Q84213041

Summary

Q84213041 is an Orion variable^[1].

Key Facts

• Q84213041's instance of is recorded as Orion variable^[2].
• Q84213041's instance of is recorded as near-infrared source^[3].
• Q84213041's instance of is recorded as variable star^[4].
• Q84213041's instance of is recorded as astrophysical X-ray source^[5].
• Q84213041's instance of is recorded as young stellar object candidate^[6].
• Q84213041's instance of is recorded as young stellar object^[7].
• Q84213041's constellation is recorded as Orion^[8].
• Q84213041's spectral class is recorded as M2.2e^[9].
• Q84213041 is part of NAME Orion Nebula Cluster^[10].
• Q84213041's catalog code is recorded as 2MASS J05335769-0540060^[11].
• Q84213041's catalog code is recorded as [DRS2009] 362^[12].
• Q84213041's catalog code is recorded as Gaia DR2 3017260022031719040^[13].
• Q84213041's catalog code is recorded as V1414 Ori^[14].
• Q84213041's catalog code is recorded as TIC 427333995^[15].
• Q84213041's catalog code is recorded as Gaia DR3 3017260022031719040^[16].
• Q84213041's type of variable star is recorded as Orion variable^[17].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.544'}^[18].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.198'}^[19].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.932'}^[20].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.852'}^[21].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.90'}^[22].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.631'}^[23].
• Q84213041's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.099239'}^[24].
• Q84213041's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5176'}^[25].
• Q84213041's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+30.52'}^[26].

Body

Definition and Type

Recorded instance of include Orion variable^[2], near-infrared source^[3], variable star^[4], astrophysical X-ray source^[5], young stellar object candidate^[6], and young stellar object^[7].

Use and Application

Q84213041 is part of NAME Orion Nebula Cluster^[10].