Q88437914
star in the constellation Taurus
Press Enter · cited answer in seconds
0 sources
Q88437914
Summary
Q88437914 is a star[1].
Key Facts
- Q88437914's instance of is recorded as star[2].
- Q88437914's constellation is recorded as Taurus[3].
- Q88437914's spectral class is recorded as G5[4].
- Q88437914's catalog code is recorded as 2MASS J03343607+0713405[5].
- Q88437914's catalog code is recorded as AG+07 378[6].
- Q88437914's catalog code is recorded as BD+06 554[7].
- Q88437914's catalog code is recorded as GSC 00070-01270[8].
- Q88437914's catalog code is recorded as HD 22183[9].
- Q88437914's catalog code is recorded as PPM 146688[10].
- Q88437914's catalog code is recorded as SAO 111267[11].
- Q88437914's catalog code is recorded as TYC 70-1270-1[12].
- Q88437914's catalog code is recorded as YZ 7 1312[13].
- Q88437914's catalog code is recorded as Gaia DR1 3277871211551566720[14].
- Q88437914's catalog code is recorded as Gaia DR2 3277871211551566720[15].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.777'}[16].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.241'}[17].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.109'}[18].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.80'}[19].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.84'}[20].
- Q88437914's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.4659'}[21].
- Q88437914's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.4434'}[22].
- Q88437914's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.58'}[23].
- Q88437914's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+290.4106'}[24].
- Q88437914's SIMBAD ID is recorded as HD 22183[25].
- Q88437914's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+53.65036380818920'}[26].