About: 17 Camelopardalis

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About: 17 Camelopardalis Goto Sponge NotDistinct Permalink

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17 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis, located roughly 960 light years away from the Sun. It is visible to the naked eye as a faint, red-hued star with an apparent visual magnitude of 5.44. This object is moving closer to the Earth with a heliocentric radial velocity of −20 km/s.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body yago:WikicatM-typeGiants yago:WikicatM-typeStars yago:Animal100015388 yago:CelestialBody109239740 yago:Giant101323781 yago:LivingThing100004258 yago:NaturalObject100019128 yago:Object100002684 yago:Organism100004475 yago:PhysicalEntity100001930 yago:WikicatHenryDraperCatalogueObjects yago:WikicatHipparcosObjects star yago:Star109444100 yago:Whole100003553
rdfs:label	17 Camelopardalis (en) 17 Camelopardalis (it) 17 Camelopardalis (sv) 鹿豹座17 (zh)
rdfs:comment	17 Camelopardalis (17 Cam) è una stella appartenente alla costellazione della Giraffa. (it) 17 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en ensam stjärna i den sydvästra delen av stjärnbilden Giraffen. Den har en genomsnittlig skenbar magnitud på ca 5,44 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 3,4 mas, beräknas den befinna sig på ett avstånd på ca 960 ljusår (ca 290 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -20 km/s. (sv) 鹿豹座17，又名BD+62 759，HD 35583、SAO 13518、HR 1802，是鹿豹座的一颗恒星，视星等为5.42，位于銀經149.08，銀緯15.46，其B1900.0坐标为赤經5h 20m 43.3s，赤緯+62° 15.46′ 1″。 (zh) 17 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis, located roughly 960 light years away from the Sun. It is visible to the naked eye as a faint, red-hued star with an apparent visual magnitude of 5.44. This object is moving closer to the Earth with a heliocentric radial velocity of −20 km/s. (en)
dcterms:subject	Bright Star Catalogue objects Camelopardalis (constellation) Durchmusterung objects Flamsteed objects Henry Draper Catalogue objects Hipparcos objects M-type giants Suspected variables
Wikipage page ID	19538773 (xsd:integer)
Wikipage revision ID	1115734603 (xsd:integer)
Link from a Wikipage to another Wikipage	Camelopardalis Camelopardalis (constellation) Stellar classification Bright Star Catalogue objects Camelopardalis (constellation) Durchmusterung objects Flamsteed objects Henry Draper Catalogue objects Hipparcos objects M-type giants Suspected variables Photosphere Effective temperature Light year Star Red giant Asymptotic giant branch Circumpolar constellation Apparent visual magnitude Radial velocity Variable star Sun's radius Luminosity of the Sun
sameAs	17 Camelopardalis 17 Camelopardalis 17 Camelopardalis 17 Camelopardalis 17 Camelopardalis 17 Camelopardalis 17 Camelopardalis 17 Camelopardalis
dbp:wikiPageUsesTemplate	dbt:Reflist dbt:Short_description 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:Stars_of_Camelopardalis dbt:Val dbt:DEC dbt:Odlist dbt:RA
absmag v	−1.85 (en)
appmag v	5.440000 (xsd:double)
class	M1IIIa (en)
constell	Camelopardalis (constellation)
epoch	J2000 (en)
gravity	0.150000 (xsd:double)
luminosity	3230 (xsd:integer)
mass	0.640000 (xsd:double)
p error	0.138000 (xsd:double)
parallax	3.042400 (xsd:double)
prop mo dec	−4.751 (en)
prop mo ra	−5.602 (en)
radius	100 (xsd:integer)
temperature	3852 (xsd:integer)
variable	suspected (en)
has abstract	17 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis, located roughly 960 light years away from the Sun. It is visible to the naked eye as a faint, red-hued star with an apparent visual magnitude of 5.44. This object is moving closer to the Earth with a heliocentric radial velocity of −20 km/s. This is an ageing red giant star, currently on the asymptotic giant branch, with a stellar classification of M1IIIa. It is a suspected small amplitude variable. The star has expanded to 100 times the Sun's radius and is radiating 3,230 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,852 K. (en)

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