Q88363792
emission-line star in the constellation Taurus
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Q88363792
Summary
Q88363792 is an emission-line star[1].
Key Facts
- Q88363792's instance of is recorded as emission-line star[2].
- Q88363792's constellation is recorded as Taurus[3].
- Q88363792's spectral class is recorded as M6e[4].
- Q88363792's catalog code is recorded as 2MASS J05352830+2352238[5].
- Q88363792's catalog code is recorded as HBHA 2214-06[6].
- Q88363792's catalog code is recorded as [KW97] 23-30[7].
- Q88363792's catalog code is recorded as Gaia DR2 3404669370664947072[8].
- Q88363792's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.6'}[9].
- Q88363792's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.337'}[10].
- Q88363792's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.745'}[11].
- Q88363792's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.569'}[12].
- Q88363792's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.3536'}[13].
- Q88363792's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9165'}[14].
- Q88363792's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.31'}[15].
- Q88363792's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1091.1075'}[16].
- Q88363792's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.86796281499320'}[17].
- Q88363792's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+23.87326455027360'}[18].
- Q88363792's epoch is recorded as J2000.0[19].
- Q88363792's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.062'}[20].
- Q88363792's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.421'}[21].
Body
Definition and Type
Q88363792's instance of is recorded as emission-line star[2].