GSTDTAP  > 地球科学
DOI10.1126/science.aal3496
Xenon isotopes in 67P/Churyumov-Gerasimenko show that comets contributed to Earth's atmosphere
Marty, B.1; Altwegg, K.2,3; Balsiger, H.2; Bar-Nun, A.4; Bekaert, D. V.1; Berthelier, J. -J.5; Bieler, A.2,6; Briois, C.7; Calmonte, U.2; Combi, M.6; De Keyser, J.8; Fiethe, B.9; Fuselier, S. A.10; Gasc, S.2; Gombosi, T. I.6; Hansen, K. C.6; Haessig, M.2,10; Jaeckel, A.2; Kopp, E.2; Korth, A.11; Le Roy, L.2; Mall, U.11; Mousis, O.12; Owen, T.13; Reme, H.14; Rubin, M.2; Semon, T.2; Tzou, C. -Y.2; Waite, J. H.10; Wurz, P.2
2017-06-09
发表期刊SCIENCE
ISSN0036-8075
EISSN1095-9203
出版年2017
卷号356期号:6342页码:1069-+
文章类型Article
语种英语
国家France; Switzerland; Israel; USA; Belgium; Germany
英文摘要

The origin of cometary matter and the potential contribution of comets to inner-planet atmospheres are long-standing problems. During a series of dedicated low-altitude orbits, the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) on the Rosetta spacecraft analyzed the isotopes of xenon in the coma of comet 67P/Churyumov-Gerasimenko. The xenon isotopic composition shows deficits in heavy xenon isotopes and matches that of a primordial atmospheric component. The present-day Earth atmosphere contains 22 +/- 5% cometary xenon, in addition to chondritic (or solar) xenon.


领域地球科学 ; 气候变化 ; 资源环境
收录类别SCI-E
WOS记录号WOS:000402871700052
WOS关键词NOBLE-GASES ; SOLAR ; ABUNDANCES ; ELEMENTS ; MISSION ; ORIGINS ; SYSTEM ; WATER
WOS类目Multidisciplinary Sciences
WOS研究方向Science & Technology - Other Topics
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/196216
专题地球科学
资源环境科学
气候变化
作者单位1.Univ Lorraine, CNRS, Ctr Rech Petrog & Geochim, 15 Rue Notre Dame Pauvres,BP 20, F-54501 Vandoeuvre Les Nancy, France;
2.Univ Bern, Phys Inst, Sidlerstr 5, CH-3012 Bern, Switzerland;
3.Univ Bern, Ctr Space & Habitabil, Sidlerstr 5, CH-3012 Bern, Switzerland;
4.Tel Aviv Univ, Dept Geosci, Tel Aviv, Israel;
5.Univ Paris 06, CNRS, Inst Pierre Simon Laplace, Lab Atmospheres Milieux Observat Spati LATMOS, 4 Ave Neptune, F-94100 St Maur, France;
6.Univ Michigan, Dept Climate & Space Sci & Engn, 2455 Hayward St, Ann Arbor, MI 48109 USA;
7.Univ Orleans, CNRS, UMR 6115, Lab Phys & Chim Environnement & Espace LPC2E, Orleans, France;
8.Inst Royal Aeron Spatiale Belg BIRA IASB, Koninklijk Belgisch Inst Ruimte Aeron, Ringlaan 3, B-1180 Brussels, Belgium;
9.Tech Univ Carolo Wilhelmina Braunschweig, Inst Comp & Network Engn IDA, Hans Sommer Str 66, D-38106 Braunschweig, Germany;
10.Southwest Res Inst, Dept Space Sci, 6220 Culebra Rd, San Antonio, TX 78228 USA;
11.Max Planck Inst Sonnensystemforsch MPS, Justus von Liebig Weg 3, D-37077 Gottingen, Germany;
12.Aix Marseille Univ, CNRS, Lab Astrophys Marseille, F-13388 Marseille, France;
13.Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA;
14.Univ Paul Sabatier, Observ Midi Pyrenees, CNRS, Inst Rech Astrophys & Planetol, 9 Ave Colonel Roche, F-31028 Toulouse 4, France
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Marty, B.,Altwegg, K.,Balsiger, H.,et al. Xenon isotopes in 67P/Churyumov-Gerasimenko show that comets contributed to Earth's atmosphere[J]. SCIENCE,2017,356(6342):1069-+.
APA Marty, B..,Altwegg, K..,Balsiger, H..,Bar-Nun, A..,Bekaert, D. V..,...&Wurz, P..(2017).Xenon isotopes in 67P/Churyumov-Gerasimenko show that comets contributed to Earth's atmosphere.SCIENCE,356(6342),1069-+.
MLA Marty, B.,et al."Xenon isotopes in 67P/Churyumov-Gerasimenko show that comets contributed to Earth's atmosphere".SCIENCE 356.6342(2017):1069-+.
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