Q87531370

Summary

Q87531370 is a long-period variable star^[1].

Key Facts

• Q87531370's instance of is recorded as long-period variable star^[2].
• Q87531370's instance of is recorded as near-infrared source^[3].
• Q87531370's constellation is recorded as Ophiuchus^[4].
• Q87531370's catalog code is recorded as 2MASS J17382766+0346006^[5].
• Q87531370's catalog code is recorded as Gaia DR2 4377179704554189056^[6].
• Q87531370's catalog code is recorded as V798 Oph^[7].
• Q87531370's catalog code is recorded as TIC 349330996^[8].
• Q87531370's catalog code is recorded as Gaia DR3 4377179704554189056^[9].
• Q87531370's type of variable star is recorded as semiregular variable star^[10].
• Q87531370's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.925'}^[11].
• Q87531370's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.025'}^[12].
• Q87531370's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.681'}^[13].
• Q87531370's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.550674'}^[14].
• Q87531370's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4307'}^[15].
• Q87531370's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-35.59'}^[16].
• Q87531370's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2321.8'}^[17].
• Q87531370's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+264.61531148746'}^[18].
• Q87531370's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+3.76689058449'}^[19].
• Q87531370's epoch is recorded as J2000.0^[20].
• Q87531370's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.143'}^[21].
• Q87531370's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.381'}^[22].

Body

Definition and Type

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