Explore
Styles
Features
Pricing
Sign in
Sign up
Sign up
Explore
Exploring the Supermassive Black Hole M87*: Gravity, Light, and Relativistic Jets
Remix
0
Share
Prompt
Scientific Context: M87* is a supermassive black hole (~6.5×10^9 M☉) at the core of galaxy M87, famous for the 2019 Event Horizon Telescope image of its shadow. Our animation should reflect known physics: intense gravity warps light into a ring, and a hot accretion disk of swirling plasma feeds the hole. Matter falling inward heats up and orbits at near-light speed, producing Doppler-brightened regions in the disk. Perpendicular to the disk, twin relativistic jets of plasma erupt from the poles. In M87 these jets extend thousands of light-years and travel at ≳0.8–0.9 c. They appear as narrow, collimated beams (often
Style
Grunge
art, cultural or historical
