Q91501023
high proper-motion star in the constellation Hercules
Press Enter · cited answer in seconds
0 sources
Q91501023
Summary
Q91501023 is a high proper-motion star[1].
Key Facts
- Q91501023's instance of is recorded as high proper-motion star[2].
- Q91501023's constellation is recorded as Hercules[3].
- Q91501023's spectral class is recorded as G5[4].
- Q91501023's catalog code is recorded as AG+15 1843[5].
- Q91501023's catalog code is recorded as BD+15 3362[6].
- Q91501023's catalog code is recorded as GEN# +1.00165803[7].
- Q91501023's catalog code is recorded as GSC 01554-01067[8].
- Q91501023's catalog code is recorded as HD 165803[9].
- Q91501023's catalog code is recorded as PPM 134285[10].
- Q91501023's catalog code is recorded as SAO 103394[11].
- Q91501023's catalog code is recorded as TYC 1554-1067-1[12].
- Q91501023's catalog code is recorded as YZ 15 6606[13].
- Q91501023's catalog code is recorded as 2MASS J18071195+1541299[14].
- Q91501023's catalog code is recorded as Gaia DR1 4498899215162893056[15].
- Q91501023's catalog code is recorded as Gaia DR2 4498899219464393728[16].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.54'}[17].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.17'}[18].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.181'}[19].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.804'}[20].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.760'}[21].
- Q91501023's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3349'}[22].
- Q91501023's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+17.6843'}[23].
- Q91501023's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.52'}[24].
- Q91501023's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+56.5473'}[25].
- Q91501023's SIMBAD ID is recorded as HD 165803[26].