Q74975392
Press Enter · cited answer in seconds
0 sources
Q74975392
Summary
Q74975392 is a star[1].
Key Facts
- Q74975392's instance of is recorded as star[2].
- Q74975392's spectral class is recorded as G9IV[3].
- Q74975392's catalog code is recorded as AG+20 1407[4].
- Q74975392's catalog code is recorded as BD+20 2813[5].
- Q74975392's catalog code is recorded as GSC 01457-00785[6].
- Q74975392's catalog code is recorded as HD 115364[7].
- Q74975392's catalog code is recorded as HIC 64776[8].
- Q74975392's catalog code is recorded as HIP 64776[9].
- Q74975392's catalog code is recorded as PPM 102503[10].
- Q74975392's catalog code is recorded as SAO 82749[11].
- Q74975392's catalog code is recorded as TYC 1457-785-1[12].
- Q74975392's catalog code is recorded as YZ 20 4740[13].
- Q74975392's catalog code is recorded as 2MASS J13163083+2005528[14].
- Q74975392's catalog code is recorded as Gaia DR1 3940179838886742144[15].
- Q74975392's catalog code is recorded as Gaia DR2 3940179843182547072[16].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.83'}[17].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.225'}[18].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.733'}[19].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.661'}[20].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.71'}[21].
- Q74975392's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5944'}[22].
- Q74975392's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.9895'}[23].
- Q74975392's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-39.07'}[24].
- Q74975392's metallicity is recorded as {'unit': '1', 'amount': '-0.29'}[25].
- Q74975392's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+200.4209'}[26].
Body
Definition and Type
Q74975392's instance of is recorded as star[2].