Small D-type asteroids in the NEO population: new targets for space missions-Reference-Cited by-同舟云学术

Small D-type asteroids in the NEO population: new targets for space missions

Published:2018-02-27 Issue:4 Volume:476 Page:4481-4487
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Barucci Maria Antonietta¹^ORCID,Perna D¹²,Popescu M¹³,Fornasier S¹^ORCID,Doressoundiram A¹,Lantz C⁴,Merlin F¹,Fulchignoni M¹,Dotto E²,Kanuchova S⁵

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, F-92195 Meudon Pricipal Cedex, France

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

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

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

5. Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranska Lomnica, Slovak Republic

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/476/4/4481/24553665/sty532.pdf

Reference58 articles.

1. Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids

2. 67P/Churyumov-Gerasimenko, a Jupiter family comet with a high D/H ratio

3. Major achievements of the Rosetta mission in connection with the origin of the solar system

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