Q92903050
high proper-motion star in the constellation Aquarius
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Q92903050
Summary
Q92903050 is a high proper-motion star[1].
Key Facts
- Q92903050's instance of is recorded as high proper-motion star[2].
- Q92903050's constellation is recorded as Aquarius[3].
- Q92903050's spectral class is recorded as M3.5[4].
- Q92903050's catalog code is recorded as 2MASS J22132883-1444538[5].
- Q92903050's catalog code is recorded as GJ 4263[6].
- Q92903050's catalog code is recorded as LTT 8914[7].
- Q92903050's catalog code is recorded as [RHG95] 3488[8].
- Q92903050's catalog code is recorded as NLTT 53230[9].
- Q92903050's catalog code is recorded as Wolf 1556[10].
- Q92903050's catalog code is recorded as RAVE J221328.8-144454[11].
- Q92903050's catalog code is recorded as WISEA J221328.57-144457.3[12].
- Q92903050's catalog code is recorded as UCAC4 377-171567[13].
- Q92903050's catalog code is recorded as PM J22134-1444E[14].
- Q92903050's catalog code is recorded as Gaia DR2 2599823487582145024[15].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.790'}[16].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.449'}[17].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.819'}[18].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.531'}[19].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.336'}[20].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.051'}[21].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.005'}[22].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.735'}[23].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.412'}[24].
- Q92903050's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.1683'}[25].
- Q92903050's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+31.8982'}[26].
Body
Definition and Type
Q92903050's instance of is recorded as high proper-motion star[2].