Q91986071

Summary

Q91986071 is a Mira variable^[1].

Key Facts

• Q91986071's instance of is recorded as Mira variable^[2].
• Q91986071's instance of is recorded as infrared source^[3].
• Q91986071's instance of is recorded as long-period variable star^[4].
• Q91986071's instance of is recorded as near-infrared source^[5].
• Q91986071's constellation is recorded as Eridanus^[6].
• Q91986071's spectral class is recorded as M6/7^[7].
• Q91986071's catalog code is recorded as 2MASS J04552388-0655501^[8].
• Q91986071's catalog code is recorded as GCRV 55622^[9].
• Q91986071's catalog code is recorded as IRAS 04529-0700^[10].
• Q91986071's catalog code is recorded as ASAS J045524-0655.9^[11].
• Q91986071's catalog code is recorded as Gaia DR2 3187255102483809152^[12].
• Q91986071's catalog code is recorded as SX Eri^[13].
• Q91986071's catalog code is recorded as AAVSO 0450-07^[14].
• Q91986071's catalog code is recorded as TIC 9456747^[15].
• Q91986071's catalog code is recorded as Gaia DR3 3187255102483809152^[16].
• Q91986071's type of variable star is recorded as long-period variable star^[17].
• Q91986071's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.960'}^[18].
• Q91986071's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.136'}^[19].
• Q91986071's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.644'}^[20].
• Q91986071's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.727676'}^[21].
• Q91986071's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2776'}^[22].
• Q91986071's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+77.0'}^[23].
• Q91986071's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+73.84953810479'}^[24].
• Q91986071's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-6.93062876212'}^[25].
• Q91986071'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].