Q84205892
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Q84205892
Summary
Q84205892 is an Orion variable[1].
Key Facts
- Q84205892's instance of is recorded as Orion variable[2].
- Q84205892's instance of is recorded as eruptive variable star[3].
- Q84205892's instance of is recorded as near-infrared source[4].
- Q84205892's instance of is recorded as T Tauri-type star[5].
- Q84205892's instance of is recorded as astrophysical X-ray source[6].
- Q84205892's instance of is recorded as young stellar object candidate[7].
- Q84205892's constellation is recorded as Orion[8].
- Q84205892's spectral class is recorded as M1.6[9].
- Q84205892's catalog code is recorded as [FKP2017] 227[10].
- Q84205892's catalog code is recorded as 2MASS J05344514-0621072[11].
- Q84205892's catalog code is recorded as SDSS J053445.16-062107.2[12].
- Q84205892's catalog code is recorded as SOXS 69[13].
- Q84205892's catalog code is recorded as Gaia DR2 3017137770082812928[14].
- Q84205892's catalog code is recorded as V775 Ori[15].
- Q84205892's catalog code is recorded as TIC 388851064[16].
- Q84205892's catalog code is recorded as Gaia DR3 3017137770082812928[17].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.386'}[18].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.041'}[19].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+19.39'}[20].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.044'}[21].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.654'}[22].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.635'}[23].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.027'}[24].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.654'}[25].
- Q84205892's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.95'}[26].
Body
Definition and Type
Recorded instance of include Orion variable[2], eruptive variable star[3], near-infrared source[4], T Tauri-type star[5], astrophysical X-ray source[6], and young stellar object candidate[7].