Q91069204
star in the constellation Draco
Press Enter · cited answer in seconds
0 sources
Q91069204
Summary
Q91069204 is a star[1].
Key Facts
- Q91069204's instance of is recorded as star[2].
- Q91069204's constellation is recorded as Draco[3].
- Q91069204's spectral class is recorded as K0[4].
- Q91069204's catalog code is recorded as 2MASS J18230163+8242215[5].
- Q91069204's catalog code is recorded as AG+82 530[6].
- Q91069204's catalog code is recorded as AGKR 16506[7].
- Q91069204's catalog code is recorded as BD+82 546[8].
- Q91069204's catalog code is recorded as GSC 04648-00162[9].
- Q91069204's catalog code is recorded as HD 172434[10].
- Q91069204's catalog code is recorded as HIC 90082[11].
- Q91069204's catalog code is recorded as HIP 90082[12].
- Q91069204's catalog code is recorded as PPM 3217[13].
- Q91069204's catalog code is recorded as SAO 3046[14].
- Q91069204's catalog code is recorded as TYC 4648-162-1[15].
- Q91069204's catalog code is recorded as Gaia DR1 2296610891111704448[16].
- Q91069204's catalog code is recorded as Gaia DR2 2296610891111704448[17].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.331'}[18].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.839'}[19].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.703'}[20].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.24'}[21].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.35'}[22].
- Q91069204's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.9390'}[23].
- Q91069204's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.4490'}[24].
- Q91069204's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.71'}[25].
- Q91069204's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+289.9391'}[26].
Body
Definition and Type
Q91069204's instance of is recorded as star[2].