The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems

We consider the possible existence of habitable Earth-like planets in four recently discovered extrasolar planetary systems. Such prospective planets must have orbits that are (1) dynamically stable, and (2) allow for surface temperatures compatible with liquid water. We find that three of the four...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Publications of the Astronomical Society of the Pacific 1996-11, Vol.108 (729), p.1018-1023
Hauptverfasser: Gehman, Curtis S., Adams, Fred C., Laughlin, Gregory
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 1023
container_issue 729
container_start_page 1018
container_title Publications of the Astronomical Society of the Pacific
container_volume 108
creator Gehman, Curtis S.
Adams, Fred C.
Laughlin, Gregory
description We consider the possible existence of habitable Earth-like planets in four recently discovered extrasolar planetary systems. Such prospective planets must have orbits that are (1) dynamically stable, and (2) allow for surface temperatures compatible with liquid water. We find that three of the four new systems (51 Peg, p¹ Cnc, and 47 UMa) are easily capable of supporting habitable planets. The fourth (70 Vir) is capable of having a habitable planet only under rather extreme circumstances. To obtain these results, we develop a probabilistic formulation for the coupled problem of orbital stability and planetary habitability.
doi_str_mv 10.1086/133826
format Article
fullrecord <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1086_133826</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40680833</jstor_id><sourcerecordid>40680833</sourcerecordid><originalsourceid>FETCH-LOGICAL-c275t-4b7fd7e7c06fde06ad430897bb6608d4cdf179513368a09ae7ad2cc4539f0f823</originalsourceid><addsrcrecordid>eNo9kEtLxDAUhYMoWEf9B0JX7qI3TZqkSxnGBxYVHNclzYN27LRDEhjn3xvp4OrAPR-Xcw5C1wTuCEh-TyiVBT9BGSmpxFQKeooyAGCYFxLO0UUIGwBCJIEMva07m3_4KeysjiF3k89XyscO1_13MgY12nTe97Hrx_x1nPZjvvqJXoVpUP7oK3_IPw8h2m24RGdODcFeHXWBvh5X6-Uzrt-fXpYPNdaFKCNmrXBGWKGBO2OBK8MoyEq0LecgDdPGEVGVqQmXCiplhTKF1qyklQMnC7pAt_NfnaIHb12z8_02BWkINH8rNPMKCbyZwU2Ik_-nGHAJklL6C_axWIc</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems</title><source>JSTOR Archive Collection A-Z Listing</source><source>Institute of Physics Journals</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Gehman, Curtis S. ; Adams, Fred C. ; Laughlin, Gregory</creator><creatorcontrib>Gehman, Curtis S. ; Adams, Fred C. ; Laughlin, Gregory</creatorcontrib><description>We consider the possible existence of habitable Earth-like planets in four recently discovered extrasolar planetary systems. Such prospective planets must have orbits that are (1) dynamically stable, and (2) allow for surface temperatures compatible with liquid water. We find that three of the four new systems (51 Peg, p¹ Cnc, and 47 UMa) are easily capable of supporting habitable planets. The fourth (70 Vir) is capable of having a habitable planet only under rather extreme circumstances. To obtain these results, we develop a probabilistic formulation for the coupled problem of orbital stability and planetary habitability.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/133826</identifier><language>eng</language><publisher>American Institute of Physics</publisher><subject>Gas giants ; Habitability ; Orbits ; Outer planets ; Planetary orbits ; Planets ; Solar orbits ; Solar systems ; Stellar orbits ; Terrestrial planets</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1996-11, Vol.108 (729), p.1018-1023</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c275t-4b7fd7e7c06fde06ad430897bb6608d4cdf179513368a09ae7ad2cc4539f0f823</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40680833$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40680833$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,803,27924,27925,58017,58250</link.rule.ids></links><search><creatorcontrib>Gehman, Curtis S.</creatorcontrib><creatorcontrib>Adams, Fred C.</creatorcontrib><creatorcontrib>Laughlin, Gregory</creatorcontrib><title>The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems</title><title>Publications of the Astronomical Society of the Pacific</title><description>We consider the possible existence of habitable Earth-like planets in four recently discovered extrasolar planetary systems. Such prospective planets must have orbits that are (1) dynamically stable, and (2) allow for surface temperatures compatible with liquid water. We find that three of the four new systems (51 Peg, p¹ Cnc, and 47 UMa) are easily capable of supporting habitable planets. The fourth (70 Vir) is capable of having a habitable planet only under rather extreme circumstances. To obtain these results, we develop a probabilistic formulation for the coupled problem of orbital stability and planetary habitability.</description><subject>Gas giants</subject><subject>Habitability</subject><subject>Orbits</subject><subject>Outer planets</subject><subject>Planetary orbits</subject><subject>Planets</subject><subject>Solar orbits</subject><subject>Solar systems</subject><subject>Stellar orbits</subject><subject>Terrestrial planets</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1996</creationdate><recordtype>article</recordtype><recordid>eNo9kEtLxDAUhYMoWEf9B0JX7qI3TZqkSxnGBxYVHNclzYN27LRDEhjn3xvp4OrAPR-Xcw5C1wTuCEh-TyiVBT9BGSmpxFQKeooyAGCYFxLO0UUIGwBCJIEMva07m3_4KeysjiF3k89XyscO1_13MgY12nTe97Hrx_x1nPZjvvqJXoVpUP7oK3_IPw8h2m24RGdODcFeHXWBvh5X6-Uzrt-fXpYPNdaFKCNmrXBGWKGBO2OBK8MoyEq0LecgDdPGEVGVqQmXCiplhTKF1qyklQMnC7pAt_NfnaIHb12z8_02BWkINH8rNPMKCbyZwU2Ik_-nGHAJklL6C_axWIc</recordid><startdate>19961101</startdate><enddate>19961101</enddate><creator>Gehman, Curtis S.</creator><creator>Adams, Fred C.</creator><creator>Laughlin, Gregory</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19961101</creationdate><title>The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems</title><author>Gehman, Curtis S. ; Adams, Fred C. ; Laughlin, Gregory</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c275t-4b7fd7e7c06fde06ad430897bb6608d4cdf179513368a09ae7ad2cc4539f0f823</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1996</creationdate><topic>Gas giants</topic><topic>Habitability</topic><topic>Orbits</topic><topic>Outer planets</topic><topic>Planetary orbits</topic><topic>Planets</topic><topic>Solar orbits</topic><topic>Solar systems</topic><topic>Stellar orbits</topic><topic>Terrestrial planets</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gehman, Curtis S.</creatorcontrib><creatorcontrib>Adams, Fred C.</creatorcontrib><creatorcontrib>Laughlin, Gregory</creatorcontrib><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gehman, Curtis S.</au><au>Adams, Fred C.</au><au>Laughlin, Gregory</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1996-11-01</date><risdate>1996</risdate><volume>108</volume><issue>729</issue><spage>1018</spage><epage>1023</epage><pages>1018-1023</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>We consider the possible existence of habitable Earth-like planets in four recently discovered extrasolar planetary systems. Such prospective planets must have orbits that are (1) dynamically stable, and (2) allow for surface temperatures compatible with liquid water. We find that three of the four new systems (51 Peg, p¹ Cnc, and 47 UMa) are easily capable of supporting habitable planets. The fourth (70 Vir) is capable of having a habitable planet only under rather extreme circumstances. To obtain these results, we develop a probabilistic formulation for the coupled problem of orbital stability and planetary habitability.</abstract><pub>American Institute of Physics</pub><doi>10.1086/133826</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-6280
ispartof Publications of the Astronomical Society of the Pacific, 1996-11, Vol.108 (729), p.1018-1023
issn 0004-6280
1538-3873
language eng
recordid cdi_crossref_primary_10_1086_133826
source JSTOR Archive Collection A-Z Listing; Institute of Physics Journals; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Gas giants
Habitability
Orbits
Outer planets
Planetary orbits
Planets
Solar orbits
Solar systems
Stellar orbits
Terrestrial planets
title The Prospects for Earth-Like Planets within Known Extrasolar Planetary Systems
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T18%3A13%3A56IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Prospects%20for%20Earth-Like%20Planets%20within%20Known%20Extrasolar%20Planetary%20Systems&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=Gehman,%20Curtis%20S.&rft.date=1996-11-01&rft.volume=108&rft.issue=729&rft.spage=1018&rft.epage=1023&rft.pages=1018-1023&rft.issn=0004-6280&rft.eissn=1538-3873&rft_id=info:doi/10.1086/133826&rft_dat=%3Cjstor_cross%3E40680833%3C/jstor_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_jstor_id=40680833&rfr_iscdi=true