notesonly.in

One notebook for every subject — open it anywhere.

Log in

Black holes: event horizon and Hawking radiation (introductory)

Galaxies and cosmology · Physics

Solar system

Interactive 3D

All eight planets in orbit around the Sun, with Saturn's rings and Earth's Moon.

Controls

Drag the sliders or type a value — the simulation updates live.

×
0×2×

Study notes

Worked example - the Schwarzschild radius of the Sun and Earth. Rs = 2GM/c^2. For the Sun: M = 2 x 10^30 kg. Rs = 2 x (6.67 x 10^-11) x (2 x 10^30) / (3 x 10^8)^2 = 2.67 x 10^20 / 9 x 10^16 = 2,960 m ~ 3 km. So the entire Sun squeezed into a 6-km-wide ball would be a black hole. For Earth: M = 6 x 10^24 kg, giving Rs ~ 8.9 mm - about the size of a marble. This shows why only collapsed stellar cores (and giant galactic centres) actually form black holes: ordinary matter is nowhere near dense enough.

← Back to topics for Physics