Very large,
massive stars burn their fuel much faster than smaller stars and may only last a few hundred thousand years.
Once known as a frozen star, a black hole is formed when
a massive star burns out and collapses upon itself, ultimately producing gravitational energy so powerful that not even light can escape from it.
Neutron stars are ultra-dense balls of neutrons, subatomic particles left behind when
a massive star burns out and collapses.
A typical supernova occurs when
a massive star burns up all of its hydrogen fuel and its core collapses.
Wilson knew that when
a massive star burns up the last of its fuel after some 10 million years, its core rapidly implodes, pulling all of the star's matter inward.
Not exact matches
For the first time, scientists using NASA's Hubble Space Telescope have witnessed a
massive object with the makeup of a comet being ripped apart and scattered in the atmosphere of a white dwarf, the
burned - out remains of a compact
star.
Another possibility is that a
massive pulse of
burning carbon from the center of the
star, emulating outwards, eliminated the lighter elements.
This
massive blue
star should have
burnt out tens of millions of years ago, but it's still going strong.
It's not clear how long it will take for the
stars to fully merge, or what will happen when that occurs: Some models of stellar evolution suggest the merged
star could explosively release a
massive amount of energy, while others hint it could simply
burn through its fuel more quickly than each
star would on its own.
A supernova — the explosion of a
massive star after it
burns through its fuel — would have to happen within 0.13 light - years of Earth, and the closest
star big enough to go supernova is nearly 147 light - years away.
According to this model, the violent wind that creates a planetary nebula is also the engine that transforms a bloated red giant into the
burnt - out cinder of a white dwarf, a metamorphosis common to all
stars of low and intermediate mass —
stars up to eight times more
massive than the sun.
Supernovae are
massive explosions that happen when a
star burns out.
But observations beginning in 2014 from NASA's NuSTAR and other space telescopes are showing that some ULXs, which glow with X-ray light equal in energy to millions of suns, are actually neutron
stars — the
burnt - out cores of
massive stars that exploded.
(Theoretically, more
massive stars would
burn faster.)
This is a counter-intuitive result, as more
massive stars have more fuel to
burn and might be expected to last longer.
Because the Universe originally lacked metals (elements heavier than lithium) that cool collapsing gas clouds today, the earliest
stars were more
massive and
burned much hotter than even the largest
stars we study today.
Many now believe that most, if not all, of the first generation of
stars (Population III) that formed from the gas and dust created by the Big Bang were
massive, fast -
burning, short - lived, and composed only of the four lightest elements, hydrogen and helium with traces of lithium and beryllium.
Researchers using NASA's Hubble Space Telescope have observed, for the first time ever, an enormous object with the composition of a comet being shredded and scattered by a white dwarf, the
burned - out husk of a
massive star.
These
massive, hot
stars burned bright for a short time, emitting so much energy in the form of starlight that they pushed nearby gas clouds far away.
Exceptions include a number of planets discovered orbiting
burned - out
star remnants called pulsars, such as PSR B1257 +12, [14] the planets orbiting the
stars Mu Arae, 55 Cancri and GJ 436, which are approximately Neptune - sized, and a planet orbiting Gliese 876 that is estimated to be about six to eight times as
massive as Earth and is probably rocky in composition.
As the
star is more
massive than Sol, it has evolved faster into a helium -
burning «clump» giant, possibly within five to eight billion years since hydrogen ignition (see Kaler's
Stars page on Arcturus).
Because they are so
massive, O - type
stars have very hot cores and
burn through their hydrogen fuel very quickly, so they are the first
stars to leave the main sequence.
While other, more
massive stars only
burn through the hydrogen at their core before coming to the end of their lifetimes, red dwarfs consume all of their hydrogen, in and out of their core.
Fear X didn't so much crash and
burn as stall on the grid, bankrupting Refn's production company Jang Go
Star and leaving him in
massive personal debt (at one point he owed his bank $ 1m).
A
star is a
massive ball of
burning gas whose main function is fusing hydrogen into helium.