[astro-ph.EP] Aims. The ratio between infrared and visible albedo, pIR/pV, provides a simple proxy for the spectral slope of asteroid surfaces between the visible and near-infrared wavelength ranges. The aim […]
astrogeology
Posted inMars
Cracks In A Martian Crater’s Ice
[NASA/JPL-Caltech/UA] Many impact craters on Mars were filled with ice in past climates. Sometimes this ice flows or slumps down the crater walls into the center and acquires concentric wrinkles […]
![Ni, Cu and Zn elemental maps of three chondrules from Paris, that show microspherule regions partitioned by zones enriched in siderophile elements (i.e., Fe, Ni, Co, Cu; pink arrows). The color bars reflect μg/g concentrations of the elements. While in BSE mode and lithophile element space, these would appear as single ~300 μm diameter chondrules, they represent aggregates of ~100 μm grape-bunch chondrules (pink spheres), where these microchondrules contained metal-rich rims. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Chondrule.png?resize=1200%2C714&ssl=1)
Posted inAstrogeology
Chondrule Formation In The Outer Disk From The Primary Three-dimensional Chemical Composition Of CM Chondrules
[astro-ph.EP] Chondrules and their associated fine-grained rims record key processes in the early protoplanetary disk, yet the links between chondrule chemistry, morphology, and matrix complementarity remain poorly constrained.
Community Workshop: The Mission to Enceladus – The ESA L4 Mission
The community workshop at ESTEC focused on “The Mission to Enceladus – The ESA L4 Mission” will be held at ESTEC December 8-10, 2026. The workshop will have a dual […]
Posted inAnalog Studies
Offworld Astrogeology Training In Iceland
Iceland’s diverse volcanic terrain is an excellent stand-in for lunar and planetary processes and provides an ideal environment in which to simulate surface science operations. Editor’s note: when it comes […]
Posted inMars
Martian Geology: Possible Evidence Of Glacial Processes
At the southern section of the floor of an impact crater is this stunning lobate (tongue-shaped) debris apron with surface banding showing high sinuosity.
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.
![(a) Schematic of Europan ice-ocean system [related image in 11]. (b) Map of sea surface temperature (◦C) showing the transition between the temperature-stratified North Atlantic Ocean and the salt-stratified Arctic Ocean; (c) Potential temperature (left) and salinity (right) profiles with depth from location near the North Pole. Different water-mass characteristics are labeled. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/What-can.png?resize=1200%2C582&ssl=1)
Posted inWater/Hycean Worlds & Oceanography
What Can Planetary Ice Shells Teach Us about Ocean Mixing and Life, and Why Salt Matters
[astro-ph.EP] Past and present climates, both on Earth and in planetary systems, maintain ice covers with underlying oceans. This can range from sea ice in the Arctic Ocean to global […]
Posted inExoplanets, -moons, -comets
The Ingredients For Planets Formed Far Earlier Than Thought
[University of Portsmouth] The building blocks of rocky planets could have started forming just 100 million years after the Big Bang – long before the first galaxies even existed, according […]
Lunar and Planetary Science Conference (LPSC) 2027
The 58th Lunar and Planetary Science Conference (LPSC) will be held as a hybrid conference on March 15–19, 2027. LPSC is a defining event in planetary research, bringing together a […]