Composition and Physical Properties of Enceladus' Surface

Observations of Saturn’s satellite Enceladus using Cassini’s Visual and Infrared Mapping Spectrometer instrument were obtained during three flybys of Enceladus in 2005. Enceladus’ surface is composed mostly of nearly pure water ice except near its south pole, where there are light organics, CO 2 , a...

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Published in:Science
Main Authors: Brown, Robert H., Clark, Roger N., Buratti, Bonnie J., Cruikshank, Dale P., Barnes, Jason W., Mastrapa, Rachel M. E., Bauer, J., Newman, S., Momary, T., Baines, K. H., Bellucci, G., Capaccioni, F., Cerroni, P., Combes, M., Coradini, A., Drossart, P., Formisano, V., Jaumann, R., Langevin, Y., Matson, D. L., McCord, T. B., Nelson, R. M., Nicholson, P. D., Sicardy, B., Sotin, C.
Format: Other Non-Article Part of Journal/Newspaper
Language:unknown
Published: 2006
Subjects:
Online Access:http://elib.dlr.de/45048/
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spelling ftdlr:oai:elib.dlr.de:45048 2023-05-15T18:22:07+02:00 Composition and Physical Properties of Enceladus' Surface Brown, Robert H. Clark, Roger N. Buratti, Bonnie J. Cruikshank, Dale P. Barnes, Jason W. Mastrapa, Rachel M. E. Bauer, J. Newman, S. Momary, T. Baines, K. H. Bellucci, G. Capaccioni, F. Cerroni, P. Combes, M. Coradini, A. Drossart, P. Formisano, V. Jaumann, R. Langevin, Y. Matson, D. L. McCord, T. B. Nelson, R. M. Nicholson, P. D. Sicardy, B. Sotin, C. 2006-03-10 http://elib.dlr.de/45048/ unknown Brown, Robert H. und Clark, Roger N. und Buratti, Bonnie J. und Cruikshank, Dale P. und Barnes, Jason W. und Mastrapa, Rachel M. E. und Bauer, J. und Newman, S. und Momary, T. und Baines, K. H. und Bellucci, G. und Capaccioni, F. und Cerroni, P. und Combes, M. und Coradini, A. und Drossart, P. und Formisano, V. und Jaumann, R. und Langevin, Y. und Matson, D. L. und McCord, T. B. und Nelson, R. M. und Nicholson, P. D. und Sicardy, B. und Sotin, C. (2006) Composition and Physical Properties of Enceladus' Surface. Science, 311 (5766), Seiten 1425-1428. DOI:10.1126/science.1121031. Planetengeologie Zeitschriftenbeitrag PeerReviewed 2006 ftdlr https://doi.org/10.1126/science.1121031 2016-03-28T20:37:14Z Observations of Saturn’s satellite Enceladus using Cassini’s Visual and Infrared Mapping Spectrometer instrument were obtained during three flybys of Enceladus in 2005. Enceladus’ surface is composed mostly of nearly pure water ice except near its south pole, where there are light organics, CO 2 , and amorphous and crystalline water ice, particularly in the region dubbed the ‘‘tiger stripes.’’ An upper limit of 5 precipitable nanometers is derived for CO in the atmospheric column above Enceladus, and 2% for NH3 in global surface deposits. Upper limits of 140 kelvin (for a filled pixel) are derived for the temperatures in the tiger stripes. Other Non-Article Part of Journal/Newspaper South pole German Aerospace Center: elib - DLR electronic library South Pole Science 311 5766 1425 1428
institution Open Polar
collection German Aerospace Center: elib - DLR electronic library
op_collection_id ftdlr
language unknown
topic Planetengeologie
spellingShingle Planetengeologie
Brown, Robert H.
Clark, Roger N.
Buratti, Bonnie J.
Cruikshank, Dale P.
Barnes, Jason W.
Mastrapa, Rachel M. E.
Bauer, J.
Newman, S.
Momary, T.
Baines, K. H.
Bellucci, G.
Capaccioni, F.
Cerroni, P.
Combes, M.
Coradini, A.
Drossart, P.
Formisano, V.
Jaumann, R.
Langevin, Y.
Matson, D. L.
McCord, T. B.
Nelson, R. M.
Nicholson, P. D.
Sicardy, B.
Sotin, C.
Composition and Physical Properties of Enceladus' Surface
topic_facet Planetengeologie
description Observations of Saturn’s satellite Enceladus using Cassini’s Visual and Infrared Mapping Spectrometer instrument were obtained during three flybys of Enceladus in 2005. Enceladus’ surface is composed mostly of nearly pure water ice except near its south pole, where there are light organics, CO 2 , and amorphous and crystalline water ice, particularly in the region dubbed the ‘‘tiger stripes.’’ An upper limit of 5 precipitable nanometers is derived for CO in the atmospheric column above Enceladus, and 2% for NH3 in global surface deposits. Upper limits of 140 kelvin (for a filled pixel) are derived for the temperatures in the tiger stripes.
format Other Non-Article Part of Journal/Newspaper
author Brown, Robert H.
Clark, Roger N.
Buratti, Bonnie J.
Cruikshank, Dale P.
Barnes, Jason W.
Mastrapa, Rachel M. E.
Bauer, J.
Newman, S.
Momary, T.
Baines, K. H.
Bellucci, G.
Capaccioni, F.
Cerroni, P.
Combes, M.
Coradini, A.
Drossart, P.
Formisano, V.
Jaumann, R.
Langevin, Y.
Matson, D. L.
McCord, T. B.
Nelson, R. M.
Nicholson, P. D.
Sicardy, B.
Sotin, C.
author_facet Brown, Robert H.
Clark, Roger N.
Buratti, Bonnie J.
Cruikshank, Dale P.
Barnes, Jason W.
Mastrapa, Rachel M. E.
Bauer, J.
Newman, S.
Momary, T.
Baines, K. H.
Bellucci, G.
Capaccioni, F.
Cerroni, P.
Combes, M.
Coradini, A.
Drossart, P.
Formisano, V.
Jaumann, R.
Langevin, Y.
Matson, D. L.
McCord, T. B.
Nelson, R. M.
Nicholson, P. D.
Sicardy, B.
Sotin, C.
author_sort Brown, Robert H.
title Composition and Physical Properties of Enceladus' Surface
title_short Composition and Physical Properties of Enceladus' Surface
title_full Composition and Physical Properties of Enceladus' Surface
title_fullStr Composition and Physical Properties of Enceladus' Surface
title_full_unstemmed Composition and Physical Properties of Enceladus' Surface
title_sort composition and physical properties of enceladus' surface
publishDate 2006
url http://elib.dlr.de/45048/
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation Brown, Robert H. und Clark, Roger N. und Buratti, Bonnie J. und Cruikshank, Dale P. und Barnes, Jason W. und Mastrapa, Rachel M. E. und Bauer, J. und Newman, S. und Momary, T. und Baines, K. H. und Bellucci, G. und Capaccioni, F. und Cerroni, P. und Combes, M. und Coradini, A. und Drossart, P. und Formisano, V. und Jaumann, R. und Langevin, Y. und Matson, D. L. und McCord, T. B. und Nelson, R. M. und Nicholson, P. D. und Sicardy, B. und Sotin, C. (2006) Composition and Physical Properties of Enceladus' Surface. Science, 311 (5766), Seiten 1425-1428. DOI:10.1126/science.1121031.
op_doi https://doi.org/10.1126/science.1121031
container_title Science
container_volume 311
container_issue 5766
container_start_page 1425
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