A surprising yellow haze of sulfur dioxide in the atmosphere of a gas “dwarf” exoplanet about 96 light years away from our own solar system makes the planet a prime […]
astrogeology
Triton and Pluto: Same Origin But Separated At Birth [Two Possible Ocean Worlds]
Assessing the origin of Pluto and Triton has profound implications for the bigger picture of Solar System formation and evolution.
Planet-forming Disks Around Very Low-mass Stars Are Different
Planets form in disks of gas and dust, orbiting young stars. The MIRI Mid-INfrared Disk Survey (MINDS), led by Thomas Henning from the Max Planck Institute for Astronomy (MPIA) in […]
Stellar Characterization and Chemical Abundances of Exoplanet Hosting M dwarfs from APOGEE Spectra: Future JWST Targets
Exoplanets hosting M dwarfs are the best targets to characterize Earth-like or super-Earth planetary atmospheres with the James Webb Space Telescope (JWST). We determine detailed stellar parameters (Teff, logg, and […]
Recipes For Forming A Carbon-rich Giant Planet
The exploration of carbon-to-oxygen ratios has yielded intriguing insights into the composition of close-in giant exoplanets, giving rise to a distinct classification: carbon-rich planets, characterized by a carbon-to-oxygen ratio ≥ […]
Sulfur Molecules From Space Seeded Early Life On Earth
Important nutrients for the first living organisms on Earth may have come from space, according to new research from the University of Hawaiʻi at Mānoa.
Phobos Photometric Properties From Mars Express HRSC Observations (Comet Capture?)
This study aims to analyze Phobos’ photometric properties using Mars Express mission observations to support the Martian Moons eXploration mission.
Europa Clipper Astrobiology Probe Arrives At Kennedy Space Center
NASA’s Europa Clipper, a spacecraft designed to investigate Jupiter’s icy moon Europa and its potential to support life, arrived in Florida on Thursday, May 23. The spacecraft, assembled at NASA’s […]
A High Internal Heat Flux and Large Core in a Warm Neptune Exoplanet
Interactions between exoplanetary atmospheres and internal properties have long been hypothesized to be drivers of the inflation mechanisms of gaseous planets and apparent atmospheric chemical disequilibrium conditions.
The Empirical and Radiative Transfer Hybrid (EaRTH) Disk Model: Merging Analyses of Protoplanetary Dust Disk Mineralogy and Structure
Our understanding of how exoplanets form and evolve relies on analyses of both the mineralogy of protoplanetary disks and their detailed structures; however, these key complementary aspects of disks are […]
