An Earth-mass planet orbiting α Centauri B
Exoplanets down to the size of Earth have been found, but not in the habitable zone—that is, at a distance from the parent star at which water, if present, would be liquid. There are planets in the habitable zone of stars cooler than our Sun, but for reasons such as tidal locking and strong stellar...
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Veröffentlicht in: | Nature (London) 2012-11, Vol.491 (7423), p.207-211 |
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creator | Dumusque, Xavier Pepe, Francesco Lovis, Christophe Ségransan, Damien Sahlmann, Johannes Benz, Willy Bouchy, François Mayor, Michel Queloz, Didier Santos, Nuno Udry, Stéphane |
description | Exoplanets down to the size of Earth have been found, but not in the habitable zone—that is, at a distance from the parent star at which water, if present, would be liquid. There are planets in the habitable zone of stars cooler than our Sun, but for reasons such as tidal locking and strong stellar activity, they are unlikely to harbour water–carbon life as we know it. The detection of a habitable Earth-mass planet orbiting a star similar to our Sun is extremely difficult, because such a signal is overwhelmed by stellar perturbations. Here we report the detection of an Earth-mass planet orbiting our neighbour star α Centauri B, a member of the closest stellar system to the Sun. The planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star (one astronomical unit is the Earth–Sun distance).
The detection of an Earth-mass planet orbiting our neighbour star α Centauri B is reported; the planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star.
A nearby Earth-mass exoplanet discovered
An exoplanet with an Earth-like mass has been discovered orbiting the nearby star α Centauri B. The planet is not in the habitable zone — it is much nearer to its star than we are to the Sun, orbiting at only about 0.04 astronomical units from its star (an astronomical unit is the mean distance between Earth and the Sun). Statistical studies suggest that low-mass planets form preferentially in multi-planet systems, so it is possible that other planets are orbiting α Centauri B, perhaps in its habitable zone. |
doi_str_mv | 10.1038/nature11572 |
format | Article |
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The detection of an Earth-mass planet orbiting our neighbour star α Centauri B is reported; the planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star.
A nearby Earth-mass exoplanet discovered
An exoplanet with an Earth-like mass has been discovered orbiting the nearby star α Centauri B. The planet is not in the habitable zone — it is much nearer to its star than we are to the Sun, orbiting at only about 0.04 astronomical units from its star (an astronomical unit is the mean distance between Earth and the Sun). Statistical studies suggest that low-mass planets form preferentially in multi-planet systems, so it is possible that other planets are orbiting α Centauri B, perhaps in its habitable zone.</description><identifier>ISSN: 0028-0836</identifier><identifier>EISSN: 1476-4687</identifier><identifier>DOI: 10.1038/nature11572</identifier><identifier>PMID: 23075844</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>639/33/34/862 ; Analysis ; Astronomical bodies ; Coolers ; Cosmic physics ; Extrasolar planets ; Harbours ; Humanities and Social Sciences ; multidisciplinary ; Observations ; Orbitals ; Orbits ; Planet detection ; Science ; Sciences of the Universe ; Spectra ; Stars ; Sun</subject><ispartof>Nature (London), 2012-11, Vol.491 (7423), p.207-211</ispartof><rights>Springer Nature Limited 2012</rights><rights>COPYRIGHT 2012 Nature Publishing Group</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c628t-101dd50c0c2ddb8f6295d26d2fa71311c4a093c57b9d03ccbd3d4d3efb0e85453</citedby><cites>FETCH-LOGICAL-c628t-101dd50c0c2ddb8f6295d26d2fa71311c4a093c57b9d03ccbd3d4d3efb0e85453</cites><orcidid>0000-0002-7613-393X ; 0000-0003-4422-2919 ; 0000-0001-7576-6236 ; 0000-0003-2355-8034 ; 0000-0001-7120-5837 ; 0000-0002-3012-0316</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,315,782,786,887,27931,27932</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/23075844$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://hal.science/hal-03645720$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>Dumusque, Xavier</creatorcontrib><creatorcontrib>Pepe, Francesco</creatorcontrib><creatorcontrib>Lovis, Christophe</creatorcontrib><creatorcontrib>Ségransan, Damien</creatorcontrib><creatorcontrib>Sahlmann, Johannes</creatorcontrib><creatorcontrib>Benz, Willy</creatorcontrib><creatorcontrib>Bouchy, François</creatorcontrib><creatorcontrib>Mayor, Michel</creatorcontrib><creatorcontrib>Queloz, Didier</creatorcontrib><creatorcontrib>Santos, Nuno</creatorcontrib><creatorcontrib>Udry, Stéphane</creatorcontrib><title>An Earth-mass planet orbiting α Centauri B</title><title>Nature (London)</title><addtitle>Nature</addtitle><addtitle>Nature</addtitle><description>Exoplanets down to the size of Earth have been found, but not in the habitable zone—that is, at a distance from the parent star at which water, if present, would be liquid. There are planets in the habitable zone of stars cooler than our Sun, but for reasons such as tidal locking and strong stellar activity, they are unlikely to harbour water–carbon life as we know it. The detection of a habitable Earth-mass planet orbiting a star similar to our Sun is extremely difficult, because such a signal is overwhelmed by stellar perturbations. Here we report the detection of an Earth-mass planet orbiting our neighbour star α Centauri B, a member of the closest stellar system to the Sun. The planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star (one astronomical unit is the Earth–Sun distance).
The detection of an Earth-mass planet orbiting our neighbour star α Centauri B is reported; the planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star.
A nearby Earth-mass exoplanet discovered
An exoplanet with an Earth-like mass has been discovered orbiting the nearby star α Centauri B. The planet is not in the habitable zone — it is much nearer to its star than we are to the Sun, orbiting at only about 0.04 astronomical units from its star (an astronomical unit is the mean distance between Earth and the Sun). Statistical studies suggest that low-mass planets form preferentially in multi-planet systems, so it is possible that other planets are orbiting α Centauri B, perhaps in its habitable zone.</description><subject>639/33/34/862</subject><subject>Analysis</subject><subject>Astronomical bodies</subject><subject>Coolers</subject><subject>Cosmic physics</subject><subject>Extrasolar planets</subject><subject>Harbours</subject><subject>Humanities and Social Sciences</subject><subject>multidisciplinary</subject><subject>Observations</subject><subject>Orbitals</subject><subject>Orbits</subject><subject>Planet detection</subject><subject>Science</subject><subject>Sciences of the Universe</subject><subject>Spectra</subject><subject>Stars</subject><subject>Sun</subject><issn>0028-0836</issn><issn>1476-4687</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqF0t9q1TAYAPAgijtOr7yX4m4cszNpkia9rIfpBgcFnXgZ0iTtMtr0LElFH8sX8ZlMOXPsQGXkIpD88pHvDwAvETxFEPN3TsbJG4QoKx6BFSKszEnJ2WOwgrDgOeS4PADPQriGEFLEyFNwUGDIKCdkBU5ql51JH6_yQYaQbXvpTMxG39hoXZf9-Z2tjYty8jZ7_xw8aWUfzIvb_RB8-3B2uT7PN58_XqzrTa7KgsccQaQ1hQqqQuuGt2VRUV2UumglQxghRSSssKKsqTTESjUaa6KxaRtoOCUUH4LjXdwr2Yutt4P0v8QorTivN2I-g7gkKVv4AyX7Zme3fryZTIhisEGZfs5jnIJAjGKKedIPU4IrxnGVPvcgRTSVHmE6Rz3a0U72RljXjtFLNXNRY8jL1AM2p5QvqM4442U_OtPadLznXy94tbU34j46XUBpaTNYtRj1eO9BMtH8jJ2cQhAXX7_s25P_2_ry-_rTolZ-DMGb9q5vCIp5SsW9KU361W15p2Yw-s7-G8sE3u5ASFeuM15cj5N3aegW4_0Fr-Tp3A</recordid><startdate>20121108</startdate><enddate>20121108</enddate><creator>Dumusque, Xavier</creator><creator>Pepe, Francesco</creator><creator>Lovis, Christophe</creator><creator>Ségransan, Damien</creator><creator>Sahlmann, Johannes</creator><creator>Benz, Willy</creator><creator>Bouchy, François</creator><creator>Mayor, Michel</creator><creator>Queloz, Didier</creator><creator>Santos, Nuno</creator><creator>Udry, Stéphane</creator><general>Nature Publishing Group UK</general><general>Nature Publishing Group</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>ATWCN</scope><scope>7X8</scope><scope>7SC</scope><scope>7SP</scope><scope>7SR</scope><scope>7TB</scope><scope>7U5</scope><scope>8BQ</scope><scope>8FD</scope><scope>F28</scope><scope>FR3</scope><scope>H8D</scope><scope>JG9</scope><scope>JQ2</scope><scope>KR7</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0002-7613-393X</orcidid><orcidid>https://orcid.org/0000-0003-4422-2919</orcidid><orcidid>https://orcid.org/0000-0001-7576-6236</orcidid><orcidid>https://orcid.org/0000-0003-2355-8034</orcidid><orcidid>https://orcid.org/0000-0001-7120-5837</orcidid><orcidid>https://orcid.org/0000-0002-3012-0316</orcidid></search><sort><creationdate>20121108</creationdate><title>An Earth-mass planet orbiting α Centauri B</title><author>Dumusque, Xavier ; 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There are planets in the habitable zone of stars cooler than our Sun, but for reasons such as tidal locking and strong stellar activity, they are unlikely to harbour water–carbon life as we know it. The detection of a habitable Earth-mass planet orbiting a star similar to our Sun is extremely difficult, because such a signal is overwhelmed by stellar perturbations. Here we report the detection of an Earth-mass planet orbiting our neighbour star α Centauri B, a member of the closest stellar system to the Sun. The planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star (one astronomical unit is the Earth–Sun distance).
The detection of an Earth-mass planet orbiting our neighbour star α Centauri B is reported; the planet has an orbital period of 3.236 days and is about 0.04 astronomical units from the star.
A nearby Earth-mass exoplanet discovered
An exoplanet with an Earth-like mass has been discovered orbiting the nearby star α Centauri B. The planet is not in the habitable zone — it is much nearer to its star than we are to the Sun, orbiting at only about 0.04 astronomical units from its star (an astronomical unit is the mean distance between Earth and the Sun). Statistical studies suggest that low-mass planets form preferentially in multi-planet systems, so it is possible that other planets are orbiting α Centauri B, perhaps in its habitable zone.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>23075844</pmid><doi>10.1038/nature11572</doi><tpages>5</tpages><orcidid>https://orcid.org/0000-0002-7613-393X</orcidid><orcidid>https://orcid.org/0000-0003-4422-2919</orcidid><orcidid>https://orcid.org/0000-0001-7576-6236</orcidid><orcidid>https://orcid.org/0000-0003-2355-8034</orcidid><orcidid>https://orcid.org/0000-0001-7120-5837</orcidid><orcidid>https://orcid.org/0000-0002-3012-0316</orcidid></addata></record> |
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subjects | 639/33/34/862 Analysis Astronomical bodies Coolers Cosmic physics Extrasolar planets Harbours Humanities and Social Sciences multidisciplinary Observations Orbitals Orbits Planet detection Science Sciences of the Universe Spectra Stars Sun |
title | An Earth-mass planet orbiting α Centauri B |
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