Q87035927
star in the constellation Taurus
Press Enter · cited answer in seconds
0 sources
Q87035927
Summary
Q87035927 is a star[1].
Key Facts
- Q87035927's instance of is recorded as star[2].
- Q87035927's constellation is recorded as Taurus[3].
- Q87035927's spectral class is recorded as F8[4].
- Q87035927's catalog code is recorded as 2MASS J04252702+2344179[5].
- Q87035927's catalog code is recorded as AG+23 404[6].
- Q87035927's catalog code is recorded as BD+23 689[7].
- Q87035927's catalog code is recorded as GSC 01816-00873[8].
- Q87035927's catalog code is recorded as HD 284421[9].
- Q87035927's catalog code is recorded as HIC 20644[10].
- Q87035927's catalog code is recorded as HIP 20644[11].
- Q87035927's catalog code is recorded as PPM 93508[12].
- Q87035927's catalog code is recorded as TYC 1816-873-1[13].
- Q87035927's catalog code is recorded as Gaia DR1 149221320075661056[14].
- Q87035927's catalog code is recorded as Gaia DR2 149221320075661056[15].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.64'}[16].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.35'}[17].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.264'}[18].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.960'}[19].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.846'}[20].
- Q87035927's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.5449'}[21].
- Q87035927's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.9431'}[22].
- Q87035927's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+58.30'}[23].
- Q87035927's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+253.6076'}[24].
- Q87035927's SIMBAD ID is recorded as HD 284421[25].
- Q87035927's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+66.36263631555260'}[26].