![Mapping of the science cases proposed by the Science Working Groups (center) to the questions and discovery areas identified by Astro2020 (left and right). The transparencies of the lines indicate the number of connections with darker lines indicating stronger links between the SWG and the Astro2020 topic. -- [astro-ph.IM]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Early-Exploration.png?resize=1200%2C711&ssl=1)
[astro-ph.IM] The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO should conduct […]
Imaging & Spectroscopy
Posted inAstrochemistry
Astrochemistry: A Cosmic Recycling System In Action In The Helix Nebula
[Northwestern University] An international team of scientists, including Northwestern University astrophysicists, has captured an unprecedented view of a dying star’s remains in the act of being recycled.
![Observed spectra compared to laboratory data for CO (left), 13CO2 (middle), and H2O (right) ices on carbonaceous dust analogs. -- [astro-ph.GA]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Molecule-specific.png?resize=1200%2C606&ssl=1)
Posted inAstrochemistry
Molecule-specific Diffusion And Desorption Of Interstellar Ices On Carbonaceous Dust
[astro-ph.GA] Interstellar ices form on dust grains in the coldest regions of molecular clouds and preserve key volatile reservoirs that could be incorporated into protoplanetary disks during star and planet […]
![Top left: (pgas, Tgas) cross-section through the terminators of WASP-69 b, with the location of the CH4 quench point overlaid (light blue line). We define the CH4 quench level as the pressure where the absolute relative difference between the equilibrium and disequilibrium concentrations first exceeds 10−3. Top right: Column densities in the line-of-sight direction in the atmosphere of WASP-69 b for [M/H] = 1.0, and C/O = 0.55 for CH44. Bottom: The same as for CH4 but now for SO2 (left) and CO2 (right). The terminator pressure scale is used as a radius axis. The hotspot offset at 10−4 bars is reflected in the column density of SO2, with larger concentrations being formed on the evening terminator. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Chemical-Tracers.png?resize=1200%2C716&ssl=1)
Posted inExoplanets, -moons, -comets
Chemical Tracers For 3D Atmospheric Asymmetries On WASP-69 b
[astro-ph.EP] Warm giant exoplanets exhibit strong three-dimensional temperature contrasts that can significantly alter atmospheric chemistry through quenching and photochemistry, yet transmission spectra are commonly interpreted using one-dimensional, limb-averaged models. Such […]
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 inMissions & Hardware
Planetary Recon: Interworld Slingshot Resource Surveys
[NASA] This proposal explores a new class of reconnaissance spacecraft that map minerals from orbit using Raman spectroscopy during high-speed flybys–without landing, sample return, or extended dwell. Editor’s note: for […]
Posted inBiosignatures & Paleobiology
Orbital Biosignature Assay: Pyramid Lake in Bloom
[NASA] The OLI-2 (Operational Land Imager-2) on the Landsat 9 satellite acquired this natural-color image of the bloom in October 2024. One day earlier, the Pyramid Lake Paiute Tribe noted […]
Posted inBiosignatures & Paleobiology
Molecular Assembly As A Universal Biosignature Measurable By Mass Spectrometry
[PNAS] Detecting life beyond Earth requires biosignatures that do not depend on the chemistry of known organisms.
Posted inBiosignatures & Paleobiology
Micropeloidal Textures – Definition, Formation And Potential As Biosignatures
[Earth-Science Reviews] Microbial biosignatures result from the interactions between microbial populations, metabolic processes, organic and mineral products, and the surrounding physicochemical environment.
Posted inMars
An Interesting Crater In Valles Marineris
[ESA] Along the equator of Mars, CaSSIS spotted a couple of interesting craters in Ganges Chasma, a mineralogically diverse canyon in the far-eastern portion of Valles Marineris.