,000 kg.
More information
This research was presented in a paper title “Localised thermonuclear bursts from accreting magnetic white dwarfs” to appear in Nature. A follow-up letter, titled “Triggering micronovae through magnetically confined accretion flows in accreting white dwarfs” has been accepted for publication in Monthly Notices of the Royal Astronomical Society.
The team on the Nature paper is composed of S. Scaringi (Centre for Extragalactic Astronomy, Department of Physics, Durham University, UK [CEA]), P. J. Groot (Department of Astrophysics, Radboud University, N?megen,the Netherlands [IMAPP] and South African Astronomical Observatory, Cape Town, South Africa [SAAO] and Department of Astronomy, University of Cape Town, South Africa [Cape Town]), C. Knigge (School of Physics and Astronomy, University of Southampton, Southampton, UK [Southampton]), A.J. Bird (Southampton) , E. Breedt (Institute of Astronomy, University of Cambridge, UK), D. A. H. Buckley (SAAO, Cape Town, Department of Physics, University of the Free State, Bloemfontein, South Africa), Y. Cavecchi (Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de México, México), N. D. Degenaar (Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, the Netherlands), D. de Martino (INAF-Osservatorio Astronomico di Capodimonte, Naples, Italy), C. Done (CEA), M. Fratta (CEA), K. Ilkiewicz (CEA), E. Koerding (IMAPP), J.-P. Lasota (Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland and Institut d’Astrophysique de Paris, CNRS et Sorbonne Universités, Paris, France), C. Littlefield (Department of Physics, University of Notre Dame, USA and Department of Astronomy, University of Washington, Seattle, USA [UW]), C. F. Manara (European Southern Observatory, Garching, Germany [ESO]), M. O’Brien (CEA), P. Szkody (UW), F. X. Timmes (School of Earth and Space Exploration, Arizona State University, Arizona, USA, Joint Institute for Nuclear Astrophysics – Center for the Evolution of the Elements, USA).
When NASA sent humans to the moon in 1969, one of the many hazards the agency had to anticipate was space rocks penetrating astronauts' spacesuits or equipment. Unlike Earth, which has a protective atmosphere in which meteoroids usually disintegrate, the moon is vulnerable to whatever rocks, or even specks, are whizzing around in space.
Thankfully, the astronauts weren't in too much danger, according to Bill Cooke, head of NASA's Meteoroid Environment Office at NASA's Marshall Space Flight Center in Alabama. "The odds of an astronaut being hit by a millimeter-sized object is like 1 in 1 million per hour per person," Cooke told Live Science. (A millimeter is the largest a meteoroid has to be to penetrate an astronaut's spacesuit.)
NASA is preparing to send humans back to the moon by 2025 and someday establish a base either orbiting the moon or on its surface, so it's more important than ever to understand the frequency with which our natural satellite experiences an impact.
So how many objects hit the moon every day? What about every year?
The answer depends on the size of the object, Cooke said. NASA's Meteoroid Environment Office studies the space environment around Earth and the moon to understand the flux of meteoroids (space rocks ranging in size from dust to small asteroids about 3 feet, or 1 meter, across), so Cooke is very familiar with what's hitting the moon every day.
For impactors smaller than a millimeter, the number cannot be precisely quantified, but Cooke estimates that 11 to 1,100 tons (10 to 1,000 metric tons) — the mass of about 5.5 cars — of dust collide with the moon per day. For larger rocks, the estimates are clearer.
"There are about 100 pingpong-ball-sized meteoroids hitting the moon per day," Cooke said. That adds up to roughly 33,000 meteoroids per year. Despite their small size, each of these pingpong-ball-size rocks impacts the surface with the force of 7 pounds (3.2 kilograms) of dynamite.
Larger meteoroids hit the moon, too, but less often. Cooke estimates that larger meteoroids, such as ones 8 feet (2.5 meters) across, slam into the moon about every four years. Those objects hit the moon with the force of a kiloton, or 1,000 tons (900 metric tons) of TNT. The moon is about 4.5 billion years old, so it's no wonder its surface is pockmarked with all kinds of craters from these impacts.
Scientists study lunar impacts in a couple of different ways. From Earth's surface, scientists point telescopes toward the moon to observe impacts. Meteoroids can hit the surface at speeds of 45,000 to 160,000 mph (20 to 72 kilometers per second), according to NASA; the impact produces a flash of light that can be observed from Earth.
Scientists can also use spacecraft orbiting the moon itself, such as NASA's Lunar Reconnaissance Orbiter (LRO), to observe the craters left behind by impacts. Because meteoroids move so fast, even an 11-pound (5 kilograms) meteoroid can leave behind a crater 30 feet (9 m) across and hurl 165,000 pounds (75,000 kg) of lunar soil and rocks from the moon's surface, according to NASA. The LRO can easily spot these craters after they form.
Although the moon experiences many impacts per year, that doesn't necessarily preclude a human presence. Considering the moon's surface area is about 14.6 million square miles (38 million square kilometers), "if you pick a square kilometer patch of ground, it will be hit by one of those pingpong-sized meteoroids once every thousand years or so," Cooke said.
So, the odds are good for our future lunar explorers and their spacecraft.
Mahabharata and Ramayana - The War of the Gods with the People?!
Mahabharata and Ramayana - The War of the Gods with the People?!
Mahabharata and Ramayana - The War of the Gods with the People ?! One of the most important questions that humanity has been trying to answer for decades refers to the distant past, was the Earth visited by extraterrestrial entities, or simply there were mysterious earthly civilizations that reached an incredible degree of development. ?
To answer this question, we need to take a look back at the darkest corners of history, which often hide impressive truths about life on Earth over 10,000 years ago. Mahabharata and Ramayana are the books that seem to outline the perfect picture of some mysterious civilizations that lived on our planet many years ago. These two ancient books are also known as the first epics in human history. They are written in Sanskrit and contain over 100,000 verses, divided into 18 chapters. Specialists who have studied them claim that these two enigmatic books are more than a historical narrative, that is, a combination of facts and myths from the ancient world. An interesting passage describes in great detail how over 12,000 years ago, the Earth was inhabited by an extremely advanced civilization from all points of view. For reasons unknown, or perhaps not mentioned in the Mahabharata passage, a large-scale nuclear war has broken out. Historian Kisari Ganguli claims that this story is very real and that it is, in fact, a description of the first nuclear explosion that took place over 12,000 years ago. Also in the verses of the Mahabharata it is related how an airplane or an ancient aircraft launched a projectile, loaded with all the power of the Universe, on two races or civilizations on Earth. No such power had ever been seen before, and the two races had disappeared altogether. The bodies were burned to such an extent that no one could recognize them.
The oldest Indian civilization appeared in the Indus Basin in the 4th - 3rd millennium BC. The most significant discoveries related to this culture were made in Harappa and Mohenjo-Daro, ancient cities located in what is now Pakistan. In the 1950s, English General Cunningham, examining the ruins near the village of Harappa, found a seal with unknown letters. However, excavations began here only in the 1920s. The culture of the newly discovered civilization was called the Harappan or Mohenjo-Daro culture.
The Harappan settlements were located in a vast area: to the east, about as far as Delhi, to the south - to the shores of the Arabian Sea. The Harappan civilization is believed to have existed from the middle of the third century to the middle of the second millennium BC. The high level of development of civilization is highlighted by the strict planning of cities, the presence of writing and works of art. Language and writing have not yet been deciphered, although many stamps with inscriptions have already been found.
Excavations in the Punjab in the 1920s by John Marshall ushered the world into a civilization that can be dated from 2500 to 2000 BC. The main fortress cities of Mohenjo-Daro and Harappa have brought us the main elements of this protohistoric civilization. Both cities were probably the capitals of the empire. A strong and advanced civilization would have flourished if not for a catastrophe that happened suddenly.
Who led it and what served as a prototype for the events of the Mahabharata? What other secrets does India keep? Among the legends of many countries there are references to a certain higher, heavenly weapon. Moreover, a weapon so powerful that, for the first time, a parallel between it and an atomic bomb was drawn by Professor Robert Oppenheimer, when, amazed by what he saw during the nuclear tests, he read aloud an excerpt. from the Mahabharata about a light brighter than a thousand suns.
Dronaparva, one of the Mahabharata books, tells of a battle during which shell explosions, similar to huge fireballs, take place. It also describes the appearance of a cloud of fungi characteristic of a thermonuclear explosion. It is compared to the opening of a huge shadow. After these explosions, the food became poisoned, the survivors became ill.
The Mahabharata provides detailed and highly realistic descriptions of the construction of missiles, aircraft and other devices. The most detailed story is about the old aircraft - the vimanas. Ramayana recounts what the god Rama and his wife Sita saw from above during a flight from Sri Lanka to India. At the same time, the author provides such details that can only be seen from a great height. And the ancient aircraft itself is characterized by incredibly high speed, fully controllable, with rooms with windows and comfortable seats.
Almost half a century has passed since humanity sent the legendary Arecibo message and scientists have created a brand new updated version. But is it a good idea?
The newly proposed “A Beacon in the Galaxy”, a binary message created by scientists as an update to the old Arecibo message, might actually be more dangerous for us than beneficial. It includes key information about us – our location, our DNA structure, and even an image of the naked human body.
Should we give aliens such vital details about Earth and humanity? This question has been around for ages and countless renowned scientists have expressed their concerns in the past. Even Stephen Hawking explained that a hypothetical alien civilization could be hostile.
Is the Beacon in the Galaxy better than the Arecibo message?
While the old radio signal included important information about Earth and humanity, it was more like a postcard with difficult-to-understand images. The new “Beacon in the Galaxy” message was created like a presentation with complex illustrations and explanations.
New universal concept
Scientists believe that complex mathematics might be unrecognizable for any potential alien intelligence while binary has a better chance to be universal. It is the simplest form because it involves simple oppositions – zero/one, yes/no, etc. Therefore, scientists assume that there is a bigger chance that aliens would understand this simple binary code.
Introducing binary and decimal systems
The new message starts with a slide that introduces binary and decimal systems, as well as prime numbers and the largest known prime number.
Particle Physics, DNA Structure, Solar System
Scientists wanted to include all the vital information about Earth and humanity in the smallest possible message. After the introduction of binary in the opening slide, they introduced the main laws of particle physics, the structure of our DNA, as well as the Solar System, and our planet in it.
A quick introduction into particle physics.
Credit: J. H. Jiang et al., 2022
Another slide shows the structure of our DNA.
Credit: J. H. Jiang et al., 2022
Location in the Milky Way and an Invitation to aliens
Scientists used globular clusters in the Milky Way that should be known to hypothetical alien astronomers to pinpoint our location in the galaxy. They also included an invitation to anyone that may find the “Beacon in the Galaxy” message to send one back to us.
How can this message be sent into space?
The team of scientists hopes to use one of two telescopes – the Allen Telescope Array in California or the FAST Telescope in China. This is mainly because these are the two telescopes that SETI researchers use in their work while most other observatories tend to close their doors to this type of work. The other issue, for now, is that both of these observatories can only search for signals and not yet send such into space.
Where will the new message be sent to?
Assuming that the new message gets approved, it will be sent towards a concentric ring that is about 13,000 light-years away from the center of the Milky Way. Scientists noted that it is impossible to guess the right direction for the radio signal. So, they picked a target that has attracted the attention of SETI researchers in the past. Previous studies suggested that if alien life exists somewhere in our galaxy, it would be near the galactic center.
Is there any point in sending more messages to the aliens?
Obviously, we have not received an answer to the Arecibo message which was sent out in 1974 and there is no surprise here. Estimations suggest that if we send the Beacon in the Galaxy, it could take 50,000 years before we get a hypothetical answer. In truth, experts hope to find signs of alien life using other more advanced and quicker methods.
Could such a message be dangerous for humanity?
How can we know if hypothetical alien civilizations would be peaceful or hostile? This argument has been around for decades since before the original Arecibo Message. What if send key information about humanity such as our location and technological level and the extraterrestrial intelligence that intercepts it wants war. My imagination can come up with various scenarios in which such a message could have a devastating result but what do you think?
Perhaps alien civilizations already know about us?
Messages like Arecibo and Beacon in the Galaxy are just a couple of examples and scientists have sent multiple other signals into space in the past. Moreover, we have practically been broadcasting our existence ever since humanity started transmitting radio waves. In other words, alien intelligence can notice us even without such messages. If alien astronomers use the same or at least similar techniques to detect technosignatures and biosignatures, they would have already found us by now.
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Sources:
Hood, A. L. (2022, March 31). NASA scientist creates new message for aliens, including human DNA. Futurism.
Jiang, J. H., Li, H., Chong, M., Jin, Q., Rosen, P. E., Jiang, X., Fahy, K. A., Taylor, S. F., Kong, Z., Hah, J., & Zhu, Z.-H. (2022, March 24). A beacon in the galaxy: Updated arecibo message for potential fast and SETI Projects. arXiv.org.
Oberhaus, D. (2022, March 30). Researchers made a new message for extraterrestrials. Scientific American.
Williams, M. (2022, March 29). Astronomers come up with a new message to let the aliens know we’re here. Universe Today.
The bright supernova SN 2018gv explodes in the spiral galaxy NGC 2525 in this Hubble Space Telescope image.
NASA, ESA, A. Riess and the SH0ES team
In the year 1054, a new star appeared in the constellation Taurus. The faint speck of light brightened rapidly, soon outshining other imposing stars in the northern sky. In a matter of days, the star’s brightness peaked. It stayed visible for weeks, even during the day, before it started to dim and slowly fade into nothingness.
The baffling star that embellished the sky in 1054 was in fact a supernova, just one of many transient sources appearing in the sky — that is, objects related to events that occur on short timescales, often changing visibly from night to night. Taking many forms and colors, some transients originate in the Milky Way, while others are objects exploding in galaxies far away.
The interest in transients has never been greater. Many surveys of the sky are discovering new sources at unprecedented rates. In 2019, astronomers reported about 20,000 newly discovered transient objects at visible wavelengths, about 100 times greater than a decade prior.
This firehose of data has the potential to transform astronomy and provide insight into subjects ranging from dark energy and dark matter to the evolution of our solar system. But it also presents unique challenges — how to make sense of the data, and how to follow up on it.
When a trickle becomes a flood
Surveys find transients by imaging the same parts of the sky with a certain cadence. A sequence of images reveals new sources and their change in brightness over time. Such information is not always enough to classify a transient. For that, one would need to obtain a spectrum of the transient, and perhaps even observe it at infrared, X-rays, or radio wavelengths.
However, the era when astronomers could follow up on every object that came along has already gone away — there are now simply too many being found. “We’re already for many years in a regime when you have to make choices [about] what you classify spectroscopically and what you don’t, and that depends on science,” says Daniel Perley, a researcher at Liverpool John Moores University in the U.K. It is telling that the community obtained the spectra for only about 10 percent of transients discovered in 2019.
Perley’s goal is to take stock of the bright transient population detected by the Zwicky Transient Facility (ZTF), which has been one of the most productive transient surveys since it began operating in 2018, spotting supernovae and fast-moving asteroids alike. By limiting the study to the brightest sources, it is feasible to take useful spectra of every object in the survey and learn, for example, how many supernovae of a certain spectral type explode in the universe.
Scientists interested in particular types of transients, like those exhibiting an especially red or blue color, have to take a different approach. For them, the initial limited amount of information determines whether a transient merits a long follow-up observation campaign. Their decision to use additional resources on a transient is based on experience, yet it always carries a bit of risk — you don’t really know a transient until you take that additional observation.
The Vera Rubin Observatory will see more than 40 times the area of the full moon. The large field of view combined with a large 8-meter mirror make the observatory a powerful machine for finding transients.
Rubin Obs/NSF/AURA
Searching for anomalies
That experience from ZTF and other transient facilities will come in handy once the Vera C. Rubin Observatory in Chile comes online in a few years. “The Rubin Observatory is going to increase the discovery rate by two orders of magnitude, from 10,000 per year to a million new supernovae and transients per year,” says Ashley Villar, an assistant professor at the Pennsylvania State University. “This is a breaking point for our field.”
The flood of transients discovered by the Rubin Observatory will include specimens that current surveys rarely find, such as very distant supernovae or very faint supernovae exploding in nearby galaxies. Scientists expect that the observatory will also discover completely new types of transients.
According to expectations, less than 0.1 percent of all transients discovered by the Rubin Observatory will get extra attention. Developing reliable techniques to recognize interesting transients in the clutter is therefore of paramount importance.
Villar plans to use a neural network, a type of machine learning, to search the data for anomalous transients with unanticipated properties. But she expects researchers will employ a wide variety of strategies to work with such massive datasets. “Some people will lean towards totally automated queue systems that just rank targets, look at their observability, and make some intelligent choice,” says Villar. “Others will want to have humans in the loops, looking at the data, asking simple questions, and deciding from there.”
Some transients emit light at different wavelengths. This timeline shows the observations of the neutron star merger GW170817. The merger emitted gravitational waves, followed by light spanning the electromagnetic spectrum
Abbott et al. (2017)
Some kinds of transients stand out based on the wavelengths of radiation they they emit — which can range from gamma rays to radio waves — and how their brightness changes over time. That means that searches tailored towards these particular kinds of transients can avoid the classification and follow-up problems encountered in searches at optical wavelengths.
For instance, fast radio bursts — immensely powerful blasts of radio waves possibly caused by flaring magnetars — are immediately distinguishable. “You can already tell from the first discovery that it’s a fast radio burst, approximately how far away it’s coming from, and its energetics,” says Emily Petroff, a radio astronomer at the University of Amsterdam.
Avoiding interference
While the transient field is flourishing, a threat looms on the horizon: the rise of light pollution across the electromagnetic spectrum. For instance, radio telescopes searching for transients are sensitive to emissions from phones, cars, airplanes, and various kinds of satellites. And the problem is getting worse. “We’re constantly playing the game of cat and mouse with new sources of interference that we’re finding at our telescope sites,” says Petroff.
So far, optical astronomers have been able to escape the pollution by observing from remote and dark oases. However, the recent upsurge in bright commercial satellites — like SpaceX’s Starlink constellation — is already disturbing observations. The anticipated fleet of satellites, which numbers in the tens of thousands, profoundly worries the community. The Rubin Observatory, in particular, has been developing a multi-pronged approach to mitigate its impact, working with SpaceX to reduce the reflectivity of its satellites and also developing algorithms to remove satellite trails from images.
It is easy enough to point a telescope at the sky. But to make sense of all the blinking lights, both cosmic and artificial, astronomers are adapting and developing clever techniques. And it is worth it, because one of those lights could turn out to be something unlike anything we have seen before.
Imagine standing on Mars, and seeing this with your own eyes.
The Perseverance rover watched as the potato-shaped moon Phobos passed in front of the Sun, from the vantage point of Jezero Crater on Mars. Perseverance used its high-resolution Mastcam-Z camera system to shoot video of Phobos, and NASA says the result is the most zoomed-in, highest frame-rate observation of a Phobos solar eclipse ever taken from the Martian surface.
The stunning eclipse took place on April 2, 2022 (Earth date, of course) and the eclipse lasted a little over 40 seconds. That means this video is very close to what Perseverance witnessed in real time. The time it takes for Phobos eclipse the Sun is much less time than a typical solar eclipse involving Earth’s Moon, since Phobos is about 157 times smaller than our own Moon. The Mastcam-Z has special solar filters that allow it to stare directly at the Sun. The video is of such high resolution, that even sunspots are visible on the Sun.
Scientists say that each time these eclipses are observed, it allow them to measure subtle shifts in Phobos’ orbit over time. The moon’s tidal forces pull on the deep interior of the Red Planet, as well as its crust and mantle, and so studying how much Phobos shifts over time reveals something about how resistant the crust and mantle are, and thus what kinds of materials they’re made of.
In 1930, astronomer Clyde Tombaugh discovered the fabled “Ninth Planet” (or “Planet X”) while working at the Lowell Observatory in Flagstaff, Arizona. The existence of this body had been predicted previously based on perturbations in the orbit of Uranus and Neptune. After receiving more than 1,000 suggestions from around the world, and a debate among the Observatory’s staff, this newfound object was named Pluto – which was proposed by a young schoolgirl from Oxford (Venetia Burney).
Since that time, Pluto has been the subject of considerable study, a naming controversy, and was visited for the first time on January 1st, 2019, by the New Horizons mission. One thing that has been clear from the beginning is the nature of Pluto’s orbit, which is highly eccentric and inclined. According to new research, Pluto’s orbit is relatively stable over longer timescales but is subject to chaotic perturbance and changes over shorter timescales.
To break it down, Pluto’s orbit is radically different from those of the planets, which follow nearly circular orbits around the Sun close to its equator, projected outward (aka. the ecliptic). In contrast, it takes 248 years for Pluto to complete a single orbit around the Sun and follows a highly-elliptical orbit that is inclined 17° to the Solar System’s ecliptic plane. The eccentric nature of its orbit also means that Pluto spends 20 years during each period orbiting closer to the Sun than Neptune.
The nature of Pluto’s orbit is an enduring mystery and something that astronomers became aware of very shortly after it was discovered. Since then, multiple efforts have been made to simulate the past and future of its orbit, which revealed a surprising property that protects Pluto from colliding with Neptune. As Dr. Malhotra told Universe Today via email, this is the orbital resonance condition known as a “mean motion resonance”:
“This condition ensures that at the time that Pluto is at the same heliocentric distance as Neptune, its longitude is nearly 90 degrees away from Neptune’s. Later another peculiar property of Pluto’s orbit was discovered: Pluto comes to perihelion at a location well above the plane of Neptune’s orbit; this is a different type of orbital resonance known as the ‘vZLK oscillation.’”
This abbreviation refers to von Zeipel, Lidov, and Kozai, who studied this phenomenon as part of the “three-body problem.” This problem consists of taking the initial positions and velocities of three massive objects (since extended to include particles) and solving for their subsequent motion according to Newton’s Three Laws of Motion and his Theory of Universal Gravitation – for which there is no general solution. As Dr. Malhotra added:
“In the late-1980s, with the availability of more powerful computers, numerical simulations revealed a third peculiar property, that Pluto’s orbit is technically chaotic, that is, small deviations of initial conditions lead to exponential divergence of the orbital solutions over tens of millions of years. However, this chaos is limited. It has been found in numerical simulations that the two special properties of Pluto’s orbit mentioned above persist over gigayear timescales, making its orbit remarkably stable, despite the chaos indicators.”
Comparison between the eight largest TNOs with Earth (all to scale).
Credit: NASA/Lexicon
For their study, Malhotra and Ito conducted numerical simulations of Pluto’s orbit for up to five billion years into the future of the Solar System.
In particular, they hoped to address unresolved questions about the peculiar orbits of Pluto and other Pluto-sized objects (aka. Plutinos). These questions have been addressed by research conducted during the past few decades, such as “planet migration theory,” but have only to a point. In particular, they hoped to address unresolved questions about the peculiar orbits of Pluto and other Pluto-sized objects (aka. Plutinos). In the past few decades, astronomers have attempted to address these questions with new theories (such as “planet migration theory”) but were met with limited success.
In this hypothesis, Pluto was pulled into its current mean motion resonance by Neptune, which migrated during the Solar System’s early history. A major prediction of this theory is that other Trans-Neptunian Objects (TNOs) would share the same resonance condition, which has since been verified with the discovery of large numbers of Plutinos. This discovery has also led to the more widespread acceptance of planet migration theory. But as Dr. Malhotra explained:
“Pluto’s orbital inclination is closely linked to its vZLK oscillation. So we reasoned that if we could understand better the conditions for Pluto’s vZLK oscillation, perhaps we could solve the mystery of its inclination. We started by investigating the individual role of the other giant planets (Jupiter, Saturn and Uranus) on Pluto’s orbit.”
To do this, Dr. Malhotra and Ito ran computer simulations where they simulated the orbital evolution of Pluto for up to 5 billion years that included eight different combinations of giant planet perturbation. These N-body simulations included interactions with:
Neptune (—NP)
Uranus and Neptune (–UNP)
Saturn and Neptune (-S-NP)
Jupiter and Neptune (J–NP)
Saturn, Uranus and Neptune (-SUNP)
Jupiter, Uranus, and Neptune (J-UNP)
Jupiter, Saturn, and Neptune (JS-NP)
Jupiter, Saturn, Uranus, and Neptune (JSUNP)
New Horizons trajectory and the orbits of Pluto and 2014 MU69.
“We found no subsets of the inner three giant planets would do to recover Pluto’s vZLK oscillation; all three – Jupiter, Saturn, and Uranus – were necessary,” said Dr. Malhotra. “But what is it about these planets that [are] essential to Pluto’s vZLK oscillation?” Dr. Malhotra added. “There are 21 parameters needed to represent the gravitational forces of Jupiter, Saturn, and Uranus on Pluto. This is a prohibitively large parameter space to explore.”
To simplify these calculations, Dr. Malhotra and Ito collapsed these into a single parameter by introducing some simplifications. This included representing each planet with a circular ring of uniform density, a total mass equal to the planet’s, and a ring radius equal to the planet’s average distance from the Sun (aka. semimajor axis). As Dr. Malhotra indicated, this yielded a single parameter representing the effect of Jupiter, Saturn, and Uranus (J2), which was equivalent to the effect of an “oblate Sun.”
“[W]e discovered a fortuitous arrangement of the masses and orbits of the giant planets that delineates a narrow range in the J2 parameter in which Pluto’s vZLK oscillation is possible, a kind of ‘Goldilock’s zone,’” she said. “This result indicates that, during the planet migration era in [the] Solar System’s history, the conditions for Trans-Neptunian objects changed in such a way as to promote many of them – including Pluto – into the vZLK oscillation state. It is likely that Pluto’s inclination originated during this dynamical evolution.”
These results are likely to have significant implications for future studies of the outer Solar System and its orbital dynamics. With further study, Dr. Malhotra believes that astronomers will learn more about the migration history of the giant planets and how they eventually settled into their current orbits. It could also lead to the discovery of a novel dynamical mechanism that will explain the origins of Pluto’s orbit and other bodies with high orbital inclinations.
This will be especially useful to astronomers dedicated to the study of Solar System dynamics. As Dr. Malhorta noted, researchers in this field were beginning to suspect that evidence that might shed light on Pluto’s orbital evolution might have been erased by the instabilities and chaotic nature of these same orbital mechanics. As Dr. Malhotra summarized:
“I think that our work raises new hope for making connection between present-day solar system dynamics and historical solar system dynamics. The origin of the orbital inclinations of minor planets throughout the solar system – including the TNOs – presents a major unsolved problem; perhaps our work will stimulate more attention to it.
“Another point that our study underscores is the value of simple(r) approximations for a complicated problem: i.e., collapsing 21 parameters into a single parameter opened the door to getting at the essential dynamical mechanisms affecting the very interesting but difficult-to-understand orbital dynamics of Pluto and Plutinos.”
The Bob Lazar Lost Tapes! Exclusive World Exclusive! Buckle Up!
The Bob Lazar Lost Tapes! Exclusive World Exclusive! Buckle Up!
The Bob Lazar Lost Tapes! Exclusive World Exclusive! Buckle Up!
Almost 30 Years Later, Audio Tapes NEVER BEFORE Heard, UNTIL NOW! Michael Schratt shares Incredible Historical Evidence Exclusively to Thirdphaseofmoon!
Drone Records UFO Over Ocean In Scotland, 1-30-2019, UFO Sighting News.
Drone Records UFO Over Ocean In Scotland, 1-30-2019, UFO Sighting News.
Date of sighting:Jan 30, 2019
Location of sighting: Fifth of Forth, Scotland
The eyewitness is a person who often records beautiful video using his drone. Here he caught some raw footage of a white disk shooting towards and below his drone at incredible speed. When the video is slowed down, I see it is a white disk. The UFO was coming from some smokestacks in the distance, which leads me to think the UFO was gathering data about the pollutants humans put into the air. When it shot toward the drone, it was no accident. The UFO was investigating the technology of the drone to record its tech in order to predict when humans will one day leave earth and create cities on other planets. Yes, aliens collect data and predict the future with it...and really accurately too.
Could aliens already be living with us? A farmer finds a mysterious creature that has never been seen before on earth, a woman claims to have been fathered by extraterrestrial life and in Nevada, a US serviceman claims to be friends with aliens living at a secret base. William Shatner believes aliens have infiltrated the human race, do you?
James Johnson hopes to drive a car again one day. If he does, he will do it using only his thoughts.
In March 2017, Johnson broke his neck in a go-carting accident, leaving him almost completely paralysed below the shoulders. He understood his new reality better than most. For decades, he had been a carer for people with paralysis. “There was a deep depression,” he says. “I thought that when this happened to me there was nothing — nothing that I could do or give.”
But then Johnson’s rehabilitation team introduced him to researchers from the nearby California Institute of Technology (Caltech) in Pasadena, who invited him to join a clinical trial of a brain–computer interface (BCI). This would first entail neurosurgery to implant two grids of electrodes into his cortex. These electrodes would record neurons in his brain as they fire, and the researchers would use algorithms to decode his thoughts and intentions. The system would then use Johnson’s brain activity to operate computer applications or to move a prosthetic device. All told, it would take years and require hundreds of intensive training sessions. “I really didn’t hesitate,” says Johnson.
The first time he used his BCI, implanted in November 2018, Johnson moved a cursor around a computer screen. “It felt like The Matrix,” he says. “We hooked up to the computer, and lo and behold I was able to move the cursor just by thinking.”
Johnson has since used the BCI to control a robotic arm, use Photoshop software, play ‘shoot-’em-up’ video games, and now to drive a simulated car through a virtual environment, changing speed, steering and reacting to hazards. “I am always stunned at what we are able to do,” he says, “and it’s frigging awesome.”
Johnson is one of an estimated 35 people who have had a BCI implanted long-term in their brain. Only around a dozen laboratories conduct such research, but that number is growing. And in the past five years, the range of skills these devices can restore has expanded enormously. Last year alone, scientists described a study participant using a robotic arm that could send sensory feedback directly to his brain1; a prosthetic speech device for someone left unable to speak by a stroke2; and a person able to communicate at record speeds by imagining himself handwriting3.
So far, the vast majority of implants for recording long-term from individual neurons have been made by a single company: Blackrock Neurotech, a medical-device developer based in Salt Lake City, Utah. But in the past seven years, commercial interest in BCIs has surged. Most notably, in 2016, entrepreneur Elon Musk launched Neuralink in San Francisco, California, with the goal of connecting humans and computers. The company has raised US$363 million. Last year, Blackrock Neurotech and several other newer BCI companies also attracted major financial backing.
Bringing a BCI to market will, however, entail transforming a bespoke technology, road-tested in only a small number of people, into a product that can be manufactured, implanted and used at scale. Large trials will need to show that BCIs can work in non-research settings and demonstrably improve the everyday lives of users — at prices that the market can support. The timeline for achieving all this is uncertain, but the field is bullish. “For thousands of years, we have been looking for some way to heal people who have paralysis,” says Matt Angle, founding chief executive of Paradromics, a neurotechnology company in Austin, Texas. “Now we’re actually on the cusp of having technologies that we can leverage for those things.”
Interface evolution
In June 2004, researchers pressed a grid of electrodes into the motor cortex of a man who had been paralysed by a stabbing. He was the first person to receive a long-term BCI implant. Like most people who have received BCIs since, his cognition was intact. He could imagine moving, but he had lost the neural pathways between his motor cortex and his muscles. After decades of work in many labs in monkeys, researchers had learnt to decode the animals’ movements from real-time recordings of activity in the motor cortex. They now hoped to infer a person’s imagined movements from brain activity in the same region.
In 2006, a landmark paper4 described how the man had learnt to move a cursor around a computer screen, control a television and use robotic arms and hands just by thinking. The study was co-led by Leigh Hochberg, a neuroscientist and critical-care neurologist at Brown University in Providence, Rhode Island, and at Massachusetts General Hospital in Boston. It was the first of a multicentre suite of trials called BrainGate, which continues today.
“It was a very simple, rudimentary demonstration,” Hochberg says. “The movements were slow or imprecise — or both. But it demonstrated that it might be possible to record from the cortex of somebody who was unable to move and to allow that person to control an external device.”
Today’s BCI users have much finer control and access to a wider range of skills. In part, this is because researchers began to implant multiple BCIs in different brain areas of the user and devised new ways to identify useful signals. But Hochberg says the biggest boost has come from machine learning, which has improved the ability to decode neural activity. Rather than trying to understand what activity patterns mean, machine learning simply identifies and links patterns to a user’s intention.
“We have neural information; we know what that person who is generating the neural data is attempting to do; and we’re asking the algorithms to create a map between the two,” says Hochberg. “That turns out to be a remarkably powerful technique.”
Motor independence
Asked what they want from assistive neurotechnology, people with paralysis most often answer “independence”. For people who are unable to move their limbs, this typically means restoring movement.
One approach is to implant electrodes that directly stimulate the muscles of a person’s own limbs and have the BCI directly control these. “If you can capture the native cortical signals related to controlling hand movements, you can essentially bypass the spinal-cord injury to go directly from brain to periphery,” says Bolu Ajiboye, a neuroscientist at Case Western Reserve University in Cleveland, Ohio.
In 2017, Ajiboye and his colleagues described a participant who used this system to perform complex arm movements, including drinking a cup of coffee and feeding himself5. “When he first started the study,” Ajiboye says, “he had to think very hard about his arm moving from point A to point B. But as he gained more training, he could just think about moving his arm and it would move.” The participant also regained a sense of ownership of the arm.
Ajiboye is now expanding the repertoire of command signals his system can decode, such as those for grip force. He also wants to give BCI users a sense of touch, a goal being pursued by several labs.
In 2015, a team led by neuroscientist Robert Gaunt at the University of Pittsburgh in Pennsylvania, reported implanting an electrode array in the hand region of a person’s somatosensory cortex, where touch information is processed6. When they used the electrodes to stimulate neurons, the person felt something akin to being touched.
Gaunt then joined forces with Pittsburgh colleague Jennifer Collinger, a neuroscientist advancing the control of robotic arms by BCIs. Together, they fashioned a robotic arm with pressure sensors embedded in its fingertips, which fed into electrodes implanted in the somatosensory cortex to evoke a synthetic sense of touch1. It was not an entirely natural feeling — sometimes it felt like pressure or being prodded, other times it was more like a buzzing, Gaunt explains. Nevertheless, tactile feedback made the prosthetic feel much more natural to use, and the time it took to pick up an object was halved, from roughly 20 seconds to 10.
Implanting arrays into brain regions that have different roles can add nuance to movement in other ways. Neuroscientist Richard Andersen — who is leading the trial at Caltech in which Johnson is participating — is trying to decode users’ more-abstract goals by tapping into the posterior parietal cortex (PPC), which forms the intention or plan to move7. That is, it might encode the thought ‘I want a drink’, whereas the motor cortex directs the hand to the coffee, then brings the coffee to the mouth.
Andersen’s group is exploring how this dual input aids BCI performance, contrasting use of the two cortical regions alone or together. Unpublished results show that Johnson’s intentions can be decoded more quickly in the PPC, “consistent with encoding the goal of the movement”, says Tyson Aflalo, a senior researcher in Andersen’s laboratory. Motor-cortex activity, by contrast, lasts throughout the whole movement, he says, “making the trajectory less jittery”.
This new type of neural input is helping Johnson and others to expand what they can do. Johnson uses the driving simulator, and another participant can play a virtual piano using her BCI.
Movement into meaning
“One of the most devastating outcomes related to brain injuries is the loss of ability to communicate,” says Edward Chang, a neurosurgeon and neuroscientist at the University of California, San Francisco. In early BCI work, participants could move a cursor around a computer screen by imagining their hand moving, and then imagining grasping to ‘click’ letters — offering a way to achieve communication. But more recently, Chang and others have made rapid progress by targeting movements that people naturally use to express themselves.
The benchmark for communication by cursor control — roughly 40 characters per minute8 — was set in 2017 by a team led by Krishna Shenoy, a neuroscientist at Stanford University in California.
Then, last year, this group reported3 an approach that enabled study participant Dennis Degray, who can speak but is paralysed from the neck down, to double the pace.
Shenoy’s colleague Frank Willett suggested to Degray that he imagine handwriting while they recorded from his motor cortex (see ‘Turning thoughts into type’). The system sometimes struggled to parse signals relating to letters that are handwritten in a similar way, such as r, n and h, but generally it could easily distinguish the letters. The decoding algorithms were 95% accurate at baseline, but when autocorrected using statistical language models that are similar to predictive text in smartphones, this jumped to 99%.
“You can decode really rapid, very fine movements,” says Shenoy, “and you’re able to do that at 90 characters per minute.”
Degray has had a functional BCI in his brain for nearly 6 years, and is a veteran of 18 studies by Shenoy’s group. He says it’s remarkable how effortless tasks become. He likens the process to learning to swim, saying, “You thrash around a lot at first, but all of a sudden, everything becomes understandable.”
Chang’s approach to restoring communication focuses on speaking rather than writing, albeit using a similar principle. Just as writing is formed of distinct letters, speech is formed of discrete units called phonemes, or individual sounds. There are around 50 phonemes in English, and each is created by a stereotyped movement of the vocal tract, tongue and lips.
Chang’s group first worked on characterizing the part of the brain that generates phonemes and, thereby, speech — an ill-defined region called the dorsal laryngeal cortex. Then, the researchers applied these insights to create a speech-decoding system that displayed the user’s intended speech as text on a screen. Last year, they reported2 that this device enabled a person left unable to talk by a brainstem stroke to communicate, using a preselected vocabulary of 50 words and at a rate of 15 words per minute. “The most important thing that we’ve learnt,” Chang says, “is that it’s no longer a theoretical; it’s truly possible to decode full words.”
Unlike other high-profile BCI breakthroughs, Chang didn’t record from single neurons. Instead, he used electrodes placed on the cortical surface that detect the averaged activity of neuronal populations. The signals are not as fine-grained as those from electrodes implanted in the cortex, but the approach is less invasive.
The most profound loss of communication occurs in people in a completely locked-in state, who remain conscious but are unable to speak or move. In March, a team including neuroscientist Ujwal Chaudhary and others at the University of Tübingen, Germany, reported9 restarting communication with a man who has amyotrophic lateral sclerosis (ALS, or motor neuron disease). The man had previously relied on eye movements to communicate, but he gradually lost the ability to move his eyes.
The team of researchers gained consent from the man’s family to implant a BCI and tried asking him to imagine movements to use his brain activity to choose letters on a screen. When this failed, they tried playing a sound that mimicked the man’s brain activity — a higher tone for more activity, lower for less — and taught him to modulate his neural activity to heighten the pitch of a tone to signal ‘yes’ and to lower it for ‘no’. That arrangement allowed him to pick out a letter every minute or so.
The method differs from that in a paper10 published in 2017, in which Chaudhary and others used a non-invasive technique to read brain activity. Questions were raised about the work and the paper was retracted, but Chaudhary stands by it.
These case studies suggest that the field is maturing rapidly, says Amy Orsborn, who researches BCIs in non-human primates at the University of Washington in Seattle. “There’s been a noticeable uptick in both the number of clinical studies and of the leaps that they’re making in the clinical space,” she says. “What comes along with that is the industrial interest”.
Lab to market
Although such achievements have attracted a flurry of attention from the media and investors, the field remains a long way from improving day-to-day life for people who’ve lost the ability to move or speak. Currently, study participants operate BCIs in brief, intensive sessions; nearly all must be physically wired to a bank of computers and supervised by a team of scientists working constantly to hone and recalibrate the decoders and associated software. “What I want,” says Hochberg, speaking as a critical-care neurologist, “is a device that is available, that can be prescribed, that is ‘off the shelf’ and can be used quickly.” In addition, such devices would ideally last users a lifetime.
Many leading academics are now collaborating with companies to develop marketable devices. Chaudhary, by contrast, has co-founded a not-for-profit company, ALS Voice, in Tübingen, to develop neurotechnologies for people in a completely locked-in state.
Blackrock Neurotech’s existing devices have been a mainstay of clinical research for 18 years, and it wants to market a BCI system within a year, according to chairman Florian Solzbacher. The company came a step closer last November, when the US Food and Drug Administration (FDA), which regulates medical devices, put the company’s products onto a fast-track review process to facilitate developing them commercially.
This possible first product would use four implanted arrays and connect through wires to a miniaturized device, which Solzbacher hopes will show how people’s lives can be improved. “We’re not talking about a 5, 10 or 30% improvement in efficacy,” he says. “People can do something they just couldn’t before.”
Blackrock Neurotech is also developing a fully implantable wireless BCI intended to be easier to use and to remove the need to have a port in the user’s cranium. Neuralink and Paradromics have aimed to have these features from the outset in the devices they are developing.
These two companies are also aiming to boost signal bandwidth, which should improve device performance, by increasing the number of recorded neurons. Paradromics’s interface — currently being tested in sheep — has 1,600 channels, divided between 4 modules.
Neuralink’s system uses very fine, flexible electrodes, called threads, that are designed to both bend with the brain and to reduce immune reactions, says Shenoy, who is a consultant and adviser to the company. The aim is to make the device more durable and recordings more stable. Neuralink has not published any peer-reviewed papers, but a 2021 blogpost reported the successful implantation of threads in a monkey’s brain to record at 1,024 sites (see go.nature.com/3jt71yq). Academics would like to see the technology published for full scrutiny, and Neuralink has so far trialled its system only in animals. But, Ajiboye says, “if what they’re claiming is true, it’s a game-changer”.
Just one other company besides Blackrock Neurotech has implanted a BCI long-term in humans — and it might prove an easier sell than other arrays. Synchron in New York City has developed a ‘stentrode’ — a set of 16 electrodes fashioned around a blood-vessel stent11. Fitted in a day in an outpatient setting, this device is threaded through the jugular vein to a vein on top of the motor cortex. First implanted in a person with ALS in August 2019, the technology was put on a fast-track review path by the FDA a year later.
Akin to the electrodes Chang uses, the stentrode lacks the resolution of other implants, so can’t be used to control complex prosthetics. But it allows people who cannot move or speak to control a cursor on a computer tablet, and so to text, surf the Internet and control connected technologies.
Synchron’s co-founder, neurologist Thomas Oxley, says the company is now submitting the results of a four-person feasibility trial for publication, in which participants used the wireless device at home whenever they chose. “There’s nothing sticking out of the body. And it’s always working,” says Oxley. The next step before applying for FDA approval, he says, is a larger-scale trial to assess whether the device meaningfully improves functionality and quality of life.
Challenges ahead
Most researchers working on BCIs are realistic about the challenges before them. “If you take a step back, it is really more complicated than any other neurological device ever built,” says Shenoy. “There’s probably going to be some hard growing years to mature the technology even more.”
Orsborn stresses that commercial devices will have to work without expert oversight for months or years — and that they need to function equally well in every user. She anticipates that advances in machine learning will address the first issue by providing recalibration steps for users to implement. But achieving consistent performance across users might present a greater challenge.
“Variability from person to person is the one where I don’t think we know what the scope of the problem is,” Orsborn says. In non-human primates, even small variations in electrode positioning can affect which circuits are tapped. She suspects there are also important idiosyncrasies in exactly how different individuals think and learn — and the ways in which users’ brains have been affected by their various conditions.
Finally, there is widespread acknowledgement that ethical oversight must keep pace with this rapidly evolving technology. BCIs present multiple concerns, from privacy to personal autonomy. Ethicists stress that users must retain full control of the devices’ outputs. And although current technologies cannot decode people’s private thoughts, developers will have records of users’ every communication, and crucial data about their brain health. Moreover, BCIs present a new type of cybersecurity risk.
There is also a risk to participants that their devices might not be supported forever, or that the companies that manufacture them fold. There are already instances in which users were let down when their implanted devices were left unsupported.
Degray, however, is eager to see BCIs reach more people. What he would like most from assistive technology is to be able to scratch his eyebrow, he says. “Everybody looks at me in the chair and they always say, ‘Oh, that poor guy, he can’t play golf any more.’ That’s bad. But the real terror is in the middle of the night when a spider walks across your face. That’s the bad stuff.”
For Johnson, it’s about human connection and tactile feedback; a hug from a loved one. “If we can map the neurons that are responsible for that and somehow filter it into a prosthetic device some day in the future, then I will feel well satisfied with my efforts in these studies.”
While working on his doctorate in theoretical physics in the early 1970s, Saul Teukolsky solved a problem that seemed purely hypothetical. Imagine a black hole, the ghostly knot of gravity that forms when, say, a massive star burns out and collapses to an infinitesimal point. Suppose you perturb it, as you might strike a bell. How does the black hole respond?
Teukolsky, then a graduate student at the California Institute of Technology (Caltech), attacked the problem with pencil, paper, and Albert Einstein's theory of gravity, general relativity. Like a bell, the black hole would oscillate at one main frequency and multiple overtones, he found. The oscillations would quickly fade as the black hole radiated gravitational waves—ripples in the fabric of space itself. It was a sweet problem, says Teukolsky, now at Cornell University. And it was completely abstract—until 5 years ago.
In February 2016, experimenters with the Laser Interferometer Gravitational-Wave Observatory (LIGO), a pair of huge instruments in Louisiana and Washington, reported the first observation of fleeting gravitational ripples, which had emanated from two black holes, each about 30 times as massive as the Sun, spiraling into each other 1.3 billion light-years away. LIGO even sensed the "ring down": the shudder of the bigger black hole produced by the merger. Teukolsky's old thesis was suddenly cutting-edge physics.
"The thought that anything I did would ever have implications for anything measurable in my lifetime was so far-fetched that the last 5 years have seemed like living in a dream world," Teukolsky says. "I have to pinch myself, it doesn't feel real."
Fantastical though it may seem, scientists can now study black holes as real objects. Gravitational wave detectors have spotted four dozen black hole mergers since LIGO's breakthrough detection. In April 2019, an international collaboration called the Event Horizon Telescope (EHT) produced the first image of a black hole. By training radio telescopes around the globe on the supermassive black hole in the heart of the nearby galaxy Messier 87 (M87), EHT imaged a fiery ring of hot gas surrounding the black hole's inky "shadow." Meanwhile, astronomers are tracking stars that zip close to the black hole in the center of our own Galaxy, following paths that may hold clues to the nature of the black hole itself.
The observations are already challenging astrophysicists' assumptions about how black holes form and influence their surroundings. The smaller black holes detected by LIGO and, now, the European gravitational wave detector Virgo in Italy have proved heavier and more varied than expected, straining astrophysicists' understanding of the massive stars from which they presumably form. And the environment around the supermassive black hole in our Galaxy appears surprisingly fertile, teeming with young stars not expected to form in such a maelstrom. But some scientists feel the pull of a more fundamental question: Are they really seeing the black holes predicted by Einstein's theory?
Some theorists say the answer is most likely a ho-hum yes. "I don't think we're going to learn anything more about general relativity or the theory of black holes from any of this," says Robert Wald, a gravitational theorist at the University of Chicago. Others aren't so sure. "Are black holes strictly the same as you would expect with general relativity or are they different?" asks Clifford Will, a gravitational theorist at the University of Florida. "That's going to be a major thrust of future observations." Any anomalies would require a rethink of Einstein's theory, which physicists suspect is not the final word on gravity, as it doesn't jibe with the other cornerstone of modern physics, quantum mechanics.
Even though it's very unlikely, it would be so amazingly important if we found that there was any deviation [from general relativity].
SEAN CARROLL
CALIFORNIA INSTITUTE OF TECHNOLOGY
Using multiple techniques, researchers are already gaining different, complementary views of these strange objects, says Andrea Ghez, an astrophysicist at the University of California, Los Angeles, who shared the 2020 Nobel Prize in Physics for inferring the existence of the supermassive black hole in the heart of our Galaxy. "We're still a long way from putting a complete picture together," she says, "but we're certainly getting more of the puzzle pieces in place."
CONSISTING OF PURE gravitational energy, a black hole is a ball of contradictions. It contains no matter, but, like a bowling ball, possesses mass and can spin. It has no surface, but has a size. It behaves like an imposing, weighty object, but is really just a peculiar region of space.
Or so says general relativity, which Einstein published in 1915. Two centuries earlier, Isaac Newton had posited that gravity is a force that somehow reaches through space to attract massive objects to one another. Einstein went deeper and argued that gravity arises because massive things such as stars and planets warp space and time—more accurately, spacetime—causing the trajectories of freely falling objects to curve into, say, the parabolic arc of a thrown ball.
Early predictions of general relativity differed only slightly from those of Newton's theory. Whereas Newton predicted that a planet should orbit its star in an ellipse, general relativity predicts that the orientation of the ellipse should advance slightly, or precess, with each orbit. In the first triumph of the theory, Einstein showed it accounted for the previously unexplained precession of the orbit of the planet Mercury. Only years later did physicists realize the theory also implied something far more radical.
In 1939, theorist J. Robert Oppenheimer and colleagues calculated that when a sufficiently massive star burned out, no known force could stop its core from collapsing to an infinitesimal point, leaving behind its gravitational field as a permanent pit in spacetime. Within a certain distance of the point, gravity would be so strong that not even light could escape. Anything closer would be cut off from the rest of the universe, David Finkelstein, a theorist at Caltech, argued in 1958. This "event horizon" isn't a physical surface. An astronaut falling past it would notice nothing special. Nevertheless, reasoned Finkelstein, who died just days before LIGO's announcement in 2016, the horizon would act like a one-way membrane, letting things fall in, but preventing anything from getting out.
According to general relativity, these objects—eventually named black holes by famed theorist John Archibald Wheeler—should also exhibit a shocking sameness. In 1963, Roy Kerr, a mathematician from New Zealand, worked out how a spinning black hole of a given mass would warp and twist spacetime. Others soon proved that, in general relativity, mass and spin are the only characteristics a black hole can have, implying that Kerr's mathematical formula, known as the Kerr metric, describes every black hole there is. Wheeler dubbed the result the no-hair theorem to emphasize that two black holes of the same mass and spin are as indistinguishable as bald pates. Wheeler himself was bald, Teukolsky notes, "so maybe it was bald pride."
Some physicists suspected black holes might not exist outside theorists' imaginations, says Sean Carroll, a theorist at Caltech. Skeptics argued that black holes might be an artifact of general relativity's subtle math, or that they might only form under unrealistic conditions, such as the collapse of a perfectly spherical star. However, in the late 1960s, Roger Penrose, a theorist at the University of Oxford, dispelled such doubts with rigorous math, for which he shared the 2020 Nobel Prize in Physics. "Penrose exactly proved that, no, no, even if you have a lumpy thing, as long as the density became high enough, it was going to collapse to a black hole," Carroll says.
Soon enough, astronomers began to see signs of actual black holes. They spotted tiny x-ray sources, such as Cygnus X-1, each in orbit around a star. Astrophysicists deduced that the x-rays came from gas flowing from the star and heating up as it fell onto the mysterious object. The temperature of the gas and the details of the orbit implied the x-ray source was too massive and too small to be anything but a black hole. Similar reasoning suggested quasars, distant galaxies spewing radiation, are powered by supermassive black holes in their centers.
But no one could be sure those black holes actually are what theorists had pictured, notes Feryal Özel, an astrophysicist at the University of Arizona (UA). For example, "Very little that we have done so far establishes the presence of an event horizon," she says. "That is an open question."
Now, with multiple ways to peer at black holes, scientists can start to test their understanding and look for surprises that could revolutionize physics. "Even though it's very unlikely, it would be so amazingly important if we found that there was any deviation" from the predictions of general relativity, Carroll says. "It's a very high-risk, high-reward question."
SCIENTISTS HOPE TO ANSWER three specific questions: Do the observed black holes really have event horizons? Are they as featureless as the no-hair theorem says? And do they distort spacetime exactly as the Kerr metric predicts?
Perhaps the simplest tool for answering them is one that Ghez developed. Since 1995, she and colleagues have used the 10-meter Keck telescope in Hawaii to track stars around a radio source known as Sagittarius A* (Sgr A*) in the center of our Galaxy. In 1998, the stars' high speeds revealed they orbit an object 4 million times as massive as the Sun. Because Sgr A* packs so much mass into such a small volume, general relativity predicts it must be a supermassive black hole. Reinhard Genzel, an astrophysicist at the Max Planck Institute for Extraterrestrial Physics, independently tracked the stars to reach the same conclusion and shared the Nobel Prize with Ghez.
Much of the information comes from a single star, dubbed SO2 by Ghez, which whips around Sgr A* once every 16 years. Just as the orbit of Mercury around the Sun precesses, so, too, should the orbit of SO2. Ghez and colleagues are now trying to tease out that precession from the extremely complicated data. "We're right on the cusp," she says. "We have a signal, but we're still trying to convince ourselves that it's real." (In April 2020, Genzel and colleagues claimed to have seen the precession.)
If they get a little lucky, Ghez and company hope to look for other anomalies that would probe the nature of the supermassive black hole. Close to the black hole, its spin should modify the precession of a star's orbit in a way that's predictable from Kerr's mathematical description. "If there were stars even closer than the ones they've seen—maybe 10 times closer—then you could test whether the Kerr metric is exactly correct," Will says.
The star tracking will likely never probe very close to the event horizon of Sgr A*, which could fit within the orbit of Mercury. But EHT, which combines data from 11 radio telescopes or arrays around the world to form, essentially, one big telescope, has offered a closer look at a different supermassive black hole, the 6.5-billion-solar-mass beast in M87.
The famous image the team released 2 years ago, which resembles a fiery circus hoop, is more complicated than it looks. The bright ring emanates from hot gas, but the dark center is not the black hole itself. Rather it is a "shadow" cast by the black hole as its gravity distorts or "lenses" the light from the gas in front of it. The edge of shadow marks not the event horizon, but rather a distance about 50% farther out where spacetime is distorted just enough so that passing light circles the black hole, neither escaping nor falling into the maw.
Even so, the image holds clues about the object at its center. The spectrum of the glowing ring could reveal, for example, whether the object has a physical surface rather than an event horizon. Matter crashing onto a surface would shine even brighter than stuff sliding into a black hole, Özel explains. (So far researchers have seen no spectral distortion.) The shadow's shape can also test the classical picture of a black hole. A spinning black hole's event horizon should bulge at the equator. However, other effects in general relativity should counteract that effect on the shadow. "Because of a very funky cancellation of squishing in different directions, the shadow still looks circular," Özel says. "That's why the shape of the shadow becomes a direct test of the no-hair theorem."
Some researchers doubt EHT can image the black hole with enough precision for such tests. Samuel Gralla, a theorist at UA, questions whether EHT is even seeing a black hole shadow or merely viewing the disk of gas swirling around the black hole from the top down, in which case the dark spot is simply the eye of that astrophysical hurricane. But Özel says that even with limited resolution, EHT can contribute significantly to testing general relativity in the conceptual terra incognita around a black hole.
Gravitational waves, in contrast, convey information straight from the black holes themselves. Churned out when black holes spiral together at half the speed of light, these ripples in spacetime pass unimpeded through ordinary matter. LIGO and Virgo have now detected mergers of black holes with masses ranging from three to 86 solar masses.
The mergers can probe the black holes in several ways, says Frank Ohme, a gravitational theorist and LIGO member at the Max Planck Institute for Gravitational Physics. Assuming the objects are classical black holes, researchers can calculate from general relativity how the chirplike gravitational wave signal from a merger should speed up, climax in a spike, and then ring down. If the massive partners are actually larger material objects, then as they draw close they should distort each other, altering the peak of the signal. So far, researchers see no alterations, Ohme says.
The merger produces a perturbed black hole just like the one in Teukolsky's old thesis, offering another test of general relativity. The final black hole undulates briefly but powerfully, at one main frequency and multiple shorter lived overtones. According to the no-hair theorem, those frequencies and lifetimes only depend on the final black hole's mass and spin. "If you analyze each mode individually, they all have to point to the same black hole mass and spin or something's wrong," Ohme says.
In September 2019, Teukolsky and colleagues teased out the main vibration and a single overtone from a particularly loud merger. If experimenters can improve the sensitivity of their detectors, Ohme says, they might be able to spot two or three overtones—enough to start to test the no-hair theorem.
FUTURE INSTRUMENTS MAY make such tests much easier. The 30-meter optical telescopes being built in Chile and Hawaii should scrutinize the neighborhood of Sgr A* with a resolution roughly 80 times better than current instruments, Ghez says, possibly spying closer stars. Similarly, EHT researchers are adding more radio dishes to their network, which should enable them to image the black hole in M87 more precisely. They're also trying to image Sgr A*.
Meanwhile, gravitational wave researchers are already planning the next generation of more sensitive detectors, including the Laser Interferometer Space Antenna (LISA), made up of three satellites flying in formation millions of kilometers apart. To be launched in the 2030s, LISA would be so sensitive that it could spot an ordinary stellar-mass black hole spiraling into a much bigger supermassive black hole in a distant galaxy, says Nicolas Yunes, a theoretical physicist at the University of Illinois, Urbana-Champaign.
The smaller black hole would serve as a precise probe of the spacetime around the bigger black hole, revealing whether it warps and twists exactly as the Kerr metric dictates. An affirmative result would cement the case that black holes are what general relativity predicts, Yunes says. "But you have to wait for LISA."
In the meantime, the sudden observability of black holes has changed the lives of gravitational physicists. Once the domain of thought experiments and elegant but abstract calculations like Teukolsky's, general relativity and black holes are suddenly the hottest things in fundamental physics, with experts in general relativity feeding vital input to billion-dollar experiments. "I felt this transition very literally myself," Ohme says. "It was really a small niche community, and with the detection of gravitational waves that all changed."
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Alternatives to black holes are scarce and strange
At one time, many physicists resisted the notion of a black hole, a ghostly, self-sustaining gravitational field so intense that not even light can escape. Now, theorists have few alternatives to these creepy holes in the universe.
Any alternative to a black hole must be some dark, dense material orb that’s slightly bigger than a black hole of the same mass. (Were the thing smaller, its own gravity would create a black hole around it.) Observers might detect the orb’s surface by spotting matter crashing onto it and heating up. Or they might deduce the greater size of the object as it swirls around a companion and tears into it before merging.
One hypothetical possibility is a gravastar: a thin material shell filled with dark energy, the mysterious space-stretching stuff that appears to be accelerating the expansion of the universe. A gravastar would have a solid surface rather than an event horizon, the point of no return that is the defining feature of a black hole. It satisfies the mathematical requirements of Albert Einstein’s theory of gravity, general relativity, says Carlos Palenzuela Luque, a gravitational theorist at the University of the Balearic Islands. However, nobody knows how a gravastar could ever form, he says.
Easier to produce might be a boson star, which would consist of exotic, massive Higgs bosons or nearly massless hypothetical particles called axions. Higgs bosons or axions could crowd into a single quantum wave, yielding a density approaching that of a black hole. However, Palenzuela Luque notes, boson stars would likely have masses in a narrow range, whereas a black hole can have any mass. Observed masses vary by factors of billions.
Black hole alternatives “is an area that’s maybe undertheorized,”says Sean Carroll, a theorist at the California Institute of Technology. But that would surely change if observations showed the current description of black holes isn’t quite right. “When we have something to guide our search, we will be able to say something new,” Palenzuela Luque says. “Right now, everything is so speculative.”
Uranus has been sadly neglected. Probes have visited Mars, Venus, Saturn, Jupiter, and Mercury. Heck, even Jupiter's moons are getting their own spacecraft. But the ice giants Uranus and Neptune, in the distant reaches of our Solar System, have not had a single dedicated visitor.
In a new report laying out the top priorities for planetary science and astrobiology, a panel of experts from the US National Academies advises that this omission be rectified. For initiation within the next decade, the committee put a Uranus probe at top priority as the next planetary flagship mission.
"The committee prioritizes the Uranus Orbiter and Probe (UOP) as the highest-priority new Flagship mission for initiation in the decade 2023–2032," the committee wrote in its report.
This probe, the report elaborated, would perform a multi-year orbital tour of Uranus, probing its stinky atmosphere. The mission would provide an unprecedented wealth of information on ice giants in general, and Uranus and its moons in particular – one of the most intriguing and mysterious major objects in the Solar System.
All this, the committee noted, suggests that Uranus warrants significant investigation, not just for its own sake, but for better understanding the evolutionary history of the entire Solar System – especially since the last probe to come close to the planet was Voyager 2 on a flyby in 1986.
The panel has identified several launch windows in the 2030s, with the earliest being 2031; planetary probes are a long game.
"Uranus is one of the most intriguing bodies in the Solar System," the scientists wrote. "Its low internal energy, active atmospheric dynamics, and complex magnetic field all present major puzzles.
"A primordial giant impact may have produced the planet's extreme axial tilt and possibly its rings and satellites, although this is uncertain. Uranus's large ice-rock moons displayed surprising evidence of geological activity in limited Voyager 2 flyby data, and are potential ocean worlds."
Ocean worlds are of great interest to astrobiologists. Scientists believe that on the ocean floors of these geologically active bodies, volcanic vents may allow entire ecosystems based on a chemosynthetic food web to thrive, much like hydrothermal vents here on Earth.
These bodies, of which several have been identified in the Solar System, are the most promising candidates for finding extraterrestrial life.
On that note, the committee identified ocean world Enceladus, a moon of Saturn, as its second-most top priority, with a mission named the Enceladus Orbilander. This ice-covered body has been observed venting plumes of vapor into space from its internal ocean. Sampling these plumes could assess the habitability of Enceladus' ocean, and perhaps even detect signs of life deep within.
A recommendation in the decadal report is a weighty one indeed, but that's no guarantee that a mission will be initiated. The previous report, Vision and Voyages for Planetary Science in the Decade 2013-2022, also recommended a Uranus mission, as well as an Enceladus mission, albeit at a lower priority.
The cost of a mission to Uranus could be over US$4 billion, but the potential scientific gain would be priceless. So, too, could be the gain from an in-depth exploration of Enceladus.
The two highest-priority missions in the previous survey were a Mars sample return mission, and a mission to Europa, an ice moon with a suspected internal ocean orbiting Jupiter. Both of those missions made the cut, and are currently in development. This bodes well for our future exploration of the outer Solar System.
Other recommendations in the new report included continuation of the Mars sample return mission; restoration of the Mars exploration program; continued support for lunar exploration; and, for the first time, improvement of NASA's program to find and track asteroids that pose a threat to life on Earth.
It may be a long road ahead to reach any or all of these goals. But the journey to the stars begins with small steps.
"This report sets out an ambitious but practicable vision for advancing the frontiers of planetary science, astrobiology, and planetary defense in the next decade," said astrophysicist Robin Canup of the Planetary Sciences Directorate at the Southwest Research Institute, and co-chair of the National Academies' steering committee for the decadal survey.
"This recommended portfolio of missions, high-priority research activities, and technology development will produce transformative advances in human knowledge and understanding about the origin and evolution of the Solar System, and of life and the habitability of other bodies beyond Earth."
The uncanny resemblance between features on Europa's frozen surface and a landform in Greenland suggest the icy-moon may be capable of harboring life.
Europa is the fourth largest moon of Jupiter and is thought to have a substantial liquid water ocean under its 15 mile thick crust of ice.
A team from Stanford University explored similarities between double ridges on the surface of Europa, and smaller versions of the features found under Greenland's ice.
Ice-penetrating radar data revealed that refreezing of liquid subsurface water drove the formation of Greenland's double ridge, and if Europa's formed the same way, it could signal the presence of large amounts of liquid water near the surface.
If Europa's features form the same way, this could signal the presence of copious amounts of liquid water - a key ingredient for life - near the surface of the thick outer ice shell of Jupiter's fourth largest moon.
The uncanny resemblance between features on Europa's frozen surface and a landform in Greenland suggest the icy-moon may be capable of harboring life
The study explored similarities between the elongated landforms, called double ridges, that are linear, with two peaks and a central trough between them, and slicing through one looks like a capital letter 'M'.
'If you sliced through one and looked at the cross section, it would look a bit like the capital letter M,' said Stanford University geophysicist Riley Culberg, lead author of the study published in the journal Nature Communications.
In the search for extraterrestrial life, Europa has attracted attention as one of the locales in our solar system that may be habitable, perhaps by microbes, owing to a global saltwater ocean detected deep beneath its ice shell.
Innumerable water pockets closer to the surface would represent a second potential habitat for organisms.
Europa is the fourth largest moon of Jupiter and is thought to have a substantial liquid water ocean under its 15 mile thick crust of ice
Ice-penetrating radar data revealed that refreezing of liquid subsurface water drove the formation of Greenland's double ridge, and if Europa's formed the same way, it could signal the presence of large amounts of liquid water near the surface
'The presence of liquid water in the ice shell would suggest that exchange between the ocean and ice shell is common, which could be important for chemical cycling that would help support life,' Culberg said.
'Shallow water in particular also means there might be easier targets for future space missions to image or sample that could at least preserve evidence of life without having to fully access the deep ocean.'
WHAT ARE DOUBLE RIDGES FOUND IN ICE FORMATIONS?
Jupiter's moon Europa is a prime candidate for extraterrestrial habitability in our solar system.
Double ridges are the most common surface feature on Europa and occur across every sector of the moon, but their formation is poorly understood.
Current hypotheses provide competing and incomplete mechanisms for the development of their distinct morphology.
A team from Stanford analyzed a double ridge in Northwest Greenland with the same gravity-scaled geometry as those found on Europa.
'Using surface elevation and radar sounding data, we show that this double ridge was formed by successive refreezing, pressurization, and fracture of a shallow water sill within the ice sheet,' they said.
If the same process is responsible for Europa's double ridges, the study suggests that shallow liquid water is spatially and temporally ubiquitous across Europa's ice shell.
This increases the possibility of finding evidence of life in these water pools.
NASA's robotic Europa Clipper spacecraft is scheduled for a 2024 launch to further investigate whether this moon possesses conditions suitable for life.
The shallow depth of Europa's potential water pockets - perhaps within six-tenths of a mile of the surface - also would place them near chemicals vital for the formation of life that may exist on its surface.
With a diameter of 1,940 miles, Europa is the fourth-largest of Jupiter's 79 known moons, a bit smaller than Earth's moon but bigger than the dwarf planet Pluto.
Europa's ocean may contain double the water of those on Earth. Life first emerged on Earth as marine microbes.
Europa's double ridges, sometimes extending hundreds miles (km), generally are around 490-650 feet tall, with the peaks about three- to six-tenths of a mile apart.
Scientists have debated how they formed. Culberg was struck by their resemblance to a landform he knew from northwestern Greenland, with peaks about 6.5 feet tall, separated by about 160 feet and extending about a half mile.
'The Greenland double ridge feature formed from the successive refreezing, pressurization and fracture of a near-surface water pocket,' Culberg said.
We see two ridges, rather than one, because the shallow water pocket was also split in two by a fracture filled with refrozen water.'
The water pocket in Greenland was about 50 feet below the surface, likely less than 33 feet thick and about a mile (1.6 km) wide.
If the same process spawned Europa's many double ridges, each associated water pocket could boast a volume similar to Lake Erie, one of North America's Great Lakes.
'Between having two potential habitats and the fact that double ridges - and the near-surface water bodies they may imply - are among the most common features on Europa's surface, it makes this moon a very exciting candidate for habitability indeed,' study co-author Dustin Schroeder added.
The study explored similarities between the elongated landforms, called double ridges, that are linear, with two peaks and a central trough between them, and slicing through one looks like a capital letter 'M'
On Earth, researchers analyze polar regions using airborne geophysical instruments to understand how the growth and retreat of ice sheets might impact sea-level rise.
Much of that study area occurs on land, where the flow of ice sheets is subject to complex hydrology – such as dynamic subglacial lakes, surface melt ponds and seasonal drainage conduits – that contributes to uncertainty in sea-level predictions.
Because a land-based subsurface is so different from Europa's subsurface ocean of liquid water, the study co-authors were surprised when they noticed that formations that streak the icy moon looked extremely similar to a minor feature on the surface of the Greenland ice sheet – an ice sheet that the group has studied in detail.
'We were working on something totally different related to climate change and its impact on the surface of Greenland when we saw these tiny double ridges – and we were able to see the ridges go from 'not formed' to 'formed,' ' Schroeder said.
If Europa's features form the same way, this could signal the presence of copious amounts of liquid water - a key ingredient for life - near the surface of the thick outer ice shell of Jupiter's fourth largest moon
The co-authors said their explanation for how the double ridges form is so complex, they couldn't have conceived it without the analog on Earth.
'The mechanism we put forward in this paper would have been almost too audacious and complicated to propose without seeing it happen in Greenland,' Schroeder said.
The findings equip researchers with a radar signature for quickly detecting this process of double ridge formation using ice-penetrating radar, which is among the instruments currently planned for exploring Europa from space.
'We are another hypothesis on top of many – we just have the advantage that our hypothesis has some observations from the formation of a similar feature on Earth to back it up,' Culberg said.
'It's opening up all these new possibilities for a very exciting discovery.'
WHAT DO WE KNOW ABOUT EUROPA AND WHY IS IT SO SPECIAL?
Jupiter's icy moon Europa is slightly smaller than Earth's moon.
Europa orbits Jupiter every 3.5 days and is tidally locked - just like Earth's Moon - so that the same side of Europa faces Jupiter at all times.
It is thought to have an iron core, a rocky mantle and a surface ocean of salty water, like Earth.
Unlike on Earth, however, this ocean is deep enough to cover the whole surface of Europa, and being far from the sun, the ocean surface is globally frozen over.
Many experts believe the hidden ocean surrounding Europa, warmed by powerful tidal forces caused by Jupiter's gravity, may have conditions favourable for life.
Nasa scientists are on the verge of exploring Jupiter's ocean moon Europa for signs of alien life.
Europa is our best shot of finding biological life in the solar system, researchers say.
The space agency is priming two probes, including one that will land on its surface, to explore the distant moon in detail within the next decade, the agency says.
Breaking News in Search for Extraterrestrial Life: Evidence of Water Near Europa’s Surface
Breaking News in Search for Extraterrestrial Life: Evidence of Water Near Europa’s Surface
BySTANFORD UNIVERSITY
This artist’s conception shows how double ridges on the surface of Jupiter’s icy moon Europa may form over shallow, refreezing water pockets within the ice shell. This mechanism is based on the study of an analogous double ridge feature found on Earth’s Greenland Ice Sheet.
Credit: Justice Blaine Wainwright
Explanation for the formation of abundant features on Europa bodes well for the search for extraterrestrial life.
Jupiter’s moon Europa is a prime candidate for life in our solar system, and scientists have been fascinated by its deep saltwater ocean for decades. However, it is encased in an icy shell that could be miles to tens of miles thick, making sampling it a difficult task. Increasing evidence suggests that the ice shell is more of a dynamic system than a barrier – and an astrobiology site with potential habitability in its own right.
Ice-penetrating radar observations that captured the formation of a “double ridge” feature in Greenland suggest that the ice shell of Europa may have an abundance of water pockets beneath similar features that are common on the surface. The findings, which will be published in the journal Nature Communications today (April 19, 2022), may be compelling for detecting potentially habitable environments within the exterior of the Jovian moon.
“Because it’s closer to the surface, where you get interesting chemicals from space, other moons, and the volcanoes of Io, there’s a possibility that life has a shot if there are pockets of water in the shell,” said study senior author Dustin Schroeder, an associate professor of geophysics at Stanford University’s School of Earth, Energy & Environmental Sciences (Stanford Earth). “If the mechanism we see in Greenland is how these things happen on Europa, it suggests there’s water everywhere.”
Ice-penetrating radar data from Greenland suggests that shallow water pockets may be common within Europa’s ice shell, increasing the potential for detecting signs of habitability near the surface of Jupiter’s moon.
A terrestrial analog
On Earth, researchers analyze polar regions using airborne geophysical instruments to understand how the growth and retreat of ice sheets might impact sea-level rise. Much of that study area occurs on land, where the flow of ice sheets is subject to complex hydrology – such as dynamic subglacial lakes, surface melt ponds, and seasonal drainage conduits – that contributes to uncertainty in sea-level predictions.
Because a land-based subsurface is so different from Europa’s subsurface ocean of liquid water, the study co-authors were surprised when, during a lab group presentation about Europa, they noticed that formations that streak the icy moon looked extremely similar to a minor feature on the surface of the Greenland ice sheet – an ice sheet that the group has studied in detail.
“We were working on something totally different related to climate change and its impact on the surface of Greenland when we saw these tiny double ridges – and we were able to see the ridges go from ‘not formed’ to ‘formed,’ ” Schroeder said.
Upon further examination, they found that the “M”-shaped crest in Greenland known as a double ridge could be a miniature version of the most prominent feature on Europa.
A view of Europa created from images taken by NASA’s Galileo spacecraft in the late 1990s.
Credit: NASA/JPL-Caltech/SETI Institute
Prominent and prevalent
Double ridges on Europa appear as dramatic gashes across the moon’s icy surface, with crests reaching nearly 1000 feet, separated by valleys about a half-mile wide. Scientists have known about the features since the moon’s surface was photographed by the Galileo spacecraft in the 1990s but have not been able to conceive a definitive explanation of how they were formed.
Through analyses of surface elevation data and ice-penetrating radar collected from 2015 to 2017 by NASA’s Operation IceBridge, the researchers revealed how the double ridge on northwest Greenland was produced when the ice fractured around a pocket of pressurized liquid water that was refreezing inside of the ice sheet, causing two peaks to rise into the distinct shape.
Europa is the smallest of Jupiter’s four Galilean moons, and the sixth-closest to the planet of all the 80 known moons of Jupiter. It is also the Solar System’s sixth-largest moon. Galileo Galilei discovered Europa in 1610, and named it after Europa, the Phoenician mother of King Minos of Crete and Zeus’ lover (the Greek equivalent of the Roman god Jupiter).
“In Greenland, this double ridge formed in a place where water from surface lakes and streams frequently drains into the near-surface and refreezes,” said lead study author Riley Culberg, a PhD student in electrical engineering at Stanford. “One way that similar shallow water pockets could form on Europa might be through water from the subsurface ocean being forced up into the ice shell through fractures – and that would suggest there could be a reasonable amount of exchange happening inside of the ice shell.”
Snowballing complexity
Rather than behaving like a block of inert ice, the shell of Europa seems to undergo a variety of geological and hydrological processes – an idea supported by this study and others, including evidence of water plumes that erupt to the surface. A dynamic ice shell supports habitability since it facilitates the exchange between the subsurface ocean and nutrients from neighboring celestial bodies accumulated on the surface.
“People have been studying these double ridges for over 20 years now, but this is the first time we were actually able to watch something similar on Earth and see nature work out its magic,” said study co-author Gregor Steinbrügge, a planetary scientist at NASA’s Jet Propulsion Laboratory (JPL) who started working on the project as a postdoctoral researcher at Stanford. “We are making a much bigger step into the direction of understanding what processes actually dominate the physics and the dynamics of Europa’s ice shell.”
The co-authors said their explanation for how the double ridges form is so complex, they couldn’t have conceived it without the analog on Earth.
“The mechanism we put forward in this paper would have been almost too audacious and complicated to propose without seeing it happen in Greenland,” Schroeder said.
The findings equip researchers with a radar signature for quickly detecting this process of double ridge formation using ice-penetrating radar, which is among the instruments currently planned for exploring Europa from space.
“We are another hypothesis on top of many – we just have the advantage that our hypothesis has some observations from the formation of a similar feature on Earth to back it up,” Culberg said. “It’s opening up all these new possibilities for a very exciting discovery.”
Reference:
“Double ridge formation over shallow water sills on Jupiter’s moon Europa” 19 April 2022, Nature Communications. DOI: 10.1038/s41467-022-29458-3
Schroeder is also a faculty affiliate with the Institute for Human-Centered Artificial Intelligence (HAI), an associate professor, by courtesy, of electrical engineering and a center fellow, by courtesy, at the Stanford Woods Institute for the Environment.
This research was supported by a National Defense Science and Engineering Graduate Fellowship and, in part, by NASA Grant NNX16AJ95G and NSF Grant 1745137.
Official history tells us that 17 missions were launched between 1961 and 1975, of which 11 were manned (Apollo 7 through Apollo 17). During this time, 6 successful landings on the lunar surface were made. The Apollo 18, 19, and 20 flights were canceled due to the lack of new scientific value at the huge expense of the state budget and taxpayers. However, in 2007, Italian freelance journalist Luca Scantamburlo took a written interview with William Rutledge, who claims to be a member of the secret Apollo 20 mission.
According to him, he was an employee of Bell Laboratories and served in the US Air Force. Rutledge attracted public attention by starting to distribute photographs and videos of the Apollo 20 mission online in 2007 which captured the same spaceship and its pilots.
What is the essence of the information from Rutledge? He claimed that during the Apollo 15 mission to the moon, an unidentified man-made object was discovered and photographed on its surface.
During missions 16 and 17, several more photographs were taken and reconnaissance of the terrain from orbit was carried out. The task of missions 18 and 19 (which was no longer officially) is not really clear: Rutledge only says that during these missions, a number of problems occurred, as a result of which research data was lost. It was originally planned to land next to an alien ship and study it using rovers.
In 1976, the Apollo 20 mission was launched, which included: William Rutledge, Aleksei Leonov, and Leona Snyder. They managed to land by the ship, get inside, inspect the interior of the ship, and the bodies of the pilots. One of the sources said that they not only examined the bodies but also took the head of one of the bodies with them.
The dimensions of the ship were 3370 x 510 meters; the age is estimated at 1.5 billion years; inside, there are many signs of biological life: remnants of vegetation in the engine compartment of the ship, stones of a triangular shape that exude a yellow liquid that has some medical properties, the remains of small bodies (about 10 cm) that lived in a network of “glass” pipes piercing the whole ship.
They found a humanoid, female, 1.65 meters. She had genitals, hair, six fingers (we assume the math is based on a dozen). She was a pilot, there was an aerobatics device connected to her fingers and eyes, the body had no clothes, and they had to cut two cables connected to the nose without nostrils. Leonov detached the device from the eyes. Blood clots or bio-fluids burst and froze in the mouth, nose, eyes, and parts of the body. Some parts of the body were in unusually good condition, hair and skin were protected by a thin transparent layer of protection. The condition seemed neither dead nor alive. The booth was full of inscriptions and formed from long, hollow hexagonal tubes.
On the other hand, one can only guess that this was the ship of the Anunnaki, about which Sitchin or some other guys wrote.
Doubts are caused by the number of fingers, these humanoids have 12 of them (6 on each hand), and we know that the Anunnaki used the hexadecimal numbering system and on all the frescoes, they have 5-fingered palms.
We also know that the Anunnaki had a parallel mission in low-Earth orbit: one part of them worked on Earth, the other part remained on the mother ship. It may well be that they used the moon and one of the ships remained there. Another interesting fact is that the team of engineers who actually implemented the Apollo project was headed by Wernher von Braun, who during Nazi Germany worked for the benefit of the Third Reich, creating for them the famous V-2 rockets.
Braun came to America along with many other German scientists removed from Germany as part of Operation Paperclip in 1945. And the colossal technological breakthrough of the engineers of the Third Reich happened due to cooperation with the occult societies of Ahnenerbe and Vril, who obtained information from the ancient egregors of the Gods related to our civilization.
Braun had an interesting chain of events: German occult societies -> moving to the USA -> working on a space program -> detecting an alien spacecraft, possibly the very same Gods who advised the Nazis. He survived until 1977 and saw the launch of Apollo 20 and, moreover, according to Rutledge, was personally present at the launch.
In recent weeks, the project took a big step forward with the installation of fiber optic amplifiers and splitters on all VLA antennas, which give COSMIC access to the data streams from the entire VLA. Once this digital backend is online, COSMIC will have access to all data provided by the VLAs 27 radio antennas, which will be able to conduct observations 24/7. In the process, COSMIC SETI will examine around 40 million stars in the Milky Way for possible signs of intelligent life.
Located in the deserts of New Mexico, the Karl G. Jansky Very Large Array is the world’s largest radio telescope array capable of operating at microwave frequencies. It was featured in the 1997 film “Contact” (based on the original novel by Carl Sagan), where Dr. Eleanor Arroway (played by Jodie Foster) and her colleagues received the first extraterrestrial communication. Interestingly enough, the VLA has never been part of a SETI effort in real life, but that’s about to change.
Jack Hickish, Digital Instrumentation Lead for COSMIC SETI, explained in a SETI Institute press release:
“Having all the VLA digital signals available to the COSMIC system is a major milestone, involving close collaboration with the NRAO VLA engineering team to ensure that the addition of the COSMIC hardware doesn’t in any way adversely affect existing VLA infrastructure.
“It is fantastic to have overcome the challenges of prototyping, testing, procurement, and installation – all conducted during both a global pandemic and semiconductor shortage – and we are excited to be able to move on to the next task of processing the many Tb/s of data to which we now have access.”
As part of this collaborative effort, the VLA will conduct observations while SETI Institute scientists will analyze that data to look for evidence of technological activity (aka. “technosignatures”). The VLA offers many important capabilities for SETI, not the least of which are its size. Each of its 27 antennas measures 25 m (82 ft) in diameter, yielding a collecting area equivalent to a single-dish antenna measuring 130 m (426 ft) in diameter.
This surface area and large amounts of metal mesh allow for almost unparalleled sensitivity levels, which is always a plus for SETI surveys (where signals are likely to be weak). In addition, each VLA antenna has eight cryogenically cooled receivers that continuously monitor the sky at frequencies ranging from 1 to 50 GHz in the radio spectrum. Some receivers can operate between 1 GHz and 54 MHz, corresponding with frequencies used for television broadcasts.
To exploit these capabilities, engineers at the VLA have installed a “splitter” that feeds a copy of the data stream provided by the VLA’s 27 antennas to locally-installed SETI equipment. This equipment consists of software and hardware that computes 64 different beams, which sorts cosmic static into hundreds of millions of narrow-band frequency channels. Said Cherry Ng, a SETI Institute COSMIC Project Scientist:
“I am excited by the ability of COSMIC to conduct the most comprehensive technosignature search ever in the Northern Hemisphere. We will be able to monitor millions of stars with a sensitivity high enough to detect an Arecibo-like transmitter out to a distance of 25 parsecs (81 light-years), covering an observing frequency range from 230 MHz to 50 GHz, which includes many parts of the spectrum that have not yet been explored for ETI signals.”
The COSMIC SETI program, which is expected to be operational by early 2023, will observe around 40 star systems in our galaxy over two years. It will be the most comprehensive SETI survey undertaken in the Northern Hemisphere, a record previously held by Breakthrough Listen. Its first major observational campaign will be conducted in parallel with the ongoing VLA Sky Survey (VLASS), which relies on the VLA to survey 82% of the sky in the 2-4GHz S-bands.
“We look forward to partnering with the SETI Institute on this exciting initiative and are pleased to see this important milestone in the technical work that will make this new science possible,” said NRAO Director Tony Beasley.
In this series we are exploring the weird and wonderful world of astronomy jargon! You’ll be the biggest thing in town after today’s topic: galaxy clusters!
Galaxy clusters are the single largest gravitationally bound structures in the Universe. The “gravitationally bound” part means that the gravity of the individual components of a galaxy cluster is strong enough to hold it together. While larger structures, known as superclusters, exist, they are not gravitationally bound and will eventually disperse.
Galaxy clusters can host a thousand galaxies or more and are typically at least 3-4 million light-years in diameter. The smallest galaxy clusters weigh 1014 solar masses, while the largest are ten to a hundred times more massive.
By far the dominant component of every galaxy cluster is dark matter, the mysterious form of matter that is invisible to light and does not interact with normal matter. Dark matter makes up around 90% of the mass of every cluster.
Of the remainder, 90% is in the form of an extremely hot but incredibly thin plasma called the intracluster medium. This medium is so hot that it emits brightly in the X-ray part of the electromagnetic spectrum. Even though the intracluster medium is so hot, it would register as a vacuum in Earth-based laboratory experiments.
Only 1% of the mass of every galaxy cluster is in the form of galaxies themselves. Those galaxies typically move through the cluster like bees in a beehive with speeds of up to a thousand kilometers per second. Those speeds can be used to weigh the cluster – more massive clusters will support faster galaxy movements without the cluster breaking apart.
The nearest cluster to Earth is the Virgo Cluster, which contains 1,000-2,000 galaxies and sits about 50 million light-years away.
Another famous cluster is the Coma Cluster, about 321 million light-years away. The main galaxies of the cluster are visible in amateur telescopes. In 1933 the astronomer Fritz Zwicky used observations of galaxy motion within the Coma Cluster to discover the existence of dark matter.
In this series we are exploring the weird and wonderful world of astronomy jargon! You’ll be off to a good start with today’s topic: the big bang theory!
The Big Bang theory is the current best understanding of the history of the Universe. The theory is a physical model, based on many lines of evidence, that says that our Universe was once smaller, hotter, and denser than it is today. In fact, according to our best measurements, about 13.77 billion years ago our entire observable Universe – including every star and galaxy that we could ever see – was once crammed into a tiny volume only a few centimeters across with a temperature of over a quadrillion degrees.
The Big Bang theory originated in the early 20th century. The first hints of the theory began with Einstein’s general theory of relativity. When he applied his equations to the study of the whole Universe, he found that a static, unchanging cosmos was highly unusual. Instead, the Universe should be either expanding or contracting. The Belgian astronomer and Catholic priest Georges Lemaître came to a similar conclusion, calling his idea of the origins of the Universe the “primeval atom.”
Scientists, including Einstein, rejected this idea. But in the 1920’s astronomer Edwin Hubble conclusively demonstrated that all galaxies are, on average, racing away from each other. The simplest explanation of this observation is that we live in an expanding Universe.
Since then, multiple lines of evidence have led scientists to conclude that the Big Bang theory is accurate. For example, models of the very early Universe successfully predict the abundance of light elements like hydrogen and helium. Early cosmologists also predicted the existence of an afterglow light pattern generated when the young Universe transitioned from a plasma to neutral state. This pattern, called the cosmic microwave background, was discovered on accident in the 1960’s.
In the Big Bang model, the primordial Universe expanded and cooled, eventually giving rise to the formation of stars and galaxies.
Today, no other theory of cosmology can successfully explain the wealth of evidence.
UFO Seen Over Las Vegas, Nevada 4-18-2022, UFO Sighting News.
UFO Seen Over Las Vegas, Nevada 4-18-2022, UFO Sighting News.
Date of sighting: April 18, 2022
Location of sighting: Las Vegas, Nevada, USA
Watch this amazing catch in Las Vegas, Nevada a few days ago. An eyewitness heard something loud that sounds like a jet and opened his phone to record, just in time to catch a strange object passing overhead. The object sounds like a jet, but looks alien made. I believe this craft could be one of USAF top secret evolutions of the TR3B, which started out as a triangle, but may have evolved into a new generation of spheres. Nellis AFB is in Las Vegas outskirts, and is a known testing ground for alien tech. Watch the video and its slow motion close up I made at the end. I have never seen a man made craft that looks like this before, and I worked on the flight line on B-1 bombers at Ellsworth AFB long ago.
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Over mijzelf
Ik ben Pieter, en gebruik soms ook wel de schuilnaam Peter2011.
Ik ben een man en woon in Linter (België) en mijn beroep is Ik ben op rust..
Ik ben geboren op 18/10/1950 en ben nu dus 74 jaar jong.
Mijn hobby's zijn: Ufologie en andere esoterische onderwerpen.
Op deze blog vind je onder artikels, werk van mezelf. Mijn dank gaat ook naar André, Ingrid, Oliver, Paul, Vincent, Georges Filer en MUFON voor de bijdragen voor de verschillende categorieën...
Veel leesplezier en geef je mening over deze blog.