New observations of Saturn's coorbital satellites
The strong planetary methane and hydrogen absorption at 2.0-2.4 microns are exploited in the present observations of the Saturnian coorbital satellites Janus and Epimetheus as they passed over the north pole of Saturn at superior conjunction. These observations confirm the orbital model results of Y...
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1992
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ftnasantrs:oai:casi.ntrs.nasa.gov:19930038738 2023-05-15T17:39:45+02:00 New observations of Saturn's coorbital satellites Nicholson, Philip D. Hamilton, Douglas P. Matthews, Keith Yoder, Charles F. Unclassified, Unlimited, Publicly available Dec. 1992 http://ntrs.nasa.gov/search.jsp?R=19930038738 unknown http://ntrs.nasa.gov/search.jsp?R=19930038738 Accession ID: 93A22735 Copyright Other Sources 91 Icarus; 100; 2; p. 464-484. 1992 ftnasantrs 2012-02-15T20:01:33Z The strong planetary methane and hydrogen absorption at 2.0-2.4 microns are exploited in the present observations of the Saturnian coorbital satellites Janus and Epimetheus as they passed over the north pole of Saturn at superior conjunction. These observations confirm the orbital model results of Yoder at al. (1989), especially in the question as to the low density of both satellites; in addition, a much stronger solution is furnished which is essentially independent of 1966 data for Epimethius. The low density results are interpreted as indicative that the objects are composed of relatively pure water ice, but with porosities of the order of 30 percent. Other/Unknown Material North Pole NASA Technical Reports Server (NTRS) North Pole Janus ENVELOPE(163.100,163.100,-71.067,-71.067) |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
language |
unknown |
topic |
91 |
spellingShingle |
91 Nicholson, Philip D. Hamilton, Douglas P. Matthews, Keith Yoder, Charles F. New observations of Saturn's coorbital satellites |
topic_facet |
91 |
description |
The strong planetary methane and hydrogen absorption at 2.0-2.4 microns are exploited in the present observations of the Saturnian coorbital satellites Janus and Epimetheus as they passed over the north pole of Saturn at superior conjunction. These observations confirm the orbital model results of Yoder at al. (1989), especially in the question as to the low density of both satellites; in addition, a much stronger solution is furnished which is essentially independent of 1966 data for Epimethius. The low density results are interpreted as indicative that the objects are composed of relatively pure water ice, but with porosities of the order of 30 percent. |
format |
Other/Unknown Material |
author |
Nicholson, Philip D. Hamilton, Douglas P. Matthews, Keith Yoder, Charles F. |
author_facet |
Nicholson, Philip D. Hamilton, Douglas P. Matthews, Keith Yoder, Charles F. |
author_sort |
Nicholson, Philip D. |
title |
New observations of Saturn's coorbital satellites |
title_short |
New observations of Saturn's coorbital satellites |
title_full |
New observations of Saturn's coorbital satellites |
title_fullStr |
New observations of Saturn's coorbital satellites |
title_full_unstemmed |
New observations of Saturn's coorbital satellites |
title_sort |
new observations of saturn's coorbital satellites |
publishDate |
1992 |
url |
http://ntrs.nasa.gov/search.jsp?R=19930038738 |
op_coverage |
Unclassified, Unlimited, Publicly available |
long_lat |
ENVELOPE(163.100,163.100,-71.067,-71.067) |
geographic |
North Pole Janus |
geographic_facet |
North Pole Janus |
genre |
North Pole |
genre_facet |
North Pole |
op_source |
Other Sources |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19930038738 Accession ID: 93A22735 |
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Copyright |
_version_ |
1766140536533549056 |