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Statements

Subject Item
dbr:22_Camelopardalis
rdf:type
yago:CelestialBody109239740 yago:NaturalObject100019128 yago:PhysicalEntity100001930 dbo:Star dbo:Location dbo:CelestialBody dbo:Place yago:Whole100003553 schema:Place yago:WikicatF-typeMain-sequenceStars yago:Object100002684 yago:WikicatFlamsteedObjects owl:Thing yago:Star109444100
rdfs:label
22 Camelopardalis 22 Camelopardalis
rdfs:comment
22 Camelopardalis is a binary star system in the northern circumpolar constellation of Camelopardalis, located 212 light years away from the Sun. It has an apparent visual magnitude of 7.03, which is below the normal limit for visibility with the naked eye. This object is moving further from the Earth with a mean heliocentric radial velocity of +10 km/s. Eggen (1991) listed it as a member of the IC 2391 supercluster. It has also been catalogued as a member of the Hyades group. However, Griffin (2005) suggests it belongs to neither. 22 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna i den södra delen av stjärnbilden Giraffen. Den har en kombinerad skenbar magnitud på ca 7,03 och kräver åtminstone en fältkikare för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 15,4 mas, beräknas den befinna sig på ett avstånd på ca 212 ljusår (ca 65 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 10 km/s. Den listades av Eggen (1991) som en medlem av superhopen IC 2391 och har också blivit katalogiserad som ingående i Hyaderna, men båda fallen betvivlades emellertid av Griffin (2005).
dcterms:subject
dbc:Spectroscopic_binaries dbc:Camelopardalis_(constellation) dbc:Durchmusterung_objects dbc:F-type_main-sequence_stars dbc:Hipparcos_objects dbc:Flamsteed_objects dbc:Henry_Draper_Catalogue_objects
dbo:wikiPageID
4976784
dbo:wikiPageRevisionID
1030485825
dbo:wikiPageWikiLink
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owl:sameAs
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dbt:DEC dbt:Convert dbt:Reflist dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:Starbox_orbit dbt:Starbox_observe dbt:Starbox_reference dbt:Odlist dbt:Stars_of_Camelopardalis dbt:Short_description dbt:RA dbt:Val
dbp:absmagV
3.14
dbp:ageGyr
1.515
dbp:appmagV
7.03
dbp:class
F5 V
dbp:constell
dbr:Camelopardalis_(constellation)
dbp:epoch
dbr:J2000.0
dbp:gravity
4.26
dbp:luminosity
5.215
dbp:mass
1.34
dbp:metalFe
0.01
dbp:pError
0.1014
dbp:parallax
15.4048
dbp:propMoDec
−131.789
dbp:propMoRa
+10.514
dbp:radius
1.68
dbo:abstract
22 Camelopardalis, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna i den södra delen av stjärnbilden Giraffen. Den har en kombinerad skenbar magnitud på ca 7,03 och kräver åtminstone en fältkikare för att kunna observeras. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 15,4 mas, beräknas den befinna sig på ett avstånd på ca 212 ljusår (ca 65 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 10 km/s. Den listades av Eggen (1991) som en medlem av superhopen IC 2391 och har också blivit katalogiserad som ingående i Hyaderna, men båda fallen betvivlades emellertid av Griffin (2005). 22 Camelopardalis is a binary star system in the northern circumpolar constellation of Camelopardalis, located 212 light years away from the Sun. It has an apparent visual magnitude of 7.03, which is below the normal limit for visibility with the naked eye. This object is moving further from the Earth with a mean heliocentric radial velocity of +10 km/s. Eggen (1991) listed it as a member of the IC 2391 supercluster. It has also been catalogued as a member of the Hyades group. However, Griffin (2005) suggests it belongs to neither. This is a single-lined spectroscopic binary system with an orbital period of 81.5 days and a significant eccentricity of 0.14. It has an 'a sin i' value of 10.57 ± 0.27 Gm (0.0707 ± 0.0018 AU), where a is the semimajor axis and i is the orbital inclination to the line of sight from the Earth. This value provides a lower bound on the true semimajor axis of their orbit. The visible component is an F-type main-sequence star with a stellar classification of F5 V. It is an estimated 1.5 billion years old with 1.3 times the mass of the Sun and 1.7 times the Sun's radius. It is radiating 5.2 times the Sun's luminosity from its photosphere at an effective temperature of 6,732 K.
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dbr:Star
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