Q88935505

Summary

Q88935505 is a Mira variable^[1].

Key Facts

• Q88935505's instance of is recorded as Mira variable^[2].
• Q88935505's instance of is recorded as infrared source^[3].
• Q88935505's instance of is recorded as long-period variable star^[4].
• Q88935505's instance of is recorded as near-infrared source^[5].
• Q88935505's constellation is recorded as Sagittarius^[6].
• Q88935505's spectral class is recorded as Me^[7].
• Q88935505's catalog code is recorded as ASAS J190838-3134.2^[8].
• Q88935505's catalog code is recorded as 2MASS J19083817-3134104^[9].
• Q88935505's catalog code is recorded as IRAS 19054-3138^[10].
• Q88935505's catalog code is recorded as GCRV 6492 E^[11].
• Q88935505's catalog code is recorded as WEB 16366^[12].
• Q88935505's catalog code is recorded as Gaia DR2 6757304624136703488^[13].
• Q88935505's catalog code is recorded as V338 Sgr^[14].
• Q88935505's catalog code is recorded as Gaia DR3 6757304624136703488^[15].
• Q88935505's catalog code is recorded as TIC 390996006^[16].
• Q88935505's type of variable star is recorded as long-period variable star^[17].
• Q88935505's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.829'}^[18].
• Q88935505's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.033'}^[19].
• Q88935505's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.593'}^[20].
• Q88935505's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.311275'}^[21].
• Q88935505's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1237'}^[22].
• Q88935505's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+118.0'}^[23].
• Q88935505's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+287.15910054693995'}^[24].
• Q88935505's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-31.56956669656001'}^[25].
• Q88935505'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].