[Science China Press] The research team, led by Dr. Yanhao Lin and Dr. Ho-kwang Mao of the Center for High Pressure Science and Technology Advanced Research (HPSTAR), together with Prof. […]
atmosphere
![[LEFT] Extended Seasonal evolution of total atmospheric optical depth across 669 Sol (a) Total atmospheric optical depth for the control simulation (b) Total atmospheric optical depth under singleinjection aluminium nanoparticle substitution (c) Total optical-depth anomaly between the seeded and control simulations, showing the temporal evolution of the radiative effect associated with the aerosol substitution Extended [RIGHT]] Seasonal evolution of aerosol optical depth across 669 Sol (a) Aerosol optical depth for the control simulation, showing the spatial and temporal distribution of the background aerosol (b) Aerosol optical depth under single-injection aluminium nanoparticle substitution (c) Aerosol optical-depth anomaly between the seeded and control simulations, showing the evolution and decay of the aerosol optical signal in the absence of continuous replenishment. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/3D-Global.png?resize=1200%2C714&ssl=1)
Posted inTerraforming & Geoengineering
3D Global Climate Simulations of Synthetic Mars Warming
[astro-ph.EP] Artificial warming via engineered aerosols presents a novel pathway to bypass volatile scarcity on modern Mars.
Posted inExoplanets, -moons, -comets
Trailblazing Technique Uncovers The Real Shape Of Scorching-hot Exoplanet Atmospheres
[University of Bristol] Until now the alien white-hot worlds of exoplanets have been depicted as circular, but new research has revealed the true shape of their atmospheres to be a […]
Posted inAtmospheres, Climate, Weather
Simulations Of The Evolving Ozone Layer: Implications For The Early Earth, Exoplanets, And The Search For Life
[astro-ph.EP] Over 4 billion years, Earth’s atmosphere has been transformed from a composition devoid of molecular oxygen (O2) to one where O2 is now 21% of our modern atmosphere by […]
![Pressures determined by ruby fluorescence measurements at different locations within the sample chamber: (a) during powder compaction, (b) after decompression. No ruby fluorescence spectrum was obtained on the sphere marked with an asterisk, likely due to insufficient Cr doping, resulting in an undetectable fluorescence signal. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/10/Elastic.png?resize=1200%2C720&ssl=1)
Posted inTitan
Elastic Properties of Titan Tholins Revealed by Brillouin Spectroscopy
[astro-ph.EP] Titan tholins, complex organic solids synthesized by simulating photochemical processes in Titan’s atmosphere, are widely regarded as analogs to organic surface materials on the Saturnian moon.
Posted inExoplanets, -moons, -comets
Ultraviolet Reflected-Light Spectroscopy of Modern Earth Analogs with Starshade Observations
[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 […]
![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.