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.

Astronomers want to build a swarm of telescopes to find life

Current plans for flagship telescopes in the 2040s are focused on answering a simple question: Are we alone? Our best telescopes to date, such as the James Webb Space Telescope (JWST), have given us only tantalizing glimpses ...

Webb and Hubble find massive star clusters emerge faster

Astronomers using the NASA/ESA/CSA James Webb Space Telescope together with the NASA/ESA Hubble Space Telescope have looked deeply at thousands of young star clusters in four nearby galaxies, studying clusters at different ...

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 ...

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