[University Of Arizona]. A Jupiter-sized world just 7.5 light-years away is cloudy, chemically complex, and, it turns out, more like home than anyone expected.
Clouds
Posted inMars
Mars’ Oddest Cloud May Be Even Odder Than We Thought
[ESA]. Scientists using the European Space Agency’s Mars Express, in combination with a state-of-the-art meteorological model of the Red Planet, have found that there may be some very exotic physics […]
![Observation and modeling of the Arsia Mons Elongated Cloud (AMEC). (A) Observation by the Mars Express VMC imager41,42, at 8.5 a.m. Local Time. (B) Reference simulation assuming only heterogeneous nucleation, at 8.1 a.m. Local Time. (C) Same as B, but with homogeneous nucleation added. See also supplementary video S1.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Homogeneous.png?resize=1200%2C720&ssl=1)
Posted inMars
Homogeneous Nucleation of Water Vapor Evidenced by Elongated Clouds on Mars
[astro-ph.EP] It is widely accepted that water vapor forms clouds by heterogeneous nucleation (condensation on pre-existing dry nuclei).
![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.
Posted inVenus
Altered Cosmic Organics As Venus’ Ultraviolet Absorbers
[astro-ph.EP] Venus’ ultraviolet (UV) absorbers significantly contribute to the atmosphere’s energy budget. However, the composition of these absorbers remains a mystery.
Posted inExoplanets, -moons, -comets
Atmospheric Diversity of Giant Planet Analogs from 3-5µm with SPHEREx
[astro-ph.EP]. The emergent spectra of giant planets peak at thermal infrared wavelengths (3-5um) and possess atmospheric features in this regime that trace carbon chemistry, vertical mixing, clouds, and composition.
Posted inExoplanets, -moons, -comets
CARMApy: An Open-Source Python Framework for Simulating Microphysical Clouds in Planetary Atmospheres
[astro-ph.EP] CARMApy is a new open-source python code that performs bin-scheme microphysical modeling of clouds in exoplanet atmospheres.
Posted inVenus
A Panspermia Origin For Venus Cloud Life
[USRA] Panspermia is the idea that life can originate on one planetary body and then be transferred to other bodies. Impacts are often the suggested method for transfer, as they […]
Posted inExoplanets, -moons, -comets
Radiatively Controlled Thermal Stability of High-Altitude Clouds in Exoplanetary Atmospheres
[astro-ph.EP] One of the most striking findings of exoplanetary science is the ubiquity of clouds. A conventional approach to infer the cloud compositions is to utilize the thermochemical equilibrium model […]
Posted inAtmospheres, Climate, Weather, Biogeochemical Cycles & Geobiology, Biophysics, Biosignatures & Paleobiology, Extremeophiles and Extreme Environments, Genomics, Proteomics, Bioinformatics, Habitable Zones, Microbiology & Virology, Status Report, Venus
Acidophilic Fungi As Possible Candidates For Living Forms In Venus’ Clouds
Present-day Venus, similar to Earth in terms of relative radius, acceleration of gravity and mean density, is characterised by a very strong greenhouse effect and full cloud cover.