HD36138
peculiar star in the constellation Pictor
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HD36138
Summary
HD36138 is a peculiar star[1].
Key Facts
- HD36138's instance of is recorded as peculiar star[2].
- HD36138's constellation is recorded as Pictor[3].
- HD36138's spectral class is recorded as A1mA3-A7[4].
- HD36138's catalog code is recorded as HD 36138[5].
- HD36138's catalog code is recorded as CPC 20 1350[6].
- HD36138's catalog code is recorded as GCRV 2088 E[7].
- HD36138's catalog code is recorded as GSC 08526-01240[8].
- HD36138's catalog code is recorded as HIC 25423[9].
- HD36138's catalog code is recorded as HIP 25423[10].
- HD36138's catalog code is recorded as 2MASS J05261484-5638418[11].
- HD36138's catalog code is recorded as PPM 334346[12].
- HD36138's catalog code is recorded as SAO 233978[13].
- HD36138's catalog code is recorded as TYC 8526-1240-1[14].
- HD36138's catalog code is recorded as WEB 4927[15].
- HD36138's catalog code is recorded as Gaia DR2 4769361590784393344[16].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.62'}[17].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.46'}[18].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4480'}[19].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.200'}[20].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.196'}[21].
- HD36138's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.140'}[22].
- HD36138's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5227'}[23].
- HD36138's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.00'}[24].
- HD36138's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+396.4007'}[25].
- HD36138's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+81.56180234486490'}[26].
Body
Definition and Type
HD36138's instance of is recorded as peculiar star[2].