Super-Luminous Astrophysics Lab: Breaking the Eddington Limit

Beaming Doppler Shift Factor

18.50x

Radiative Efficiency (η)

32.4%

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Physical Presets

System Parameters

Black Hole Mass (M☉) 1.70e+10 M☉

Central gravitational mass well (10^6 to 10^11 solar masses).

Mass Accretion Rate (M☉/yr) 410 M☉/yr

Infalling baryonic mass converted to photon radiation per year.

Kerr Spin Parameter (a*) 0.980

Dimensionless black hole angular momentum driving disk efficiency η.

Line-of-Sight Jet Angle (θ) 12°

Relativistic beaming angle between polar jet axis and Earth observer.

Radiation vs Gravity Balance

Hydrostatic Pressure Ratio L / L_Edd = 2.60

Sub-Eddington (Sub-Critical) 1.0 Limit Super-Eddington Outflow

Observed Telemetry

Apparent Solar Luminosity (L☉)

570 Billion L☉

3.828 × 10^26 W × 5.70e11

Milky Way Multiplier

20.4x Galaxy Output

vs 2.8 × 10^10 L☉ total MW

Eddington Ratio (L/L_Edd)

2.60

1.1 Solar Masses / day

Accretion Regime Status

Super-Eddington Accretion Phase (L/L_Edd = 2.6)

How Brightness Defies Classical Limits: Relativistic Doppler beaming boosts jet radiation along the line of sight by 18.5x. Furthermore, high spin (a* = 0.98) unlocks an accretion efficiency of 32.4%, allowing mass consumption of 410 M☉ / year to yield extreme brightness.

⚡ Astrophysical Telemetry Export