Q91672402
high proper-motion star in the constellation Cassiopeia
Press Enter · cited answer in seconds
0 sources
Q91672402
Summary
Q91672402 is a high proper-motion star[1].
Key Facts
- Q91672402's instance of is recorded as high proper-motion star[2].
- Q91672402's constellation is recorded as Cassiopeia[3].
- Q91672402's spectral class is recorded as G5[4].
- Q91672402's catalog code is recorded as AG+63 98[5].
- Q91672402's catalog code is recorded as BD+62 201[6].
- Q91672402's catalog code is recorded as GSC 04021-01131[7].
- Q91672402's catalog code is recorded as HD 6522[8].
- Q91672402's catalog code is recorded as PPM 12737[9].
- Q91672402's catalog code is recorded as SAO 11582[10].
- Q91672402's catalog code is recorded as TYC 4021-1131-1[11].
- Q91672402's catalog code is recorded as uvby98 100006522[12].
- Q91672402's catalog code is recorded as 2MASS J01072603+6329597[13].
- Q91672402's catalog code is recorded as Gaia DR1 523323794876202112[14].
- Q91672402's catalog code is recorded as GEN# +1.00006522[15].
- Q91672402's catalog code is recorded as Gaia DR2 523323799178732032[16].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.37'}[17].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.645'}[18].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.231'}[19].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.147'}[20].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.12'}[21].
- Q91672402's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.0949'}[22].
- Q91672402's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.5682'}[23].
- Q91672402's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-31.58'}[24].
- Q91672402's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+280.2533'}[25].
- Q91672402's SIMBAD ID is recorded as HD 6522[26].