[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 […]
lava world
Posted inExoplanets, -moons, -comets
An Evolving Cosmic Shoreline and Sandbar Bounding the Rocky Airless Valley
[astro-ph.EP] Recent JWST observations challenge the traditional ‘cosmic shoreline’ from both sides, revealing thick volatile atmospheres on the hottest close-in ‘lava worlds,’ where irradiation should drive the most extreme escape, […]
![An artist’s rendering of “cosmic sandbar” planet TOI-561b orbiting its star, with its atmosphere illuminated. (Image credit: NASA, ESA, CSA, Ralf Crawford [STScI])](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Why-Some.jpg?resize=1200%2C719&ssl=1)
Posted inLava / magma ocean / Volcanic Worlds
Why Some Planets Have Theory-defying Atmospheres
[Stanford University] Stanford researchers have offered a compelling explanation for why some sizzling, lava-covered worlds nestled tightly around their stars can keep hold of their atmospheres. At such close quarters, […]
Posted inIo
Lava World Recon: Juno Measures Subsurface Temperature Of Io
[SwRI] NASA’s Juno mission has made the first direct measurements of the temperature below the surface of Jupiter’s moon Io, which reveal significant heating in the upper few feet of […]
Posted inVenus
Venus: Dead? Far From It
[ETH Zurich] Simulations conducted by researchers at ETH Zurich suggest a strong likelihood that Venus’s rift valleys are still geologically active rather than being mere relics of a bygone era, […]
Posted inIo
Lava World Recon: Juno Studies Io’s Volcanoes
[NASA] NASA’s Juno mission has provided the first measurements of the temperature below the surface of Jupiter’s moon Io, revealing significant heating within the shallow subsurface of the most volcanically […]
Posted inBiogeochemical Cycles & Geobiology
Fire And Ice: Were Yellowstone’s Past Volcanic Eruptions And Glaciations Related?
[USGS/Yellowstone Volcano Observatory] Yellowstone is a land of fire and ice. Not only does it have a history of different styles of volcanic eruptions, but it has also been covered […]
![Numerical computations corresponding to the candidate pattern in the H–alpha filter (λ0 = 656 nm), for the total flux (left) and the polarized flux (right). The background polarization signal has been subtracted from the latter. The decrease in spatial resolution due to the Earth’s atmosphere is not included. The planetary atmosphere is assumed to be horizontally homogeneous except for the gas density variations. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Planet-wide.png?resize=1200%2C711&ssl=1)
Posted inVenus
Planet-wide, Concentric Density Waves in Venus’s Upper Atmosphere Revealed through Polarimetry?
[astro-ph.EP] We report observations of faint (10−6), concentric, planet-wide rings in the polarized flux of sunlight that is reflected by Venus, obtained during a serendipitous, 36-minute run in 2010, with […]
![Schematic of the coupled interior-atmosphere evolutionary framework PROTEUS, showing the links between interior, surface, atmosphere, and stellar modules. Core components include SPIDER (mantle dynamics), CALLIOPE (surface in-/outgassing), AGNI/JANUS (radiativeand prescribed-convective atmospheres), ZEPHYRUS (atmospheric escape), and MORS (XUV stellar evolution). Modules exchange energy fluxes at each planetary interfaces—including core cooling, volatile outgassing, heat transport, heat loss to space, escape and stellar irradiation—while C–H–O–N–S volatiles are tracked throughout the mantle and atmosphere. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Atmospheric-evolution.png?resize=1200%2C718&ssl=1)
Posted inAtmospheres, Climate, Weather
Atmospheric Evolution Through Outgassing And Escape On Young Molten Rocky Exoplanets
[astro-ph.EP] The earliest rocky planet atmospheres are shaped by competition between initial volatile inventories and atmospheric escape. On young magma ocean planets, outgassing competes with atmospheric escape, controlling volatile retention […]
![Reflation events (red) occur across a range of ages and with different magnitudes across the evolution of irradiated super-Earths. The plot shows the normalised bulk density evolution of individual simulations, versus the time elapsed since planet formation. The red lines indicate cases where a reflation event occurs, while blue lines indicate those where it does not occur. The evolution tracks that end with a dot indicate the planet has reached an airless state and complete atmospheric erosion by hydrodynamic escape has taken place. The evolution of the two select cases for Figure 1 are highlighted and denoted with a R and D. These cases illustrate in more detail a representative reflation (red) and deflation case (blue). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/07/Reflation.png?resize=1200%2C717&ssl=1)
Posted inAstrogeology
Reflation: Redox-driven Atmospheric Inflation As Tracer Of Super-Earth Geochemistry
[astro-ph.EP] We demonstrate that the redox-sensitivity of mantle outgassing can trigger transient episodes of atmospheric re-inflation in highly irradiated and geochemically-reduced super-Earths, a mechanism we term reflation.