Triple F-a comet nucleus sample return mission

被引：15

作者：

Kueppers, Michael ^{[1
,2
]}

Keller, H. U. ^{[1
]}

Kuehrt, E. ^{[3
]}

A'Hearn, M. F. ^{[4
]}

Altwegg, K. ^{[5
]}

Bertrand, R. ^{[6
]}

Busemann, H. ^{[7
]}

Capria, M. T. ^{[8
]}

Colangeli, L. ^{[9
]}

Davidsson, B. ^{[10
]}

Ehrenfreund, P. ^{[11
]}

Knollenberg, J. ^{[3
]}

Mottola, S. ^{[3
]}

Rathke, A. ^{[12
]}

Weiss, P. ^{[13
]}

Zolensky, M. ^{[14
]}

Akim, E. ^{[15
]}

Basilevsky, A. ^{[16
]}

Galimov, E. ^{[16
]}

Gerasimov, M. ^{[17
]}

Korablev, O. ^{[17
]}

Lomakin, I. ^{[18
]}

Marov, M. ^{[15
]}

Martynov, M. ^{[18
]}

Nazarov, M. ^{[16
]}

Zakharov, A. ^{[17
]}

Zelenyi, L. ^{[17
]}

Aronica, A. ^{[19
]}

Ball, A. J. ^{[7
]}

Barbieri, C. ^{[20
]}

Bar-Nun, A. ^{[21
]}

Benkhoff, J. ^{[3
]}

Biele, J. ^{[3
]}

Biver, N. ^{[55
]}

Blum, J. ^{[22
]}

Bockelee-Morvan, D. ^{[55
]}

Botta, O. ^{[23
]}

Bredehoeft, J. -H. ^{[24
]}

Capaccioni, F. ^{[8
]}

Charnley, S. ^{[54
]}

Cloutis, E. ^{[25
]}

Cottin, H. ^{[26
]}

Cremonese, G. ^{[20
]}

Crovisier, J. ^{[55
]}

Crowther, S. A. ^{[53
]}

Epifani, E. M. ^{[9
]}

Esposito, F. ^{[9
]}

Ferrari, A. C. ^{[52
]}

Ferri, F. ^{[20
]}

Fulle, M. ^{[51
]}

机构：

[1] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany

[2] European Space Astron Ctr, Madrid 28691, Spain

[3] DLR, Berlin, Germany

[4] Univ Maryland, College Pk, MD 20742 USA

[5] Univ Bern, Bern, Switzerland

[6] CNES, Toulouse, France

[7] Open Univ, Milton Keynes MK7 6AA, Bucks, England

[8] IASF INAF, Rome, Italy

[9] Osserv Astron Capodimonte, INAF, I-80131 Naples, Italy

[10] Uppsala Univ, Uppsala, Sweden

[11] Leiden Univ, Leiden, Netherlands

[12] EADS Astrium, Friedrichshafen, Germany

[13] Hong Kong Polytech Univ, Hong Kong, Hong Kong, Peoples R China

[14] NASA, Lyndon B Johnson Space Ctr, Houston, TX 77058 USA

[15] Keldysh Inst, Moscow, Russia

[16] Vernadskij Inst, Moscow, Russia

[17] Space Res Inst, Moscow, Russia

[18] Lavochkin Assoc, Moscow, Russia

[19] Univ Naples Federico II, Naples, Italy

[20] Univ Padua, Padua, Italy

[21] Tel Aviv Univ, IL-69978 Tel Aviv, Israel

[22] Tech Univ Carolo Wilhelmina Braunschweig, Braunschweig, Germany

[23] Int Space Sci Inst, Bern, Switzerland

[24] Univ Bremen, Bremen, Germany

[25] Univ Winnipeg, Winnipeg, MB R3B 2E9, Canada

[26] Univ Paris, F-75252 Paris, France

[27] MPIfK, Heidelberg, Germany

[28] CSIC, IAA, Granada, Spain

[29] ESA, Estec, Noordwijk, Netherlands

[30] Natl Cent Univ, Taipei, Taiwan

[31] Univ Munster, Munster, Germany

[32] IWF, Graz, Austria

[33] Univ Warsaw, Warsaw, Poland

[34] IAC, Tenerife, Spain

[35] Queens Univ Belfast, Belfast, Antrim, North Ireland

[36] Kobe Univ, Kobe, Hyogo 657, Japan

[37] CNRS, F-91405 Orsay, France

[38] Univ Nice, Nice, France

[39] Carnegie Inst Sci, Washington, DC 20005 USA

[40] Univ Cologne, Cologne, Germany

[41] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA

[42] USA, Res Lab, Washington, DC 20310 USA

[43] PAS, Space Res Ctr, Warsaw, Poland

[44] DLR, Cologne, Germany

[45] Cardiff Univ, Cardiff, Wales

[46] Krakow Tech Univ, PL-31155 Krakow, Poland

[47] JPL, Pasadena, CA USA

[48] ETH, Zurich, Switzerland

[49] Univ London Imperial Coll Sci Technol & Med, London, England

[50] LAM, Marseille, France

来源：

EXPERIMENTAL ASTRONOMY | 2009年 / 23卷 / 03期

关键词：

Comets; Cosmogony; Sample return; Space mission; DEEP IMPACT; MECHANICAL-PROPERTIES; ROSETTA MISSION; ORGANIC-MATTER; WATER ICE; ORIGIN; SURFACE; SPECTROMETER; 81P/WILD-2; FAMILY;

D O I：

10.1007/s10686-008-9115-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Triple F (Fresh From the Fridge) mission, a Comet Nucleus Sample Return, has been proposed to ESA's Cosmic Vision program. A sample return from a comet enables us to reach the ultimate goal of cometary research. Since comets are the least processed bodies in the solar system, the proposal goes far beyond cometary science topics (like the explanation of cometary activity) and delivers invaluable information about the formation of the solar system and the interstellar molecular cloud from which it formed. The proposed mission would extract three sample cores of the upper 50 cm from three locations on a cometary nucleus and return them cooled to Earth for analysis in the laboratory. The simple mission concept with a touch-and-go sampling by a single spacecraft was proposed as an M-class mission in collaboration with the Russian space agency ROSCOSMOS.

引用

页码：809 / 847

页数：39

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