AMBITION – comet nucleus cryogenic sample return
Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprint...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bockelée-Morvan, D. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s) 2021 |
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| Übergeordnetes Werk: |
Enthalten in: Experimental astronomy - Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989, 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 |
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| Übergeordnetes Werk: |
volume:54 ; year:2021 ; number:2-3 ; day:21 ; month:07 ; pages:1077-1128 |
| Links: |
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| DOI / URN: |
10.1007/s10686-021-09770-4 |
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| Katalog-ID: |
SPR049616757 |
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| 520 | |a Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. | ||
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| 700 | 1 | |a Filacchione, Gianrico |0 (orcid)0000-0001-9567-0055 |4 aut | |
| 700 | 1 | |a Altwegg, Kathrin |4 aut | |
| 700 | 1 | |a Bianchi, Eleonora |4 aut | |
| 700 | 1 | |a Bizzarro, Martin |4 aut | |
| 700 | 1 | |a Blum, Jürgen |4 aut | |
| 700 | 1 | |a Bonal, Lydie |4 aut | |
| 700 | 1 | |a Capaccioni, Fabrizio |4 aut | |
| 700 | 1 | |a Choukroun, Mathieu |4 aut | |
| 700 | 1 | |a Codella, Claudio |4 aut | |
| 700 | 1 | |a Cottin, Hervé |4 aut | |
| 700 | 1 | |a Davidsson, Björn |4 aut | |
| 700 | 1 | |a De Sanctis, Maria Cristina |4 aut | |
| 700 | 1 | |a Drozdovskaya, Maria N. |4 aut | |
| 700 | 1 | |a Engrand, Cécile |4 aut | |
| 700 | 1 | |a Galand, Marina |4 aut | |
| 700 | 1 | |a Güttler, Carsten |4 aut | |
| 700 | 1 | |a Henri, Pierre |4 aut | |
| 700 | 1 | |a Herique, Alain |4 aut | |
| 700 | 1 | |a Ivanovski, Stavro |4 aut | |
| 700 | 1 | |a Kokotanekova, Rosita |4 aut | |
| 700 | 1 | |a Levasseur-Regourd, Anny-Chantal |4 aut | |
| 700 | 1 | |a Miller, Kelly E. |4 aut | |
| 700 | 1 | |a Rotundi, Alessandra |4 aut | |
| 700 | 1 | |a Schönbächler, Maria |4 aut | |
| 700 | 1 | |a Snodgrass, Colin |4 aut | |
| 700 | 1 | |a Thomas, Nicolas |4 aut | |
| 700 | 1 | |a Tubiana, Cecilia |4 aut | |
| 700 | 1 | |a Ulamec, Stephan |4 aut | |
| 700 | 1 | |a Vincent, Jean-Baptiste |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Experimental astronomy |d Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 |g 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 |w (DE-627)312841116 |w (DE-600)2012330-9 |x 1572-9508 |7 nnns |
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10.1007/s10686-021-09770-4 doi (DE-627)SPR049616757 (SPR)s10686-021-09770-4-e DE-627 ger DE-627 rakwb eng Bockelée-Morvan, D. verfasserin aut AMBITION – comet nucleus cryogenic sample return 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 Filacchione, Gianrico (orcid)0000-0001-9567-0055 aut Altwegg, Kathrin aut Bianchi, Eleonora aut Bizzarro, Martin aut Blum, Jürgen aut Bonal, Lydie aut Capaccioni, Fabrizio aut Choukroun, Mathieu aut Codella, Claudio aut Cottin, Hervé aut Davidsson, Björn aut De Sanctis, Maria Cristina aut Drozdovskaya, Maria N. aut Engrand, Cécile aut Galand, Marina aut Güttler, Carsten aut Henri, Pierre aut Herique, Alain aut Ivanovski, Stavro aut Kokotanekova, Rosita aut Levasseur-Regourd, Anny-Chantal aut Miller, Kelly E. aut Rotundi, Alessandra aut Schönbächler, Maria aut Snodgrass, Colin aut Thomas, Nicolas aut Tubiana, Cecilia aut Ulamec, Stephan aut Vincent, Jean-Baptiste aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:54 year:2021 number:2-3 day:21 month:07 pages:1077-1128 https://dx.doi.org/10.1007/s10686-021-09770-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 54 2021 2-3 21 07 1077-1128 |
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10.1007/s10686-021-09770-4 doi (DE-627)SPR049616757 (SPR)s10686-021-09770-4-e DE-627 ger DE-627 rakwb eng Bockelée-Morvan, D. verfasserin aut AMBITION – comet nucleus cryogenic sample return 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 Filacchione, Gianrico (orcid)0000-0001-9567-0055 aut Altwegg, Kathrin aut Bianchi, Eleonora aut Bizzarro, Martin aut Blum, Jürgen aut Bonal, Lydie aut Capaccioni, Fabrizio aut Choukroun, Mathieu aut Codella, Claudio aut Cottin, Hervé aut Davidsson, Björn aut De Sanctis, Maria Cristina aut Drozdovskaya, Maria N. aut Engrand, Cécile aut Galand, Marina aut Güttler, Carsten aut Henri, Pierre aut Herique, Alain aut Ivanovski, Stavro aut Kokotanekova, Rosita aut Levasseur-Regourd, Anny-Chantal aut Miller, Kelly E. aut Rotundi, Alessandra aut Schönbächler, Maria aut Snodgrass, Colin aut Thomas, Nicolas aut Tubiana, Cecilia aut Ulamec, Stephan aut Vincent, Jean-Baptiste aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:54 year:2021 number:2-3 day:21 month:07 pages:1077-1128 https://dx.doi.org/10.1007/s10686-021-09770-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 54 2021 2-3 21 07 1077-1128 |
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10.1007/s10686-021-09770-4 doi (DE-627)SPR049616757 (SPR)s10686-021-09770-4-e DE-627 ger DE-627 rakwb eng Bockelée-Morvan, D. verfasserin aut AMBITION – comet nucleus cryogenic sample return 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 Filacchione, Gianrico (orcid)0000-0001-9567-0055 aut Altwegg, Kathrin aut Bianchi, Eleonora aut Bizzarro, Martin aut Blum, Jürgen aut Bonal, Lydie aut Capaccioni, Fabrizio aut Choukroun, Mathieu aut Codella, Claudio aut Cottin, Hervé aut Davidsson, Björn aut De Sanctis, Maria Cristina aut Drozdovskaya, Maria N. aut Engrand, Cécile aut Galand, Marina aut Güttler, Carsten aut Henri, Pierre aut Herique, Alain aut Ivanovski, Stavro aut Kokotanekova, Rosita aut Levasseur-Regourd, Anny-Chantal aut Miller, Kelly E. aut Rotundi, Alessandra aut Schönbächler, Maria aut Snodgrass, Colin aut Thomas, Nicolas aut Tubiana, Cecilia aut Ulamec, Stephan aut Vincent, Jean-Baptiste aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:54 year:2021 number:2-3 day:21 month:07 pages:1077-1128 https://dx.doi.org/10.1007/s10686-021-09770-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 54 2021 2-3 21 07 1077-1128 |
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10.1007/s10686-021-09770-4 doi (DE-627)SPR049616757 (SPR)s10686-021-09770-4-e DE-627 ger DE-627 rakwb eng Bockelée-Morvan, D. verfasserin aut AMBITION – comet nucleus cryogenic sample return 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 Filacchione, Gianrico (orcid)0000-0001-9567-0055 aut Altwegg, Kathrin aut Bianchi, Eleonora aut Bizzarro, Martin aut Blum, Jürgen aut Bonal, Lydie aut Capaccioni, Fabrizio aut Choukroun, Mathieu aut Codella, Claudio aut Cottin, Hervé aut Davidsson, Björn aut De Sanctis, Maria Cristina aut Drozdovskaya, Maria N. aut Engrand, Cécile aut Galand, Marina aut Güttler, Carsten aut Henri, Pierre aut Herique, Alain aut Ivanovski, Stavro aut Kokotanekova, Rosita aut Levasseur-Regourd, Anny-Chantal aut Miller, Kelly E. aut Rotundi, Alessandra aut Schönbächler, Maria aut Snodgrass, Colin aut Thomas, Nicolas aut Tubiana, Cecilia aut Ulamec, Stephan aut Vincent, Jean-Baptiste aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:54 year:2021 number:2-3 day:21 month:07 pages:1077-1128 https://dx.doi.org/10.1007/s10686-021-09770-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 54 2021 2-3 21 07 1077-1128 |
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10.1007/s10686-021-09770-4 doi (DE-627)SPR049616757 (SPR)s10686-021-09770-4-e DE-627 ger DE-627 rakwb eng Bockelée-Morvan, D. verfasserin aut AMBITION – comet nucleus cryogenic sample return 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2021 Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 Filacchione, Gianrico (orcid)0000-0001-9567-0055 aut Altwegg, Kathrin aut Bianchi, Eleonora aut Bizzarro, Martin aut Blum, Jürgen aut Bonal, Lydie aut Capaccioni, Fabrizio aut Choukroun, Mathieu aut Codella, Claudio aut Cottin, Hervé aut Davidsson, Björn aut De Sanctis, Maria Cristina aut Drozdovskaya, Maria N. aut Engrand, Cécile aut Galand, Marina aut Güttler, Carsten aut Henri, Pierre aut Herique, Alain aut Ivanovski, Stavro aut Kokotanekova, Rosita aut Levasseur-Regourd, Anny-Chantal aut Miller, Kelly E. aut Rotundi, Alessandra aut Schönbächler, Maria aut Snodgrass, Colin aut Thomas, Nicolas aut Tubiana, Cecilia aut Ulamec, Stephan aut Vincent, Jean-Baptiste aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 54(2021), 2-3 vom: 21. Juli, Seite 1077-1128 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:54 year:2021 number:2-3 day:21 month:07 pages:1077-1128 https://dx.doi.org/10.1007/s10686-021-09770-4 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 54 2021 2-3 21 07 1077-1128 |
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Bockelée-Morvan, D. @@aut@@ Filacchione, Gianrico @@aut@@ Altwegg, Kathrin @@aut@@ Bianchi, Eleonora @@aut@@ Bizzarro, Martin @@aut@@ Blum, Jürgen @@aut@@ Bonal, Lydie @@aut@@ Capaccioni, Fabrizio @@aut@@ Choukroun, Mathieu @@aut@@ Codella, Claudio @@aut@@ Cottin, Hervé @@aut@@ Davidsson, Björn @@aut@@ De Sanctis, Maria Cristina @@aut@@ Drozdovskaya, Maria N. @@aut@@ Engrand, Cécile @@aut@@ Galand, Marina @@aut@@ Güttler, Carsten @@aut@@ Henri, Pierre @@aut@@ Herique, Alain @@aut@@ Ivanovski, Stavro @@aut@@ Kokotanekova, Rosita @@aut@@ Levasseur-Regourd, Anny-Chantal @@aut@@ Miller, Kelly E. @@aut@@ Rotundi, Alessandra @@aut@@ Schönbächler, Maria @@aut@@ Snodgrass, Colin @@aut@@ Thomas, Nicolas @@aut@@ Tubiana, Cecilia @@aut@@ Ulamec, Stephan @@aut@@ Vincent, Jean-Baptiste @@aut@@ |
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Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. 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Bockelée-Morvan, D. |
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AMBITION – comet nucleus cryogenic sample return Space missions (dpeaa)DE-He213 Solar system (dpeaa)DE-He213 Comets (dpeaa)DE-He213 |
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AMBITION – comet nucleus cryogenic sample return |
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Bockelée-Morvan, D. Filacchione, Gianrico Altwegg, Kathrin Bianchi, Eleonora Bizzarro, Martin Blum, Jürgen Bonal, Lydie Capaccioni, Fabrizio Choukroun, Mathieu Codella, Claudio Cottin, Hervé Davidsson, Björn De Sanctis, Maria Cristina Drozdovskaya, Maria N. Engrand, Cécile Galand, Marina Güttler, Carsten Henri, Pierre Herique, Alain Ivanovski, Stavro Kokotanekova, Rosita Levasseur-Regourd, Anny-Chantal Miller, Kelly E. Rotundi, Alessandra Schönbächler, Maria Snodgrass, Colin Thomas, Nicolas Tubiana, Cecilia Ulamec, Stephan Vincent, Jean-Baptiste |
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Elektronische Aufsätze |
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ambition – comet nucleus cryogenic sample return |
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AMBITION – comet nucleus cryogenic sample return |
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Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. © The Author(s) 2021 |
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Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. © The Author(s) 2021 |
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Abstract We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration. © The Author(s) 2021 |
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Filacchione, Gianrico Altwegg, Kathrin Bianchi, Eleonora Bizzarro, Martin Blum, Jürgen Bonal, Lydie Capaccioni, Fabrizio Choukroun, Mathieu Codella, Claudio Cottin, Hervé Davidsson, Björn De Sanctis, Maria Cristina Drozdovskaya, Maria N. Engrand, Cécile Galand, Marina Güttler, Carsten Henri, Pierre Herique, Alain Ivanovski, Stavro Kokotanekova, Rosita Levasseur-Regourd, Anny-Chantal Miller, Kelly E. Rotundi, Alessandra Schönbächler, Maria Snodgrass, Colin Thomas, Nicolas Tubiana, Cecilia Ulamec, Stephan Vincent, Jean-Baptiste |
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| score |
7.3994865 |