HD93731
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HD93731
Summary
HD93731 is a peculiar star[1].
Key Facts
- HD93731's instance of is recorded as peculiar star[2].
- HD93731's instance of is recorded as high proper-motion star[3].
- HD93731's constellation is recorded as Hydra[4].
- HD93731's spectral class is recorded as A3III(m)[5].
- HD93731's catalog code is recorded as HD 93731[6].
- HD93731's catalog code is recorded as GSC 06642-01326[7].
- HD93731's catalog code is recorded as HIC 52883[8].
- HD93731's catalog code is recorded as HIP 52883[9].
- HD93731's catalog code is recorded as 2MASS J10485764-2755041[10].
- HD93731's catalog code is recorded as PPM 258170[11].
- HD93731's catalog code is recorded as SAO 179248[12].
- HD93731's catalog code is recorded as uvby98 100093731[13].
- HD93731's catalog code is recorded as YZ 117 7125[14].
- HD93731's catalog code is recorded as TYC 6642-1326-1[15].
- HD93731's catalog code is recorded as Gaia DR2 5457287533378238848[16].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.17'}[17].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.93'}[18].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.8888'}[19].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.491'}[20].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.462'}[21].
- HD93731's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.384'}[22].
- HD93731's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.7455'}[23].
- HD93731's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+22.60'}[24].
- HD93731's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+148.2470'}[25].
- HD93731's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+162.24023456289560'}[26].
Body
Definition and Type
Recorded instance of include peculiar star[2] and high proper-motion star[3].