Q89101709
star in the constellation Libra
Press Enter · cited answer in seconds
0 sources
Q89101709
Summary
Q89101709 is a star[1].
Key Facts
- Q89101709's instance of is recorded as star[2].
- Q89101709's constellation is recorded as Libra[3].
- Q89101709's spectral class is recorded as A4V[4].
- Q89101709's catalog code is recorded as BD-16 4123[5].
- Q89101709's catalog code is recorded as GSC 06185-00885[6].
- Q89101709's catalog code is recorded as HD 139249[7].
- Q89101709's catalog code is recorded as HIC 76522[8].
- Q89101709's catalog code is recorded as HIP 76522[9].
- Q89101709's catalog code is recorded as PPM 230497[10].
- Q89101709's catalog code is recorded as SAO 159393[11].
- Q89101709's catalog code is recorded as SRS 13052[12].
- Q89101709's catalog code is recorded as TYC 6185-885-1[13].
- Q89101709's catalog code is recorded as YZ 106 5722[14].
- Q89101709's catalog code is recorded as 2MASS J15373992-1643528[15].
- Q89101709's catalog code is recorded as RAVE J153739.9-164353[16].
- Q89101709's catalog code is recorded as Gaia DR2 6261480474060306176[17].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.749'}[18].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.693'}[19].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.596'}[20].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.32'}[21].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.59'}[22].
- Q89101709's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.2660'}[23].
- Q89101709's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.1374'}[24].
- Q89101709's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.42'}[25].
- Q89101709's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+162.9354'}[26].
Body
Definition and Type
Q89101709's instance of is recorded as star[2].