[Climate of the Past] It is believed that the atmospheric circulation on Snowball Earth produced a net ablation zone exposing bare sea ice.
atmosphere
![Schematic of the flow-map encoder–operator–decoder architecture used to emulate chemical kinetics. The encoder maps the current normalized input state (and global parameters) to a latent space. The latent dynamics operator evolves this latent state using the time step and global parameters, and the decoder reconstructs the predicted future normalized species state. Optional residual connections can be applied in latent space and/or on the normalized model outputs.-- astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Accelerating.png?resize=1200%2C718&ssl=1)
Posted inExoplanets, -moons, -comets
Accelerating Chemical Kinetics For Exoplanet Atmospheres Using Neural Networks
[astro-ph.EP] Observations increasingly reveal the coupled radiative, chemical, and dynamical processes that shape exoplanet atmospheres. Interpreting these atmospheres requires models that can capture this complexity.
Posted inLava / magma ocean / Volcanic Worlds
Atmosphere Detected On The Coldest Lava World To Date
[University of Chicago] In the search for extraterrestrial life, it makes sense to first look for rocky planets with an atmosphere, like Earth. Without an atmosphere, a planet can’t have […]
Posted inExoplanets, -moons, -comets
Stellar Flares Rather Than High Tint As Possible Cause For the Missing Methane In Young Exoplanets: The Case Study of V1298-Tau b
[astro-ph.EP] Recent observations of V1298-Tau b, a warm sub-Neptune (R=9.85±0.3R⊕, M=13.1±5.3,M⊕, Teq=670K) orbiting a young (10-30Myr) K star, show depleted methane and surprising abundances of CO2 in its atmosphere.
![Figure showing the structure of pure carbon planets ranging from 0.1 to 20 Earth masses with a surface temperature of 300K. Color bar indicates density in g/cm3 . -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/09/Modeling-Carbon.png?resize=1200%2C719&ssl=1)
Posted inExoplanets, -moons, -comets
Modeling Carbon-Based Planets with MAGRATHEA
[astro-ph.EP] A planet’s interior structure not only influences its habitability, but it also provides information about the planet’s formation and history.
Posted inTitan
Experimental Measurements of Benzene Ice Critical Saturation Ratios on Titan Tholins and Impact on the Microphysical Modeling of Titan’s South Polar Benzene Cloud
[The Planetary Science Journal] The Cassini Composite Infrared Spectrometer revealed the presence of a benzene (C6H6) ice cloud in Titan’s autumn south polar stratosphere following the northern spring equinox in […]
Posted inExoplanets, -moons, -comets
A Clearer View of HAT-P-1 b: JWST NIRSpec G395H Reveals Water, Carbon Dioxide, and Possibly Hydrogen Sulfide
[astro-ph.EP] As part of JWST’s Exoplanet Grand Tour Survey, we use panchromatic transmission spectroscopy to connect HAT-P-1 b’s previously studied optical and near-infrared atmosphere to the longer-wavelength molecular bands accessible […]
Posted inExtremeophiles and Extreme Environments
Cultivation Of Halophilic Archaea In Shallow Subsurface Martian Conditions Has Implications For Extant Life On Mars
[biorxiv.org] The present-day martian surface is generally considered inhospitable to life because of low atmospheric pressure, intense surface radiation, global desiccation, and oxidizing chemistry which has been increasing since the […]
Posted inAtmospheres, Climate, Weather
Atmospheric Retrieval of Combined JWST, HST, and Ground-Based Observations Reveals a Featureless Transmission Spectrum for GJ 1132 b
[astro-ph.EP] We present a panchromatic transmission spectrum of GJ1132b spanning 0.71–5.16 μm, combining published transit observations from Magellan/LDSS3C, HST/WFC3 G141, and JWST/NIRSpec (G395H and G395M).
![Global Temperature contour maps of Venus with VEX RO serving as the primary reference dataset. The data binning is the same as in Figure 4. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Study-on.png?resize=1200%2C720&ssl=1)
Posted inVenus
Study On The Venusian Atmospheric Thermal Structure: A Comparative Analysis Between VEX/Akatsuki And Venus-GRAM/VCD
[astro-ph.EP] We investigate the thermal structure of the Venusian middle atmosphere between 45 and 80 km using radio occultation (RO) measurements from Venus Express and Akatsuki spanning 2006-2024.