Q84009415

Summary

Q84009415 is a Mira variable^[1].

Key Facts

• Q84009415's instance of is recorded as Mira variable^[2].
• Q84009415's instance of is recorded as infrared source^[3].
• Q84009415's instance of is recorded as long-period variable star^[4].
• Q84009415's instance of is recorded as near-infrared source^[5].
• Q84009415's constellation is recorded as Sagittarius^[6].
• Q84009415's spectral class is recorded as Me^[7].
• Q84009415's catalog code is recorded as IRAS 18502-2623^[8].
• Q84009415's catalog code is recorded as ASAS J185323-2620.2^[9].
• Q84009415's catalog code is recorded as 2MASS J18532358-2620122^[10].
• Q84009415's catalog code is recorded as GCRV 6385 E^[11].
• Q84009415's catalog code is recorded as WEB 16039^[12].
• Q84009415's catalog code is recorded as Gaia DR2 4073795657307645440^[13].
• Q84009415's catalog code is recorded as OP Sgr^[14].
• Q84009415's catalog code is recorded as TIC 90408648^[15].
• Q84009415's catalog code is recorded as Gaia DR3 4073795657307645440^[16].
• Q84009415's type of variable star is recorded as long-period variable star^[17].
• Q84009415's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.849'}^[18].
• Q84009415's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.746'}^[19].
• Q84009415's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.235'}^[20].
• Q84009415's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.980345'}^[21].
• Q84009415's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6829'}^[22].
• Q84009415's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+23.0'}^[23].
• Q84009415's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+283.34829342882'}^[24].
• Q84009415's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-26.33681227396'}^[25].
• Q84009415's epoch is recorded as J2000.0^[26].

Body

Definition and Type

Recorded instance of include Mira variable^[2], infrared source^[3], long-period variable star^[4], and near-infrared source^[5].