Q94572079
star
Press Enter · cited answer in seconds
0 sources
Q94572079
Summary
Q94572079 is a star[1].
Key Facts
- Q94572079's instance of is recorded as star[2].
- Q94572079's constellation is recorded as Scorpius[3].
- Q94572079's spectral class is recorded as A2IV/V[4].
- Q94572079's catalog code is recorded as Braes 98[5].
- Q94572079's catalog code is recorded as CD-40 10789[6].
- Q94572079's catalog code is recorded as CPC 0 15371[7].
- Q94572079's catalog code is recorded as CPD-40 7538[8].
- Q94572079's catalog code is recorded as GSC 07872-01648[9].
- Q94572079's catalog code is recorded as HD 151643[10].
- Q94572079's catalog code is recorded as PPM 322256[11].
- Q94572079's catalog code is recorded as SAO 227291[12].
- Q94572079's catalog code is recorded as TYC 7872-1648-1[13].
- Q94572079's catalog code is recorded as 2MASS J16502964-4045333[14].
- Q94572079's catalog code is recorded as RAVE J165029.6-404533[15].
- Q94572079's catalog code is recorded as Gaia DR1 5969811817672170112[16].
- Q94572079's catalog code is recorded as Gaia DR2 5969811822023982848[17].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.855'}[18].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.815'}[19].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.750'}[20].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.37'}[21].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.53'}[22].
- Q94572079's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.3169'}[23].
- Q94572079's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5421'}[24].
- Q94572079's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-5.68'}[25].
- Q94572079's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+393.3756'}[26].
Body
Definition and Type
Q94572079's instance of is recorded as star[2].