[astro-ph.EP] Characterizing rocky, habitable zone planets in reflected light is a key science objective for future direct imaging missions, and the ultraviolet (UV) is uniquely suited for supporting the characterization […]
atmosphere
![Latitude-longitude maps of mean water vapour and hydrogen chloride volume mixing ratios and coefficient of variation (standard deviation divided by the mean) in percentage form at 20.91 km altitude. The values are calculated over four Venus solar days (468 Earth days). --[astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/How-long.png?resize=1200%2C717&ssl=1)
Posted inVenus
How Long Could Volcanic Plumes Persist In The Venus Atmosphere?
[astro-ph.EP] Resolving the ambiguity surrounding current Venusian volcanism is a primary objective for upcoming missions like EnVision and VERITAS.
![Set Transformer actor–critic architecture used by the RL policy. The input candidate set 𝑋 ∈ R 𝑁×𝐹 is first projected into a latent 𝑑-dimensional representation and processed by 𝐿 Induced Set Attention Blocks (ISABs). Learned inducing tokens provide the queries in the first attention operation of each ISAB, after which information is redistributed to the candidate tokens. The actor combines each contextualised target representation with the global mission state to produce one logit per available observation. Each logit is then converted into a probability to select a corresponding observation. The critic uses Pooling by Multihead Attention (PMA) to obtain a permutation-invariant summary of the candidate set, which is combined with the same global state to estimate 𝑉 (𝑠). -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/aRieL-Reinforcement.png?resize=1200%2C715&ssl=1)
Posted inAriel Mission
aRieL – Reinforcement Learning For The Ariel Space Telescope Scheduling
[astro-ph.EP] The Ariel mission will conduct a population level survey of hundreds of exoplanet atmospheres, requiring observations to be scheduled across a large and diverse catalogue of potential targets.
Posted inExoplanets, -moons, -comets
The Accretionally Heated Atmospheres Of Protoplanets And Brown Dwarfs
[astro-ph.EP] The ranks of accreting planets and brown dwarfs are growing. To help interpret their spectra, we study how accretion affects a planet’s atmosphere. The atmosphere is irradiated from above […]
![[Left]: A concept raytrace showing the IFS, with just the FUV channels shown. The NUV channels take the zero-order from each FUV grating and reflect it towards the IFS fold mirror (on either side) into a similar format NUV IFS (see Haughton et al., 2026 for a depiction of the INFUSE design that this IFS is based on13). The IFS assembly is forward (out of the page) from the MOS at the focal plane, with the IFS fold mirror canted slightly to move the slicer, gratings, and detectors over 0.7 meters from the MOS optical path. [Right]: The slicer-based IFS operates by reflecting portions of the image plane to different gratings, which then focus a spectrogram to a unique portion of the detector. In essence, each reflective slice operates like a long-slit spectrograph, with the slicer geometry separating the multi-slit spectrograph to avoid spectral confusion.-- astro-ph.IM](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/An-Ultraviolet.png?resize=1200%2C563&ssl=1)
Posted inAstronomy & Telescopes
An Ultraviolet Instrument On The Habitable Worlds Observatory: Considerations and Capability Trades On The Multi-Object, Integral-field, and High-resolution Modes Of A Potential UVI
[astro-ph.IM] The Habitable Worlds Observatory (HWO) is NASA’s next-generation astrophysics platform, delivering transformative capability in the search for life and study of the origins of the universe.
![A comparison of the upwards and downwards long-wave radiative fluxes (left and middle column) after 2000 years using a tidally-locked co-ordinate system. AS, T and SS denote the antistellar point, terminator and substellar point respectively. The right-hand column shows the difference in fluxes in filled contours, which are overlain by solid black contours that indicate the percentage increase of specific humidity in the 100 m versus the 10 m simulation.-- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/The-Hydrological.png?resize=1200%2C720&ssl=1)
Posted inExoplanets, -moons, -comets
The Hydrological Cycle and Circulation of Tidally-Locked Planets with A Finite Moisture Inventory
[astro-ph.EP] Tidally-locked planets express a range of climate regimes distinct from those found in our solar system.
Posted inBiogeochemical Cycles & Geobiology
Material Cycling Across Earth’s Spheres And Triggers Of Cambrian Explosion: A Tectonic Perspective
[ELSP] A comprehensive model of the Cambrian explosion featuring “multi-factors coupling and multi-sphere driving”. Supercontinent breakup and mantle plume activity served as the initial trigger of environmental change in the […]
Posted inAtmospheres, Climate, Weather
Where Does Earth’s Nitrogen Go? Two Atoms Offer A Clue
[Science] Nitrogen is one of life’s building blocks, but it’s only helpful in the right amounts. Too much nitrogen in water, for example, can lead to poor water quality and […]
Posted inBrown Dwarfs
First Detection Of Variable Water Clouds Outside Of Our Solar System
[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.
Posted inBrown Dwarfs
SPHEREx Telescope Sees Menagerie Of Brown Dwarfs
[NASA] NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) space telescope is shedding light on brown dwarfs, celestial objects that blur the line […]