Q95970979
high proper-motion star in the constellation Leo
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Q95970979
Summary
Q95970979 is a high proper-motion star[1].
Key Facts
- Q95970979's instance of is recorded as high proper-motion star[2].
- Q95970979's constellation is recorded as Leo[3].
- Q95970979's catalog code is recorded as LP 431-13 B[4].
- Q95970979's catalog code is recorded as Gaia DR2 3986730279283800704[5].
- Q95970979's catalog code is recorded as WDS J10476+2008B[6].
- Q95970979's catalog code is recorded as G 58-18B[7].
- Q95970979's catalog code is recorded as 2MASS J10473327+2007406[8].
- Q95970979's catalog code is recorded as USNO-B1.0 1101-00185878[9].
- Q95970979's catalog code is recorded as NLTT 25362[10].
- Q95970979's catalog code is recorded as LSPM J1047+2007E[11].
- Q95970979's catalog code is recorded as UCAC4 551-048607[12].
- Q95970979's catalog code is recorded as PM J10475+2007E[13].
- Q95970979's type of variable star is recorded as rotating variable star[14].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.602'}[15].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.844'}[16].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.439'}[17].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.96'}[18].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.2850'}[19].
- Q95970979's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.6'}[20].
- Q95970979's metallicity is recorded as {'unit': '1', 'amount': '+0.0'}[21].
- Q95970979's SIMBAD ID is recorded as G 58-18B[22].
- Q95970979's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.00'}[23].
- Q95970979's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+161.8885092000'}[24].
- Q95970979's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+20.1276767000'}[25].
- Q95970979's epoch is recorded as J2000.0[26].