Q95268878
high proper-motion star in the constellation Vulpecula
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Q95268878
Summary
Q95268878 is a high proper-motion star[1].
Key Facts
- Q95268878's instance of is recorded as high proper-motion star[2].
- Q95268878's constellation is recorded as Vulpecula[3].
- Q95268878's spectral class is recorded as G5[4].
- Q95268878's catalog code is recorded as LSPM J1933+2331[5].
- Q95268878's catalog code is recorded as ASCC 803272[6].
- Q95268878's catalog code is recorded as UCAC2 40235783[7].
- Q95268878's catalog code is recorded as USNO-B1.0 1135-00387878[8].
- Q95268878's catalog code is recorded as GSC 02138-01581[9].
- Q95268878's catalog code is recorded as HD 344546[10].
- Q95268878's catalog code is recorded as HIC 96192[11].
- Q95268878's catalog code is recorded as HIP 96192[12].
- Q95268878's catalog code is recorded as LP 393-12[13].
- Q95268878's catalog code is recorded as NLTT 47941[14].
- Q95268878's catalog code is recorded as TYC 2138-1581-1[15].
- Q95268878's catalog code is recorded as 2MASS J19333473+2331483[16].
- Q95268878's catalog code is recorded as Gaia DR1 2019556810140986240[17].
- Q95268878's catalog code is recorded as Gaia DR2 2019556814492396544[18].
- Q95268878's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.732'}[19].
- Q95268878's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.354'}[20].
- Q95268878's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.253'}[21].
- Q95268878's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8'}[22].
- Q95268878's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.9274'}[23].
- Q95268878's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.5546'}[24].
- Q95268878's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.31'}[25].
- Q95268878's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+86.5456'}[26].
Body
Definition and Type
Q95268878's instance of is recorded as high proper-motion star[2].