The Moon and Extra-Solar Planets
We have used ISO, the Infrared Space Observatory, to perform a systematic search for protoplanetary discs around nearby main-sequence stars. We find a strong correlation with stellar age: more than half of the stars younger than 400Myr do have such a disc, whereas less than 10% of the older stars ex...
Gespeichert in:
| Veröffentlicht in: | Earth, moon, and planets moon, and planets, 1999-01, Vol.85-86 (1-3), p.201-207 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 207 |
|---|---|
| container_issue | 1-3 |
| container_start_page | 201 |
| container_title | Earth, moon, and planets |
| container_volume | 85-86 |
| creator | Jourdain de Muizon, M Laureijs, R. J Habing, H. J Leech, K Kessler, M. F Metcalfe, L Salama, A Siebenmorgen, R Dominik, C Trams, N Bouchet, P |
| description | We have used ISO, the Infrared Space Observatory, to perform a systematic search for protoplanetary discs around nearby main-sequence stars. We find a strong correlation with stellar age: more than half of the stars younger than 400Myr do have such a disc, whereas less than 10% of the older stars exhibit disc emission. Such discs seem thus to decay on a timescale of a few hundred Myr. Both the stability of the discs during this period and their decay can be explained by collisions of planetesimals. Such collisions produce the dust which is necessary to replenish the disc. The process stops as soon as the planetesimals run out, either because they are all destroyed, have escaped, or merged into planets, which implies the decay of the disc. The timescale for the dissipation of protoplanetary discs is remarkably similar to the timescale of the heavy bombardment in our Solar System. The cratering of the Moon is a clear signature of the heavy bombardment which may provide further fundamental clues to the formation of planetary systems. |
| doi_str_mv | 10.1023/A:1017067915613 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_miscellaneous_787213402</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2908966873</sourcerecordid><originalsourceid>FETCH-LOGICAL-p186t-da9da958e0aba147ccac361ce43316f0951248cfeb89dfad77ce956d302a61463</originalsourceid><addsrcrecordid>eNp90E1LxDAQBuAgCtbq2WtR0FN1JpNkEm_Lsn7AioLrecmmKbrUdm264M-3oidBYWAuDy_zjhDHCBcIki4nVwjIYNihNkg7IkPNVAI7tSsyQMOlk07vi4OU1gCgpJWZKBYvsbjvurbwbVXMPobel09d4_visfFtHNKh2Kt9k-LRz87F8_VsMb0t5w83d9PJvNygNUNZeTeOthH8yqPiEHwggyEqIjQ1OI1S2VDHlXVV7SvmEJ02FYH0BpWhXJx_52767n0b07B8e00hNl9XdNu0ZMsSSY1Nc3H2r5Q8voFAj_DkF1x3274dWyxZSSOlIxzR6V9IOrDOGMtEn-AUZSk</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2908966873</pqid></control><display><type>article</type><title>The Moon and Extra-Solar Planets</title><source>EZB-FREE-00999 freely available EZB journals</source><creator>Jourdain de Muizon, M ; Laureijs, R. J ; Habing, H. J ; Leech, K ; Kessler, M. F ; Metcalfe, L ; Salama, A ; Siebenmorgen, R ; Dominik, C ; Trams, N ; Bouchet, P</creator><creatorcontrib>Jourdain de Muizon, M ; Laureijs, R. J ; Habing, H. J ; Leech, K ; Kessler, M. F ; Metcalfe, L ; Salama, A ; Siebenmorgen, R ; Dominik, C ; Trams, N ; Bouchet, P</creatorcontrib><description>We have used ISO, the Infrared Space Observatory, to perform a systematic search for protoplanetary discs around nearby main-sequence stars. We find a strong correlation with stellar age: more than half of the stars younger than 400Myr do have such a disc, whereas less than 10% of the older stars exhibit disc emission. Such discs seem thus to decay on a timescale of a few hundred Myr. Both the stability of the discs during this period and their decay can be explained by collisions of planetesimals. Such collisions produce the dust which is necessary to replenish the disc. The process stops as soon as the planetesimals run out, either because they are all destroyed, have escaped, or merged into planets, which implies the decay of the disc. The timescale for the dissipation of protoplanetary discs is remarkably similar to the timescale of the heavy bombardment in our Solar System. The cratering of the Moon is a clear signature of the heavy bombardment which may provide further fundamental clues to the formation of planetary systems.</description><identifier>ISSN: 0167-9295</identifier><identifier>EISSN: 1573-0794</identifier><identifier>DOI: 10.1023/A:1017067915613</identifier><language>eng</language><publisher>Dordrecht: Springer Nature B.V</publisher><subject>Bombardment ; Collisions ; Decay ; Extrasolar planets ; Infrared Space Observatory (ISO) ; Lunar surface ; Main sequence stars ; Moon ; Planet formation ; Planetary systems ; Planets ; Protoplanetary disks ; Solar system ; Stars ; Stars & galaxies ; Stellar age ; Time</subject><ispartof>Earth, moon, and planets, 1999-01, Vol.85-86 (1-3), p.201-207</ispartof><rights>Kluwer Academic Publishers 1999.</rights><rights>Kluwer Academic Publishers 1999</rights><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Jourdain de Muizon, M</creatorcontrib><creatorcontrib>Laureijs, R. J</creatorcontrib><creatorcontrib>Habing, H. J</creatorcontrib><creatorcontrib>Leech, K</creatorcontrib><creatorcontrib>Kessler, M. F</creatorcontrib><creatorcontrib>Metcalfe, L</creatorcontrib><creatorcontrib>Salama, A</creatorcontrib><creatorcontrib>Siebenmorgen, R</creatorcontrib><creatorcontrib>Dominik, C</creatorcontrib><creatorcontrib>Trams, N</creatorcontrib><creatorcontrib>Bouchet, P</creatorcontrib><title>The Moon and Extra-Solar Planets</title><title>Earth, moon, and planets</title><description>We have used ISO, the Infrared Space Observatory, to perform a systematic search for protoplanetary discs around nearby main-sequence stars. We find a strong correlation with stellar age: more than half of the stars younger than 400Myr do have such a disc, whereas less than 10% of the older stars exhibit disc emission. Such discs seem thus to decay on a timescale of a few hundred Myr. Both the stability of the discs during this period and their decay can be explained by collisions of planetesimals. Such collisions produce the dust which is necessary to replenish the disc. The process stops as soon as the planetesimals run out, either because they are all destroyed, have escaped, or merged into planets, which implies the decay of the disc. The timescale for the dissipation of protoplanetary discs is remarkably similar to the timescale of the heavy bombardment in our Solar System. The cratering of the Moon is a clear signature of the heavy bombardment which may provide further fundamental clues to the formation of planetary systems.</description><subject>Bombardment</subject><subject>Collisions</subject><subject>Decay</subject><subject>Extrasolar planets</subject><subject>Infrared Space Observatory (ISO)</subject><subject>Lunar surface</subject><subject>Main sequence stars</subject><subject>Moon</subject><subject>Planet formation</subject><subject>Planetary systems</subject><subject>Planets</subject><subject>Protoplanetary disks</subject><subject>Solar system</subject><subject>Stars</subject><subject>Stars & galaxies</subject><subject>Stellar age</subject><subject>Time</subject><issn>0167-9295</issn><issn>1573-0794</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1999</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNp90E1LxDAQBuAgCtbq2WtR0FN1JpNkEm_Lsn7AioLrecmmKbrUdm264M-3oidBYWAuDy_zjhDHCBcIki4nVwjIYNihNkg7IkPNVAI7tSsyQMOlk07vi4OU1gCgpJWZKBYvsbjvurbwbVXMPobel09d4_visfFtHNKh2Kt9k-LRz87F8_VsMb0t5w83d9PJvNygNUNZeTeOthH8yqPiEHwggyEqIjQ1OI1S2VDHlXVV7SvmEJ02FYH0BpWhXJx_52767n0b07B8e00hNl9XdNu0ZMsSSY1Nc3H2r5Q8voFAj_DkF1x3274dWyxZSSOlIxzR6V9IOrDOGMtEn-AUZSk</recordid><startdate>19990101</startdate><enddate>19990101</enddate><creator>Jourdain de Muizon, M</creator><creator>Laureijs, R. J</creator><creator>Habing, H. J</creator><creator>Leech, K</creator><creator>Kessler, M. F</creator><creator>Metcalfe, L</creator><creator>Salama, A</creator><creator>Siebenmorgen, R</creator><creator>Dominik, C</creator><creator>Trams, N</creator><creator>Bouchet, P</creator><general>Springer Nature B.V</general><scope>3V.</scope><scope>7TG</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>8G5</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L7M</scope><scope>M2O</scope><scope>M2P</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>PADUT</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>Q9U</scope></search><sort><creationdate>19990101</creationdate><title>The Moon and Extra-Solar Planets</title><author>Jourdain de Muizon, M ; Laureijs, R. J ; Habing, H. J ; Leech, K ; Kessler, M. F ; Metcalfe, L ; Salama, A ; Siebenmorgen, R ; Dominik, C ; Trams, N ; Bouchet, P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p186t-da9da958e0aba147ccac361ce43316f0951248cfeb89dfad77ce956d302a61463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1999</creationdate><topic>Bombardment</topic><topic>Collisions</topic><topic>Decay</topic><topic>Extrasolar planets</topic><topic>Infrared Space Observatory (ISO)</topic><topic>Lunar surface</topic><topic>Main sequence stars</topic><topic>Moon</topic><topic>Planet formation</topic><topic>Planetary systems</topic><topic>Planets</topic><topic>Protoplanetary disks</topic><topic>Solar system</topic><topic>Stars</topic><topic>Stars & galaxies</topic><topic>Stellar age</topic><topic>Time</topic><toplevel>online_resources</toplevel><creatorcontrib>Jourdain de Muizon, M</creatorcontrib><creatorcontrib>Laureijs, R. J</creatorcontrib><creatorcontrib>Habing, H. J</creatorcontrib><creatorcontrib>Leech, K</creatorcontrib><creatorcontrib>Kessler, M. F</creatorcontrib><creatorcontrib>Metcalfe, L</creatorcontrib><creatorcontrib>Salama, A</creatorcontrib><creatorcontrib>Siebenmorgen, R</creatorcontrib><creatorcontrib>Dominik, C</creatorcontrib><creatorcontrib>Trams, N</creatorcontrib><creatorcontrib>Bouchet, P</creatorcontrib><collection>ProQuest Central (Corporate)</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Research Library</collection><collection>Science Database</collection><collection>Research Library (Corporate)</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Research Library China</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central Basic</collection><jtitle>Earth, moon, and planets</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Jourdain de Muizon, M</au><au>Laureijs, R. J</au><au>Habing, H. J</au><au>Leech, K</au><au>Kessler, M. F</au><au>Metcalfe, L</au><au>Salama, A</au><au>Siebenmorgen, R</au><au>Dominik, C</au><au>Trams, N</au><au>Bouchet, P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Moon and Extra-Solar Planets</atitle><jtitle>Earth, moon, and planets</jtitle><date>1999-01-01</date><risdate>1999</risdate><volume>85-86</volume><issue>1-3</issue><spage>201</spage><epage>207</epage><pages>201-207</pages><issn>0167-9295</issn><eissn>1573-0794</eissn><abstract>We have used ISO, the Infrared Space Observatory, to perform a systematic search for protoplanetary discs around nearby main-sequence stars. We find a strong correlation with stellar age: more than half of the stars younger than 400Myr do have such a disc, whereas less than 10% of the older stars exhibit disc emission. Such discs seem thus to decay on a timescale of a few hundred Myr. Both the stability of the discs during this period and their decay can be explained by collisions of planetesimals. Such collisions produce the dust which is necessary to replenish the disc. The process stops as soon as the planetesimals run out, either because they are all destroyed, have escaped, or merged into planets, which implies the decay of the disc. The timescale for the dissipation of protoplanetary discs is remarkably similar to the timescale of the heavy bombardment in our Solar System. The cratering of the Moon is a clear signature of the heavy bombardment which may provide further fundamental clues to the formation of planetary systems.</abstract><cop>Dordrecht</cop><pub>Springer Nature B.V</pub><doi>10.1023/A:1017067915613</doi><tpages>7</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0167-9295 |
| ispartof | Earth, moon, and planets, 1999-01, Vol.85-86 (1-3), p.201-207 |
| issn | 0167-9295 1573-0794 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_787213402 |
| source | EZB-FREE-00999 freely available EZB journals |
| subjects | Bombardment Collisions Decay Extrasolar planets Infrared Space Observatory (ISO) Lunar surface Main sequence stars Moon Planet formation Planetary systems Planets Protoplanetary disks Solar system Stars Stars & galaxies Stellar age Time |
| title | The Moon and Extra-Solar Planets |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-26T11%3A23%3A03IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=The%20Moon%20and%20Extra-Solar%20Planets&rft.jtitle=Earth,%20moon,%20and%20planets&rft.au=Jourdain%20de%20Muizon,%20M&rft.date=1999-01-01&rft.volume=85-86&rft.issue=1-3&rft.spage=201&rft.epage=207&rft.pages=201-207&rft.issn=0167-9295&rft.eissn=1573-0794&rft_id=info:doi/10.1023/A:1017067915613&rft_dat=%3Cproquest%3E2908966873%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2908966873&rft_id=info:pmid/&rfr_iscdi=true |