Q75781311

Summary

Q75781311 is a high proper-motion star^[1].

Key Facts

• Q75781311's instance of is recorded as high proper-motion star^[2].
• Q75781311's instance of is recorded as spectroscopic binary^[3].
• Q75781311's constellation is recorded as Boötes^[4].
• Q75781311's spectral class is recorded as M1.65^[5].
• Q75781311's catalog code is recorded as LSPM J1456+1648^[6].
• Q75781311's catalog code is recorded as NLTT 38848^[7].
• Q75781311's catalog code is recorded as 2MASS J14562809+1648342^[8].
• Q75781311's catalog code is recorded as G 136-35^[9].
• Q75781311's catalog code is recorded as USNO-B1.0 1068-00263899^[10].
• Q75781311's catalog code is recorded as WISEA J145628.13+164830.7^[11].
• Q75781311's catalog code is recorded as UCAC4 535-056841^[12].
• Q75781311's catalog code is recorded as PM J14564+1648W^[13].
• Q75781311's catalog code is recorded as Gaia DR2 1188044308340155648^[14].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.7'}^[15].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.752'}^[16].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.896'}^[17].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.583'}^[18].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.688'}^[19].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.960'}^[20].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.328'}^[21].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.077'}^[22].
• Q75781311's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.3249'}^[23].
• Q75781311's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+22.7442'}^[24].
• Q75781311's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+18.557'}^[25].
• Q75781311's metallicity is recorded as {'unit': '1', 'amount': '+0.11'}^[26].

Body

Definition and Type

Recorded instance of include high proper-motion star^[2] and spectroscopic binary^[3].