Q76842157
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Q76842157
Summary
Q76842157 is a T Tauri-type star[1].
Key Facts
- Q76842157's instance of is recorded as T Tauri-type star[2].
- Q76842157's constellation is recorded as Cepheus[3].
- Q76842157's spectral class is recorded as G1.5[4].
- Q76842157's catalog code is recorded as 2MASS J21360723+5734324[5].
- Q76842157's catalog code is recorded as [SHB2004] Trumpler 37 73-537[6].
- Q76842157's catalog code is recorded as Gaia DR2 2178446174630143360[7].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.05'}[8].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.30'}[9].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.27'}[10].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.25'}[11].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.16'}[12].
- Q76842157's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.3011'}[13].
- Q76842157's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1396'}[14].
- Q76842157's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-20.5'}[15].
- Q76842157's stellar rotational velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+11.7'}[16].
- Q76842157's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+324.03017373841910'}[17].
- Q76842157's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+57.57567536617310'}[18].
- Q76842157's epoch is recorded as J2000.0[19].
- Q76842157's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.658'}[20].
- Q76842157's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.047'}[21].
Body
Definition and Type
Q76842157's instance of is recorded as T Tauri-type star[2].