Q84210902

Summary

Q84210902 is an Orion variable^[1].

Key Facts

• Q84210902's instance of is recorded as Orion variable^[2].
• Q84210902's instance of is recorded as near-infrared source^[3].
• Q84210902's instance of is recorded as variable star^[4].
• Q84210902's instance of is recorded as astrophysical X-ray source^[5].
• Q84210902's instance of is recorded as young stellar object^[6].
• Q84210902's constellation is recorded as Orion^[7].
• Q84210902's spectral class is recorded as M4.5^[8].
• Q84210902's catalog code is recorded as 2MASS J05344791-0535438^[9].
• Q84210902's catalog code is recorded as [AD95] 379^[10].
• Q84210902's catalog code is recorded as [DRS2009] 970^[11].
• Q84210902's catalog code is recorded as Gaia DR2 3017263148767891456^[12].
• Q84210902's catalog code is recorded as V2034 Ori^[13].
• Q84210902's catalog code is recorded as TIC 427373752^[14].
• Q84210902's catalog code is recorded as Gaia DR3 3017263148767891456^[15].
• Q84210902's type of variable star is recorded as T Tauri-type star^[16].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+21.323'}^[17].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.76'}^[18].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.113'}^[19].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.860'}^[20].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.075'}^[21].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.08'}^[22].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.646'}^[23].
• Q84210902's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.150848'}^[24].
• Q84210902's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.7018'}^[25].
• Q84210902's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+28.1161'}^[26].

Body

Definition and Type

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