Pallas collisional family Archives

Spectral slope versus the size of the observed Pallas family members. The spectral slopes are calculated from Gaia’s Data Release 3 (DR3) observations (Gaia Collaboration et al. 2016, 2023b) and the sizes are obtained from the 2019 NEOWISE diameters and albedos archive. -- astro-ph.EP

Astrochemistry, Astrogeology, Astronomy & Telescopes, Biochemistry & Organic Chemistry, Biogeochemical Cycles & Geobiology, Comets and Asteroids, Icy Worlds, Imaging & Spectroscopy, Status Report

Near-infrared Spectroscopic Characterization Of The Pallas Family

by Keith CowingMarch 18, 2025March 18, 2025

The Pallas collisional family of asteroids, named after (2) Pallas, is notable for its high orbital inclination and the distinct blue color of Pallas and a few larger B-type family […]

Pallas collisional family

Near-infrared Spectroscopic Characterization Of The Pallas Family

The Role Of Minerals In Prebiotic Evolution: Implications For Identifying Worlds With The Potential For Life’s Origin

Gen-EBM: An Energy Balance Model For Terrestrial Planets. Climate Multistability From Snowball To Post-runaway Greenhouse Climates

Astrometric Planet Search Around Southern Ultracool Dwarfs: V. Discovery Of The Exoplanet Candidate PALTA-1 b

Hubble Space Telescope Observations of Active Asteroid (101955) Bennu

SOPHIE And TESS Characterization Of Fourteen TESS Objects Of Interest: Nine Planetary Systems And Five Low-mass Stellar Companions