Q84218424
Press Enter · cited answer in seconds
0 sources
Q84218424
Summary
Q84218424 is a T Tauri-type star[1].
Key Facts
- Q84218424's instance of is recorded as T Tauri-type star[2].
- Q84218424's constellation is recorded as Orion[3].
- Q84218424's spectral class is recorded as M1.8[4].
- Q84218424 is part of Q84210325[5].
- Q84218424 is part of NAME Orion Nebula Cluster[6].
- Q84218424's catalog code is recorded as [FKP2017] 615[7].
- Q84218424's catalog code is recorded as 2MASS J05364753-0608203[8].
- Q84218424's catalog code is recorded as KKO 27[9].
- Q84218424's catalog code is recorded as SV* SVS 1886[10].
- Q84218424's catalog code is recorded as [CHS2001] 16879[11].
- Q84218424's catalog code is recorded as [FHM2008] F31-ap177[12].
- Q84218424's catalog code is recorded as [MGM2012] 1038[13].
- Q84218424's catalog code is recorded as [FKV2013] 82[14].
- Q84218424's catalog code is recorded as SDSS J053647.54-060820.4[15].
- Q84218424's catalog code is recorded as ESO-HA 1550[16].
- Q84218424's catalog code is recorded as Gaia DR2 3016980711716911488[17].
- Q84218424's catalog code is recorded as V991 Ori[18].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.1'}[19].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.797'}[20].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.322'}[21].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.93'}[22].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.655'}[23].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.219'}[24].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.066'}[25].
- Q84218424's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.379'}[26].
Body
Definition and Type
Q84218424's instance of is recorded as T Tauri-type star[2].
Use and Application
Part of include Q84210325[5], a molecular cloud[27] and NAME Orion Nebula Cluster[6], an open cluster[28].