Q80298543
carbon star in the constellation Eridanus
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Q80298543
Summary
Q80298543 is a carbon star[1].
Key Facts
- Q80298543's instance of is recorded as carbon star[2].
- Q80298543's constellation is recorded as Eridanus[3].
- Q80298543's spectral class is recorded as C[4].
- Q80298543's catalog code is recorded as 2MASS J04461089-1841396[5].
- Q80298543's catalog code is recorded as HE 0443-1847[6].
- Q80298543's catalog code is recorded as Gaia DR2 2977952442680871040[7].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.90'}[8].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.17'}[9].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.704'}[10].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.169'}[11].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.012'}[12].
- Q80298543's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4496'}[13].
- Q80298543's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4545'}[14].
- Q80298543's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.47'}[15].
- Q80298543's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2200.2200'}[16].
- Q80298543's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+71.54539510754650'}[17].
- Q80298543's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-18.69434203722830'}[18].
- Q80298543's epoch is recorded as J2000.0[19].
- Q80298543's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.114'}[20].
- Q80298543's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.487'}[21].
Body
Definition and Type
Q80298543's instance of is recorded as carbon star[2].