Q74000589
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Q74000589
Summary
Q74000589 is a high proper-motion star[1].
Key Facts
- Q74000589's instance of is recorded as high proper-motion star[2].
- Q74000589's instance of is recorded as near-infrared source[3].
- Q74000589's constellation is recorded as Andromeda[4].
- Q74000589's spectral class is recorded as M1.5V[5].
- Q74000589's catalog code is recorded as Karmn J23306+466[6].
- Q74000589's catalog code is recorded as LSPM J2330+4639[7].
- Q74000589's catalog code is recorded as Ci 20 1430[8].
- Q74000589's catalog code is recorded as LHS 5406[9].
- Q74000589's catalog code is recorded as LTT 16912[10].
- Q74000589's catalog code is recorded as NLTT 57076[11].
- Q74000589's catalog code is recorded as 2MASS J23304170+4639562[12].
- Q74000589's catalog code is recorded as UCAC4 684-128708[13].
- Q74000589's catalog code is recorded as PM J23306+4639[14].
- Q74000589's catalog code is recorded as Gaia DR2 1938475489813398400[15].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.7'}[16].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.967'}[17].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.362'}[18].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.124'}[19].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.948'}[20].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.738'}[21].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.643'}[22].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.658'}[23].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.4552'}[24].
- Q74000589's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.443639'}[25].
- Q74000589's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+24.7257'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2] and near-infrared source[3].