Q88604169
carbon star in the constellation Eridanus
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Q88604169
Summary
Q88604169 is a carbon star[1].
Key Facts
- Q88604169's instance of is recorded as carbon star[2].
- Q88604169's constellation is recorded as Eridanus[3].
- Q88604169's spectral class is recorded as C[4].
- Q88604169's catalog code is recorded as 2MASS J04194683-0506172[5].
- Q88604169's catalog code is recorded as HE 0417-0513[6].
- Q88604169's catalog code is recorded as Gaia DR2 3202598512371692800[7].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.70'}[8].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.01'}[9].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.169'}[10].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.524'}[11].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.386'}[12].
- Q88604169's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8504'}[13].
- Q88604169's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4310'}[14].
- Q88604169's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-30.53'}[15].
- Q88604169's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2320.1856'}[16].
- Q88604169's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+64.94513750601270'}[17].
- Q88604169's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-5.10478069798640'}[18].
- Q88604169's epoch is recorded as J2000.0[19].
- Q88604169's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.087'}[20].
- Q88604169's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.755'}[21].
Body
Definition and Type
Q88604169's instance of is recorded as carbon star[2].