Q85426711
emission-line star in the constellation Mensa
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Q85426711
Summary
Q85426711 is an emission-line star[1].
Key Facts
- Q85426711's instance of is recorded as emission-line star[2].
- Q85426711's constellation is recorded as Mensa[3].
- Q85426711's spectral class is recorded as B1Ve[4].
- Q85426711's catalog code is recorded as [RP2006] 574[5].
- Q85426711's catalog code is recorded as UCAC4 098-010187[6].
- Q85426711's catalog code is recorded as [H2013] LMCe 1193[7].
- Q85426711's catalog code is recorded as Gaia DR2 4657131518426432640[8].
- Q85426711's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.255'}[9].
- Q85426711's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.970'}[10].
- Q85426711's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.825'}[11].
- Q85426711's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.470'}[12].
- Q85426711's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.8896'}[13].
- Q85426711's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0071'}[14].
- Q85426711's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+251'}[15].
- Q85426711's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+217'}[16].
- Q85426711's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.43506818125630'}[17].
- Q85426711's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-70.55589482570480'}[18].
- Q85426711's epoch is recorded as J2000.0[19].
- Q85426711's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.524'}[20].
- Q85426711's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+2.244'}[21].
Body
Definition and Type
Q85426711's instance of is recorded as emission-line star[2].