GD 61 (original) (raw)
GD 61 est une naine blanche située à ∼175 a.l. (∼53,7 pc) de la Terre dans la constellation de Persée. Elle possède un système planétaire, dont un astéroïde qui contiendrait de l'eau. Il s'agit du premier astre extrasolaire sur lequel est détecté de l'eau sous forme solide ou liquide.
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| dbo:abstract | GD 61 is a white dwarf with a planetary system located 150 light-years from Earth in the constellation Perseus. It is thought to have been a main-sequence star of spectral type A0V with around three times the mass of the Sun that has aged and passed through a red-giant phase, leaving a dense, hot remnant that has around 70% of the Sun's mass and a surface temperature of 17,280 K. It is thought to be around 600 million years old, including both its life as a main-sequence star and as a white dwarf. It has an apparent magnitude of 14.8. GD 61 was first noted as a potential degenerate star in 1965, in a survey of white-dwarf suspects by astronomers from the Lowell Observatory in Arizona. In 2013, a circumstellar disk that resulted from the destruction of a water-rich asteroid was detected in close orbit around GD 61, which makes this the first detection of solid or liquid water on an extrasolar body. This asteroid would originally have been 26% water by mass, close to the water content of Ceres. This evidence suggests that a planet, with a rocky surface similar to Earth's, may have existed in the past, with the asteroid thus being an artifact from this period, now possibly part of a debris field from the hypothetical planet's breakup. Such a planet would have had both a rocky surface and water, two key ingredients for life. The researchers used the Cosmic Origins Spectrograph on the Hubble Space Telescope to determine the elemental composition. The elements magnesium, silicon, iron, and oxygen were detected, all components of rocky planets, although the levels of oxygen were much higher than what could be accounted for. The lack of associated carbon left only one candidate for the oxygen excess—water. (en) GD 61 est une naine blanche située à ∼175 a.l. (∼53,7 pc) de la Terre dans la constellation de Persée. Elle possède un système planétaire, dont un astéroïde qui contiendrait de l'eau. Il s'agit du premier astre extrasolaire sur lequel est détecté de l'eau sous forme solide ou liquide. (fr) GD 61 (WD 0435+410) es una enana blanca en la constelación de Perseo de magnitud aparente +14,80.Se encuentra a 52 pársecs (170 años luz) de distancia del Sistema Solar. (es) GD 61是一顆位於英仙座的有行星系統存在的白矮星，距離地球150光年。 (zh) |
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| dbo:wikiPageWikiLink | dbr:Perseus_(constellation) dbc:Astronomical_objects_discovered_in_2013 dbc:Perseus_(constellation) dbc:White_dwarfs dbr:Cosmic_Origins_Spectrograph dbr:Lowell_Observatory dbr:Ceres_(dwarf_planet) dbr:White_dwarf dbr:24_Themis dbr:Extraterrestrial_liquid_water dbr:Red_giant dbc:Astrobiology dbr:Wikt:extrasolar |
| dbp:ageMyr | 600 (xsd:integer) |
| dbp:appmagV | 14.800000 (xsd:double) |
| dbp:constell | dbr:Perseus_(constellation) |
| dbp:epoch | J2000 (en) |
| dbp:mass | 70.0 |
| dbp:temperature | 17280 (xsd:integer) |
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| dcterms:subject | dbc:Astronomical_objects_discovered_in_2013 dbc:Perseus_(constellation) dbc:White_dwarfs dbc:Astrobiology |
| gold:hypernym | dbr:Dwarf |
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| rdfs:comment | GD 61 est une naine blanche située à ∼175 a.l. (∼53,7 pc) de la Terre dans la constellation de Persée. Elle possède un système planétaire, dont un astéroïde qui contiendrait de l'eau. Il s'agit du premier astre extrasolaire sur lequel est détecté de l'eau sous forme solide ou liquide. (fr) GD 61 (WD 0435+410) es una enana blanca en la constelación de Perseo de magnitud aparente +14,80.Se encuentra a 52 pársecs (170 años luz) de distancia del Sistema Solar. (es) GD 61是一顆位於英仙座的有行星系統存在的白矮星，距離地球150光年。 (zh) GD 61 is a white dwarf with a planetary system located 150 light-years from Earth in the constellation Perseus. It is thought to have been a main-sequence star of spectral type A0V with around three times the mass of the Sun that has aged and passed through a red-giant phase, leaving a dense, hot remnant that has around 70% of the Sun's mass and a surface temperature of 17,280 K. It is thought to be around 600 million years old, including both its life as a main-sequence star and as a white dwarf. It has an apparent magnitude of 14.8. GD 61 was first noted as a potential degenerate star in 1965, in a survey of white-dwarf suspects by astronomers from the Lowell Observatory in Arizona. (en) |
| rdfs:label | GD 61 (es) GD 61 (en) GD 61 (fr) GD 61 (zh) |
| owl:sameAs | freebase:GD 61 yago-res:GD 61 wikidata:GD 61 http://ast.dbpedia.org/resource/GD_61 dbpedia-es:GD 61 dbpedia-fr:GD 61 dbpedia-simple:GD 61 http://ta.dbpedia.org/resource/ஜி.டி_61 dbpedia-zh:GD 61 https://global.dbpedia.org/id/4mwNT |
| prov:wasDerivedFrom | wikipedia-en:GD_61?oldid=1052595038&ns=0 |
| foaf:isPrimaryTopicOf | wikipedia-en:GD_61 |
| foaf:name | GD 61 (en) |
| is dbo:wikiPageWikiLink of | dbr:List_of_extrasolar_candidates_for_liquid_water dbr:Timeline_of_astronomy dbr:GD_40 dbr:Extraterrestrial_liquid_water dbr:Asteroid dbr:Extrasolar_object |
| is foaf:primaryTopic of | wikipedia-en:GD_61 |