HD91303
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HD91303
Summary
HD91303 is a peculiar star[1].
Key Facts
- HD91303's instance of is recorded as peculiar star[2].
- HD91303's instance of is recorded as infrared source[3].
- HD91303's constellation is recorded as Vela[4].
- HD91303's spectral class is recorded as A1mA9-A9[5].
- HD91303's catalog code is recorded as HD 91303[6].
- HD91303's catalog code is recorded as CPC 0 8648[7].
- HD91303's catalog code is recorded as GSC 08197-01576[8].
- HD91303's catalog code is recorded as HIC 51537[9].
- HD91303's catalog code is recorded as HIP 51537[10].
- HD91303's catalog code is recorded as 2MASS J10313521-4527155[11].
- HD91303's catalog code is recorded as PPM 315438[12].
- HD91303's catalog code is recorded as SAO 222120[13].
- HD91303's catalog code is recorded as TYC 8197-1576-1[14].
- HD91303's catalog code is recorded as Gaia DR1 5367280923115641728[15].
- HD91303's catalog code is recorded as Gaia DR2 5367280927418045824[16].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.50'}[17].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.19'}[18].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1333'}[19].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.660'}[20].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.527'}[21].
- HD91303's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.506'}[22].
- HD91303's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.4222'}[23].
- HD91303's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+226.1318'}[24].
- HD91303's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+157.89669667268150'}[25].
- HD91303's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-45.45432638404340'}[26].
Body
Definition and Type
Recorded instance of include peculiar star[2] and infrared source[3].