Q80680969
star in the constellation Auriga
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Q80680969
Summary
Q80680969 is a star[1].
Key Facts
- Q80680969's instance of is recorded as star[2].
- Q80680969's constellation is recorded as Auriga[3].
- Q80680969's spectral class is recorded as F8[4].
- Q80680969's catalog code is recorded as AG+48 628[5].
- Q80680969's catalog code is recorded as BD+48 1394[6].
- Q80680969's catalog code is recorded as GSC 03380-00251[7].
- Q80680969's catalog code is recorded as PPM 49105[8].
- Q80680969's catalog code is recorded as SAO 41139[9].
- Q80680969's catalog code is recorded as TYC 3380-251-1[10].
- Q80680969's catalog code is recorded as Gaia DR1 967586999995209216[11].
- Q80680969's catalog code is recorded as Gaia DR2 967587004292313856[12].
- Q80680969's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.46'}[13].
- Q80680969's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.02'}[14].
- Q80680969's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3485'}[15].
- Q80680969's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.7923'}[16].
- Q80680969's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+31.95'}[17].
- Q80680969's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+172.6430'}[18].
- Q80680969's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+97.76369300258900'}[19].
- Q80680969's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.61414087880160'}[20].
- Q80680969's epoch is recorded as J2000.0[21].
- Q80680969's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-35.667'}[22].
- Q80680969's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.986'}[23].
Body
Definition and Type
Q80680969's instance of is recorded as star[2].