Infrared absorption spectra from organic matter in the asteroid Ryugu samples: Some unique properties compared to unheated carbonaceous chondrites

被引：9

作者：

Kebukawa, Yoko ^{[1
]}

Quirico, Eric ^{[2
]}

Dartois, Emmanuel ^{[3
]}

Yabuta, Hikaru ^{[4
]}

Bejach, Laure ^{[5
]}

Bonal, Lydie ^{[2
]}

Dazzi, Alexandre ^{[6
]}

Deniset-Besseau, Ariane ^{[6
]}

Duprat, Jean ^{[7
]}

Engrand, Cecile ^{[5
]}

Mathurin, Jeremie ^{[6
]}

Barosch, Jens ^{[8
]}

Cody, George D. ^{[8
]}

De Gregorio, Bradley ^{[9
]}

Hashiguchi, Minako ^{[10
]}

Kamide, Kanami ^{[4
]}

Kilcoyne, David ^{[11
]}

Komatsu, Mutsumi ^{[12
,13
]}

Martins, Zita ^{[14
]}

Montagnac, Gilles ^{[15
]}

Mostefaoui, Smail ^{[7
]}

Nittler, Larry R. ^{[8
,16
]}

Ohigashi, Takuji ^{[17
]}

Okumura, Taiga ^{[18
]}

Remusat, Laurent ^{[7
]}

Sandford, Scott ^{[19
]}

Shigenaka, Miho ^{[4
]}

Stroud, Rhonda ^{[9
,16
]}

Suga, Hiroki ^{[20
]}

Takahashi, Yoshio ^{[18
]}

Takeichi, Yasuo ^{[21
]}

Tamenori, Yusuke ^{[20
]}

Verdier-Paoletti, Maximilien ^{[7
]}

Wakabayashi, Daisuke ^{[21
]}

Yamashita, Shohei ^{[21
]}

Yurimoto, Hisayoshi ^{[22
]}

Nakamura, Tomoki ^{[23
]}

Noguchi, Takaaki ^{[24
]}

Okazaki, Ryuji ^{[25
]}

Naraoka, Hiroshi ^{[25
]}

Sakamoto, Kanako ^{[26
]}

Tachibana, Shogo ^{[18
]}

Yada, Toru ^{[26
]}

Nishimura, Masahiro ^{[26
]}

Nakato, Aiko ^{[26
]}

Miyazaki, Akiko ^{[26
]}

Yogata, Kasumi ^{[26
]}

Abe, Masanao ^{[26
]}

Okada, Tatsuaki ^{[26
]}

Usui, Tomohiro ^{[26
]}

机构：

[1] Yokohama Natl Univ, Dept Chem & Life Sci, Yokohama, Kanagawa, Japan

[2] Univ Grenoble Alpes, CNRS, Inst Planetol & Astrophys IPAG, UMR 5274, Grenoble, France

[3] Univ Paris Saclay, Inst Sci Mol Orsay, CNRS, Orsay, France

[4] Hiroshima Univ, Dept Earth & Planetary Syst Sci, Hiroshima, Japan

[5] Univ Paris Saclay, CNRS, Lab Phys 2 Infinis Irene Joliot Curie, Orsay, France

[6] Univ Paris Saclay, CNRS, Inst Chim Phys, Orsay, France

[7] Sorbonne Univ, CNRS, Museum Natl Hist Nat, Inst Mineral Phys Mat & Cosmochim, Paris, France

[8] Carnegie Inst Sci, Earth & Planets Lab, Washington, DC USA

[9] US Naval Res Lab, Mat Sci & Technol Div, Washington, DC USA

[10] Nagoya Univ, Grad Sch Environm Studies, Nagoya, Aichi, Japan

[11] Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA USA

[12] Saitama Prefectural Univ, Ctr Univ Wide Educ, Saitama, Japan

[13] Waseda Univ, Dept Earth Sci, Tokyo, Japan

[14] Univ Lisbon, Inst Mol Sci, Inst Super Tecn, Dept Chem Engn,Ctr Quim Estrutural, Lisbon, Portugal

[15] Univ Lyon 1, Ecole Normale Super Lyon, Lyon, France

[16] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA

[17] UVSOR Synchrotron Facil, Inst Mol Sci, Okazaki, Aichi, Japan

[18] Univ Tokyo, Dept Earth & Planetary Sci, Tokyo, Japan

[19] NASA, Ames Res Ctr, Moffett Field, CA USA

[20] Japan Synchrotron Radiat Res Inst, Sayo, Hyogo, Japan

[21] High Energy Accelerator Res Org, Inst Mat Struct Sci, Tsukuba, Ibaraki, Japan

[22] Hokkaido Univ, Dept Earth & Planetary Sci, Sapporo, Hokkaido, Japan

[23] Tohoku Univ, Dept Earth Sci, Sendai, Miyagi, Japan

[24] Kyoto Univ, Dept Earth & Planetary Sci, Kyoto, Japan

[25] Kyushu Univ, Dept Earth & Planetary Sci, Fukuoka, Japan

[26] Japan Aerosp Explorat Agcy JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan

[27] Kanagawa Inst Technol, Atsugi, Kanagawa, Japan

来源：

METEORITICS & PLANETARY SCIENCE | 2024年 / 59卷 / 08期

基金：

日本学术振兴会;

关键词：

SOLAR-SYSTEM; ANTARCTIC MICROMETEORITES; CR; SPECTROSCOPY; STARDUST; ORIGIN; DUST; CM; MINERALOGY; PARTICLES;

D O I：

10.1111/maps.14064

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

The infrared spectral characteristics of organic-rich acid residues prepared from Ryugu samples returned by the JAXA Hayabusa2 mission generally match those from unheated carbonaceous chondrite meteorites, but the residues from Ryugu are richer in methyl and methylene functional groups and have higher CH2/CH3 ratios. Moreover, two distinct outlier carbonaceous phases are found; one with spectral characteristics of N-H functional groups, likely amides, and a second phase containing less nitrogen. Such infrared characteristics of Ryugu organic matter might indicate the pristine nature of the freshly collected samples and reflect the near-surface chemistry in the parent asteroid.

引用

页码：1845 / 1858

页数：14

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