2M0437 b (original) (raw)
2M0437 b, or 2MASS J04372171+2651014 b, is an extrasolar planet that orbits the red dwarf of the pre-main sequence 2MASS J04372171+2651014, 418 light-years away in the constellation of Taurus. It is a gas giant, with a mass 4 times that of Jupiter. It is one of the few exoplanets directly imaged. The planet is of importance to astronomers as it challenges models of planet formation by nucleus accretion and disk instability.
| Property | Value |
|---|---|
| dbo:abstract | 2M0437 b, or 2MASS J04372171+2651014 b, is an extrasolar planet that orbits the red dwarf of the pre-main sequence 2MASS J04372171+2651014, 418 light-years away in the constellation of Taurus. It is a gas giant, with a mass 4 times that of Jupiter. It is one of the few exoplanets directly imaged. The planet is of importance to astronomers as it challenges models of planet formation by nucleus accretion and disk instability. (en) 2M0437 b es un planeta extrasolar que orbita la enana roja de la pre-secuencia principal a 418 años luz en la constelación de Tauro. Es un Gigante gaseoso, con una masa 4 veces superior a la de Júpiter. (es) 2MASS J04372171+2651014 b（2M0437b）とは、地球からおうし座の方向に約421光年離れた場所に存在しているスペクトル分類がM型の恒星 （2M0437） の周囲を公転している太陽系外惑星である。TIC 125843782 b等の別名も持つ。 (ja) |
| dbo:detectionMethod | Imaged |
| dbo:wikiPageID | 69330661 (xsd:integer) |
| dbo:wikiPageLength | 6150 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1123846979 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Subaru_Telescope dbc:Gas_giants dbr:Exoplanet dbc:Exoplanets_detected_by_direct_imaging dbr:Hawaii dbr:Taurus_(constellation) dbr:Red_dwarf |
| dbp:apsis | astron (en) |
| dbp:discovered | October 2021 (en) |
| dbp:discoverer | Gaidos et al. (en) |
| dbp:discoveryMethod | Imaged (en) |
| dbp:discoverySite | Subaru Telescope, Hawaii, USA (en) |
| dbp:extrasolarplanet | yes (en) |
| dbp:mass | ~4 (en) |
| dbp:name | 2 (xsd:integer) |
| dbp:singleTemperature | ~1400–1500 K (en) |
| dbp:wikiPageUsesTemplate | dbt:Convert dbt:Infobox_planet dbt:Jupiter_mass dbt:Reflist |
| dcterms:subject | dbc:Gas_giants dbc:Exoplanets_detected_by_direct_imaging |
| rdf:type | owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody wikidata:Q634 dbo:Planet |
| rdfs:comment | 2M0437 b, or 2MASS J04372171+2651014 b, is an extrasolar planet that orbits the red dwarf of the pre-main sequence 2MASS J04372171+2651014, 418 light-years away in the constellation of Taurus. It is a gas giant, with a mass 4 times that of Jupiter. It is one of the few exoplanets directly imaged. The planet is of importance to astronomers as it challenges models of planet formation by nucleus accretion and disk instability. (en) 2M0437 b es un planeta extrasolar que orbita la enana roja de la pre-secuencia principal a 418 años luz en la constelación de Tauro. Es un Gigante gaseoso, con una masa 4 veces superior a la de Júpiter. (es) 2MASS J04372171+2651014 b（2M0437b）とは、地球からおうし座の方向に約421光年離れた場所に存在しているスペクトル分類がM型の恒星 （2M0437） の周囲を公転している太陽系外惑星である。TIC 125843782 b等の別名も持つ。 (ja) |
| rdfs:label | 2M0437 b (en) 2MASS J04372171+2651014 b (es) 2MASS J04372171+2651014 b (ja) |
| owl:sameAs | wikidata:2M0437 b dbpedia-es:2M0437 b dbpedia-ja:2M0437 b https://global.dbpedia.org/id/G63Zp |
| prov:wasDerivedFrom | wikipedia-en:2M0437_b?oldid=1123846979&ns=0 |
| foaf:isPrimaryTopicOf | wikipedia-en:2M0437_b |
| foaf:name | 2M0437b (en) |
| is foaf:primaryTopic of | wikipedia-en:2M0437_b |