Q80122176
star in the constellation Eridanus
Press Enter · cited answer in seconds
0 sources
Q80122176
Summary
Q80122176 is a star[1].
Key Facts
- Q80122176's instance of is recorded as star[2].
- Q80122176's constellation is recorded as Eridanus[3].
- Q80122176's spectral class is recorded as K0III-IV[4].
- Q80122176's catalog code is recorded as 2MASS J05082155-0839474[5].
- Q80122176's catalog code is recorded as ADS 3722 B[6].
- Q80122176's catalog code is recorded as BD-08 1038[7].
- Q80122176's catalog code is recorded as CCDM J05083-0839B[8].
- Q80122176's catalog code is recorded as IDS 05036-0848 B[9].
- Q80122176's catalog code is recorded as PPM 187739[10].
- Q80122176's catalog code is recorded as SAO 131807[11].
- Q80122176's catalog code is recorded as YZ 98 1354[12].
- Q80122176's catalog code is recorded as WDS J05083-0840B[13].
- Q80122176's catalog code is recorded as Gaia DR2 3182907530429023872[14].
- Q80122176's catalog code is recorded as TYC 5330-1724-1[15].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8'}[16].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7'}[17].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.124'}[18].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.629'}[19].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.462'}[20].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6926'}[21].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.83'}[22].
- Q80122176's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.05'}[23].
- Q80122176's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.3351'}[24].
- Q80122176's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+74.96'}[25].
- Q80122176's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+428.2472'}[26].