When these massive
stars run out of fuel in their center, their core collapses down to a neutron star and a supersonic shockwave is sent out to blow up the entire star.
When these massive
stars run out of fuel in their center, their core collapses down to a neutron star and a supersonic shock wave is sent out.
But once
stars run out of fuel and their fusion reactions end, they can no longer hold up this weight and collapse onto themselves.
Supernovas happen when huge
stars run out of fuel and collapse, creating an explosion that can briefly outshine their host galaxy.
When a massive
star runs out of fuel at the end of its life, it collapses and triggers a violent explosion known as a supernova.
When these supercharged early
stars ran out of fuel and exploded as supernovae, they would have blasted the interstellar gas right out of the galaxy.
When such
a star runs out of fuel, there is no longer enough heat and energy to fight back against the force of their own gravity.
The property results from the way they form: When a giant
star runs out of fuel and can no longer fight against the crushing force of its gravity, its core shrinks to the size of an asteroid, and most of its mass is blasted away in a titanic explosion called a supernova.
When
the star runs out of fuel and its core becomes too hefty, it collapses, triggering an explosion.
When a massive
star runs out of fuel, it can collapse onto itself and create a spectacular explosion that briefly outshines an entire galaxy, dispersing vital elements into space.
When
a star runs out of fuel, it collapses inward on itself.
Not exact matches
It will follow the evolution
of similar
stars, eventually
running out of hydrogen
fuel, at which point it will shift to burning helium at a much higher temperature, and will eventually, 5 billion years from now, gradually become a red giant with a diameter greater than the Earth's present orbit.
A neutron
star is the crushed core
of a massive
star that
ran out of fuel, collapsed under its own weight, and exploded as a supernova.
When a
star runs out of hydrogen
fuel in its core, it expands into a bloated red giant.
Astronomers figured this must be a short - lived phase, because a normal galaxy forming
stars that fast would soon
run out of fuel (gas and dust).
In the first stage
of this process, the more massive
star of the pair begins to
run out of fuel, transferring its outer layers to its less massive companion — which is destined to become the magnetar — causing it to rotate more and more quickly.
This immediately raised the question
of what happened to much heavier
stars when they
ran out of fuel — did they go on contracting for ever until they became what we would now call a black hole?
Known as 2014J, this was a Type la supernova caused by the explosion
of a white dwarf
star, the inner core
of star once it has
run out of nuclear
fuel and ejected its outer layers.
This
star - making frenzy gives rise to galactic wind that pushes
out more gas than the system keeps in, leading astronomers to estimate that M82 will
run out of fuel in just 8 million years.
Coupled with the fact that 98 %
of all
stars become white dwarfs when they
run out of nuclear
fuel, he says that suggests «the fraction
of stars that create rocky planets is high».
As
stars run out of hydrogen
fuel and burn helium instead, their luminosity waxes and wanes during several phases
of pulsation, interspersed with times
of relative calm.
When a
star runs out of hydrogen
fuel its core collapses inward under gravity and, hitting rock bottom, sends
out a shockwave that blasts away the
star's outer layers as a supernova.
When a
star runs out of nuclear
fuel, for example, the waste that remains collapses in on itself, fast and hard.
First, if a
star grows massive enough, its nuclear fires can no longer overcome the crushing force
of its gravity, in which case it
runs out of fuel and collapses.
What happens to a
star when it
runs out of fuel at the end
of its life depends on its mass.
Astronomers aren't sure why, but they posit that the tiny galaxy
ran out of the gases that
fuel star birth early on.
When a large
star runs out of nuclear
fuel, the core collapses in milliseconds.
When the nuclear reactions that power them
run out of fuel, the
stars can no longer resist their own intense gravity; they collapse and trigger the massive explosions called supernovae.
The explosions drive huge amounts
of gas
out of the galaxies and with most
of the rest consumed in
star formation, the galaxies soon
run out of fuel.
After 10 billion years
of guzzling the hydrogen in its core, a sun - size
star runs out of nuclear
fuel and becomes unstable.
When a
star runs out of hydrogen
fuel in its center, the core contracts and heats up, inflating the
star into a bloated red giant.
Most occur when massive
stars run out of nuclear
fuel.
«In a few billion years, when the Sun has
run out of fuel and the solar system has ceased to exist, TRAPPIST - 1 will still be only an infant
star.
A black hole is formed when a massive
star starts
running out of nuclear
fuel at its interior (mainly hydrogen and helium) and begins to collapse under its own gravity.
The glowing gaseous shrouds in the nebula were shed by the central
star after it
ran out of fuel to sustain the nuclear reactions in its core.
When a massive
star runs out of nuclear
fuel, it collapses under its own weight and forms a black hole.
A pulsar is formed when a massive
star runs out of nuclear
fuel and dies in a cataclysmic explosion called a supernova.
When a very massive
star begins to
run out of hydrogen and other nuclear
fuels, it can collapse so suddenly that almost all its electrons are driven into nuclei.
When a
star less than eight times the mass
of our Sun
runs out of the supply
of hydrogen
fueling the thermonuclear reaction raging in its stellar core, it may transform into a red giant instead
of ending its life in a dramatic supernova explosion.
The idea behind the death
of a massive
star is relatively straightforward: It gets old,
runs out of fuel, collapses under gravity and then explodes as a supernova.
Eventually, however, the hydrogen
fuel that powers the nuclear reactions within
stars will begin to
run out, and they will enter the final phases
of their lifetime.
These are black holes that are a few to a few dozen times the mass
of our sun that were likely formed by the death
of very massive
stars after they'd
run out of fuel and exploded as supernovas billions
of years ago.
All
stars, including our sun, will eventually
run out of the hydrogen gas that
fuels the nuclear fusion reactions in their cores.