Q66649627
Press Enter · cited answer in seconds
0 sources
Q66649627
Summary
Q66649627 is a high proper-motion star[1].
Key Facts
- Q66649627's instance of is recorded as high proper-motion star[2].
- Q66649627's spectral class is recorded as G5[3].
- Q66649627's catalog code is recorded as HD 59555[4].
- Q66649627's catalog code is recorded as GSC 03406-01470[5].
- Q66649627's catalog code is recorded as HIC 36672[6].
- Q66649627's catalog code is recorded as HIP 36672[7].
- Q66649627's catalog code is recorded as 2MASS J07323992+4632054[8].
- Q66649627's catalog code is recorded as PPM 49941[9].
- Q66649627's catalog code is recorded as 1RXS J073239.5+463217[10].
- Q66649627's catalog code is recorded as SAO 41841[11].
- Q66649627's catalog code is recorded as uvby98 100059555[12].
- Q66649627's catalog code is recorded as AG+46 653[13].
- Q66649627's catalog code is recorded as BD+46 1277[14].
- Q66649627's catalog code is recorded as TYC 3406-1470-1[15].
- Q66649627's catalog code is recorded as Gaia DR1 975357351748144384[16].
- Q66649627's catalog code is recorded as Gaia DR2 975357356044685312[17].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.29'}[18].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.65'}[19].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.4707'}[20].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.425'}[21].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.155'}[22].
- Q66649627's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.082'}[23].
- Q66649627's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.7480'}[24].
- Q66649627's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-30.62'}[25].
- Q66649627's metallicity is recorded as {'unit': '1', 'amount': '-0.24'}[26].
Body
Definition and Type
Q66649627's instance of is recorded as high proper-motion star[2].