3D Workspace
Home
Assets
Affiliate Program
Sign up/Log in
?
Upgrade
DCC Bridge
Anonymous1769053202
01-22 03:59
Model Name
gas giant 3d model
Tags
nature & environment
rendering
space
Prompt
Non-rotating (Schwarzschild) black hole: perfectly spherical – the event horizon is an ideal sphere with radius exactly the Schwarzschild radius (r_s = 2GM/c²) Rotating (Kerr) black hole: oblate (flattened at the poles, bulging at the equator) due to centrifugal effects from spin The faster the spin (higher a*), the more pronounced the oblateness – at near-extremal spin (a* ≈ 0.999), the horizon is significantly squashed Additional feature in Kerr: the ergosphere – an oblong/football-shaped region outside the horizon where spacetime is dragged so strongly that nothing can remain stationary - the horizon as a perfect void (zero albedo, absorb all light) with strong gravitational lensing distortion around it - Spinning BH: apply frame-dragging effects in particle/accretion disk simulation – asymmetric Doppler boosting (one side brighter/blueshifted) the horizon has no material properties; it's a mathematical boundary
Detailed Info
Related Models
Enter invite code
Enter invite code to get credits!
Anonymous1769053202
Anonymous1769053202