Morse, A. D.; Altwegg, K.; Andrews, D. J.; Auster, H. U.; Carr, C. M.; Galand, M.; Goesmann, F.; Gulkis, S.; Lee, S.; Richter, I.; Sheridan, S.; Stern, S. A.; A'Hearn, M. F.; Feldman, P.; Parker, J.; Retherford, K. D.; Weaver, H. A. and Wright, I. P.
|DOI (Digital Object Identifier) Link:||https://doi.org/10.1016/j.pss.2012.01.003|
|Google Scholar:||Look up in Google Scholar|
On 10th July 2010 the Rosetta spacecraft passed within 3160 km of asteroid 21 Lutetia during which seven instruments attempted to detect an exosphere. A comparison of the sensitivity is made between the different instruments based on a simple spherical out-gassing point source model, which was used to infer that the Lutetia exosphere production rate was determined by MIRO to be <4.3×1023 molecules s-1 for water and by ROSINA RTOF to be <1.7×1025 molecules s-1 for carbon monoxide. Consideration of the flyby geometry and combined instrument operations places further constraints on the exosphere structure and gas production rate. Experience gained during the flyby will prove invaluable for operations planning during Rosetta's approach and orbit of comet 67P/Churyumov–Gerasimenko in 2014.
|Item Type:||Journal Article|
|Copyright Holders:||2012 Elsevier Ltd.|
|Keywords:||Rosetta; Lutetia; exosphere; asteroid; comet|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Andrew Morse|
|Date Deposited:||17 Feb 2012 14:14|
|Last Modified:||17 Nov 2016 11:08|
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