Q79499842
high proper-motion star in the constellation Vulpecula
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Q79499842
Summary
Q79499842 is a high proper-motion star[1].
Key Facts
- Q79499842's instance of is recorded as high proper-motion star[2].
- Q79499842's constellation is recorded as Vulpecula[3].
- Q79499842's spectral class is recorded as G0[4].
- Q79499842's catalog code is recorded as AG+27 2351[5].
- Q79499842's catalog code is recorded as BD+26 4051[6].
- Q79499842's catalog code is recorded as GCRV 7790 E[7].
- Q79499842's catalog code is recorded as GSC 02180-01069[8].
- Q79499842's catalog code is recorded as HD 341397[9].
- Q79499842's catalog code is recorded as PPM 112305[10].
- Q79499842's catalog code is recorded as SAO 89381[11].
- Q79499842's catalog code is recorded as TYC 2180-1069-1[12].
- Q79499842's catalog code is recorded as YZ 27 12015[13].
- Q79499842's catalog code is recorded as 2MASS J21014681+2714497[14].
- Q79499842's catalog code is recorded as Gaia DR1 1845152447540434048[15].
- Q79499842's catalog code is recorded as WEB 18888[16].
- Q79499842's catalog code is recorded as Gaia DR2 1845152451841587328[17].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.677'}[18].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.436'}[19].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.373'}[20].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.82'}[21].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.43'}[22].
- Q79499842's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6683'}[23].
- Q79499842's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.7650'}[24].
- Q79499842's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-6.29'}[25].
- Q79499842's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+173.4605'}[26].
Body
Definition and Type
Q79499842's instance of is recorded as high proper-motion star[2].