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.

NASA's tiny spacecraft sends first exoplanet images

With the first images from the spacecraft now in hand, the team behind NASA's Star-Planet Activity Research CubeSat, or SPARCS, is ready to begin charting the energetic lives of the galaxy's most common stars to help answer ...

Comet 3I/ATLAS: Europa Clipper captures rare ultraviolet view

The Southwest Research Institute-led Ultraviolet Spectrograph (UVS) aboard NASA's Europa Clipper spacecraft has made valuable observations of the interstellar comet 3I/ATLAS, which in July became the third officially recognized ...

Puzzling ultraviolet radiation in the birthplaces of stars

Researchers used the MIRI instrument onboard the James Webb Space Telescope (JWST) to identify the presence of ultraviolet radiation in five young stars in the Ophiuchus region, and to understand its role in the formation ...

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