Q77975264
star in the constellation Ursa Major
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Q77975264
Summary
Q77975264 is a star[1].
Key Facts
- Q77975264's instance of is recorded as star[2].
- Q77975264's constellation is recorded as Ursa Major[3].
- Q77975264's spectral class is recorded as sdA[4].
- Q77975264's catalog code is recorded as SDSS J101409.26+591753.0[5].
- Q77975264's catalog code is recorded as SDSS J101409.26+591753.3[6].
- Q77975264's catalog code is recorded as Gaia DR2 1046784719464709376[7].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.082'}[8].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.932'}[9].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.923'}[10].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.035'}[11].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.288'}[12].
- Q77975264's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.1263'}[13].
- Q77975264's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+159.5'}[14].
- Q77975264's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+153.53860512021910'}[15].
- Q77975264's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+59.29805887327720'}[16].
- Q77975264's epoch is recorded as J2000.0[17].
- Q77975264's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+8228'}[18].
- Q77975264's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+1816000'}[19].
- Q77975264's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.288'}[20].
- Q77975264's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.343'}[21].
Body
Definition and Type
Q77975264's instance of is recorded as star[2].