Sentences with phrase «carinae explodes as a supernova»

After a star explodes as a supernova, it usually leaves behind either a black hole or what's called a neutron star — the collapsed, high - density core of the former star.

Most stars end their lives either slowly fading away or exploding as a supernova.

The most massive stars in the original cluster will have already run through their brief but brilliant lives and exploded as supernovae long ago.

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.

Lower velocity runaway stars can be produced when one half of a binary pair explodes as a supernova, blasting its partner away.

If they are jettisoned out of the galaxy and then explode as supernovae, the heavy elements they contain could be released into this medium.

Long gamma - ray bursts, which flash for up to 100 seconds or longer, are believed to occur when massive stars explode as supernovae.

Stars exploding as supernovae are the main sources of heavy chemical elements in the Universe.

Larger stars — those with more than about eight solar masses — will explode as supernovas.

There, young stars, born during the merger, will explode as supernovas, and a quasar — a giant black hole ignited by the galactic collision — might spew energetic radiation.

First, a massive star exploded as a supernova, blasting its debris out into space.

When a star explodes as a supernova, it shines brightly for a few weeks or months before fading away.

Cassiopeia A Just before it explodes as a supernova, a massive star is like an onion, with layers of different chemical compositions atop one another.

Stars that are eight or more times the mass of the sun explode as supernovae at the end of their lives.

When a giant star explodes as a supernova, it can outshine its own galaxy as it dishes out heat, X-rays, and the highest - energy radiation of all, gamma rays.

When a massive star dies, it explodes as a supernova, which includes a short burst of visible light, as in this illustration.

Black holes this size are «born» when a heavyweight star — more than ten times the mass of the Sun — explodes as a supernova at the end of its life.

Overall, supernovas are rare, but as the solar system circles through the Milky Way, it sometimes passes through one of our galaxy's spiral arms, where large numbers of massive stars form and explode as supernovas.

A neutron star forms when a massive star explodes as a supernova, blowing off its outer layers while its core collapses.

As this cluster is relatively old, a part of this lost mass will be due to the most massive stars in the cluster having already reached the ends of their lives and exploded as supernovae.

Various lines of evidence, including observations from NASA's Fermi Gamma - ray Space Telescope, support the idea that shock waves from the expanding debris of stars that exploded as supernovas accelerate cosmic rays up to energies of 1,000 trillion electron volts (PeV).

Shortly after their birth, they exploded as supernovas, ejecting newly formed carbon, oxygen, and nitrogen atoms into space.

That meant the X-ray source and Geminga were one and the same pulsar: the dense, rapidly spinning core of a star that exploded as a supernova.

These stars are rapidly working their way through their vast supplies of hydrogen, and have only a few million years of life left before they meet a dramatic demise and explode as supernovae.

Or, the Wolf - Rayet could explode as a supernova.

(When big stars reach the end of their life, they explode as supernovae, leaving neutron stars or black holes behind.)

Neutron stars are the superdense remains of massive stars that have exploded as supernovas.

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.

That's according to a new analysis — part of the biggest census of star - forming regions to date — that focused on stars eight times the mass of our sun or larger (the size that eventually explode as supernovae) at a very early stage in their lifetime, when they'd still be inside the clouds of gas and dust where they formed.

According to the popular «collapsar» theory, a GRB occurs when a very massive star explodes as a supernova and collapses into a black hole.

The results of the simulations thus lend support to basic perceptions of the dynamical processes that are involved when a star explodes as supernova.

At the end of its life, a massive star inevitably explodes as a supernova.

These neighbouring bubbles eventually merged to form a superbubble, and the short life spans of the stars at its heart meant that they exploded as supernovae at similar times, expanding the superbubble even further, to the point that it merged with other superbubbles, which is when the supershell was formed.

Sobral adds: «But star formation at this rate leads to a lot of massive, short - lived stars coming into being, which explode as supernovae a few million years later.

Any heavier than that, and it will explode as a supernova.

If a runaway star accumulates between 800 and 3000 times the Sun's mass before exploding as a supernova, it can produce a midsize black hole whose mass is 100 to 1000 times the Sun's.

After exploding as a supernova, the star would have faded from view within a year or so — and eventually from living memory, until, 25 years ago, a radio telescope near Canberra, Australia, found its curious remains.

The Crab pulsar is the corpse left over when the star that created the Crab nebula exploded as a supernova.

When massive stars explode as supernovae, they disperse the heavier elements they have built into space, where they become the building blocks of the next generation of stars.

It will likely explode as a supernova within 10,000 years, or maybe sooner.

Eventually, they explode as supernovae (see Székely & Benedekfi (2007) for more on the death of stars).

originate from fusion reactions in the heart of stars and are spewed out when those stars explode as supernovae, the relatively high metallicity of the galaxy suggests that it had already seen the birth and death of generations of stars by the time the universe was 700 million years old.»

Before 1987, astronomers believed that only red supergiants would explode as supernovae, but this observation proved that other types of evolved stars can produce these explosions too.

Pulsars are the spinning remnants of stars that have exploded as supernovae.

In other cases, in which the mass of the star is several solar masses or more, the star may explode as a supernova.

Since pulsars are superdense, spinning neutron stars left over when a massive star explodes as a supernova, it was logical to assume that the Monogem Ring, the shell of debris from a supernova explosion, was the remnant of the blast that created the pulsar.

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.

Evolutionists therefore believe that the hundred or so heavier chemical elements (97 % of all chemical elements) were produced either deep inside stars or when some stars exploded as supernovas.

A fourth theory assumed that two helium nuclei and several neutrons might merge when helium - rich stars exploded as supernovas.

The second process relies on the fact that stars also contain smaller amounts of carbon produced in previous generations of stars that exploded as supernovas.