Q85914675

Summary

Q85914675 is a carbon star^[1].

Key Facts

• Q85914675's instance of is recorded as carbon star^[2].
• Q85914675's instance of is recorded as infrared source^[3].
• Q85914675's instance of is recorded as long-period variable star^[4].
• Q85914675's instance of is recorded as near-infrared source^[5].
• Q85914675's instance of is recorded as spectroscopic binary^[6].
• Q85914675's constellation is recorded as Chamaeleon^[7].
• Q85914675's spectral class is recorded as C^[8].
• Q85914675's catalog code is recorded as CGCS 2967^[9].
• Q85914675's catalog code is recorded as IRAS 11065-8131^[10].
• Q85914675's catalog code is recorded as 2MASS J11072122-8147364^[11].
• Q85914675's catalog code is recorded as Gaia DR1 5197686683370693120^[12].
• Q85914675's catalog code is recorded as Gaia DR2 5197686687668124160^[13].
• Q85914675's catalog code is recorded as CI Cha^[14].
• Q85914675's catalog code is recorded as TYC 9422-908-1^[15].
• Q85914675's catalog code is recorded as TIC 395009792^[16].
• Q85914675's catalog code is recorded as Gaia DR3 5197686687668124160^[17].
• Q85914675's type of variable star is recorded as long-period variable star^[18].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.01'}^[19].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.43'}^[20].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.555'}^[21].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.190'}^[22].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.528'}^[23].
• Q85914675's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.368615'}^[24].
• Q85914675's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.8557'}^[25].
• Q85914675's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1168.634'}^[26].

Body

Definition and Type

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