The Diverse Population Of Small Bodies Of The Solar System
Abstract
Small bodies are rocky and/or icy objects, usually ranging in size from a few meters to a few hundreds of kilometers. They comprise near-Earth and main belt asteroids, Jupiter Trojans, trans-Neptunian objects, Centaurs, comets, and a recently discovered category called the transitional objects. Their physical nature, distribution, formation, and evolution are fundamental to understand how the solar system formed and evolved and, ultimately, how planetary systems are formed in other stars. The number of discoveries regarding exoplanets and debris disks is continuously increasing, and therefore it is crucial to first understand our own solar system's provenance and evolution in order to better interpret what is going on in newly discovered planetary systems. In this chapter we review the main physical and compositional properties of the different populations of small bodies of the solar system.
Publication Date
11-3-2018
Publication Title
Handbook of Exoplanets
Number of Pages
395-419
Document Type
Article; Book Chapter
Personal Identifier
scopus
DOI Link
https://doi.org/10.1007/978-3-319-55333-7_55
Copyright Status
Unknown
Socpus ID
85086424768 (Scopus)
Source API URL
https://api.elsevier.com/content/abstract/scopus_id/85086424768
STARS Citation
de León, Julia; Licandro, Javier; and Pinilla-Alonso, Noemí, "The Diverse Population Of Small Bodies Of The Solar System" (2018). Scopus Export 2015-2019. 10019.
https://stars.library.ucf.edu/scopus2015/10019