There is a great, short essay by Gary Gibbons about Michell's prediction, why it was forgotten for so long, and some of his other contributions to physics.
Did you know that Michell designed the torsion balance experiment used by Cavendish to measure the density of the Earth?
Gary's essay appeared in New Scientist in 1979. It appears they've removed it from the web, but here's a copy Gary posted on his old website.
In 1783, Newton’s law of gravitation was newer than general relativity is today.
Michell surveyed the heavens, extrapolated the properties of the objects he observed, and realized that the Universe (as he understood it) allowed exotic and fantastic gravitational phenomena.
In that sense, he had a lot in common with modern physicists and astronomers.
But even though Michell envisioned something a bit different than the phenomenon we understand in general relativity, this is still a momentous event in the history of black holes.
His paper predates Laplace's 1796 prediction of "invisible bodies" by 13 years, and Schwarzschild's black hole solution of general relativity by 132 years.
In general relativity, the causal structure of spacetime traps things behind a horizon. No rocket can overcome that.
Think of general relativity as laying out rules for how things are allowed to move. The rules in a black hole spacetime simply don’t allow trajectories that pass behind the horizon of a black hole and then make it back outside. Once something crosses over, the only allowed motions take it further in.
This sounds like a black hole, right? Escape velocity greater than the speed limit built into our Universe?
Not quite. Escape velocity assumes no further acceleration. Newtonian physics would allow a rocket with enough fuel to escape Michell's object, it would just need to maintain sufficient acceleration for long enough.
But the black holes that arise in general relativity are an entirely different phenomenon.
"Escape velocity" is the speed needed at takeoff for a rocket (or any projectile) to escape the gravitational pull of whatever it is taking off from, without any further acceleration.
In 1783 the speed of light was known to be finite. Michell pointed out that if an object was dense enough, the escape velocity would exceed the speed of light and therefore "all light emitted from such a body would be made to return towards it, by its own proper gravity."
What Michell predicted was the existence of bodies with an escape velocity greater than the speed of light. It's fair to call that a "Newtonian Black Hole."
It's not quite the same thing as a black hole in general relativity, where crossing the horizon means it's impossible to move in any way that takes you back outside.
The Reverend John Michell read a paper before the Royal Society #OTD in 1783 that included the first prediction of what, given the understanding of gravity at the time, you might call a Black Hole.
Can anyone recommend a clickity-clackity mechanical keyboard that is nice to type on, but has a low barrier to entry? (That is, you don’t have to make lots of decisions about keycaps, switches, etc.) Bonus if it does Bluetooth.
Charles Darwin's "On the Origin of Species by Means of Natural Selection" was published #OTD in 1859.
Yesterday I was thankful for his explanation of the process by which certain saurischian dinosaurs became, over millions of years, delicious and small enough to fit on a plate:🦖→🦃.