Q87264188
high proper-motion star in the constellation Cetus
Press Enter · cited answer in seconds
0 sources
Q87264188
Summary
Q87264188 is a high proper-motion star[1].
Key Facts
- Q87264188's instance of is recorded as high proper-motion star[2].
- Q87264188's constellation is recorded as Cetus[3].
- Q87264188's spectral class is recorded as G1V[4].
- Q87264188's catalog code is recorded as 2MASS J02035133-1427450[5].
- Q87264188's catalog code is recorded as BD-15 363[6].
- Q87264188's catalog code is recorded as GSC 05283-00989[7].
- Q87264188's catalog code is recorded as HD 12684[8].
- Q87264188's catalog code is recorded as HIC 9637[9].
- Q87264188's catalog code is recorded as HIP 9637[10].
- Q87264188's catalog code is recorded as PPM 211008[11].
- Q87264188's catalog code is recorded as SAO 148177[12].
- Q87264188's catalog code is recorded as TYC 5283-989-1[13].
- Q87264188's catalog code is recorded as YZ 104 531[14].
- Q87264188's catalog code is recorded as RAVE J020351.3-142745[15].
- Q87264188's catalog code is recorded as Gaia DR1 5148552635460095232[16].
- Q87264188's catalog code is recorded as Gaia DR2 5148552635460095232[17].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.288'}[18].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.029'}[19].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.919'}[20].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.001'}[21].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.547'}[22].
- Q87264188's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2423'}[23].
- Q87264188's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.1380'}[24].
- Q87264188's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.02'}[25].
- Q87264188's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+162.9195'}[26].