HD290634
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HD290634
Summary
HD290634 is a peculiar star[1].
Key Facts
- HD290634's instance of is recorded as peculiar star[2].
- HD290634's instance of is recorded as infrared source[3].
- HD290634's constellation is recorded as Orion[4].
- HD290634's spectral class is recorded as A0[5].
- HD290634's catalog code is recorded as HD 290634[6].
- HD290634's catalog code is recorded as GSC 00114-01937[7].
- HD290634's catalog code is recorded as 2MASS J05352345+0014213[8].
- HD290634's catalog code is recorded as TYC 114-1937-1[9].
- HD290634's catalog code is recorded as Gaia DR2 3220893423784483840[10].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7889'}[11].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.404'}[12].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.324'}[13].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.269'}[14].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.07'}[15].
- HD290634's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.83'}[16].
- HD290634's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.2659'}[17].
- HD290634's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+306.1943'}[18].
- HD290634's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.84771610111250'}[19].
- HD290634's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+0.23926480227730'}[20].
- HD290634's epoch is recorded as J2000.0[21].
- HD290634's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.600'}[22].
- HD290634's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.785'}[23].
Body
Definition and Type
Recorded instance of include peculiar star[2] and infrared source[3].