Results 101 to 110 of about 218,932 (203)
Arrival and magnetization of carbonaceous chondrites in the asteroid belt before 4562 million years ago. [PDF]
O'Brien T +6 more
europepmc +1 more source
Identifying LL Chondrite Near-Earth Asteroids Using LL Chondrite Reflectance Spectra
Most near-Earth objects are thought to originate from the collisional fragments of the main asteroid belt. One question that remains to be resolved is the proportion of near-Earth objects sampling the core area material of the parent body to the outer ...
Pengyue Wang +3 more
doaj +1 more source
Meteoritics &Planetary Science, Volume 61, Issue 10, Page 2413-2414, October 2026.
wiley +1 more source
Exploring the Bimodal Solar System via Sample Return from the Main Asteroid Belt: The Case for Revisiting Ceres. [PDF]
Burbine TH, Greenwood RC.
europepmc +1 more source
Photometric observations of main-belt asteroid (10422) 1999 AN22 [PDF]
Photometric observations of main-belt asteroid (10422) 1999 AN22 were obtained from May 20 to July 09, 2019, in order to determine its synodic rotation period. Observations were acquired from two observatories in Malta and one from Spain. Through our
Galdies, Charles +2 more
core
Evaluation of a gas dischange transducer and associated instrumentation necessary for the asteroid belt meteoroid experiment [PDF]
Evaluation of gas discharge transducer and associated instrumentation for asteroid belt meteoroid experiment with Pioneer probes F/
Parker, C. D.
core
The main asteroid belt has lost > 99:9% of its solid mass since the time at which the planets were forming, according to models for the protoplanetary disk.
Chambers And Wetherill +2 more
core
Keck and Gemini Characterization of Hayabusa2# Rendezvous Target 1998 KY26
Near-Earth object (NEO) 1998 KY _26 is a target of the Hayabusa2# spacecraft, which it will rendezvous with in 2031 July. The asteroid has been noted to rotate rapidly and has a large out-of-plane nongravitational acceleration.
Bryce T. Bolin +9 more
doaj +1 more source
Collaborative asteroid photometry of six main-belt asteroids
Synodic rotation periods of six main-belt asteroids were derived from photometric observations obtained from 2021 July 21 through November 2 from three observatories situated in Malta and one from Spain. We provide lightcurve rotation periods for (1713) Banchilon, (2232) Altaj, (2458) Veniakaverin, (6681) Prokopovich, (6787) 1991 PF15, and (18863) 1999
Brincat, Stephen M. +3 more
openaire +1 more source
88th Annual Meeting of the Meteoritical Society 2026: Abstracts
Meteoritics &Planetary Science, Volume 61, Issue S1, Page S48-S551, August 2026.
wiley +1 more source

