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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 05973naa a2201705 4500 | |
| 001 | oai:DiVA.org:uu-130791 | |
| 003 | SwePub | |
| 008 | 100913s2009 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-1307912 URI |
| 024 | 7 | a https://doi.org/10.1007/s10686-008-9115-82 DOI |
| 040 | a (SwePub)uu | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Kueppers, Michael4 aut |
| 245 | 1 0 | a Triple F-a comet nucleus sample return mission |
| 264 | c 2008-08-07 | |
| 264 | 1 | b Springer Science and Business Media LLC,c 2009 |
| 338 | a print2 rdacarrier | |
| 520 | a 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. | |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a Comets | |
| 653 | a Cosmogony | |
| 653 | a Sample return | |
| 653 | a Space mission | |
| 653 | a Physics | |
| 653 | a Fysik | |
| 700 | 1 | a Keller, H. U.4 aut |
| 700 | 1 | a Kuehrt, E4 aut |
| 700 | 1 | a A'Hearn, M. F.4 aut |
| 700 | 1 | a Altwegg, K4 aut |
| 700 | 1 | a Bertrand, R4 aut |
| 700 | 1 | a Busemann, H4 aut |
| 700 | 1 | a Capria, T4 aut |
| 700 | 1 | a Colangeli, L4 aut |
| 700 | 1 | a Davidsson, Björnu Uppsala universitet,Institutionen för fysik och astronomi4 aut |
| 700 | 1 | a Ehrenfreund, P4 aut |
| 700 | 1 | a Knollenberg, J4 aut |
| 700 | 1 | a Mottola, S4 aut |
| 700 | 1 | a Rathke, A4 aut |
| 700 | 1 | a Weiss, P4 aut |
| 700 | 1 | a Zolensky, M4 aut |
| 700 | 1 | a Akim, E4 aut |
| 700 | 1 | a Basilevsky, A4 aut |
| 700 | 1 | a Galimov, E4 aut |
| 700 | 1 | a Gerasimov, M4 aut |
| 700 | 1 | a Korablev, O4 aut |
| 700 | 1 | a Lomakin, I4 aut |
| 700 | 1 | a Marov, M4 aut |
| 700 | 1 | a Martynov, M4 aut |
| 700 | 1 | a Nazarov, M4 aut |
| 700 | 1 | a Zakharov, A4 aut |
| 700 | 1 | a Zelenyi, L4 aut |
| 700 | 1 | a Aronica, A4 aut |
| 700 | 1 | a Ball, J4 aut |
| 700 | 1 | a Barbieri, C4 aut |
| 700 | 1 | a Bar-Nun, A4 aut |
| 700 | 1 | a Benkhoff, J4 aut |
| 700 | 1 | a Biele, J4 aut |
| 700 | 1 | a Biver, N4 aut |
| 700 | 1 | a Blum, J4 aut |
| 700 | 1 | a Bockelee-Morvan, D4 aut |
| 700 | 1 | a Botta, O4 aut |
| 700 | 1 | a Bredehoeft, J.-H.4 aut |
| 700 | 1 | a Capaccioni, F4 aut |
| 700 | 1 | a Charnley, S4 aut |
| 700 | 1 | a Cloutis, E4 aut |
| 700 | 1 | a Cottin, H4 aut |
| 700 | 1 | a Cremonese, G4 aut |
| 700 | 1 | a Crovisier, J4 aut |
| 700 | 1 | a Crowther, S. A.4 aut |
| 700 | 1 | a Epifani, M4 aut |
| 700 | 1 | a Esposito, F4 aut |
| 700 | 1 | a Ferrari, C4 aut |
| 700 | 1 | a Ferri, F4 aut |
| 700 | 1 | a Fulle, M4 aut |
| 700 | 1 | a Gilmour, J4 aut |
| 700 | 1 | a Goesmann, F4 aut |
| 700 | 1 | a Gortsas, N4 aut |
| 700 | 1 | a Green, F4 aut |
| 700 | 1 | a Groussin, O4 aut |
| 700 | 1 | a Gruen, E4 aut |
| 700 | 1 | a Gutierrez, P. J.4 aut |
| 700 | 1 | a Hartogh, P4 aut |
| 700 | 1 | a Henkel, T4 aut |
| 700 | 1 | a Hilchenbach, M4 aut |
| 700 | 1 | a Ho, T.-M.4 aut |
| 700 | 1 | a Horneck, G4 aut |
| 700 | 1 | a Hviid, F4 aut |
| 700 | 1 | a Ip, W.-H.4 aut |
| 700 | 1 | a Jaeckel, A4 aut |
| 700 | 1 | a Jessberger, E4 aut |
| 700 | 1 | a Kallenbach, R4 aut |
| 700 | 1 | a Kargl, G4 aut |
| 700 | 1 | a Koemle, I4 aut |
| 700 | 1 | a Korth, A4 aut |
| 700 | 1 | a Kossacki, K4 aut |
| 700 | 1 | a Krause, C4 aut |
| 700 | 1 | a Krueger, H4 aut |
| 700 | 1 | a Li, Z.-Y.4 aut |
| 700 | 1 | a Licandro, J4 aut |
| 700 | 1 | a Lopez-Moreno, J4 aut |
| 700 | 1 | a Lowry, C4 aut |
| 700 | 1 | a Lyon, I4 aut |
| 700 | 1 | a Magni, G4 aut |
| 700 | 1 | a Mall, U4 aut |
| 700 | 1 | a Mann, I4 aut |
| 700 | 1 | a Markiewicz, W4 aut |
| 700 | 1 | a Martins, Z4 aut |
| 700 | 1 | a Maurette, M4 aut |
| 700 | 1 | a Meierhenrich, U4 aut |
| 700 | 1 | a Mennella, V4 aut |
| 700 | 1 | a Ng, C4 aut |
| 700 | 1 | a Nittler, R4 aut |
| 700 | 1 | a Palumbo, P4 aut |
| 700 | 1 | a Paetzold, M4 aut |
| 700 | 1 | a Prialnik, D4 aut |
| 700 | 1 | a Rengel, M4 aut |
| 700 | 1 | a Rickman, Hansu Uppsala universitet,Institutionen för fysik och astronomi4 aut |
| 700 | 1 | a Rodriguez, J4 aut |
| 700 | 1 | a Roll, R4 aut |
| 700 | 1 | a Rost, D4 aut |
| 700 | 1 | a Rotundi, A4 aut |
| 700 | 1 | a Sandford, S4 aut |
| 700 | 1 | a Schoenbaechler, M4 aut |
| 700 | 1 | a Sierks, H4 aut |
| 700 | 1 | a Srama, R4 aut |
| 700 | 1 | a Stroud, M4 aut |
| 700 | 1 | a Szutowicz, S4 aut |
| 700 | 1 | a Tornow, C4 aut |
| 700 | 1 | a Ulamec, S4 aut |
| 700 | 1 | a Wallis, M4 aut |
| 700 | 1 | a Waniak, W4 aut |
| 700 | 1 | a Weissman, P4 aut |
| 700 | 1 | a Wieler, R4 aut |
| 700 | 1 | a Wurz, P4 aut |
| 700 | 1 | a Yung, L4 aut |
| 700 | 1 | a Zarnecki, C4 aut |
| 710 | 2 | a Uppsala universitetb Institutionen för fysik och astronomi4 org |
| 773 | 0 | t Experimental astronomyd : Springer Science and Business Media LLCg 23:3, s. 809-847q 23:3<809-847x 0922-6435x 1572-9508 |
| 856 | 4 | u https://link.springer.com/content/pdf/10.1007%2Fs10686-008-9115-8.pdf |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-130791 |
| 856 | 4 8 | u https://doi.org/10.1007/s10686-008-9115-8 |
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