Q80591952
high proper-motion star in the constellation Leo
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Q80591952
Summary
Q80591952 is a high proper-motion star[1].
Key Facts
- Q80591952's instance of is recorded as high proper-motion star[2].
- Q80591952's constellation is recorded as Leo[3].
- Q80591952's spectral class is recorded as K3[4].
- Q80591952's child astronomical body is recorded as TOI-5720 b[5].
- Q80591952's catalog code is recorded as LSPM J1121+2516[6].
- Q80591952's catalog code is recorded as NLTT 27110[7].
- Q80591952's catalog code is recorded as ASCC 683374[8].
- Q80591952's catalog code is recorded as 2MASS J11211567+2516255[9].
- Q80591952's catalog code is recorded as USNO-B1.0 1152-00184840[10].
- Q80591952's catalog code is recorded as G 120-35[11].
- Q80591952's catalog code is recorded as LP 374-31[12].
- Q80591952's catalog code is recorded as LTT 13066[13].
- Q80591952's catalog code is recorded as WISEA J112115.38+251624.4[14].
- Q80591952's catalog code is recorded as Gaia DR2 3994047048130880384[15].
- Q80591952's catalog code is recorded as TOI-5720[16].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.123'}[17].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.485'}[18].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.288'}[19].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.59'}[20].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.6'}[21].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8215'}[22].
- Q80591952's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.8'}[23].
- Q80591952's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.38'}[24].
- Q80591952's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.38'}[25].
- Q80591952's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+27.8846'}[26].
Body
Definition and Type
Q80591952's instance of is recorded as high proper-motion star[2].