Q66534158
Press Enter · cited answer in seconds
0 sources
Q66534158
Summary
Q66534158 is a star[1].
Key Facts
- Q66534158's instance of is recorded as star[2].
- Q66534158's spectral class is recorded as K0[3].
- Q66534158's catalog code is recorded as HD 58184[4].
- Q66534158's catalog code is recorded as GSC 04116-01773[5].
- Q66534158's catalog code is recorded as HIC 36306[6].
- Q66534158's catalog code is recorded as HIP 36306[7].
- Q66534158's catalog code is recorded as IRAS 07238+6158[8].
- Q66534158's catalog code is recorded as 2MASS J07282392+6152393[9].
- Q66534158's catalog code is recorded as PPM 16202[10].
- Q66534158's catalog code is recorded as SAO 14206[11].
- Q66534158's catalog code is recorded as AG+61 540[12].
- Q66534158's catalog code is recorded as BD+62 926[13].
- Q66534158's catalog code is recorded as TYC 4116-1773-1[14].
- Q66534158's catalog code is recorded as Gaia DR1 1087280729148344960[15].
- Q66534158's catalog code is recorded as Gaia DR2 1087280733444272000[16].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.51'}[17].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.35'}[18].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.0098'}[19].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.388'}[20].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.852'}[21].
- Q66534158's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.718'}[22].
- Q66534158's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.6076'}[23].
- Q66534158's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-0.23'}[24].
- Q66534158's metallicity is recorded as {'unit': '1', 'amount': '+0.30'}[25].
- Q66534158's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+131.4475'}[26].
Body
Definition and Type
Q66534158's instance of is recorded as star[2].