Q75155020
Mira variable star in the constellation Cygnus
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Q75155020
Summary
Q75155020 is a Mira variable[1].
Key Facts
- Q75155020's instance of is recorded as Mira variable[2].
- Q75155020's instance of is recorded as infrared source[3].
- Q75155020's instance of is recorded as long-period variable star[4].
- Q75155020's instance of is recorded as near-infrared source[5].
- Q75155020's constellation is recorded as Cygnus[6].
- Q75155020's spectral class is recorded as M7[7].
- Q75155020's catalog code is recorded as GSC 02673-04122[8].
- Q75155020's catalog code is recorded as IRAS 19536+3237[9].
- Q75155020's catalog code is recorded as IRC +30400[10].
- Q75155020's catalog code is recorded as RAFGL 5444S[11].
- Q75155020's catalog code is recorded as V468 Cyg[12].
- Q75155020's catalog code is recorded as 2MASS J19553815+3245338[13].
- Q75155020's catalog code is recorded as AAVSO 1951+32[14].
- Q75155020's catalog code is recorded as Gaia DR2 2034277140553486848[15].
- Q75155020's catalog code is recorded as TIC 87085603[16].
- Q75155020's catalog code is recorded as Gaia DR3 2034277144845873280[17].
- Q75155020's type of variable star is recorded as Mira variable[18].
- Q75155020's type of variable star is recorded as long-period variable star[19].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.098'}[20].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.969'}[21].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.470'}[22].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.04'}[23].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.02'}[24].
- Q75155020's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.758516'}[25].
- Q75155020's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1132'}[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].