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Browsing Tag

Exoplanet

111 posts
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
Ultraviolet-Driven Atmospheric Degeneracies Challenge Conventional Biosignature Frameworks for Terrestrial Planets with Ultracool M Dwarf Hosts: An Archean-Analog TRAPPIST-1 e Case Study
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Ultraviolet-Driven Atmospheric Degeneracies Challenge Conventional Biosignature Frameworks for Terrestrial Planets with Ultracool M Dwarf Hosts: An Archean-Analog TRAPPIST-1 e Case Study

  • June 8, 2026
Comparison of input SEDs used in this study and molecular photoabsorption cross sections relevant to Archean-analog photochemistry. The…
SScience
Predictive Rankings of the Probability for Temperate Terrestrial Worlds for the HWO ExEP Mission Star List
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Predictive Rankings of the Probability for Temperate Terrestrial Worlds for the HWO ExEP Mission Star List

  • June 5, 2026
The simulated occurrence rates of planets in both simulated (blue) and known (orange) planetary systems around nearby stars.…
SScience
NASA’s Roman Mission Preps to Unveil New Populations of Faraway Worlds
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NASA’s Roman Mission Preps to Unveil New Populations of Faraway Worlds

  • May 30, 2026
This plot shows currently known exoplanets, with different categories highlighted. Roman will help fill in the bottom-right of…
SScience
Red Dwarf Stars Detected ‘Eating’ Earth-like Planets
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Red Dwarf Stars Detected ‘Eating’ Earth-like Planets

  • May 30, 2026
This artist’s impression shows two Earth-sized worlds passing in front of their parent red dwarf star in the…
SScience
The Unique Ability Of The Hubble Space Telescope To Characterize Young Exoplanet Environments
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The Unique Ability Of The Hubble Space Telescope To Characterize Young Exoplanet Environments

  • May 30, 2026
Modified Pass et al. (2025) Figure 2 showing an updated Cosmic Shoreline for exoplanets orbiting full convective M…
SScience
Weighing Newborn Planets Using Their Dusty Fingerprints
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Weighing Newborn Planets Using Their Dusty Fingerprints

  • May 29, 2026
Simulation of a planet embedded in a protoplanetary disc, causing disc material to pile up in a ring…
SSpace
Gas Giant Exoplanet TOI 4465 B Orbiting Distant Star
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NASA Finds a “Goldilocks” Giant Planet Wrapped in Methane

  • May 29, 2026
Artist’s impression of a gas giant planet orbiting its distant host star. New research, led by astronomers at…
SSpace
Gas Giant Planet Formation
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Super Jupiters Expose a Long Standing Space Mystery

  • May 26, 2026
One way gas giants form is through core accretion, where solid cores gradually grow in a disk by…
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
HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
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HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory

  • May 25, 2026
Upper panels: Equatorial rotational velocity (veq) vs. projected rotational velocity (v sin i) for stars in Tiers 1,…
SScience
Constraints On The Crystallinity Of Water Ice In Planet-forming Disks From Infrared Scattered-Light Spectra
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Constraints On The Crystallinity Of Water Ice In Planet-forming Disks From Infrared Scattered-Light Spectra

  • May 24, 2026
Protoplanetary disk images (top row) and scattered-/transmitted-light spectra (bottom-left and bottom-middle) obtained from the radiative-transfer simulations, together with…
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