Q79621810
long period variable
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Q79621810
Summary
Q79621810 is a long-period variable star[1].
Key Facts
- Q79621810's instance of is recorded as long-period variable star[2].
- Q79621810's instance of is recorded as carbon star[3].
- Q79621810's instance of is recorded as near-infrared source[4].
- Q79621810's constellation is recorded as Centaurus[5].
- Q79621810's spectral class is recorded as M5[6].
- Q79621810's catalog code is recorded as CGCS 3100[7].
- Q79621810's catalog code is recorded as ASAS J114613-5704.1[8].
- Q79621810's catalog code is recorded as UCAC3 66-162235[9].
- Q79621810's catalog code is recorded as UCAC4 165-077819[10].
- Q79621810's catalog code is recorded as 2MASS J11461303-5704045[11].
- Q79621810's catalog code is recorded as Gaia DR2 5342227524214437376[12].
- Q79621810's catalog code is recorded as V1236 Cen[13].
- Q79621810's catalog code is recorded as Gaia DR3 5342227524214437376[14].
- Q79621810's catalog code is recorded as TIC 268033664[15].
- Q79621810's type of variable star is recorded as long-period variable star[16].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.36'}[17].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.20'}[18].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.76'}[19].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.974'}[20].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.04'}[21].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.672'}[22].
- Q79621810's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.143246'}[23].
- Q79621810's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2877'}[24].
- Q79621810's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.60'}[25].
- Q79621810's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3475.843'}[26].