Along with black holes, neutron stars are the result of stars
collapsing under gravity once their fuel burns out, until their density is about the same as that of the nucleus of an atom, at which point the protons and electrons «melt» into pure neutrons.
A cable made of carbon nanotubes, which have the highest known ratio of tensile strength to weight, would have to be so thick at the far end that it would
collapse under gravity.
An extremely compact ball of neutrons created from the central core of a star that
collapsed under gravity during a 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.
All stars are believed to form within clouds of gas and dust that
collapse under gravity.
The map stretches halfway back to the beginning of the universe and shows how dark matter has grown increasingly «clumpy» as
it collapses under gravity.
Not exact matches
Stars are born when a cloud of gas hundreds of times more massive than our Sun begins to
collapse under its own
gravity.
When the core reaches about 1.5 times the mass of the Sun, it
collapses under the influence of its own
gravity and forms a neutron star.
You probably know that black holes are stars that have
collapsed under their own
gravity, producing gravitational forces so strong that even light can't escape.
Such stars get so hot that they convert gamma rays, whose high energy helped keep the star from
collapsing under its own
gravity, into electrons and their antimatter counterparts, positrons.
The traditional model of how stars and their planets form dates back to the 18th century, when scientists proposed that a slowly rotating cloud of dust and gas could
collapse under its own
gravity.
This gas gives rise to newborn stars — it gradually
collapses under the force of its own
gravity until it is sufficiently compressed to form a protostar — the precursor to a star.
New simulations suggest that dense swarms of boulders
collapsed under their own
gravity to make the building blocks of our solar system.
«What probably happens is that after the supernova, the remaining stellar core
collapses under its own
gravity to form a black hole,» Reeves says.
Impey speculates that the dark matter which lurks in these dim galaxies could make up a substantial chunk of the extra mass that would be needed to make the Universe dense enough to eventually
collapse under its own
gravity.
Scientifically, Hawking's name will forever be tied to black holes, the ultraintense gravitational fields left behind when massive stars
collapse under their own
gravity into infinitesimal points.
When a massive star
collapses under its own
gravity during a supernova explosion it forms either a neutron star or black hole.
Unlike run - of - the - mill black holes that form from
collapsing stars, such primordial black holes could have formed when dense regions of the very early universe
collapsed under their own
gravity, some theories suggest.
When too much matter is put into too small a space, it
collapses under its own
gravity and forms a black hole.
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.
Dimitrios Psaltis, an astrophysicist at the University of Arizona, is helping to test what may be general relativity's most extreme prediction: that large - enough stars will eventually
collapse under their own
gravity to form these infinitely dense objects.
Eventually, these lumps became large enough and dense enough to
collapse and form galaxies, which themselves clumped
under the influence of
gravity to form clusters and superclusters of galaxies, and so on.
They simulated two streams of interstellar gas coming together to form a cloud that, over a few million years,
collapsed under its own
gravity to make a cluster of stars.
The protoplanetary disc took shape when a spherical cloud of ultra-cold gas and dust began to
collapse under its own
gravity.
NAKED singularities and cosmic censorship may sound like lurid terms from the tabloids, but in fact these phrases lie at the heart of a troubling question for modern cosmology: what happens when our known laws of space and time break down, as happens in the final moments of a star
collapsing to a point
under its own
gravity?
Decades of research indicate that when a star heftier than eight suns burns up its nuclear fuel, it will begin to
collapse under its own
gravity, starting at the core.
Once a star has exhausted its fuel, it will
collapse under its own
gravity.
In the modern universe, black holes typically form from massive stars that
collapse under their own
gravity at the ends of their lives.
Dense pockets of material in these clouds
collapse under their own
gravity and grow by accumulating more and more star - forming gas from their parent clouds.
As a ball of dust and gas contracts
under its own
gravity, it begins to shrink and its core begins
collapsing faster and faster.
We know that these huge clouds
collapse under for force of
gravity to form stars.
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 core of the star, with 40 percent more mass than our Sun,
collapses under its own
gravity to a sphere only about 10 miles in diameter, composed mostly of neutrons.
The more numerous faint stars are still in the process of
collapsing under their own
gravity, but have become hot enough in their centers to be self luminous bodies.
These concentrations become ever more dense until they
collapse inward
under gravity to form protoplanets.
Groups of stars such as those in Orion are born when a cloud of gas hundreds of times more massive than our Sun begins to
collapse under its own
gravity.
Those gamma rays help to keep the star from
collapsing under its own
gravity.
«The atmosphere does not
collapse under the downward pull of
gravity because of the energy embedded in the movement of the air molecules.