Q83102201
high proper-motion star in the constellation Cetus
Press Enter · cited answer in seconds
0 sources
Q83102201
Summary
Q83102201 is a high proper-motion star[1].
Key Facts
- Q83102201's instance of is recorded as high proper-motion star[2].
- Q83102201's constellation is recorded as Cetus[3].
- Q83102201's spectral class is recorded as K0[4].
- Q83102201's catalog code is recorded as 2MASS J02080102-0458572[5].
- Q83102201's catalog code is recorded as BD-05 393[6].
- Q83102201's catalog code is recorded as GSC 04692-00577[7].
- Q83102201's catalog code is recorded as HIC 9946[8].
- Q83102201's catalog code is recorded as HIP 9946[9].
- Q83102201's catalog code is recorded as NLTT 7089[10].
- Q83102201's catalog code is recorded as PPM 184265[11].
- Q83102201's catalog code is recorded as SAO 129711[12].
- Q83102201's catalog code is recorded as TYC 4692-577-1[13].
- Q83102201's catalog code is recorded as YZ 95 507[14].
- Q83102201's catalog code is recorded as WISEA J020801.15-045855.6[15].
- Q83102201's catalog code is recorded as Gaia DR1 2491371886865667072[16].
- Q83102201's catalog code is recorded as Gaia DR2 2491371891160914688[17].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.190'}[18].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.832'}[19].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.788'}[20].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.43'}[21].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.12'}[22].
- Q83102201's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2823'}[23].
- Q83102201's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+15.6528'}[24].
- Q83102201's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.91'}[25].
- Q83102201's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+63.8863'}[26].