About: WOH G17

Property	Value
dbo:abstract	WOH G17 is a possible red supergiant (RSG) located in the Large Magellanic Cloud (LMC) or a Mira variable asymptotic giant branch (AGB) star in the constellation of Mensa. The star is often considered to be a foreground object; much closer than the LMC, probably in the Milky Way, and therefore is potentially much smaller and less luminous. As a red supergiant, it would be one of the largest known stars, with a luminosity of 933,000 L☉ and temperature of 3,300 K implying a radius of about 2,955 solar radii (2.056×109 km; 13.74 au), which is somewhat on par with the largest red supergiants known. This would correspond to a volume 25.8 billion times bigger than the Sun. If placed at the center of the Solar system its photosphere would engulf the orbit of Saturn and reach to about 3/4 the distance to Uranus’s orbit. (en)
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dbo:wikiPageLength	5265 (xsd:nonNegativeInteger)
dbo:wikiPageRevisionID	1122005934 (xsd:integer)
dbo:wikiPageWikiLink	dbr:Saturn dbr:Mira_variable dbr:List_of_largest_stars dbr:Uranus dbc:Asymptotic-giant-branch_stars dbc:IRAS_catalogue_objects dbc:M-type_supergiants dbc:TIC_objects dbr:Mensa_(constellation) dbr:Photosphere dbr:Stephenson_2-18 dbr:WOH_G64 dbr:Long-period_variable_star dbr:2MASS dbc:2MASS_objects dbc:Extragalactic_stars dbr:Asymptotic_giant_branch dbc:Mensa_(constellation) dbr:Large_Magellanic_Cloud dbr:Sun dbr:Red_supergiant dbc:Large_Magellanic_Cloud dbc:Mira_variables dbr:Solar_System dbr:IRAS dbr:Milky_Way dbr:Red_supergiant_star dbr:Semiregular_variable
dbp:appmag	5.520000 (xsd:double) 5.590000 (xsd:double) 6.920000 (xsd:double) 11.150000 (xsd:double)
dbp:appmag1Passband	K (en)
dbp:appmag2Passband	G (en)
dbp:appmag3Passband	H (en)
dbp:appmag4Passband	J (en)
dbp:appmagV	13.800000 (xsd:double)
dbp:class	M (en)
dbp:constell	dbr:Mensa_(constellation)
dbp:epoch	J2000 (en)
dbp:gravity	+0.5 (en)
dbp:luminosity	932967 (xsd:integer)
dbp:pError	0.043500 (xsd:double)
dbp:parallax	0.177300 (xsd:double)
dbp:propMoDec	7.034000 (xsd:double)
dbp:propMoRa	2.293000 (xsd:double)
dbp:radialV	101.213000 (xsd:double)
dbp:temperature	3300 (xsd:integer)
dbp:type	RSG or AGB (en)
dbp:variable	LPV (en)
dbp:wikiPageUsesTemplate	dbt:Convert dbt:Reflist dbt:Short_description dbt:Solar_luminosity dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_observe dbt:Starbox_reference dbt:Val dbt:DEC dbt:RA dbt:Stars_of_Mensa
dcterms:subject	dbc:Asymptotic-giant-branch_stars dbc:IRAS_catalogue_objects dbc:M-type_supergiants dbc:TIC_objects dbc:2MASS_objects dbc:Extragalactic_stars dbc:Mensa_(constellation) dbc:Large_Magellanic_Cloud dbc:Mira_variables
rdf:type	owl:Thing dbo:Place dbo:Location schema:Place dbo:CelestialBody dbo:Star
rdfs:comment	WOH G17 is a possible red supergiant (RSG) located in the Large Magellanic Cloud (LMC) or a Mira variable asymptotic giant branch (AGB) star in the constellation of Mensa. The star is often considered to be a foreground object; much closer than the LMC, probably in the Milky Way, and therefore is potentially much smaller and less luminous. (en)
rdfs:label	WOH G17 (en)
owl:sameAs	wikidata:WOH G17 https://global.dbpedia.org/id/C2w5S
prov:wasDerivedFrom	wikipedia-en:WOH_G17?oldid=1122005934&ns=0
foaf:isPrimaryTopicOf	wikipedia-en:WOH_G17
foaf:name	WOH G17 (en)
is dbo:wikiPageWikiLink of	dbr:WOH_G64 dbr:WOH_S264 dbr:WOH_S279 dbr:WOH_S281 dbr:IRAS_05280–6910
is foaf:primaryTopic of	wikipedia-en:WOH_G17