UFO'S of UAP'S, ASTRONOMIE, RUIMTEVAART, ARCHEOLOGIE, OUDHEIDKUNDE, SF-SNUFJES EN ANDERE ESOTERISCHE WETENSCHAPPEN

What happens when a spiral and an elliptical galaxy collide? To celebrate the second anniversary of the “first light” for the Webb telescope, NASA released an amazing infrared view of two galaxies locked in a tight dance. They’re called the Penguin and the Egg and their dance will last hundreds of millions of years.

“In just two years, Webb has transformed our view of the universe, enabling the kind of world-class science that drove NASA to make this mission a reality,” said Mark Clampin, director of the Astrophysics Division at NASA Headquarters in Washington. “Webb is providing insights into longstanding mysteries about the early Universe.”

Webb Witnesses a Galactic Dance

The telescope targeted a collision scene named Arp 142 containing both galaxies—a scene that the Hubble Space Telescope has also explored. They lie about 326 million light-years away. Their first close encounter began somewhere between 25 and 75 million years ago. That’s when two partner galaxies had the first of many passages that will distort their shapes more than they already appear here.

The Hubble Space Telescope captured visible light when observing Arp 142, nicknamed the Penguin and the Egg, in 2013.

At right is the James Webb Space Telescope’s near-infrared light view of the same region. Courtesy NASA, ESA, CSA, STScI

The Hubble Space Telescope captured visible light when observing Arp 142, nicknamed the Penguin and the Egg, in 2013. The Webb view (right) shows the near-infrared view.

Courtesy NASA, ESA, CSA, STScI

Webb’s observations, which combine near- and mid-infrared light from Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), respectively, clearly show that a hazy cloud of gas and stars (blue) links them together. The close approach also set off tremendous bursts of star birth in the colliding clouds of gas and dust.

Eventually, after several close approaches in their cosmic dance, these two galaxies will merge completely. Observers hundreds of millions of years in the future will look at Arp 142 and see one massive elliptical galaxy.

Interestingly, Webb’s sharp infrared eyes also picked out very distant galaxies. Some lie beyond this cosmic collision, although at least one lies about a hundred million light-years closer to Earth. It bristles with hot, young, newborn stars.

How The Arp 142 Galaxies Experience a Merger

The Penguin and Egg galaxies lie about 100,000 light-years apart but they affect each other. The Egg’s gravitational pull distorts the spiral and that interaction is “sculpting” the Penguin. The core makes up the eye of a penguin. The slowly unwinding spiral arms form a beak, head, backbone, and tail.

Webb’s infrared view reveals otherwise unseen activity between the two. For example, the Penguin is rich in dust. Webb’s view shows us how gravitational interactions pull that dust away from the Penguin. There are also scads of new stars in the galaxy, surrounded by what looks like smoke. Webb’s view shows this hydrogen cloud. It’s rich in carbon-based molecules called polycyclic aromatic hydrocarbons (PAHs). These are incredibly abundant in the Universe and astronomers find them just about everywhere they point a telescope.

Webb’s mid-infrared view of interacting galaxies Arp 142 seems to sing in primary colors. The background of space is like a yawning darkness speckled with bright, multi-colored beads.

This image was taken by MIRI, the telescope’s Mid-Infrared Instrument, which astronomers use to study cooler and older objects, dust, and extremely distant galaxies.

Here, the Egg appears as an exceptionally small teal oval with gauzy layers. Mid-infrared light predominantly shows the oldest stars in the elliptical galaxy, which has lost or used up most of its gas and dust. This is why the view is so different from the combined image, which includes near-infrared light.NASA, ESA, CSA, STScI

Webb’s mid-infrared MIRI image shows the Egg as a small teal oval. Mid-infrared light predominantly shows the oldest stars in the elliptical galaxy, which has lost or used up most of its gas and dust. This is why the view is so different from the combined image, which includes near-infrared light.

Courtesy: NASA, ESA, CSA, STScI

By contrast, in Webb’s view, the Egg looks like it’s hardly been touched—it’s still an egg-shaped elliptical. It has much older stars than the Penguin. Past epochs of star birth have pretty much used up the available star-making material. So, even though the two galaxies have about the same mass, the Egg just doesn’t have as much material to get stretched out or turned into stars.

Zeroing in on Webb’s Two Views

If you look at both of Webb’s infrared views of the galaxy collision, you can see marked differences in them. That’s because each one prioritizes a different set of infrared wavelengths. In the mid-infrared view, the egg looks tiny and washed out. That’s because the instrument sees only the old stars in the Egg. By contrast, the Penguin’s distorted core and spiral arms are brimming with young stars embedded in the PAH-rich hydrogen clouds.

The combined near- and mid-infrared view shows more of the gas clouds as the Egg tears them away from the Penguin. These regions will glitter in the future with the light of newly formed stars. For now, however, only cooler, older stars are visible in the combined image. The younger ones are there, but the mid-infrared-sensitive instrument doesn’t spot them.

Here’s a flythrough visualization of Arp 142. NASA, ESA, CSA, Ralf Crawford (STScI), Joseph DePasquale (STScI), Christian Nieves (STScI), Joseph Olmsted (STScI), Alyssa Pagan (STScI), Frank Summers (STScI), Greg Bacon (STScI)

Why Does Webb Study Galaxy Collisions?

By studying this galactic collision site, the Webb telescope further probes the activity as galaxies evolve. Collisions are an integral part of this process. Our Milky Way Galaxy will dance with the nearby Andromeda Galaxy, starting in about 5 billion years. Images and data from observations of other galaxies doing the same thing give astronomers a chance to understand the process and forecast the distant future when something called “Milkdromeda” will contain the stars and planets of two spirals that once were close neighbors.

For More Information

Vivid Portrait of Interacting Galaxies Marks Webb’s Second Anniversary
Galaxy Evolution

Various forms of hopping robots have crept into development for us[e in different space exploration missions. We’ve reported on their use on asteroids and even our own Moon. But a study funded by NASA’s Institute for Advanced Concepts (NIAC) in 2018 planned a mission to a type of world where hopping may not be as noticeable an advantage—Europa.

The mission, developed by engineers at NASA’s Jet Propulsion Laboratory, Purdue University, and Honeybee Robotics, is known as the Steam Propelled Autonomous Retrieval Robot for Ocean Worlds, or SPARROW. It’s about the size and shape of a soccer ball, with the logic, power, and control systems inside a spherical outer hollow shell.

SPARROW wouldn’t be able to operate on its own, however. It would require a lander to deposit it onto the surface and serve as a refueling and sample collection storage base. Europa Clipper, the only currently planned NASA mission to the icy moon, would have been good for hitching a ride, but its lack of a lander made it unsuitable for SPARROW.

Budget constraints are always a problem for innovative missions – as Fraser explains with Dr. Manasvi Lingam.

However, the hopping robot itself is well suited for the environment in Europa. Its designers intended to make it “terrain agnostic,” meaning it could traverse even the harshest terrain the icy moon could throw at it. These would include penitentes, shards of ice that could be meters tall, and difficult for ground-based robots to traverse.

SPARROW could fly over them, collect interesting samples, and return to the lander to refuel and deposit them. Then, it could go out again in a different direction. To model this system architecture, the JPL team spent Phase I trying to determine the best propulsion system for the robot and modeling control algorithms for the flights.

First, let’s tackle the propulsion system. The lander accompanying SPARROW would have to mine ice off the moon’s surface, then heat it and store it as water. When SPARROW returned from a hop, it would use the water to refuel. Five different propulsion methods were considered as part of the study. Still, the best turned out to be a “hot water thruster,” where SPARROW would internally heat the water supplied by the lander, then eject that out in a burst of propulsive force to launch the robot off the surface.

Exploring the surface of Europa is only one part of its mystery – as Fraser explains.

The second major part of the paper was controlling that propulsion. Trajectory correction is critical to mission success, but in this case, the designers believe that no matter where the robot ends up, it will be able to collect a sample and return to the lander. This is due to its gimballed design, which allows the robot to consistently orient correctly, even after bouncing along a frozen surface for a while.

There is still much work to do before the mission is ready to go, though. Some of the most pressing questions are how to stop ice from forming in the robot’s propulsion nozzle and throughout its structural cage. Such blockages could easily throw off any existing trajectory calculations and theoretically immobilize the hopper entirely if they were severe enough.

However, no work is planned to solve those problems for now as the project has yet to receive Phase II funding from NIAC, and work on it appears to have stalled. Dr. Gareth Meirion-Griffith, the primary investigator on the project, has moved on from JPL to take a job at Collins Aerospace. Even so, someday, the author’s ideas might be integrated into a Europa lander mission—we’ll have to wait and see.

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