Q88435753
RR Lyrae variable star in the constellation Aries
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Q88435753
Summary
Q88435753 is a RR Lyrae variable[1].
Key Facts
- Q88435753's instance of is recorded as RR Lyrae variable[2].
- Q88435753's instance of is recorded as near-infrared source[3].
- Q88435753's constellation is recorded as Aries[4].
- Q88435753's spectral class is recorded as B8[5].
- Q88435753's catalog code is recorded as 2MASS J02160372+1731590[6].
- Q88435753's catalog code is recorded as GCRV 1252[7].
- Q88435753's catalog code is recorded as GSC 01217-01508[8].
- Q88435753's catalog code is recorded as UCAC3 216-9084[9].
- Q88435753's catalog code is recorded as CRTS J021603.7+173159[10].
- Q88435753's catalog code is recorded as Gaia DR1 80556921999940096[11].
- Q88435753's catalog code is recorded as WEB 2223[12].
- Q88435753's catalog code is recorded as Gaia DR2 80556926295542528[13].
- Q88435753's catalog code is recorded as RW Ari[14].
- Q88435753's catalog code is recorded as TYC 1217-1508-1[15].
- Q88435753's catalog code is recorded as TIC 408568560[16].
- Q88435753's catalog code is recorded as Gaia DR3 80556926295542528[17].
- Q88435753's type of variable star is recorded as RR Lyrae variables with nearly symmetric light curves[18].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.496'}[19].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.237'}[20].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.215'}[21].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.51'}[22].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.47'}[23].
- Q88435753's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.173477'}[24].
- Q88435753's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.487'}[25].
- Q88435753's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-54.15'}[26].
Body
Definition and Type
Recorded instance of include RR Lyrae variable[2] and near-infrared source[3].