Q78260899
star in the constellation Lyra
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Q78260899
Summary
Q78260899 is a star[1].
Key Facts
- Q78260899's instance of is recorded as star[2].
- Q78260899's constellation is recorded as Lyra[3].
- Q78260899's spectral class is recorded as F2[4].
- Q78260899's catalog code is recorded as AG+42 1589[5].
- Q78260899's catalog code is recorded as BD+42 3077[6].
- Q78260899's catalog code is recorded as GSC 03112-00071[7].
- Q78260899's catalog code is recorded as PPM 57127[8].
- Q78260899's catalog code is recorded as SAO 47489[9].
- Q78260899's catalog code is recorded as TYC 3112-71-1[10].
- Q78260899's catalog code is recorded as Gaia DR1 2111929908724377728[11].
- Q78260899's catalog code is recorded as Gaia DR2 2111929908724377728[12].
- Q78260899's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.18'}[13].
- Q78260899's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.63'}[14].
- Q78260899's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1440'}[15].
- Q78260899's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.9587'}[16].
- Q78260899's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-22.34'}[17].
- Q78260899's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+167.8218'}[18].
- Q78260899's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+276.52287848904580'}[19].
- Q78260899's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+42.98974603389010'}[20].
- Q78260899's epoch is recorded as J2000.0[21].
- Q78260899's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+28.704'}[22].
- Q78260899's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.181'}[23].
Body
Definition and Type
Q78260899's instance of is recorded as star[2].