Q77593558
carbon star in the constellation Carina
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Q77593558
Summary
Q77593558 is a carbon star[1].
Key Facts
- Q77593558's instance of is recorded as carbon star[2].
- Q77593558's instance of is recorded as infrared source[3].
- Q77593558's instance of is recorded as long-period variable star[4].
- Q77593558's instance of is recorded as near-infrared source[5].
- Q77593558's constellation is recorded as Carina[6].
- Q77593558's spectral class is recorded as C[7].
- Q77593558's catalog code is recorded as CGCS 6426[8].
- Q77593558's catalog code is recorded as IRAS 10509-6036[9].
- Q77593558's catalog code is recorded as 2MASS J10525544-6052102[10].
- Q77593558's catalog code is recorded as Gaia DR2 5338192488354938752[11].
- Q77593558's catalog code is recorded as V755 Car[12].
- Q77593558's catalog code is recorded as TIC 465384707[13].
- Q77593558's catalog code is recorded as OGLE GD1369.18.00022[14].
- Q77593558's catalog code is recorded as OGLE GD-LPV-1386[15].
- Q77593558's catalog code is recorded as Gaia DR3 5338192488354938752[16].
- Q77593558's type of variable star is recorded as Mira variable[17].
- Q77593558's type of variable star is recorded as long-period variable star[18].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.68'}[19].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.93'}[20].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.673'}[21].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.178018'}[22].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.998'}[23].
- Q77593558's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.534'}[24].
- Q77593558's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1064'}[25].
- Q77593558's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+17.91'}[26].
Body
Definition and Type
Recorded instance of include carbon star[2], infrared source[3], long-period variable star[4], and near-infrared source[5].