SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets
The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee & Taylor 2001), as well as contributions to a...
Gespeichert in:
Veröffentlicht in: | arXiv.org 2007-04 |
---|---|
Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Shao, M Marcy, G Unwin, S Allen, R Beichman, C Catanzarite, J Chaboyer, B Ciardi, D Edberg, S J Gallagher, D Gould, A Henry, T Johnston, K Kulkarni, S Law, N Majewski, S Marr, J Pan, X Shaklan, S Shaya, E Tanner, A Tomsick, J Wehrle, A Worthey, G |
description | The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee & Taylor 2001), as well as contributions to a broad range of problems in astrophysics. Numerous committees of the National Research Council as well as NASA Roadmaps have similarly highlighted SIM as the one technology that offers detection and characterization of rocky planets around nearby stars and which is technically ready. To date, SIM remains the only program with the capability of detecting and confirming rocky planets in the habitable zones of nearby solar-type stars. Moreover, SIM measures masses and three-dimensional orbits of habitable planets around nearby stars (within 25 pc); these are the only stars for which follow-up by other techniques is feasible, such as space-based spectroscopy, ground-based interferometry, and of course TPF. |
doi_str_mv | 10.48550/arxiv.0704.0952 |
format | Article |
fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_0704_0952</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2089897201</sourcerecordid><originalsourceid>FETCH-LOGICAL-a511-8d9f26ecac832ed1d65735ebbe35a9b0fb4b16c831e7529e219ed556d8fc09c33</originalsourceid><addsrcrecordid>eNotkEtPwkAUhScmJhJk78pM4pbiPDptx50BERIqGLtvZtpbGdIHzBQjf8NfbAus7s09Jyf3fAg9UDLxIyHIs7K_5mdCQuJPiBTsBg0Y59SLfMbu0Mi5HSGEBSETgg_Q39cyxptS1dB-HsG1LzjZAo4b1-KNbSrjTP2NP0BZLwFb4QSybW0OR8Btg2fQQtaO8dzUOY6Vc-DGWHV7L9jK1NCFWQBvZiqonWlqVeK11aZ1uCnOqfqEF6o7KF3C9Q13j24LVToYXecQJfO3ZLrwVuv35fR15SlBuzq5LFgAmcoiziCneSBCLkBr4EJJTQrtaxp0IoVQMAmMSsiFCPKoyIjMOB-ix0vsmVe6t6ZS9pT23NKeW2d4uhj2tjn0bNJdc7RdB5cyEslIhoxQ_g-jAXFZ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2089897201</pqid></control><display><type>article</type><title>SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets</title><source>Freely Accessible Journals</source><source>arXiv.org</source><creator>Shao, M ; Marcy, G ; Unwin, S ; Allen, R ; Beichman, C ; Catanzarite, J ; Chaboyer, B ; Ciardi, D ; Edberg, S J ; Gallagher, D ; Gould, A ; Henry, T ; Johnston, K ; Kulkarni, S ; Law, N ; Majewski, S ; Marr, J ; Pan, X ; Shaklan, S ; Shaya, E ; Tanner, A ; Tomsick, J ; Wehrle, A ; Worthey, G</creator><creatorcontrib>Shao, M ; Marcy, G ; Unwin, S ; Allen, R ; Beichman, C ; Catanzarite, J ; Chaboyer, B ; Ciardi, D ; Edberg, S J ; Gallagher, D ; Gould, A ; Henry, T ; Johnston, K ; Kulkarni, S ; Law, N ; Majewski, S ; Marr, J ; Pan, X ; Shaklan, S ; Shaya, E ; Tanner, A ; Tomsick, J ; Wehrle, A ; Worthey, G</creatorcontrib><description>The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee & Taylor 2001), as well as contributions to a broad range of problems in astrophysics. Numerous committees of the National Research Council as well as NASA Roadmaps have similarly highlighted SIM as the one technology that offers detection and characterization of rocky planets around nearby stars and which is technically ready. To date, SIM remains the only program with the capability of detecting and confirming rocky planets in the habitable zones of nearby solar-type stars. Moreover, SIM measures masses and three-dimensional orbits of habitable planets around nearby stars (within 25 pc); these are the only stars for which follow-up by other techniques is feasible, such as space-based spectroscopy, ground-based interferometry, and of course TPF.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0704.0952</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astronomy ; Astrophysics ; Circumstellar habitable zone ; Interferometry ; Orbits ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Planet detection ; Planets ; R&D ; Research & development ; Stars ; Terrestrial planets</subject><ispartof>arXiv.org, 2007-04</ispartof><rights>Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the associated terms available at http://arxiv.org/abs/0704.0952.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.0704.0952$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1117/12.734671$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Shao, M</creatorcontrib><creatorcontrib>Marcy, G</creatorcontrib><creatorcontrib>Unwin, S</creatorcontrib><creatorcontrib>Allen, R</creatorcontrib><creatorcontrib>Beichman, C</creatorcontrib><creatorcontrib>Catanzarite, J</creatorcontrib><creatorcontrib>Chaboyer, B</creatorcontrib><creatorcontrib>Ciardi, D</creatorcontrib><creatorcontrib>Edberg, S J</creatorcontrib><creatorcontrib>Gallagher, D</creatorcontrib><creatorcontrib>Gould, A</creatorcontrib><creatorcontrib>Henry, T</creatorcontrib><creatorcontrib>Johnston, K</creatorcontrib><creatorcontrib>Kulkarni, S</creatorcontrib><creatorcontrib>Law, N</creatorcontrib><creatorcontrib>Majewski, S</creatorcontrib><creatorcontrib>Marr, J</creatorcontrib><creatorcontrib>Pan, X</creatorcontrib><creatorcontrib>Shaklan, S</creatorcontrib><creatorcontrib>Shaya, E</creatorcontrib><creatorcontrib>Tanner, A</creatorcontrib><creatorcontrib>Tomsick, J</creatorcontrib><creatorcontrib>Wehrle, A</creatorcontrib><creatorcontrib>Worthey, G</creatorcontrib><title>SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets</title><title>arXiv.org</title><description>The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee & Taylor 2001), as well as contributions to a broad range of problems in astrophysics. Numerous committees of the National Research Council as well as NASA Roadmaps have similarly highlighted SIM as the one technology that offers detection and characterization of rocky planets around nearby stars and which is technically ready. To date, SIM remains the only program with the capability of detecting and confirming rocky planets in the habitable zones of nearby solar-type stars. Moreover, SIM measures masses and three-dimensional orbits of habitable planets around nearby stars (within 25 pc); these are the only stars for which follow-up by other techniques is feasible, such as space-based spectroscopy, ground-based interferometry, and of course TPF.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Circumstellar habitable zone</subject><subject>Interferometry</subject><subject>Orbits</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Planet detection</subject><subject>Planets</subject><subject>R&D</subject><subject>Research & development</subject><subject>Stars</subject><subject>Terrestrial planets</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotkEtPwkAUhScmJhJk78pM4pbiPDptx50BERIqGLtvZtpbGdIHzBQjf8NfbAus7s09Jyf3fAg9UDLxIyHIs7K_5mdCQuJPiBTsBg0Y59SLfMbu0Mi5HSGEBSETgg_Q39cyxptS1dB-HsG1LzjZAo4b1-KNbSrjTP2NP0BZLwFb4QSybW0OR8Btg2fQQtaO8dzUOY6Vc-DGWHV7L9jK1NCFWQBvZiqonWlqVeK11aZ1uCnOqfqEF6o7KF3C9Q13j24LVToYXecQJfO3ZLrwVuv35fR15SlBuzq5LFgAmcoiziCneSBCLkBr4EJJTQrtaxp0IoVQMAmMSsiFCPKoyIjMOB-ix0vsmVe6t6ZS9pT23NKeW2d4uhj2tjn0bNJdc7RdB5cyEslIhoxQ_g-jAXFZ</recordid><startdate>20070406</startdate><enddate>20070406</enddate><creator>Shao, M</creator><creator>Marcy, G</creator><creator>Unwin, S</creator><creator>Allen, R</creator><creator>Beichman, C</creator><creator>Catanzarite, J</creator><creator>Chaboyer, B</creator><creator>Ciardi, D</creator><creator>Edberg, S J</creator><creator>Gallagher, D</creator><creator>Gould, A</creator><creator>Henry, T</creator><creator>Johnston, K</creator><creator>Kulkarni, S</creator><creator>Law, N</creator><creator>Majewski, S</creator><creator>Marr, J</creator><creator>Pan, X</creator><creator>Shaklan, S</creator><creator>Shaya, E</creator><creator>Tanner, A</creator><creator>Tomsick, J</creator><creator>Wehrle, A</creator><creator>Worthey, G</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20070406</creationdate><title>SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets</title><author>Shao, M ; Marcy, G ; Unwin, S ; Allen, R ; Beichman, C ; Catanzarite, J ; Chaboyer, B ; Ciardi, D ; Edberg, S J ; Gallagher, D ; Gould, A ; Henry, T ; Johnston, K ; Kulkarni, S ; Law, N ; Majewski, S ; Marr, J ; Pan, X ; Shaklan, S ; Shaya, E ; Tanner, A ; Tomsick, J ; Wehrle, A ; Worthey, G</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a511-8d9f26ecac832ed1d65735ebbe35a9b0fb4b16c831e7529e219ed556d8fc09c33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Circumstellar habitable zone</topic><topic>Interferometry</topic><topic>Orbits</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Planet detection</topic><topic>Planets</topic><topic>R&D</topic><topic>Research & development</topic><topic>Stars</topic><topic>Terrestrial planets</topic><toplevel>online_resources</toplevel><creatorcontrib>Shao, M</creatorcontrib><creatorcontrib>Marcy, G</creatorcontrib><creatorcontrib>Unwin, S</creatorcontrib><creatorcontrib>Allen, R</creatorcontrib><creatorcontrib>Beichman, C</creatorcontrib><creatorcontrib>Catanzarite, J</creatorcontrib><creatorcontrib>Chaboyer, B</creatorcontrib><creatorcontrib>Ciardi, D</creatorcontrib><creatorcontrib>Edberg, S J</creatorcontrib><creatorcontrib>Gallagher, D</creatorcontrib><creatorcontrib>Gould, A</creatorcontrib><creatorcontrib>Henry, T</creatorcontrib><creatorcontrib>Johnston, K</creatorcontrib><creatorcontrib>Kulkarni, S</creatorcontrib><creatorcontrib>Law, N</creatorcontrib><creatorcontrib>Majewski, S</creatorcontrib><creatorcontrib>Marr, J</creatorcontrib><creatorcontrib>Pan, X</creatorcontrib><creatorcontrib>Shaklan, S</creatorcontrib><creatorcontrib>Shaya, E</creatorcontrib><creatorcontrib>Tanner, A</creatorcontrib><creatorcontrib>Tomsick, J</creatorcontrib><creatorcontrib>Wehrle, A</creatorcontrib><creatorcontrib>Worthey, G</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</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>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</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 China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Shao, M</au><au>Marcy, G</au><au>Unwin, S</au><au>Allen, R</au><au>Beichman, C</au><au>Catanzarite, J</au><au>Chaboyer, B</au><au>Ciardi, D</au><au>Edberg, S J</au><au>Gallagher, D</au><au>Gould, A</au><au>Henry, T</au><au>Johnston, K</au><au>Kulkarni, S</au><au>Law, N</au><au>Majewski, S</au><au>Marr, J</au><au>Pan, X</au><au>Shaklan, S</au><au>Shaya, E</au><au>Tanner, A</au><au>Tomsick, J</au><au>Wehrle, A</au><au>Worthey, G</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets</atitle><jtitle>arXiv.org</jtitle><date>2007-04-06</date><risdate>2007</risdate><eissn>2331-8422</eissn><abstract>The past two Decadal Surveys in Astronomy and Astrophysics recommended the completion of a space-based interferometry mission, known today as SIM PlanetQuest, for its unique ability to detect and characterize nearby rocky planets (Bahcall 1991, McKee & Taylor 2001), as well as contributions to a broad range of problems in astrophysics. Numerous committees of the National Research Council as well as NASA Roadmaps have similarly highlighted SIM as the one technology that offers detection and characterization of rocky planets around nearby stars and which is technically ready. To date, SIM remains the only program with the capability of detecting and confirming rocky planets in the habitable zones of nearby solar-type stars. Moreover, SIM measures masses and three-dimensional orbits of habitable planets around nearby stars (within 25 pc); these are the only stars for which follow-up by other techniques is feasible, such as space-based spectroscopy, ground-based interferometry, and of course TPF.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0704.0952</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2007-04 |
issn | 2331-8422 |
language | eng |
recordid | cdi_arxiv_primary_0704_0952 |
source | Freely Accessible Journals; arXiv.org |
subjects | Astronomy Astrophysics Circumstellar habitable zone Interferometry Orbits Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Planet detection Planets R&D Research & development Stars Terrestrial planets |
title | SIM PlanetQuest: The Most Promising Near-Term Technique to Detect, Find Masses, and Determine Three-Dimensional Orbits of Nearby Habitable Planets |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-05T10%3A41%3A25IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=SIM%20PlanetQuest:%20The%20Most%20Promising%20Near-Term%20Technique%20to%20Detect,%20Find%20Masses,%20and%20Determine%20Three-Dimensional%20Orbits%20of%20Nearby%20Habitable%20Planets&rft.jtitle=arXiv.org&rft.au=Shao,%20M&rft.date=2007-04-06&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.0704.0952&rft_dat=%3Cproquest_arxiv%3E2089897201%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2089897201&rft_id=info:pmid/&rfr_iscdi=true |