Q88966892

Summary

Q88966892 is a long-period variable star^[1].

Key Facts

• Q88966892's instance of is recorded as long-period variable star^[2].
• Q88966892's instance of is recorded as near-infrared source^[3].
• Q88966892's constellation is recorded as Scorpius^[4].
• Q88966892's catalog code is recorded as 2MASS J17355619-3428064^[5].
• Q88966892's catalog code is recorded as Gaia DR2 4053557943240169344^[6].
• Q88966892's catalog code is recorded as V489 Sco^[7].
• Q88966892's catalog code is recorded as Gaia DR3 4053557943240169344^[8].
• Q88966892's type of variable star is recorded as slow irregular variables of late spectral types^[9].
• Q88966892's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.018'}^[10].
• Q88966892's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.953'}^[11].
• Q88966892's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.518'}^[12].
• Q88966892's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.71694'}^[13].
• Q88966892's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3293'}^[14].
• Q88966892's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.22'}^[15].
• Q88966892's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3036.745'}^[16].
• Q88966892's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+263.98416300210994'}^[17].
• Q88966892's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-34.46845623762001'}^[18].
• Q88966892's epoch is recorded as J2000.0^[19].
• Q88966892's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.191'}^[20].
• Q88966892's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.184'}^[21].

Body

Definition and Type

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