Q89004520
high proper-motion star in the constellation Taurus
Press Enter · cited answer in seconds
0 sources
Q89004520
Summary
Q89004520 is a high proper-motion star[1].
Key Facts
- Q89004520's instance of is recorded as high proper-motion star[2].
- Q89004520's constellation is recorded as Taurus[3].
- Q89004520's spectral class is recorded as G5[4].
- Q89004520's catalog code is recorded as LP 301-76[5].
- Q89004520's catalog code is recorded as 2MASS J04072963+2835214[6].
- Q89004520's catalog code is recorded as LSPM J0407+2835[7].
- Q89004520's catalog code is recorded as ASCC 658690[8].
- Q89004520's catalog code is recorded as UCAC2 41838371[9].
- Q89004520's catalog code is recorded as USNO-B1.0 1185-00051845[10].
- Q89004520's catalog code is recorded as BD+28 621[11].
- Q89004520's catalog code is recorded as GSC 01826-01400[12].
- Q89004520's catalog code is recorded as HD 283364[13].
- Q89004520's catalog code is recorded as TYC 1826-1400-1[14].
- Q89004520's catalog code is recorded as Gaia DR1 163958933416099712[15].
- Q89004520's catalog code is recorded as Gaia DR2 163958937714783872[16].
- Q89004520's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.729'}[17].
- Q89004520's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.378'}[18].
- Q89004520's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.286'}[19].
- Q89004520's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.6'}[20].
- Q89004520's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.9097'}[21].
- Q89004520's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.5451'}[22].
- Q89004520's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+62.03'}[23].
- Q89004520's metallicity is recorded as {'unit': '1', 'amount': '-0.08'}[24].
- Q89004520's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+86.6168'}[25].
- Q89004520's SIMBAD ID is recorded as HD 283364[26].