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Statements

Subject Item
dbr:NR_Vulpeculae
rdf:type
dbo:Location dbo:Place owl:Thing dbo:Star dbo:CelestialBody schema:Place
rdfs:label
NR Vulpeculae 狐狸座NR NR Vulpeculae
rdfs:comment
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. 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。 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.
foaf:name
NR Vulpeculae
dbp:name
NR Vulpeculae
foaf:depiction
n8:NRVulLightCurve.png
dcterms:subject
dbc:Objects_with_variable_star_designations dbc:Slow_irregular_variables dbc:Vulpecula dbc:Henry_Draper_Catalogue_objects dbc:M-type_supergiants dbc:Durchmusterung_objects dbc:2MASS_objects dbc:K-type_supergiants dbc:IRAS_catalogue_objects
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54147053
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1089953508
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wikidata:Q25390181 dbpedia-zh:狐狸座NR n17:2PKxN dbpedia-fr:NR_Vulpeculae
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dbt:Starbox_reference dbt:Stars_of_Vulpecula dbt:Short_description dbt:Variable-star-stub dbt:Val dbt:RA dbt:Reflist dbt:DEC dbt:Supergiant-star-stub dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_catalogue dbt:Starbox_character dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_begin dbt:Starbox_astrometry
dbo:thumbnail
n8:NRVulLightCurve.png?width=300
dbp:appmagV
9.130000000000001
dbp:class
M1Ia
dbp:constell
dbr:Vulpecula_(constellation)
dbp:epoch
J2000
dbp:gravity
−0.13
dbp:luminosity
111000
dbp:mass
4.92
dbp:metalFe
+0.093
dbp:pError
0.0516
dbp:parallax
0.5633
dbp:radius
553
dbp:type
dbr:Red_supergiant
dbp:variable
dbr:Slow_irregular_variable
dbo:abstract
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). 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. 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。
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wikipedia-en:NR_Vulpeculae?oldid=1089953508&ns=0
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6187
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wikipedia-en:NR_Vulpeculae