Olivine-rich asteroids in the near-Earth space-Reference-Cited by-同舟云学术

Olivine-rich asteroids in the near-Earth space

Published:2018-03-15 Issue:2 Volume:477 Page:2786-2795
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Popescu Marcel¹²,Perna D¹³,Barucci M A¹^ORCID,Fornasier S¹^ORCID,Doressoundiram A¹,Lantz C¹⁴,Merlin F¹,Belskaya I N¹⁵,Fulchignoni M¹

Affiliation:

1. LESIA, Observatoire de Paris, PSL Research University, CNRS, Univ. Paris Diderot, Sorbonne Paris Cité, UPMC Univ., Paris 06, Sorbonne Universités, 5 Place J. Janssen, Meudon Pricipal Cedex F-92195, France

2. Astronomical Institute of the Romanian Academy, 5 Cuţitul de Argint, 040557 Bucharest, Romania

3. INAF-Osservatorio Astronomico di Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Rome, Italy

4. IAS, UMR 8617, CNRS, Université Paris-Sud, Bat 121, F-91405 Orsay, France

5. Institute of Astronomy, V.N. Karazin Kharkiv National University, 35 Sumska Str, UA-61022 Kharkiv, Ukraine

Funder

Horizon 2020

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/477/2/2786/25009959/sty704.pdf

Reference48 articles.

1. Classification of asteroids using G-mode analysis

2. Spectral observations for near-Earth objects including potential target 4660 Nereus : Results from Meudon remote observations at the NASA Infrared Telescope Facility (IRTF)

3. Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes

4. The olivine-dominated composition of the Eureka family of Mars Trojan asteroids

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