Bananas for Scale
Black Hole — Stellar Mass

Photo from Wikimedia Commons

Black Hole — Stellar Mass

A dead star so dense that light itself cannot escape/Deep Space

A stellar-mass black hole forms when a massive star (at least 20-25 times the mass of the Sun) collapses at the end of its life. A typical stellar black hole has about 10 solar masses and an event horizon diameter of about 60 km. Within that boundary, the escape velocity exceeds the speed of light, making it a one-way trip for anything that crosses it. Despite their fearsome reputation, stellar black holes are relatively common — there may be 100 million of them in the Milky Way alone.

Measurements

Mass20 nonillion kg
111 octillionMale gorillas
556 septillionLoaded semi trucks
200 octillionBaby elephants

About 10 solar masses

Event horizon diameter60,000 m
240,000Tambourine diameters
72.5Burj Khalifas
6 millionThumb tack lengths

About 60 km across; smaller than a city

Escape velocity (at horizon)300 million m/s
1Light speed
14,990Meteorites

The speed of light; that is the whole point

Schwarzschild radius30,000 m
10.7 quintillionElectron radii
10 millionSesame seeds
410,959Lipstick tubes

About 30 km

Tidal force at 1000 km50 billion N
5 quadrillionSand grain weights
5 trillionWet noodle flicks
2.5 millionHydraulic jacks

Extreme tidal stretching (spaghettification)

Hawking temperature6 billionths K
13.3 trillionthsBaking ovens
16.4 trillionthsHot Pocket centers
17 trillionthsFresh bread loaves

About 6 nanokelvin; essentially zero

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