Q83247890

Summary

Q83247890 is a long-period variable star^[1].

Key Facts

• Q83247890's instance of is recorded as long-period variable star^[2].
• Q83247890's instance of is recorded as infrared source^[3].
• Q83247890's instance of is recorded as near-infrared source^[4].
• Q83247890's constellation is recorded as Ophiuchus^[5].
• Q83247890's spectral class is recorded as M4^[6].
• Q83247890's catalog code is recorded as BD+12 3429^[7].
• Q83247890's catalog code is recorded as IRAS 18112+1227^[8].
• Q83247890's catalog code is recorded as IRC +10352^[9].
• Q83247890's catalog code is recorded as RAFGL 5211S^[10].
• Q83247890's catalog code is recorded as 2MASS J18133316+1228036^[11].
• Q83247890's catalog code is recorded as Gaia DR2 4484878350264848000^[12].
• Q83247890's catalog code is recorded as V454 Oph^[13].
• Q83247890's catalog code is recorded as TYC 1017-648-1^[14].
• Q83247890's catalog code is recorded as TIC 166270801^[15].
• Q83247890's catalog code is recorded as Gaia DR3 4484878350264848000^[16].
• Q83247890's type of variable star is recorded as semiregular variable star^[17].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.85'}^[18].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.92'}^[19].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.58'}^[20].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.62'}^[21].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.58'}^[22].
• Q83247890's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.435482'}^[23].
• Q83247890's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5953'}^[24].
• Q83247890's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+0.72'}^[25].
• Q83247890's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+626.841'}^[26].

Body

Definition and Type

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