HD107526
star in the constellation Centaurus
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HD107526
Summary
HD107526 is a star[1].
Key Facts
- HD107526's instance of is recorded as star[2].
- HD107526's constellation is recorded as Centaurus[3].
- HD107526's spectral class is recorded as A5/7V(m)[4].
- HD107526's catalog code is recorded as HD 107526[5].
- HD107526's catalog code is recorded as GSC 08637-01228[6].
- HD107526's catalog code is recorded as 2MASS J12215007-5424009[7].
- HD107526's catalog code is recorded as SAO 239876[8].
- HD107526's catalog code is recorded as HIP 60296[9].
- HD107526's catalog code is recorded as CPC 19 4642[10].
- HD107526's catalog code is recorded as CPD-53 5092[11].
- HD107526's catalog code is recorded as HIC 60296[12].
- HD107526's catalog code is recorded as PPM 340913[13].
- HD107526's catalog code is recorded as TYC 8637-1228-1[14].
- HD107526's catalog code is recorded as Gaia DR2 6076246712214033408[15].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.36'}[16].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.11'}[17].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.0532'}[18].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.618'}[19].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.523'}[20].
- HD107526's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.514'}[21].
- HD107526's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4074'}[22].
- HD107526's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+415.3859'}[23].
- HD107526's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+185.45863460641420'}[24].
- HD107526's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-54.40026704664280'}[25].
- HD107526's epoch is recorded as J2000.0[26].
Body
Definition and Type
HD107526's instance of is recorded as star[2].