Candidate Main-belt Asteroids for Surface Heterogeneity

Candidate Main-belt Asteroids for Surface Heterogeneity

Large terrestrial bodies in our solar system like the Earth, Mars, Mercury, and the Moon exhibit geologically complex surfaces with compositional heterogeneity. From past studies using large telescopes and spacecraft, it was shown that asteroids with diameters larger than 100 km also show surface he...

Celý popis

Podrobná bibliografie
Hlavní autoři: Sunao Hasegawa, Michaël Marsset, Francesca E. DeMeo, Josef Hanuš, Richard P. Binzel, Schelte J. Bus, Brian Burt, David Polishook, Cristina A. Thomas, Jooyeon Geem, Masateru Ishiguro, Daisuke Kuroda, Pierre Vernazza
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2024-01-01
Edice:The Astronomical Journal
Témata:
Small Solar System bodies
Asteroids
Main belt asteroids
Asteroid surfaces
On-line přístup:https://doi.org/10.3847/1538-3881/ad3045

Internet

https://doi.org/10.3847/1538-3881/ad3045

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