HD55540
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HD55540
Summary
HD55540 is a peculiar star[1].
Key Facts
- HD55540's instance of is recorded as peculiar star[2].
- HD55540's instance of is recorded as infrared source[3].
- HD55540's constellation is recorded as Canis Major[4].
- HD55540's spectral class is recorded as ApEuCr[5].
- HD55540's catalog code is recorded as HD 55540[6].
- HD55540's catalog code is recorded as GSC 05977-01025[7].
- HD55540's catalog code is recorded as 2MASS J07123042-2103537[8].
- HD55540's catalog code is recorded as PPM 251872[9].
- HD55540's catalog code is recorded as SAO 173199[10].
- HD55540's catalog code is recorded as YZ 110 2794[11].
- HD55540's catalog code is recorded as BD-20 1779[12].
- HD55540's catalog code is recorded as TYC 5977-1025-1[13].
- HD55540's catalog code is recorded as Gaia DR1 2928451638924970880[14].
- HD55540's catalog code is recorded as Gaia DR2 2928451643230872832[15].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.39'}[16].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.37'}[17].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3717'}[18].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.385'}[19].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.365'}[20].
- HD55540's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.391'}[21].
- HD55540's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.8200'}[22].
- HD55540's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+549.4505'}[23].
- HD55540's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+108.12676644845890'}[24].
- HD55540's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-21.06493759642760'}[25].
- HD55540's epoch is recorded as J2000.0[26].
Body
Definition and Type
Recorded instance of include peculiar star[2] and infrared source[3].