Q90940190
star in the constellation Leo
Press Enter · cited answer in seconds
0 sources
Q90940190
Summary
Q90940190 is a star[1].
Key Facts
- Q90940190's instance of is recorded as star[2].
- Q90940190's constellation is recorded as Leo[3].
- Q90940190's spectral class is recorded as K5[4].
- Q90940190's catalog code is recorded as AG+19 1044[5].
- Q90940190's catalog code is recorded as AGKR 9217[6].
- Q90940190's catalog code is recorded as BD+19 2321[7].
- Q90940190's catalog code is recorded as GSC 01422-00700[8].
- Q90940190's catalog code is recorded as HIC 50207[9].
- Q90940190's catalog code is recorded as HIP 50207[10].
- Q90940190's catalog code is recorded as PPM 127245[11].
- Q90940190's catalog code is recorded as SAO 99022[12].
- Q90940190's catalog code is recorded as TYC 1422-700-1[13].
- Q90940190's catalog code is recorded as YZ 19 4090[14].
- Q90940190's catalog code is recorded as 2MASS J10145910+1905535[15].
- Q90940190's catalog code is recorded as Gaia DR1 625034358520340224[16].
- Q90940190's catalog code is recorded as Gaia DR2 625034358520340224[17].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.320'}[18].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.824'}[19].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.686'}[20].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.27'}[21].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.31'}[22].
- Q90940190's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9174'}[23].
- Q90940190's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.9493'}[24].
- Q90940190's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.83'}[25].
- Q90940190's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+253.2094'}[26].
Body
Definition and Type
Q90940190's instance of is recorded as star[2].