Q76924436
star in the constellation Leo
Press Enter · cited answer in seconds
0 sources
Q76924436
Summary
Q76924436 is a star[1].
Key Facts
- Q76924436's instance of is recorded as star[2].
- Q76924436's constellation is recorded as Leo[3].
- Q76924436's spectral class is recorded as K0[4].
- Q76924436's catalog code is recorded as AG+10 1434[5].
- Q76924436's catalog code is recorded as BD+11 2357[6].
- Q76924436's catalog code is recorded as GSC 00859-01142[7].
- Q76924436's catalog code is recorded as HD 99664[8].
- Q76924436's catalog code is recorded as HIC 55962[9].
- Q76924436's catalog code is recorded as HIP 55962[10].
- Q76924436's catalog code is recorded as PPM 128275[11].
- Q76924436's catalog code is recorded as SAO 99618[12].
- Q76924436's catalog code is recorded as TYC 859-1142-1[13].
- Q76924436's catalog code is recorded as YZ 10 4299[14].
- Q76924436's catalog code is recorded as 2MASS J11280486+1040178[15].
- Q76924436's catalog code is recorded as Gaia DR1 3915531914928511616[16].
- Q76924436's catalog code is recorded as Gaia DR2 3915531919223900416[17].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.561'}[18].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.053'}[19].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.954'}[20].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.26'}[21].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.25'}[22].
- Q76924436's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.9841'}[23].
- Q76924436's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.0925'}[24].
- Q76924436's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+32.20'}[25].
- Q76924436's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+323.3630'}[26].
Body
Definition and Type
Q76924436's instance of is recorded as star[2].