Page 3: Research news on Ultraviolet astronomy

Ultraviolet astronomy is the research area focused on observing and interpreting electromagnetic radiation in the ultraviolet (UV) spectral range, typically ~10–400 nm, to investigate astrophysical plasmas and high-energy processes. Because Earth’s atmosphere absorbs most UV photons, the field relies on space-based observatories and suborbital platforms equipped with specialized optics, coatings, and photon-counting detectors. Ultraviolet observations probe hot stars, the interstellar and intergalactic medium, accretion disks, stellar winds, and shock fronts via resonance lines and continua, enabling measurements of temperature, composition, ionization state, kinematics, and mass loss. This domain is crucial for constraining models of star formation, galaxy evolution, feedback, and the baryon cycle in cosmic structures.

Image: Hubble reveals Jupiter in ultraviolet light

This NASA Hubble Space Telescope image shows the planet Jupiter in a color composite of ultraviolet wavelengths. Released on Nov. 3, 2023, in honor of Jupiter reaching opposition, which occurs when the planet and the sun ...

Image: Earth in far-ultraviolet

On April 21, 1972, NASA astronaut John W. Young, commander of the Apollo 16 mission, took a far-ultraviolet photo of Earth with an ultraviolet camera. Young's original black-and-white picture was printed on Agfacontour professional ...

MAUVE: An ultraviolet astrophysics probe mission concept

For the past 30 years, NASA's Great Observatories—the Hubble, Spitzer, Compton, and Chandra space telescopes—have revealed some amazing things about the universe. In addition to some of the deepest views of the universe provided ...

Instrument aboard Jupiter-bound spacecraft nails in-flight test

As European Space Agency (ESA)'s Jupiter Icy moons Explorer (Juice) spacecraft hurtled past the moon and Earth in mid-August to provide its first gravity assist maneuver to the Jovian system, the Southwest Research Institute-led ...

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