Q84632290

Summary

Q84632290 is a S-type star^[1].

Key Facts

• Q84632290's instance of is recorded as S-type star^[2].
• Q84632290's instance of is recorded as carbon star^[3].
• Q84632290's instance of is recorded as infrared source^[4].
• Q84632290's instance of is recorded as long-period variable star^[5].
• Q84632290's instance of is recorded as near-infrared source^[6].
• Q84632290's constellation is recorded as Centaurus^[7].
• Q84632290's spectral class is recorded as S^[8].
• Q84632290's catalog code is recorded as GSC 08677-00117^[9].
• Q84632290's catalog code is recorded as IRAS 14069-5905^[10].
• Q84632290's catalog code is recorded as 2MASS J14103255-5919380^[11].
• Q84632290's catalog code is recorded as Gaia DR2 5867790577604855936^[12].
• Q84632290's catalog code is recorded as V335 Cen^[13].
• Q84632290's catalog code is recorded as Gaia DR3 5867790577604855936^[14].
• Q84632290's catalog code is recorded as TIC 210714096^[15].
• Q84632290's type of variable star is recorded as SRa semi-regular variable star^[16].
• Q84632290's type of variable star is recorded as Mira variable^[17].
• Q84632290's type of variable star is recorded as long-period variable star^[18].
• Q84632290's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.50'}^[19].
• Q84632290's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.591'}^[20].
• Q84632290's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.414'}^[21].
• Q84632290's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.992'}^[22].
• Q84632290's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.071148'}^[23].
• Q84632290's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6921'}^[24].
• Q84632290's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-32.43'}^[25].
• Q84632290's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1444.878'}^[26].

Body

Definition and Type

Recorded instance of include S-type star^[2], carbon star^[3], infrared source^[4], long-period variable star^[5], and near-infrared source^[6].