Q86894990

Summary

Q86894990 is a long-period variable star^[1].

Key Facts

• Q86894990's instance of is recorded as long-period variable star^[2].
• Q86894990's instance of is recorded as near-infrared source^[3].
• Q86894990's constellation is recorded as Pisces^[4].
• Q86894990's spectral class is recorded as M0^[5].
• Q86894990's catalog code is recorded as 2MASS J00231864-0133344^[6].
• Q86894990's catalog code is recorded as GSC 04665-00921^[7].
• Q86894990's catalog code is recorded as HIC 1843^[8].
• Q86894990's catalog code is recorded as HIP 1843^[9].
• Q86894990's catalog code is recorded as PPM 174712^[10].
• Q86894990's catalog code is recorded as Gaia DR1 2541834316619460608^[11].
• Q86894990's catalog code is recorded as Gaia DR2 2541834320915645312^[12].
• Q86894990's catalog code is recorded as CC Psc^[13].
• Q86894990's catalog code is recorded as TYC 4665-921-1^[14].
• Q86894990's catalog code is recorded as TIC 284077894^[15].
• Q86894990's catalog code is recorded as Gaia DR3 2541834320915645312^[16].
• Q86894990's type of variable star is recorded as SRb semi-regular variable star^[17].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.417'}^[18].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.589'}^[19].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.302'}^[20].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.92'}^[21].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.63'}^[22].
• Q86894990's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.040562'}^[23].
• Q86894990's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5812'}^[24].
• Q86894990's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+16.76'}^[25].
• Q86894990's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1720.58'}^[26].

Body

Definition and Type

Recorded instance of include long-period variable star^[2] and near-infrared source^[3].