Q92122600
RR Lyrae variable star in the constellation Vela
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Q92122600
Summary
Q92122600 is a RR Lyrae variable[1].
Key Facts
- Q92122600's instance of is recorded as RR Lyrae variable[2].
- Q92122600's instance of is recorded as near-infrared source[3].
- Q92122600's instance of is recorded as variable star[4].
- Q92122600's constellation is recorded as Vela[5].
- Q92122600's spectral class is recorded as kA2hA5[6].
- Q92122600's catalog code is recorded as CSV 1647[7].
- Q92122600's catalog code is recorded as GCRV 61603[8].
- Q92122600's catalog code is recorded as GSC 07735-00975[9].
- Q92122600's catalog code is recorded as 2MASS J10460030-4359170[10].
- Q92122600's catalog code is recorded as CRTS J104600.5-435916[11].
- Q92122600's catalog code is recorded as Gaia DR1 5390917846133815040[12].
- Q92122600's catalog code is recorded as Gaia DR2 5390917850431396224[13].
- Q92122600's catalog code is recorded as FS Vel[14].
- Q92122600's catalog code is recorded as TYC 7735-975-1[15].
- Q92122600's catalog code is recorded as TIC 147022379[16].
- Q92122600's catalog code is recorded as Gaia DR3 5390917850431396224[17].
- Q92122600's type of variable star is recorded as RR Lyrae variable with asymmetric light curves[18].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.48'}[19].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.798'}[20].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.528'}[21].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.368'}[22].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.04'}[23].
- Q92122600's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.062923'}[24].
- Q92122600's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7592'}[25].
- Q92122600's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+286.46'}[26].
Body
Definition and Type
Recorded instance of include RR Lyrae variable[2], near-infrared source[3], and variable star[4].