Kepler-91b: a planet at the end of its life: Planet and giant host star properties via light-curve variations

The evolution of planetary systems is intimately linked to the evolution of their host stars. Although several theories have been proposed, the question of how planets die remains open owing to the small number statistics, making it clear that the sample of planets around post-main sequence stars ne...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astronomy and astrophysics (Berlin) 2014-02, Vol.562, p.np-np
Hauptverfasser: Lillo-Box, J, Barrado, D, Moya, A, Montesinos, B, Montalban, J, Bayo, A, Barbieri, M, Regulo, C, Mancini, L, Bouy, H, Henning, T
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page np
container_issue
container_start_page np
container_title Astronomy and astrophysics (Berlin)
container_volume 562
creator Lillo-Box, J
Barrado, D
Moya, A
Montesinos, B
Montalban, J
Bayo, A
Barbieri, M
Regulo, C
Mancini, L
Bouy, H
Henning, T
description The evolution of planetary systems is intimately linked to the evolution of their host stars. Although several theories have been proposed, the question of how planets die remains open owing to the small number statistics, making it clear that the sample of planets around post-main sequence stars needs to be enlarged. In this work we study the giant star Kepler-91 (KOI-2133) in order to determine the nature of a transiting companion. However, its planetary confirmation is needed due to the large pixel size of the Kepler camera, which can hide other stellar configurations able to mimic planet-like transit events. Kepler-91b could be the previous stage of the planet engulfment, which has recently been detected for BD+48 740. Our estimations show that Kepler-91b will be swallowed by its host star in less than 55 Myr. At pericentre, the star subtends an angle of 48[degrees], covering around 10% of the sky as seen from the planet. The planetary atmosphere seems to be inflated probably due to the high stellar irradiation.
doi_str_mv 10.1051/0004-6361/201322001
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1651404710</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1651404710</sourcerecordid><originalsourceid>FETCH-LOGICAL-c265t-e3b9bbf0f296a0e39ee8472d90ed2c9204817614afe03ee58f88cb6bc5fbb75e3</originalsourceid><addsrcrecordid>eNqNkMFKAzEURYMoWKtf4CZLQca-l2QyiTspVsWCG12HJPOCI9POOJku_Hs7VLp2dblwuFwOY9cIdwglLgBAFVpqXAhAKQQAnrAZKikKqJQ-ZbMjcc4ucv7aV4FGztjtK_UtDYXFcM8971u_pZH7kY-fxGlb8y7xZsy8bRJdsrPk20xXfzlnH6vH9-VzsX57elk-rIsodDkWJIMNIUESVnsgaYmMqkRtgWoRrQBlsNKofCKQRKVJxsSgQyxTCFVJcs5uDrv90H3vKI9u0-RI7fSt22WHukQFqkL4ByqtNVog7lF5QOPQ5TxQcv3QbPzw4xDcZNFNjtzkyB0tyl-C9mGD</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1639986211</pqid></control><display><type>article</type><title>Kepler-91b: a planet at the end of its life: Planet and giant host star properties via light-curve variations</title><source>EDP Sciences</source><source>EZB Electronic Journals Library</source><source>EDP Sciences - Revues - Licences nationales - accès par la plateforme ISTEX</source><creator>Lillo-Box, J ; Barrado, D ; Moya, A ; Montesinos, B ; Montalban, J ; Bayo, A ; Barbieri, M ; Regulo, C ; Mancini, L ; Bouy, H ; Henning, T</creator><creatorcontrib>Lillo-Box, J ; Barrado, D ; Moya, A ; Montesinos, B ; Montalban, J ; Bayo, A ; Barbieri, M ; Regulo, C ; Mancini, L ; Bouy, H ; Henning, T</creatorcontrib><description>The evolution of planetary systems is intimately linked to the evolution of their host stars. Although several theories have been proposed, the question of how planets die remains open owing to the small number statistics, making it clear that the sample of planets around post-main sequence stars needs to be enlarged. In this work we study the giant star Kepler-91 (KOI-2133) in order to determine the nature of a transiting companion. However, its planetary confirmation is needed due to the large pixel size of the Kepler camera, which can hide other stellar configurations able to mimic planet-like transit events. Kepler-91b could be the previous stage of the planet engulfment, which has recently been detected for BD+48 740. Our estimations show that Kepler-91b will be swallowed by its host star in less than 55 Myr. At pericentre, the star subtends an angle of 48[degrees], covering around 10% of the sky as seen from the planet. The planetary atmosphere seems to be inflated probably due to the high stellar irradiation.</description><identifier>ISSN: 0004-6361</identifier><identifier>EISSN: 1432-0746</identifier><identifier>DOI: 10.1051/0004-6361/201322001</identifier><language>eng</language><subject>Planetary systems ; Planets ; Samples ; Stars ; Statistical methods ; Statistics ; Stellar evolution ; Transit</subject><ispartof>Astronomy and astrophysics (Berlin), 2014-02, Vol.562, p.np-np</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c265t-e3b9bbf0f296a0e39ee8472d90ed2c9204817614afe03ee58f88cb6bc5fbb75e3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,3714,27901,27902</link.rule.ids></links><search><creatorcontrib>Lillo-Box, J</creatorcontrib><creatorcontrib>Barrado, D</creatorcontrib><creatorcontrib>Moya, A</creatorcontrib><creatorcontrib>Montesinos, B</creatorcontrib><creatorcontrib>Montalban, J</creatorcontrib><creatorcontrib>Bayo, A</creatorcontrib><creatorcontrib>Barbieri, M</creatorcontrib><creatorcontrib>Regulo, C</creatorcontrib><creatorcontrib>Mancini, L</creatorcontrib><creatorcontrib>Bouy, H</creatorcontrib><creatorcontrib>Henning, T</creatorcontrib><title>Kepler-91b: a planet at the end of its life: Planet and giant host star properties via light-curve variations</title><title>Astronomy and astrophysics (Berlin)</title><description>The evolution of planetary systems is intimately linked to the evolution of their host stars. Although several theories have been proposed, the question of how planets die remains open owing to the small number statistics, making it clear that the sample of planets around post-main sequence stars needs to be enlarged. In this work we study the giant star Kepler-91 (KOI-2133) in order to determine the nature of a transiting companion. However, its planetary confirmation is needed due to the large pixel size of the Kepler camera, which can hide other stellar configurations able to mimic planet-like transit events. Kepler-91b could be the previous stage of the planet engulfment, which has recently been detected for BD+48 740. Our estimations show that Kepler-91b will be swallowed by its host star in less than 55 Myr. At pericentre, the star subtends an angle of 48[degrees], covering around 10% of the sky as seen from the planet. The planetary atmosphere seems to be inflated probably due to the high stellar irradiation.</description><subject>Planetary systems</subject><subject>Planets</subject><subject>Samples</subject><subject>Stars</subject><subject>Statistical methods</subject><subject>Statistics</subject><subject>Stellar evolution</subject><subject>Transit</subject><issn>0004-6361</issn><issn>1432-0746</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqNkMFKAzEURYMoWKtf4CZLQca-l2QyiTspVsWCG12HJPOCI9POOJku_Hs7VLp2dblwuFwOY9cIdwglLgBAFVpqXAhAKQQAnrAZKikKqJQ-ZbMjcc4ucv7aV4FGztjtK_UtDYXFcM8971u_pZH7kY-fxGlb8y7xZsy8bRJdsrPk20xXfzlnH6vH9-VzsX57elk-rIsodDkWJIMNIUESVnsgaYmMqkRtgWoRrQBlsNKofCKQRKVJxsSgQyxTCFVJcs5uDrv90H3vKI9u0-RI7fSt22WHukQFqkL4ByqtNVog7lF5QOPQ5TxQcv3QbPzw4xDcZNFNjtzkyB0tyl-C9mGD</recordid><startdate>20140201</startdate><enddate>20140201</enddate><creator>Lillo-Box, J</creator><creator>Barrado, D</creator><creator>Moya, A</creator><creator>Montesinos, B</creator><creator>Montalban, J</creator><creator>Bayo, A</creator><creator>Barbieri, M</creator><creator>Regulo, C</creator><creator>Mancini, L</creator><creator>Bouy, H</creator><creator>Henning, T</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20140201</creationdate><title>Kepler-91b: a planet at the end of its life</title><author>Lillo-Box, J ; Barrado, D ; Moya, A ; Montesinos, B ; Montalban, J ; Bayo, A ; Barbieri, M ; Regulo, C ; Mancini, L ; Bouy, H ; Henning, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c265t-e3b9bbf0f296a0e39ee8472d90ed2c9204817614afe03ee58f88cb6bc5fbb75e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Planetary systems</topic><topic>Planets</topic><topic>Samples</topic><topic>Stars</topic><topic>Statistical methods</topic><topic>Statistics</topic><topic>Stellar evolution</topic><topic>Transit</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Lillo-Box, J</creatorcontrib><creatorcontrib>Barrado, D</creatorcontrib><creatorcontrib>Moya, A</creatorcontrib><creatorcontrib>Montesinos, B</creatorcontrib><creatorcontrib>Montalban, J</creatorcontrib><creatorcontrib>Bayo, A</creatorcontrib><creatorcontrib>Barbieri, M</creatorcontrib><creatorcontrib>Regulo, C</creatorcontrib><creatorcontrib>Mancini, L</creatorcontrib><creatorcontrib>Bouy, H</creatorcontrib><creatorcontrib>Henning, T</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy and astrophysics (Berlin)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Lillo-Box, J</au><au>Barrado, D</au><au>Moya, A</au><au>Montesinos, B</au><au>Montalban, J</au><au>Bayo, A</au><au>Barbieri, M</au><au>Regulo, C</au><au>Mancini, L</au><au>Bouy, H</au><au>Henning, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Kepler-91b: a planet at the end of its life: Planet and giant host star properties via light-curve variations</atitle><jtitle>Astronomy and astrophysics (Berlin)</jtitle><date>2014-02-01</date><risdate>2014</risdate><volume>562</volume><spage>np</spage><epage>np</epage><pages>np-np</pages><issn>0004-6361</issn><eissn>1432-0746</eissn><abstract>The evolution of planetary systems is intimately linked to the evolution of their host stars. Although several theories have been proposed, the question of how planets die remains open owing to the small number statistics, making it clear that the sample of planets around post-main sequence stars needs to be enlarged. In this work we study the giant star Kepler-91 (KOI-2133) in order to determine the nature of a transiting companion. However, its planetary confirmation is needed due to the large pixel size of the Kepler camera, which can hide other stellar configurations able to mimic planet-like transit events. Kepler-91b could be the previous stage of the planet engulfment, which has recently been detected for BD+48 740. Our estimations show that Kepler-91b will be swallowed by its host star in less than 55 Myr. At pericentre, the star subtends an angle of 48[degrees], covering around 10% of the sky as seen from the planet. The planetary atmosphere seems to be inflated probably due to the high stellar irradiation.</abstract><doi>10.1051/0004-6361/201322001</doi></addata></record>
fulltext fulltext
identifier ISSN: 0004-6361
ispartof Astronomy and astrophysics (Berlin), 2014-02, Vol.562, p.np-np
issn 0004-6361
1432-0746
language eng
recordid cdi_proquest_miscellaneous_1651404710
source EDP Sciences; EZB Electronic Journals Library; EDP Sciences - Revues - Licences nationales - accès par la plateforme ISTEX
subjects Planetary systems
Planets
Samples
Stars
Statistical methods
Statistics
Stellar evolution
Transit
title Kepler-91b: a planet at the end of its life: Planet and giant host star properties via light-curve variations
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-29T10%3A59%3A27IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Kepler-91b:%20a%20planet%20at%20the%20end%20of%20its%20life:%20Planet%20and%20giant%20host%20star%20properties%20via%20light-curve%20variations&rft.jtitle=Astronomy%20and%20astrophysics%20(Berlin)&rft.au=Lillo-Box,%20J&rft.date=2014-02-01&rft.volume=562&rft.spage=np&rft.epage=np&rft.pages=np-np&rft.issn=0004-6361&rft.eissn=1432-0746&rft_id=info:doi/10.1051/0004-6361/201322001&rft_dat=%3Cproquest_cross%3E1651404710%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1639986211&rft_id=info:pmid/&rfr_iscdi=true