Your weight depends on your mass and the strength of the gravity where you are. A neutron star has a mass 2-3 times that of the sun compacted into a very small area, resulting in a surface gravity billions of times stronger than on Earth. As a result, at the surface of a neutron star you would weigh several billion times what you do now.
A subgiant star is bigger than a neutron star. Neutron stars are incredibly dense and compact, with a radius of about 10-15 kilometers, while subgiant stars have a larger radius of several million kilometers.
A neutron star is the collapsed remains of a supernova. It is an incredibly dense - and incredibly hot - pile of stellar ash. What is happening in it is slow cooling. One well-known physicist (James S. Trefil) states that the full cooling of a neutron star would take longer than the current known age of the universe (15 billion years).
A subgiant star is larger than a neutron star. Neutron stars are incredibly dense and compact remnants of massive stars, while subgiant stars are in a transitional phase between main sequence and red giant stages, typically larger and more diffuse than neutron stars.
When you combine an electron with a proton you make a neutron. Therefore you make a "neutron" star.
Neutron stars are so heavy because they are the compact core of a star that is 8 time the mass of our Sun. The most massive neutron stars possible are 3 times the mass of our Sun.
A teaspoon of a neutron star would weigh as much as a car due to its incredibly high density. Neutron stars are formed when the core of a massive star collapses under its own gravity during a supernova explosion, packing an immense amount of mass into a small volume. This results in a teaspoon of neutron star material being incredibly dense and heavy.
A teaspoon of material from a neutron star would weigh about 6 billion tons.
A neutron star is formed when a large star collapses from gravity, but, the star is able to cling on to life because as it collapses, the neutrons in the atoms that make up the star repel each other, pushing outwards against the gravitational force, keeping the star alive, but incredibly dense.
A subgiant star is bigger than a neutron star. Neutron stars are incredibly dense and compact, with a radius of about 10-15 kilometers, while subgiant stars have a larger radius of several million kilometers.
A neutron star is the collapsed remains of a supernova. It is an incredibly dense - and incredibly hot - pile of stellar ash. What is happening in it is slow cooling. One well-known physicist (James S. Trefil) states that the full cooling of a neutron star would take longer than the current known age of the universe (15 billion years).
A dead star with the density of an atomic nuclei is called a neutron star. Neutron stars are incredibly dense and are composed mostly of tightly packed neutrons. They form when massive stars explode in a supernova and their cores collapse under gravity.
A subgiant star is larger than a neutron star. Neutron stars are incredibly dense and compact remnants of massive stars, while subgiant stars are in a transitional phase between main sequence and red giant stages, typically larger and more diffuse than neutron stars.
When you combine an electron with a proton you make a neutron. Therefore you make a "neutron" star.
Neutron stars are so heavy because they are the compact core of a star that is 8 time the mass of our Sun. The most massive neutron stars possible are 3 times the mass of our Sun.
Depends on the age of the neutron star. As a neutron star no longer has any method to produce heat, it will slowly cool over time. A young neutron star will have a core temperature of about 106 kelvin.
A neutron star is what is left of the core of a massive star after it dies. The core collapses under the force of gravity, crushing itself from a size far larger than Earth to about the size of a city but still with a mass up to 3 times that of the sun. If it is any more massive it becomes a black hole.
The description matches that of a neutron star, which is formed after a supernova explosion of a massive star. Neutron stars are incredibly dense, with matter packed tightly together. Due to their high gravitational pull, a small amount of neutron star material would have an extremely high mass.