NR Vulpeculae (original) (raw)
NR Vulpeculae is a red supergiant and irregular variable star in the constellation Vulpecula. It has an effective temperature around 4,000 K, a radius of 553 times larger than the sun, which means that if it were in the place of the Sun, its surface would reach beyond Mars's orbit. Consequently, NR Vulpeculae is also a luminous star, radiating 111,000 - 223,000 times as much energy as the sun. It is considered a likely member of the Vulpecula OB1 stellar association.
| Property | Value |
|---|---|
| dbo:abstract | NR Vulpeculae is a red supergiant and irregular variable star in the constellation Vulpecula. It has an effective temperature around 4,000 K, a radius of 553 times larger than the sun, which means that if it were in the place of the Sun, its surface would reach beyond Mars's orbit. Consequently, NR Vulpeculae is also a luminous star, radiating 111,000 - 223,000 times as much energy as the sun. It is considered a likely member of the Vulpecula OB1 stellar association. (en) NR Vulpeculae est une supergéante rouge de la constellation du Petit Renard. Elle possède une température de surface d'environ 4 000 K et son rayon est environ 550 fois plus grand que celui du Soleil ; cela signifie que si elle était placée dans le système solaire, sa surface s'étendrait au-delà de l'orbite de Mars. Par conséquent, NR Vulpeculae est également une étoile très lumineuse, étant 70 000 à 111 000 fois plus lumineuse que le Soleil. L'étoile est une variable irrégulière à longue période, dont la magnitude apparente varie entre 9,13 et 9,61. Elle est probablement membre de l'association stellaire (Vul OB1). (fr) 狐狸座NR是一颗位于狐狸座的红特超巨星，狐狸座NR属于慢不规则变星，并且是已知的最大恒星之一。 (zh) |
| dbo:thumbnail | wiki-commons:Special:FilePath/NRVulLightCurve.png?width=300 |
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| dbo:wikiPageLength | 6187 (xsd:nonNegativeInteger) |
| dbo:wikiPageRevisionID | 1089953508 (xsd:integer) |
| dbo:wikiPageWikiLink | dbr:Bonner_Durchmusterung dbr:All_Sky_Automated_Survey_for_SuperNovae dbr:Light_curve dbc:Durchmusterung_objects dbc:Henry_Draper_Catalogue_objects dbc:IRAS_catalogue_objects dbc:K-type_supergiants dbc:M-type_supergiants dbc:Objects_with_variable_star_designations dbc:Slow_irregular_variables dbc:Vulpecula dbr:Constellation dbr:Effective_temperature dbr:Henry_Draper_Catalogue dbr:Two-Micron_Sky_Survey dbr:USNO_CCD_Astrograph_Catalog dbr:Vulpecula dbr:Vulpecula_OB1 dbr:2MASS dbc:2MASS_objects dbr:Red_supergiant dbr:Mars dbr:Guide_Star_Catalog dbr:IRAS dbr:Tycho-2_Catalogue dbr:RAFGL dbr:Slow_irregular_variable dbr:Photometric_system dbr:Vulpecula_(constellation) dbr:Variable_star_designation dbr:Stellar_association dbr:AAVSO dbr:File:NRVulLightCurve.png |
| dbp:appmagV | 9.130000 (xsd:double) |
| dbp:class | M1Ia (en) |
| dbp:constell | dbr:Vulpecula_(constellation) |
| dbp:epoch | J2000 (en) |
| dbp:gravity | −0.13 (en) |
| dbp:luminosity | 111000 (xsd:integer) |
| dbp:mass | 4.920000 (xsd:double) |
| dbp:metalFe | +0.093 (en) |
| dbp:name | NR Vulpeculae (en) |
| dbp:pError | 0.051600 (xsd:double) |
| dbp:parallax | 0.563300 (xsd:double) |
| dbp:radius | 553 (xsd:integer) |
| dbp:type | dbr:Red_supergiant |
| dbp:variable | dbr:Slow_irregular_variable |
| dbp:wikiPageUsesTemplate | dbt:Reflist dbt:Short_description dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalogue dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_reference dbt:Stars_of_Vulpecula dbt:Supergiant-star-stub dbt:Val dbt:DEC dbt:RA dbt:Variable-star-stub |
| dcterms:subject | dbc:Durchmusterung_objects dbc:Henry_Draper_Catalogue_objects dbc:IRAS_catalogue_objects dbc:K-type_supergiants dbc:M-type_supergiants dbc:Objects_with_variable_star_designations dbc:Slow_irregular_variables dbc:Vulpecula dbc:2MASS_objects |
| rdf:type | owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody dbo:Star |
| rdfs:comment | NR Vulpeculae is a red supergiant and irregular variable star in the constellation Vulpecula. It has an effective temperature around 4,000 K, a radius of 553 times larger than the sun, which means that if it were in the place of the Sun, its surface would reach beyond Mars's orbit. Consequently, NR Vulpeculae is also a luminous star, radiating 111,000 - 223,000 times as much energy as the sun. It is considered a likely member of the Vulpecula OB1 stellar association. (en) 狐狸座NR是一颗位于狐狸座的红特超巨星，狐狸座NR属于慢不规则变星，并且是已知的最大恒星之一。 (zh) NR Vulpeculae est une supergéante rouge de la constellation du Petit Renard. Elle possède une température de surface d'environ 4 000 K et son rayon est environ 550 fois plus grand que celui du Soleil ; cela signifie que si elle était placée dans le système solaire, sa surface s'étendrait au-delà de l'orbite de Mars. Par conséquent, NR Vulpeculae est également une étoile très lumineuse, étant 70 000 à 111 000 fois plus lumineuse que le Soleil. (fr) |
| rdfs:label | NR Vulpeculae (fr) NR Vulpeculae (en) 狐狸座NR (zh) |
| owl:sameAs | wikidata:NR Vulpeculae dbpedia-fr:NR Vulpeculae dbpedia-zh:NR Vulpeculae https://global.dbpedia.org/id/2PKxN |
| prov:wasDerivedFrom | wikipedia-en:NR_Vulpeculae?oldid=1089953508&ns=0 |
| foaf:depiction | wiki-commons:Special:FilePath/NRVulLightCurve.png |
| foaf:isPrimaryTopicOf | wikipedia-en:NR_Vulpeculae |
| foaf:name | NR Vulpeculae (en) |
| is dbo:wikiPageDisambiguates of | dbr:NR |
| is dbo:wikiPageWikiLink of | dbr:NR |
| is foaf:primaryTopic of | wikipedia-en:NR_Vulpeculae |
