How does astronomy use the electromagnetic spectrum? - PART II

How does astronomy use the electromagnetic spectrum? - PART II

Parts of the electromagnetic spectrum invisible to human eyes reveal a vast amount of information about the universe, but it took a long time for astronomers to learn how to view it.
For thousands of years, humans were looking up at the star-studded night sky using just their eyes sensitive to the optical wavelength of the electromagnetic spectrum. The first telescopes, invented in the early 17th century, enhanced the ability of human eyes by magnifying distant objects.
But as physicists started discovering in the 19th century that there are other, invisible, types of light in the natural world around us, astronomers realized that there must be such light emanating also from the universe.
WHAT DOES ULTRAVIOLET LIGHT TEACH US ABOUT THE UNIVERSE?
The great Hubble is also the world's main observer of ultraviolet light that emanates from sources in the universe. Ultraviolet light has shorter wavelengths and carries higher energies than visible light and points astronomers to hot, energetic processes, such as those taking place in young stars and in young star-forming galaxies. Massive stars that orbit each other in binary systems also emit ultraviolet light and so do powerful auroras on giant gaseous planets like Jupiter.
Ultraviolet light gets absorbed by the ozone layer in Earth's atmosphere, which is good for organisms living on Earth (as these wavelengths are known to cause tissue-damage and cancer). For astronomy, however, the limited ability of ultraviolet light to penetrate the atmospheres means that telescopes designed to study it need to orbit in space.
Famous ultraviolet telescopes
Apart from the Hubble Space Telescope, solar observatories such as the European Solar Orbiter or NASA's Solar Dynamics Observatory carry ultraviolet imagers to observe highly energetic processes on the sun. NASA's Jupiter explorer Juno also carries an instrument for studying ultraviolet light.
WHAT DO X-RAYS TEACH US ABOUT THE UNIVERSE?
Things get even more heated and energetic with X-rays. Discovered accidentally by German physicist Wilhelm Roentgen in 1895, these matter-penetrating rays are generated in vast amounts during some of the most extraordinary processes in the universe, such as when supermassive black holes or extremely massive neutron stars suck in matter from their surroundings, or during supernova explosions of dying stars.
X-rays come from the hottest places in the universe including black hole and neutron stars' accretion disks where matter spirals at extreme speeds. High-temperature plasma that fills space between galaxies in galaxy clusters also emits X-rays, and so do stars including our sun.
Astronomers recently discovered that comets can emit X-rays, Wibisono said, and that Jupiter, in addition to its ultraviolet aurora, also produces an aurora that shines in X-rays.
"X-rays are a really powerful part of the spectrum because you get fluorescence in X-rays," said Wibisono. "Rocky surfaces of moons and planets give off X-rays for fluorescence. The atmospheres around terrestrial planets also fluoresce and X-rays, the gas giants scatter solar X-rays, so they act like a mirror to the solar X-rays."
Fluorescence is the ability of a surface to absorb and subsequently emit light that originally arrived from another source.
Infamous for their potential to cause DNA mutations that may lead to cancer, X-rays get, just like ultraviolet rays, fortunately filtered out by Earth's atmosphere. X-ray astronomy could therefore only take off once humans were able to send objects to space. Astronomers knew prior to that that the sun is a powerful source of X-rays, but the first instruments capable of detecting other sources of cosmic X-rays were only launched aboard sounding rockets in the 1960s.
One of the problems with the detection of cosmic X-rays is their ability to penetrate matter. Just like they penetrate human tissue to reveal broken bones, X-rays also pass through mirrors that astronomers may want to use to concentrate them.
Building sensitive X-ray detectors therefore requires some engineering ingenuity. Scientists have to design mirrors for X-ray telescopes in a way that the energetic rays hit the reflecting surface at a shallow angle "like a stone skipping across the surface of a pond," according to NASA(opens in new tab).
X-ray telescopes require multiple mirrors (opens in new tab)positioned at gradually increasing angles to deflect the X-rays onto a detector. Such contraptions, however, tend to be rather chunky and require large satellites to accommodate them. NASA's Chandra, for example, at 45-feet-long (13 m), is the largest satellite launched by the Space Shuttle, about a three feet (1 m) longer than Hubble.
The matter-penetrating ability of X-rays, however, also has its advantages, as these rays easily escape from dust-shrouded regions, such as galactic centers where black holes munch on the infalling matter.
Famous X-ray telescopes
NASA's Chandra X-ray observatory is the current flagship X-ray telescope. In space since 1999, Chandra travels around Earth on an elliptical orbit that takes it as far as 83,000 miles (133,000 km) away from the planet's surface where no residual atmosphere obstructs the X-ray views. During its more than two decades in orbit, Chandra has imaged jets of matter shooting from supermassive black holes in galactic centers and even traced the separation of dark matter from normal matter in the collisions of galaxies in galactic clusters.
ESA also has its X-ray space observer, the XMM-Newton space telescope, also launched in 1999.
WHAT DO GAMMA-RAYS TEACH US ABOUT THE UNIVERSE?
Gamma-rays are the highest energy type of radiation present in the universe. Just like X-rays, they come from extremely hot and energetic processes in the universe, such as supernova explosions and accreting black holes. Even more capable of penetrating matter than X-rays, gamma-rays are also produced during nuclear explosions on Earth, and, in smaller quantities, in thunderstorms and during radioactive decay. Stars such as our sun also produce occasional gamma-ray flashes in the form of solar flares.
Just like many other types of astronomy, gamma-ray astronomy came about by accident. In the 1960s, American military satellites were looking for signs of the USSR's testing of nuclear weapons, when they detected inexplicable flashes of extremely energetic gamma-rays. Lasting from fractions of seconds to several minutes, these gamma-ray bursts, as they became known, were coming regularly from all parts of the universe.
It took until the 1990s for astronomers to figure out that these bursts come from extremely powerful explosions that mark the birth of new black holes when massive stars die. The shorter types of gamma-ray bursts are produced in collisions of superdense stellar remnants called the neutron stars.
Gamma-ray bursts point astronomers to the fact that a cataclysmic event has just occurred somewhere in the universe. By measuring the intensity of the burst, astronomers can learn something about the intensity and distance of the event. However, they need to search for the source of the flash afterward, using other types of telescopes. When they manage to locate the region in the sky where the burst has come from, they can then observe the area in other parts of the electromagnetic spectrum to gain more insight into the processes involved.
Famous gamma-ray telescopes
NASA's space telescopes Fermi and Swift together with ESA's Integral are the world's current gamma-ray burst spotting workhorses. However, only Swift, which covers about 9% of the sky, has the ability to locate sources of these giant explosions.
Astronomers are therefore looking for new approaches to gamma-ray burst detection. In 2021, a team of scientists from Hungary and Slovakia launched a tiny cubesat called GRB Alpha, that has been successfully detecting gamma-ray bursts ever since. In October 2022, GRBAlpha made an accurate detection of the peak intensity of the brightest gamma-ray burst ever seen, while the event completely blinded detectors on NASA's Fermi.
The researchers envision that a fleet of such cubesats would make it possible to find sources of gamma-ray bursts across the entire sky through the so-called triangulation, the same method used to pinpoint a location on Earth with the help of GPS.
- Follow Tereza Pultarova on Twitter @TerezaPultarova(opens in new tab). Follow us on Twitter @Spacedotcom(opens in new tab) and on Facebook(opens in new tab).
ADDITIONAL RESOURCES
Astronomy Cast, produced by the Planetary Science Institute in collaboration with Universe Today has a great series on the different kinds of astronomy based on the electromagnetic spectrum. You can listen to their radio astronomy(opens in new tab), submillimeter astronomy(opens in new tab), infrared astronomy(opens in new tab), optical astronomy, ultraviolet astronomy, X-ray astronomy(opens in new tab) and gamma-ray astronomy(opens in new tab).
BIBLIOGRAPHY
- National Radio Astronomy Observatory: The History of Radio Astronomy, accessed April 2023 from: https://public.nrao.edu/radio-astronomy/the-history-of-radio-astronomy/(opens in new tab)
- Walker, J. H. A brief history of infrared astronomy, Astronomy & Geophysics, Volume 41, Issue 5, October 2000, Pages 5.10–5.13: https://doi.org/10.1046/j.1468-4004.2000.41510.x(opens in new tab)
- ESA: Seeing with infrared eyes: A brief history of infrared astronomy, July 2020, accessed April 2023 from: https://sci.esa.int/web/herschel/-/59550-a-brief-history-of-infrared-astronomy(opens in new tab)
- Harvard University: History of X-Ray Astronomy, accessed April 2023 from: https://chandra.harvard.edu/xray_astro/history.html(opens in new tab)
- ESA: History of X-ray astronomy in Europe: From Exosat to ATHENA, accessed April 2023 from:https://sci.esa.int/web/athena/-/60759-history-of-x-ray-astronomy-in-europe-from-exosat-to-athena(opens in new tab)
- Pinkau, K. History of gamma-ray telescopes and astronomy, Experimental Astronomy, Volume 25, Issue 1-3, pp. 157-171, August 2009: https://ui.adsabs.harvard.edu/abs/2009ExA....25..157P/abstract













































