V602 Carinae (original) (raw)
りゅうこつ座V602星は、太陽から約 1,977 パーセク離れたところにある 赤色超巨星で、半径は太陽の約1000倍以上あり、光度は太陽の約200,000倍あるとされている。この恒星はりゅうこつ座の中に位置しており、7.6等と9.2等の間を変光するSRC型の脈動変光星である。
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dbo:abstract | V602 Carinae (V602 Car, HD 97671) is a red supergiant and variable star of spectral type of M3 in the constellation Carina. It is one of largest known stars. In 2005, V602 Car was calculated to have a bolometric luminosity below 110,000 L☉ and a radius around 860 R☉ based on the assumption of an effective temperature of 3,550 K. A 2015 study derived a slightly higher bolometric luminosity of 138,000+66,000−45,000 L☉ based on the measured flux and an assumed distance, and a larger radius of 1,050±165 R☉ based on the measured angular diameter and luminosity. An effective temperature of 3,432±280 K was then calculated from the luminosity and radius. More recent measurements based on a Gaia Data Release 2 parallax of 0.4366±0.0698 mas gives a luminosity at 125,000–131,000 L☉ with a corresponding radius of 932 R☉ based on the same effective temperature derived in 2005. V602 Car has an estimated mass loss rate of 1.9×10−6 M☉ per year. An excess of emission at long wavelengths from this star, as well as a small amount of silicate emission, suggests that it may be enclosed by an extensive cloud of dust. V602 Car is a semiregular variable star with a maximum brightness range of magnitude 7.6 - 9.1 and a period of 635 or 672 days. Despite the large amplitude of variation, it was only named as a variable star in 2006. (en) りゅうこつ座V602星は、太陽から約 1,977 パーセク離れたところにある 赤色超巨星で、半径は太陽の約1000倍以上あり、光度は太陽の約200,000倍あるとされている。この恒星はりゅうこつ座の中に位置しており、7.6等と9.2等の間を変光するSRC型の脈動変光星である。 (ja) V602 Киля — красный сверхгигант, переменная звезда в созвездии Киля. (ru) |
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dbp:absmagV | –4.83 (en) |
dbp:appmagV | 8.390000 (xsd:double) (en) |
dbp:bV | +2.52 (en) |
dbp:caption | Location of V602 Car (en) |
dbp:class | M3 Ia-Iab (en) |
dbp:constell | dbr:Carina_(constellation) |
dbp:epoch | dbr:J2000.0 |
dbp:equinox | J2000.0 (en) |
dbp:luminosity | 125000 (xsd:integer) |
dbp:mass | 17.700000 (xsd:double) |
dbp:pError | 0.069800 (xsd:double) |
dbp:parallax | 0.436600 (xsd:double) |
dbp:propMoDec | 2.183000 (xsd:double) |
dbp:propMoRa | −5.425 (en) |
dbp:radius | 932 (xsd:integer) |
dbp:uB | +2.59 (en) |
dbp:variable | dbr:Semiregular_variable_star |
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gold:hypernym | dbr:Star |
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rdfs:comment | りゅうこつ座V602星は、太陽から約 1,977 パーセク離れたところにある 赤色超巨星で、半径は太陽の約1000倍以上あり、光度は太陽の約200,000倍あるとされている。この恒星はりゅうこつ座の中に位置しており、7.6等と9.2等の間を変光するSRC型の脈動変光星である。 (ja) V602 Киля — красный сверхгигант, переменная звезда в созвездии Киля. (ru) V602 Carinae (V602 Car, HD 97671) is a red supergiant and variable star of spectral type of M3 in the constellation Carina. It is one of largest known stars. In 2005, V602 Car was calculated to have a bolometric luminosity below 110,000 L☉ and a radius around 860 R☉ based on the assumption of an effective temperature of 3,550 K. A 2015 study derived a slightly higher bolometric luminosity of 138,000+66,000−45,000 L☉ based on the measured flux and an assumed distance, and a larger radius of 1,050±165 R☉ based on the measured angular diameter and luminosity. An effective temperature of 3,432±280 K was then calculated from the luminosity and radius. More recent measurements based on a Gaia Data Release 2 parallax of 0.4366±0.0698 mas gives a luminosity at 125,000–131,000 L☉ with a correspondi (en) |
rdfs:label | りゅうこつ座V602星 (ja) V602 Carinae (en) V602 Киля (ru) |
owl:sameAs | freebase:V602 Carinae yago-res:V602 Carinae wikidata:V602 Carinae dbpedia-he:V602 Carinae dbpedia-ja:V602 Carinae dbpedia-ru:V602 Carinae https://global.dbpedia.org/id/4hrXG |
prov:wasDerivedFrom | wikipedia-en:V602_Carinae?oldid=1073197198&ns=0 |
foaf:depiction | wiki-commons:Special:FilePath/Carina_constellation_map.svg wiki-commons:Special:FilePath/V602CarLightCurve.png |
foaf:isPrimaryTopicOf | wikipedia-en:V602_Carinae |
foaf:name | V602 Carinae (en) |
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is foaf:primaryTopic of | wikipedia-en:V602_Carinae |