Q87221446
star in the constellation Phoenix
Press Enter · cited answer in seconds
0 sources
Q87221446
Summary
Q87221446 is a star[1].
Key Facts
- Q87221446's instance of is recorded as star[2].
- Q87221446's constellation is recorded as Phoenix[3].
- Q87221446's spectral class is recorded as K3III[4].
- Q87221446's catalog code is recorded as CD-57 8875[5].
- Q87221446's catalog code is recorded as CPC 20 7575[6].
- Q87221446's catalog code is recorded as CPD-57 10351[7].
- Q87221446's catalog code is recorded as GSC 08836-00334[8].
- Q87221446's catalog code is recorded as HD 223237[9].
- Q87221446's catalog code is recorded as HIC 117378[10].
- Q87221446's catalog code is recorded as HIP 117378[11].
- Q87221446's catalog code is recorded as PPM 351407[12].
- Q87221446's catalog code is recorded as SAO 248022[13].
- Q87221446's catalog code is recorded as SRS 18290[14].
- Q87221446's catalog code is recorded as TYC 8836-334-1[15].
- Q87221446's catalog code is recorded as 2MASS J23475867-5711270[16].
- Q87221446's catalog code is recorded as Gaia DR2 6495102574420609408[17].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.662'}[18].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.024'}[19].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.823'}[20].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.92'}[21].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.27'}[22].
- Q87221446's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5172'}[23].
- Q87221446's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.4271'}[24].
- Q87221446's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.48'}[25].
- Q87221446's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+412.0143'}[26].
Body
Definition and Type
Q87221446's instance of is recorded as star[2].