Physics Simulation

GRAVITATIONAL WAVES

Interactive visualization of spacetime ripples from binary merger. Watch orbits shrink, see LIGO signals, and explore the physics of gravitational waves.

📡 Source Configuration

30 M☉
Solar masses (1 M☉ ≈ 1.989 × 10³¹ kg)
30 M☉
Solar masses
5000 km
Orbital distance (Schwarzschild radii)
2.0×
Time compression factor

Binary System

Top-down view

Spacetime Deformation

Test masses in GW field

LIGO Interferometer

Laser arm length difference

GW Strain Signal h(t)

Detected amplitude vs time (Chirp → Merger → Ringdown)

Live Statistics

Orbital Frequency
0.0 Hz
GW Frequency
0.0 Hz
Strain Amplitude
0.0 × 10⁻²¹
Separation
5000 km
Time to Merger
Energy Radiated
0 M☉c²
Orbital Speed (M1)
0 km/s
Orbital Period