HD32262
peculiar star in the constellation Orion
Press Enter · cited answer in seconds
0 sources
HD32262
Summary
HD32262 is a peculiar star[1].
Key Facts
- HD32262's instance of is recorded as peculiar star[2].
- HD32262's constellation is recorded as Orion[3].
- HD32262's spectral class is recorded as A2/3mA8-F2/3[4].
- HD32262's catalog code is recorded as HD 32262[5].
- HD32262's catalog code is recorded as GSC 00102-01178[6].
- HD32262's catalog code is recorded as HIC 23417[7].
- HD32262's catalog code is recorded as HIP 23417[8].
- HD32262's catalog code is recorded as 2MASS J05015838+0203514[9].
- HD32262's catalog code is recorded as PPM 148336[10].
- HD32262's catalog code is recorded as SAO 112339[11].
- HD32262's catalog code is recorded as YZ 1 1536[12].
- HD32262's catalog code is recorded as AG+01 516[13].
- HD32262's catalog code is recorded as BD+01 884[14].
- HD32262's catalog code is recorded as TYC 102-1178-1[15].
- HD32262's catalog code is recorded as Gaia DR1 3232047827513267712[16].
- HD32262's catalog code is recorded as Gaia DR2 3232047831810595200[17].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.73'}[18].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.33'}[19].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2385'}[20].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.602'}[21].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.551'}[22].
- HD32262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.461'}[23].
- HD32262's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.1692'}[24].
- HD32262's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+315.5370'}[25].
- HD32262's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+75.49328920053960'}[26].
Body
Definition and Type
HD32262's instance of is recorded as peculiar star[2].