A black hole’s “surface” is its event horizon. This boundary defines where you’d have to go faster than light – so much faster than anything can go – to escape the black hole. 2/6pic.twitter.com/wN0JtTPSi6
-
-
Show this thread
-
Two main types of black holes have been extensively observed — stellar-mass and supermassive. The type depends on how much stuff is crammed inside. Tens of times our Sun’s mass for a stellar-mass one; millions to billions for a supermassive one! 3/6pic.twitter.com/S82rcoC9R9
Show this thread -
Stellar-mass black holes form when a huge star — with at least 20 times the mass of our Sun — runs out of fuel. It collapses under its own weight and leaves behind a crushed remnant — a black hole.

4/6pic.twitter.com/wLMWcvEYa7Show this thread -
Supermassive black holes reside at the centers of most (and maybe all) large galaxies.
Scientists are still trying to figure out where they come from.
But we do know that they existed in the very earliest days of a galaxy’s lifetime. 5/6pic.twitter.com/APncyjXy2gShow this thread -
There *should* be a class of black hole somewhere between the stellar and supermassive ones. While some evidence of these “intermediate mass” black holes has been found, they seem to be more shy than the others! 6/6pic.twitter.com/2WTsmDU6X0
Show this thread
End of conversation
New conversation -
-
-
Thanks. Twitter will use this to make your timeline better. UndoUndo
-
-
-
Thanks. Twitter will use this to make your timeline better. UndoUndo
-
-
-
Movie pitch title: Blackholenado?
Thanks. Twitter will use this to make your timeline better. UndoUndo
-
-
-
This is just brilliant stuff right herepic.twitter.com/BEb8qQV3DR
Thanks. Twitter will use this to make your timeline better. UndoUndo
-
Loading seems to be taking a while.
Twitter may be over capacity or experiencing a momentary hiccup. Try again or visit Twitter Status for more information.