Accretional heating of the satellites of Saturn and Uranus
Voyager images of the satellites of Saturn and Uranus have shown that these bodies are characterized by remarkable diversity and surprisingly complex geologic histories. Despite their small sizes, a number of the satellites show unambiguous evidence for resurfacing. The goal was to develop a detaile...
Gespeichert in:
Hauptverfasser: | , , , |
---|---|
Format: | Report |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | |
container_volume | |
creator | Squyres, Steven W. Reynolds, Ray T. Summers, Audrey L. Shung, Felix |
description | Voyager images of the satellites of Saturn and Uranus have shown that these bodies are characterized by remarkable diversity and surprisingly complex geologic histories. Despite their small sizes, a number of the satellites show unambiguous evidence for resurfacing. The goal was to develop a detailed model for heating of these small satellites, and then to explore the consequences of variations in the free parameters in the model. Specifically an attempt was made to determine for what range of conditions melting will occur in these satellites. Along with varying a number of model parameters, the important effects of inclusion of small amounts of ammonia and methane in the system were considered. |
format | Report |
fullrecord | <record><control><sourceid>nasa_CYI</sourceid><recordid>TN_cdi_nasa_ntrs_19870013922</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>19870013922</sourcerecordid><originalsourceid>FETCH-nasa_ntrs_198700139223</originalsourceid><addsrcrecordid>eNrjZLByTE4uSi3JzM9LzFHISE0sycxLV8hPUyjJSFUoTixJzcnJLEktBokEJ5aUFuUpJOalKIQWJeaVFvMwsKYl5hSn8kJpbgYZN9cQZw_dvMTixPi8kqLieENLC3MDA0NjSyMjYwLSAGnZKrs</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>report</recordtype></control><display><type>report</type><title>Accretional heating of the satellites of Saturn and Uranus</title><source>NASA Technical Reports Server</source><creator>Squyres, Steven W. ; Reynolds, Ray T. ; Summers, Audrey L. ; Shung, Felix</creator><creatorcontrib>Squyres, Steven W. ; Reynolds, Ray T. ; Summers, Audrey L. ; Shung, Felix</creatorcontrib><description>Voyager images of the satellites of Saturn and Uranus have shown that these bodies are characterized by remarkable diversity and surprisingly complex geologic histories. Despite their small sizes, a number of the satellites show unambiguous evidence for resurfacing. The goal was to develop a detailed model for heating of these small satellites, and then to explore the consequences of variations in the free parameters in the model. Specifically an attempt was made to determine for what range of conditions melting will occur in these satellites. Along with varying a number of model parameters, the important effects of inclusion of small amounts of ammonia and methane in the system were considered.</description><language>eng</language><publisher>Legacy CDMS</publisher><subject>Lunar And Planetary Exploration</subject><creationdate>1987</creationdate><rights>Copyright Determination: GOV_PUBLIC_USE_PERMITTED</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,796,4475</link.rule.ids><linktorsrc>$$Uhttps://ntrs.nasa.gov/citations/19870013922$$EView_record_in_NASA$$FView_record_in_$$GNASA$$Hfree_for_read</linktorsrc></links><search><creatorcontrib>Squyres, Steven W.</creatorcontrib><creatorcontrib>Reynolds, Ray T.</creatorcontrib><creatorcontrib>Summers, Audrey L.</creatorcontrib><creatorcontrib>Shung, Felix</creatorcontrib><title>Accretional heating of the satellites of Saturn and Uranus</title><description>Voyager images of the satellites of Saturn and Uranus have shown that these bodies are characterized by remarkable diversity and surprisingly complex geologic histories. Despite their small sizes, a number of the satellites show unambiguous evidence for resurfacing. The goal was to develop a detailed model for heating of these small satellites, and then to explore the consequences of variations in the free parameters in the model. Specifically an attempt was made to determine for what range of conditions melting will occur in these satellites. Along with varying a number of model parameters, the important effects of inclusion of small amounts of ammonia and methane in the system were considered.</description><subject>Lunar And Planetary Exploration</subject><fulltext>true</fulltext><rsrctype>report</rsrctype><creationdate>1987</creationdate><recordtype>report</recordtype><sourceid>CYI</sourceid><recordid>eNrjZLByTE4uSi3JzM9LzFHISE0sycxLV8hPUyjJSFUoTixJzcnJLEktBokEJ5aUFuUpJOalKIQWJeaVFvMwsKYl5hSn8kJpbgYZN9cQZw_dvMTixPi8kqLieENLC3MDA0NjSyMjYwLSAGnZKrs</recordid><startdate>19870501</startdate><enddate>19870501</enddate><creator>Squyres, Steven W.</creator><creator>Reynolds, Ray T.</creator><creator>Summers, Audrey L.</creator><creator>Shung, Felix</creator><scope>CYE</scope><scope>CYI</scope></search><sort><creationdate>19870501</creationdate><title>Accretional heating of the satellites of Saturn and Uranus</title><author>Squyres, Steven W. ; Reynolds, Ray T. ; Summers, Audrey L. ; Shung, Felix</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-nasa_ntrs_198700139223</frbrgroupid><rsrctype>reports</rsrctype><prefilter>reports</prefilter><language>eng</language><creationdate>1987</creationdate><topic>Lunar And Planetary Exploration</topic><toplevel>online_resources</toplevel><creatorcontrib>Squyres, Steven W.</creatorcontrib><creatorcontrib>Reynolds, Ray T.</creatorcontrib><creatorcontrib>Summers, Audrey L.</creatorcontrib><creatorcontrib>Shung, Felix</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Squyres, Steven W.</au><au>Reynolds, Ray T.</au><au>Summers, Audrey L.</au><au>Shung, Felix</au><format>book</format><genre>unknown</genre><ristype>RPRT</ristype><btitle>Accretional heating of the satellites of Saturn and Uranus</btitle><date>1987-05-01</date><risdate>1987</risdate><abstract>Voyager images of the satellites of Saturn and Uranus have shown that these bodies are characterized by remarkable diversity and surprisingly complex geologic histories. Despite their small sizes, a number of the satellites show unambiguous evidence for resurfacing. The goal was to develop a detailed model for heating of these small satellites, and then to explore the consequences of variations in the free parameters in the model. Specifically an attempt was made to determine for what range of conditions melting will occur in these satellites. Along with varying a number of model parameters, the important effects of inclusion of small amounts of ammonia and methane in the system were considered.</abstract><cop>Legacy CDMS</cop><oa>free_for_read</oa></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | |
ispartof | |
issn | |
language | eng |
recordid | cdi_nasa_ntrs_19870013922 |
source | NASA Technical Reports Server |
subjects | Lunar And Planetary Exploration |
title | Accretional heating of the satellites of Saturn and Uranus |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-22T13%3A46%3A58IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-nasa_CYI&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=unknown&rft.btitle=Accretional%20heating%20of%20the%20satellites%20of%20Saturn%20and%20Uranus&rft.au=Squyres,%20Steven%20W.&rft.date=1987-05-01&rft_id=info:doi/&rft_dat=%3Cnasa_CYI%3E19870013922%3C/nasa_CYI%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |