Q87226722
classical Cepheid variable star in the constellation Serpens
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Q87226722
Summary
Q87226722 is a classical Cepheid variable[1].
Key Facts
- Q87226722's instance of is recorded as classical Cepheid variable[2].
- Q87226722's instance of is recorded as infrared source[3].
- Q87226722's instance of is recorded as near-infrared source[4].
- Q87226722's instance of is recorded as variable star[5].
- Q87226722's constellation is recorded as Serpens[6].
- Q87226722's spectral class is recorded as K5[7].
- Q87226722's catalog code is recorded as GCRV 11130[8].
- Q87226722's catalog code is recorded as IRAS 18387-0109[9].
- Q87226722's catalog code is recorded as 2MASS J18412175-0106403[10].
- Q87226722's catalog code is recorded as WEB 15760[11].
- Q87226722's catalog code is recorded as Gaia DR2 4260210878780635904[12].
- Q87226722's catalog code is recorded as AA Ser[13].
- Q87226722's catalog code is recorded as ASAS J184122-0106.7[14].
- Q87226722's catalog code is recorded as TIC 179892079[15].
- Q87226722's catalog code is recorded as Gaia DR3 4260210878780635904[16].
- Q87226722's type of variable star is recorded as classical Cepheid variable[17].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.54'}[18].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.572'}[19].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.544'}[20].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.722'}[21].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.326'}[22].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.081848'}[23].
- Q87226722's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.09'}[24].
- Q87226722's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2408'}[25].
- Q87226722's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-55.16'}[26].
Body
Definition and Type
Recorded instance of include classical Cepheid variable[2], infrared source[3], near-infrared source[4], and variable star[5].