Q87865529
high proper-motion star in the constellation Libra
Press Enter · cited answer in seconds
0 sources
Q87865529
Summary
Q87865529 is a high proper-motion star[1].
Key Facts
- Q87865529's instance of is recorded as high proper-motion star[2].
- Q87865529's constellation is recorded as Libra[3].
- Q87865529's spectral class is recorded as G3V[4].
- Q87865529's catalog code is recorded as BD-22 3830[5].
- Q87865529's catalog code is recorded as CD-22 10611[6].
- Q87865529's catalog code is recorded as CPD-22 5820[7].
- Q87865529's catalog code is recorded as GSC 06746-00610[8].
- Q87865529's catalog code is recorded as HD 129320[9].
- Q87865529's catalog code is recorded as PPM 263281[10].
- Q87865529's catalog code is recorded as SAO 182785[11].
- Q87865529's catalog code is recorded as TYC 6746-610-1[12].
- Q87865529's catalog code is recorded as YZ 112 10572[13].
- Q87865529's catalog code is recorded as 2MASS J14422748-2246378[14].
- Q87865529's catalog code is recorded as RAVE J144227.5-224638[15].
- Q87865529's catalog code is recorded as Gaia DR1 6278660442022446592[16].
- Q87865529's catalog code is recorded as Gaia DR2 6278660446318233472[17].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.699'}[18].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.385'}[19].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.292'}[20].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.571'}[21].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.996'}[22].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.316'}[23].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.816'}[24].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.572'}[25].
- Q87865529's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.7649'}[26].
Body
Definition and Type
Q87865529's instance of is recorded as high proper-motion star[2].