Q76925145
star in the constellation Leo
Press Enter · cited answer in seconds
0 sources
Q76925145
Summary
Q76925145 is a star[1].
Key Facts
- Q76925145's instance of is recorded as star[2].
- Q76925145's constellation is recorded as Leo[3].
- Q76925145's spectral class is recorded as F5[4].
- Q76925145's catalog code is recorded as AG+11 1343[5].
- Q76925145's catalog code is recorded as BD+12 2353[6].
- Q76925145's catalog code is recorded as GSC 00860-00301[7].
- Q76925145's catalog code is recorded as HD 100871[8].
- Q76925145's catalog code is recorded as HIC 56636[9].
- Q76925145's catalog code is recorded as HIP 56636[10].
- Q76925145's catalog code is recorded as PPM 128400[11].
- Q76925145's catalog code is recorded as SAO 99693[12].
- Q76925145's catalog code is recorded as TYC 860-301-1[13].
- Q76925145's catalog code is recorded as YZ 11 4345[14].
- Q76925145's catalog code is recorded as 2MASS J11364269+1140113[15].
- Q76925145's catalog code is recorded as Gaia DR1 3916427157911605376[16].
- Q76925145's catalog code is recorded as Gaia DR2 3916427157911605376[17].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.156'}[18].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.025'}[19].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.003'}[20].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.93'}[21].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.29'}[22].
- Q76925145's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8394'}[23].
- Q76925145's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.1309'}[24].
- Q76925145's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.85'}[25].
- Q76925145's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+242.0780'}[26].
Body
Definition and Type
Q76925145's instance of is recorded as star[2].