Organic Matter in the Solar System-Implications for Future on-Site and Sample Return Missions

被引：24
作者：
Martins, Zita [1 ]
Chan, Queenie Hoi Shan [2 ,3 ]
Bonal, Lydie [4 ]
King, Ashley [2 ,5 ]
Yabuta, Hikaru [6 ]
机构：
[1] Univ Lisbon, Ctr Quim Estrutural, Dept Engn Quim, Inst Super Tecn, Ave Rovisco Pais 1, P-1049001 Lisbon, Portugal
[2] Open Univ, Planetary & Space Sci, Sch Phys Sci, Walton Hall, Milton Keynes MK7 6AA, Bucks, England
[3] Royal Holloway Univ London, Dept Earth Sci, Egham TW20 0EX, Surrey, England
[4] Univ Grenoble Alpes, Inst Planetol & Astrophys Grenoble, CNRS, CNES, F-38000 Grenoble, France
[5] Nat Hist Museum, Cromwell Rd, London SW7 5BD, England
[6] Hiroshima Univ, Dept Earth & Planetary Syst Sci, 1-3-1 Kagamiyama, Hiroshima 7398526, Japan
来源：
SPACE SCIENCE REVIEWS | 2020年 / 216卷 / 04期
基金：
英国科学技术设施理事会; 欧盟地平线“2020”;
关键词：
Organic matter; Solar system; Comets; Asteroids; Extraterrestrial samples; Sample return mission; INTERPLANETARY DUST PARTICLES; SPECTRAL REFLECTANCE PROPERTIES; ANTARCTIC CARBONACEOUS CHONDRITES; POLYCYCLIC AROMATIC-HYDROCARBONS; EXTRATERRESTRIAL AMINO-ACIDS; OXYGEN ISOTOPIC COMPOSITIONS; MOLECULAR-CLOUD MATERIAL; COMPOUND-SPECIFIC CARBON; MURCHISON METEORITE; AQUEOUS ALTERATION;
D O I：
10.1007/s11214-020-00679-6
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Solar system bodies like comets, asteroids, meteorites and dust particles contain organic matter with different abundances, structures and chemical composition. This chapter compares the similarities and differences of the organic composition in these planetary bodies. Furthermore, these links are explored in the context of detecting the most pristine organic material, either by on-site analysis or sample return missions. Finally, we discuss the targets of potential future sample return missions, as well as the contamination controls that should be in place in order to successfully study pristine organic matter.
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页数：23
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