Q78464698
high proper-motion star in the constellation Pegasus
Press Enter · cited answer in seconds
0 sources
Q78464698
Summary
Q78464698 is a high proper-motion star[1].
Key Facts
- Q78464698's instance of is recorded as high proper-motion star[2].
- Q78464698's constellation is recorded as Pegasus[3].
- Q78464698's spectral class is recorded as M2.5[4].
- Q78464698 is part of ** GIC 188[5].
- Q78464698's catalog code is recorded as LSPM J2306+1236N[6].
- Q78464698's catalog code is recorded as UCAC2 36395678[7].
- Q78464698's catalog code is recorded as 2MASS J23062530+1236570[8].
- Q78464698's catalog code is recorded as USNO-B1.0 1026-00760905[9].
- Q78464698's catalog code is recorded as CCDM J23064+1236B[10].
- Q78464698's catalog code is recorded as G 67-47[11].
- Q78464698's catalog code is recorded as IDS 23014+1203 B[12].
- Q78464698's catalog code is recorded as NLTT 55835[13].
- Q78464698's catalog code is recorded as [ZEH2003] RX J2306.4+1236 2[14].
- Q78464698's catalog code is recorded as WDS J23064+1235B[15].
- Q78464698's catalog code is recorded as UCAC3 206-309366[16].
- Q78464698's catalog code is recorded as UCAC3 206-309367[17].
- Q78464698's catalog code is recorded as UCAC4 514-140180[18].
- Q78464698's catalog code is recorded as WISEA J230625.57+123656.2[19].
- Q78464698's catalog code is recorded as Gaia DR2 2814796530710871424[20].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.97'}[21].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.351'}[22].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.779'}[23].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.524'}[24].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.89'}[25].
- Q78464698's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.0992'}[26].
Body
Definition and Type
Q78464698's instance of is recorded as high proper-motion star[2].
Use and Application
Q78464698 is part of ** GIC 188[5].