Dust Measurements in the Coma of Comet 67P/Churyumov-Gerasimenko Inbound to the Sun Between 3.7 and 3.4 AU
Date Issued
2015
Author(s)
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Lopez-Moreno, J. J.
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Rodriguez, J.
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Bussoletti, E.
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Crifo, J.
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Green, S. F.
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Gruen, E.
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Lamy, P. L.
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McDonnell, J. A. M.
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Molina, A.
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Morales, R.
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Moreno, F.
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Ortiz, J. L.
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Perrin, J.
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Rodrigo, R.
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Weissman, P.
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Zarnecki, J. C.
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Cosi, M.
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Giovane, F.
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Gustafson, B.
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Herranz, M. L.
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Jeronimo, J. M.
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Leese, M. R.
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Lopez-Jimenez, A. C.
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Altobelli, N.
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Sierks, H.
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Agarwal, J.
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Bertini, I.
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Fornasier, S.
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Gutierrez, P. J.
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Lara, L.
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Guettler, C.
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Marzari, F.
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Oaklay, N.
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Snodgrass, C.
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Vincenzo, J. B.
Abstract
GIADA and OSIRIS dust data, combined with data from MIRO and ROSINA instruments onboard Rosetta, from 3.7 to 3.4 AU inbound provide a dust/gas ratio of 4 ± 2.
Coverage
46th Lunar and Planetary Science Conference
Issue
1832
Start page
2420
Conferenece
46th Lunar and Planetary Science Conference
Conferenece place
The Woodlands, Houston, USA
Conferenece date
16-20 March, 2015
Ads BibCode
2015LPI....46.2420F
Rights
open.access
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