GARGANTUA

SUPERMASSIVE BLACK HOLE · 1.0 × 10⁸ M☉

SCHWARZSCHILD METRIC // NULL-GEODESIC RAYTRACING

MISSION ELAPSED

00:00:00

OBSERVER DISTANCE26.00 Rs

DISK INCLINATION6.0°

GRAV. TIME DILATION1.020 ×

GEODESIC STEPS280

RENDER PROFILECINEMATIC

FRAME RATE—

DISK INCLINATION 6°

DISK BRIGHTNESS 1.00

DOPPLER BEAMING 1.00

DISK OUTER RADIUS 12.0

DRAG ORBIT · SCROLL ZOOM · 1–4 VIEWS · C CINEMATIC · M SOUND · P PARAMS · H HUD

№ 02 — A DAINER.AI STUDY
RAW WEBGL2 · NO ENGINE · NO LIBRARIES
NO AUDIO FILES · SEE THE COLLECTION

GARGANTUA

Light does not travel straight here. Every photon you are about to see was integrated along a null geodesic through curved spacetime — bent, beamed and redshifted by a hundred million solar masses.
The sound is generated from that same physics. Headphones help.

This instrument needs WebGL2. Your browser or device did not provide a WebGL2 context, so the raytracer cannot run.

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