Q88438080
star in the constellation Taurus
Press Enter · cited answer in seconds
0 sources
Q88438080
Summary
Q88438080 is a star[1].
Key Facts
- Q88438080's instance of is recorded as star[2].
- Q88438080's constellation is recorded as Taurus[3].
- Q88438080's spectral class is recorded as K0[4].
- Q88438080's catalog code is recorded as 2MASS J03441383+0941484[5].
- Q88438080's catalog code is recorded as AG+09 340[6].
- Q88438080's catalog code is recorded as AGKR 3295[7].
- Q88438080's catalog code is recorded as BD+09 477[8].
- Q88438080's catalog code is recorded as GSC 00657-00183[9].
- Q88438080's catalog code is recorded as HIC 17444[10].
- Q88438080's catalog code is recorded as HIP 17444[11].
- Q88438080's catalog code is recorded as PPM 146865[12].
- Q88438080's catalog code is recorded as SAO 111383[13].
- Q88438080's catalog code is recorded as TYC 657-183-1[14].
- Q88438080's catalog code is recorded as YZ 9 1372[15].
- Q88438080's catalog code is recorded as Gaia DR1 12015188190925696[16].
- Q88438080's catalog code is recorded as Gaia DR2 12015188190925696[17].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.37'}[18].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.76'}[19].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.851'}[20].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.176'}[21].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.968'}[22].
- Q88438080's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8964'}[23].
- Q88438080's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4063'}[24].
- Q88438080's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.19'}[25].
- Q88438080's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+711.0858'}[26].
Body
Definition and Type
Q88438080's instance of is recorded as star[2].