Q75175470

Summary

Q75175470 is a high proper-motion star^[1].

Key Facts

• Q75175470's instance of is recorded as high proper-motion star^[2].
• Q75175470's spectral class is recorded as M4V^[3].
• Q75175470's catalog code is recorded as LSPM J0920+2643^[4].
• Q75175470's catalog code is recorded as UCAC2 41194031^[5].
• Q75175470's catalog code is recorded as USNO-B1.0 1167-00176400^[6].
• Q75175470's catalog code is recorded as GJ 3552^[7].
• Q75175470's catalog code is recorded as LHS 266^[8].
• Q75175470's catalog code is recorded as LP 313-42^[9].
• Q75175470's catalog code is recorded as NLTT 21489^[10].
• Q75175470's catalog code is recorded as USNO 714^[11].
• Q75175470's catalog code is recorded as [RHG95] 1476^[12].
• Q75175470's catalog code is recorded as 2MASS J09202188+2643434^[13].
• Q75175470's catalog code is recorded as PLX 2222.01^[14].
• Q75175470's catalog code is recorded as WISEA J092022.64+264337.2^[15].
• Q75175470's catalog code is recorded as Gaia DR2 694072869723271296^[16].
• Q75175470's type of variable star is recorded as rotating variable star^[17].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.48'}^[18].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.073'}^[19].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.571'}^[20].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.290'}^[21].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.5'}^[22].
• Q75175470's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1023'}^[23].
• Q75175470's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+53.1690'}^[24].
• Q75175470's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.1'}^[25].
• Q75175470's metallicity is recorded as {'unit': '1', 'amount': '-0.63'}^[26].

Body

Definition and Type

Q75175470's instance of is recorded as high proper-motion star^[2].