Q76805887
high proper-motion star in the constellation Reticulum
Press Enter · cited answer in seconds
0 sources
Q76805887
Summary
Q76805887 is a high proper-motion star[1].
Key Facts
- Q76805887's instance of is recorded as high proper-motion star[2].
- Q76805887's constellation is recorded as Reticulum[3].
- Q76805887's spectral class is recorded as F6V[4].
- Q76805887's catalog code is recorded as 2MASS J03522894-6555327[5].
- Q76805887's catalog code is recorded as CD-66 195[6].
- Q76805887's catalog code is recorded as CPC 21 682[7].
- Q76805887's catalog code is recorded as CPD-66 225[8].
- Q76805887's catalog code is recorded as GSC 08874-01333[9].
- Q76805887's catalog code is recorded as HD 24814[10].
- Q76805887's catalog code is recorded as HIC 18121[11].
- Q76805887's catalog code is recorded as HIP 18121[12].
- Q76805887's catalog code is recorded as PPM 353769[13].
- Q76805887's catalog code is recorded as TYC 8874-1333-1[14].
- Q76805887's catalog code is recorded as RAVE J035229.0-655533[15].
- Q76805887's catalog code is recorded as Gaia DR1 4669601384671531008[16].
- Q76805887's catalog code is recorded as Gaia DR2 4669601388967902848[17].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.535'}[18].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.328'}[19].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.246'}[20].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.215'}[21].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.811'}[22].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.562'}[23].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.740'}[24].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.230'}[25].
- Q76805887's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3432'}[26].
Body
Definition and Type
Q76805887's instance of is recorded as high proper-motion star[2].