Q83744913
high proper-motion star in the constellation Dorado
Press Enter · cited answer in seconds
0 sources
Q83744913
Summary
Q83744913 is a high proper-motion star[1].
Key Facts
- Q83744913's instance of is recorded as high proper-motion star[2].
- Q83744913's constellation is recorded as Dorado[3].
- Q83744913's spectral class is recorded as K0III[4].
- Q83744913's catalog code is recorded as 2MASS J04291336-5424249[5].
- Q83744913's catalog code is recorded as CD-54 871[6].
- Q83744913's catalog code is recorded as CPC 19 1372[7].
- Q83744913's catalog code is recorded as CPD-54 671[8].
- Q83744913's catalog code is recorded as GSC 08509-01719[9].
- Q83744913's catalog code is recorded as HD 28777[10].
- Q83744913's catalog code is recorded as HIC 20927[11].
- Q83744913's catalog code is recorded as HIP 20927[12].
- Q83744913's catalog code is recorded as PPM 333531[13].
- Q83744913's catalog code is recorded as SAO 233536[14].
- Q83744913's catalog code is recorded as TYC 8509-1719-1[15].
- Q83744913's catalog code is recorded as Gaia DR1 4779068624893749376[16].
- Q83744913's catalog code is recorded as Gaia DR2 4779068629189718016[17].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.139'}[18].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.555'}[19].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.460'}[20].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.01'}[21].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.13'}[22].
- Q83744913's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7119'}[23].
- Q83744913's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.3902'}[24].
- Q83744913's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+29.85'}[25].
- Q83744913's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+294.9678'}[26].