Q93210474
Mira variable star in the constellation Delphinus
Press Enter · cited answer in seconds
0 sources
Q93210474
Summary
Q93210474 is a Mira variable[1].
Key Facts
- Q93210474's instance of is recorded as Mira variable[2].
- Q93210474's instance of is recorded as OH/IR star[3].
- Q93210474's instance of is recorded as infrared source[4].
- Q93210474's instance of is recorded as long-period variable star[5].
- Q93210474's instance of is recorded as near-infrared source[6].
- Q93210474's constellation is recorded as Delphinus[7].
- Q93210474's spectral class is recorded as M8[8].
- Q93210474's catalog code is recorded as GCRV 71403[9].
- Q93210474's catalog code is recorded as IRAS 20440+0412[10].
- Q93210474's catalog code is recorded as [TVH89] 431[11].
- Q93210474's catalog code is recorded as 2MASS J20463316+0423364[12].
- Q93210474's catalog code is recorded as Gaia DR2 1735162531272902784[13].
- Q93210474's catalog code is recorded as BR Del[14].
- Q93210474's catalog code is recorded as AAVSO 2041+04[15].
- Q93210474's catalog code is recorded as TIC 393867767[16].
- Q93210474's catalog code is recorded as Gaia DR3 1735162531271418240[17].
- Q93210474's type of variable star is recorded as Mira variable[18].
- Q93210474's type of variable star is recorded as long-period variable star[19].
- Q93210474's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.82'}[20].
- Q93210474's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.72'}[21].
- Q93210474's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.29'}[22].
- Q93210474's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.619705'}[23].
- Q93210474's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3498'}[24].
- Q93210474's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-81.0'}[25].
- Q93210474's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+311.63814561986'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], OH/IR star[3], infrared source[4], long-period variable star[5], and near-infrared source[6].