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Browsing Tag

Gas giant

22 posts
SScience
Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b
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Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b

  • July 9, 2026
Using the upgraded GRAVITY+ instrument on ESO’s Very Large Telescope Interferometer (VLTI), astronomers have measured the ratio of…
SScience
An artist’s impression of the hot-Jupiter exoplanet HD 80606b. Image credit: NASA / ESA / CSA / Joseph Olmsted, STScI.
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Webb Sees Jupiter-Size Exoplanet Being Roasted by Its Star

  • June 22, 2026
HD 80606b has one of the most extreme orbits of any known exoplanet and the NASA/ESA/CSA James Webb…
SScience
James Webb Space Telescope Finds a Hot Jupiter Roasting on a 111-Day Skewer
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James Webb Space Telescope Finds a Hot Jupiter Roasting on a 111-Day Skewer

  • June 18, 2026
Comparison of best-fit size of the exoplanet HD 80606 b with Jupiter. Credit: Wikimedia Commons Jupiter’s cloud tops hover around –145°C.…
PPhysics
As planets and stars travel through the streams of charged particles flowing across space, their magnetic fields act like obstacles; incoming particles are slowed and deflected, forming a boundary called the bow shock; just ahead of this boundary lies the foreshock, a variable region where magnetic conditions can accelerate some particles to nearly the speed of light. Image credit: Ben C. Smith, Johns Hopkins Applied Physics Laboratory.
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Jupiter Accelerates Electrons to Near-Light Speed, Offering Clues to Cosmic Ray Origins

  • June 11, 2026
The giant planet’s bow shock isn’t just deflecting the solar wind, it’s acting as a powerful particle accelerator,…
SScience
This illustration shows magnetic activity in an ultra-hot Jupiter. Image credit: ESO / M. Kornmesser / L. Calçada.
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Astronomers Detect Clearest Signs Yet of Magnetic Fields on Extrasolar Planets

  • June 2, 2026
By tracking fierce winds racing through the atmospheres of seven ultra-hot Jupiters, astronomers have uncovered the strongest evidence…
SScience
Webb Detects Methane in Atmosphere of Exo-Saturn TOI-199b
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Webb Detects Methane in Atmosphere of Exo-Saturn TOI-199b

  • May 25, 2026
Using spectral data from the Near-Infrared Spectrograph (NIRSpec) onboard the NASA/ESA/CSA James Webb Space Telescope, astronomers analyzed the…
SScience
An artist’s impression of Epsilon Indi Ab with water clouds atop its ammonia-dominated atmosphere. Image credit: E.C. Matthews, MPIA / T. Müller, HdA.
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Webb Spots Icy Clouds on Distant Jupiter-Like Exoplanet

  • April 24, 2026
Using the NASA/ESA/CSA James Webb Space Telescope, astronomers have detected water-ice clouds swirling through the atmosphere of Epsilon…
SScience
The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
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The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere

  • April 18, 2026
The retrieved transmission spectrum using the results from the free retrieval plotted as a black line, along with…
SScience
An artist’s impression of the asteroid 2025 MN45. Image credit: NSF-DOE Vera C. Rubin Observatory / NOIRLab / SLAC / AURA / P. Marenfeld.
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Earth’s Building Blocks Came from Close to Home, Planetary Scientists Say

  • March 31, 2026
A new analysis of isotopic signatures across planets and meteorite parent bodies suggests our home world formed entirely…
SScience
These Webb (left) and Hubble (right) images reveal Saturn in infrared and visible light. Image credit: NASA / ESA / CSA / STScI / A. Simon, NASA-GSFC / M. Wong, University of California / J. DePasquale, STScI.
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Webb and Hubble Telescopes Capture Saturn in Unprecedented Detail

  • March 27, 2026
By combining infrared observations from the NASA/ESA/CSA James Webb Space Telescope with visible-light imagery from the NASA/ESA Hubble…
SScience
These images, taken with ESO’s Very Large Telescope, show a planetary system being born around the young star WISPIT 2. Image credit: ESO / Lawlor et al.
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Two Protoplanets Emerge from Dusty Disk around Nearby Young Star

  • March 24, 2026
Using ESO’s Very Large Telescope (VLT) and VLT Interferometer (VLTI) in Chile, astronomers have directly observed two gas…
SScience
Webb captured the auroral footprints of Io and Europa, providing spectral measurements for the first time, and revealing extreme changes in the physical properties within Io’s auroral footprint that are likely linked to the electrons crashing into the top of Jupiter’s atmosphere. Image credit: NASA / ESA / CSA / Webb / NIRCam / Jupiter ERS Team / Judy Schmidt / Katie L. Knowles, Northumbria University.
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Webb Captures Io’s and Europa’s Auroral Footprints in Jupiter’s Atmosphere

  • March 6, 2026
The NASA/ESA/CSA James Webb Space Telescope conducted a clockwise scan around the entire limb of Jupiter, chasing aurora…
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