Results 111 to 120 of about 218,932 (203)
Passive sorting of asteroid material using solar radiation pressure [PDF]
Understanding dust dynamics in asteroid environments is key for future science missions to asteroids and, in the long-term, also for asteroid exploitation.
Sanchez Cuartielles, Joan-Pau +2 more
core +1 more source
Context. Asteroid (469219) Kamo‘oalewa is the target of the Tianwen-2 sample-return mission by the China National Space Administration. Because of its orbit and its peculiar spectral properties, it was proposed that Kamo‘oalewa originated from the Moon ...
Fenucci Marco +3 more
doaj +1 more source
Depletion and Excitation of the Asteroid Belt by Migrating Planets
International audienceA model of early inner Solar System evolution whereby the gas-driven migration of Jupiter and Saturn truncates the disk of planetesimals and creates a depleted and dynamically excited asteroid belt populated from two parent ...
Mandell, A. M. +4 more
core
Geochemical Modeling from the Asteroid Belt to the Kuiper Belt: Systematic Review
The high costs and time-consuming nature of space exploration missions are among the major barriers to studying deep space. The lack of samples and limited information make such studies challenging, highlighting the need for innovative solutions ...
Arash Yoosefdoost, Rafael M. Santos
doaj +1 more source
Depletion and Excitation of the Asteroid Belt by Migrating Planets
International audienceA model of early inner Solar System evolution whereby the gas-driven migration of Jupiter and Saturn truncates the disk of planetesimals and creates a depleted and dynamically excited asteroid belt populated from two parent ...
Mandell, A. M. +4 more
core
Pulsar Timing Noise from Brownian Motion of the Sun
Recently, pulsar timing arrays (PTAs) reported a signal at nanohertz frequencies consistent with a stochastic gravitational-wave background. Here, I show that the Brownian motion of the Sun as a result of its random gravitational interactions with the ...
Abraham Loeb
doaj +1 more source
SPECTROPHOTOMETRIC STUDIES OF ASTEROIDS II: TAXONOMIC TYPE
Analysis of spectral observations of a number of Main Belt asteroids, the Apollo family asteroid (NEO) 30825 (1990 TG1), and the rare asteroid 1951 Lick was used to determine their taxonomic types.
G.K. Aimanova +3 more
doaj +1 more source
Satellite Formation around the Largest Asteroids
Satellites around large asteroids are preferentially found among those with the most rapid rotation and elongated shape. The taxonomic statistics are similarly skewed; in total, 13 asteroids larger than 100 km are known to have satellites, but none have ...
Kevin J. Walsh +5 more
doaj +1 more source
A Spectroscopically Unique Main Belt Asteroid: 10537
We present visible and near-infrared reflectance spectra and interpreted surface mineralogy for asteroid 10537 (1991 RY16). The spectrum of this object is without precedent among the main-belt asteroids. A unique absorption band centered at 0.63 mm could
Schelte J Bus +6 more
core

