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  2. Neutron star - Wikipedia

    en.wikipedia.org/wiki/Neutron_star

    A neutron star is so dense that one teaspoon (5 milliliters) of its material would have a mass over 5.5 × 10 12 kg, about 900 times the mass of the Great Pyramid of Giza. [b] The entire mass of the Earth at neutron star density would fit into a sphere 305 m in diameter, about the size of the Arecibo Telescope.

  3. Nuclear pasta - Wikipedia

    en.wikipedia.org/wiki/Nuclear_pasta

    For a typical neutron star of 1.4 solar masses (M ☉) and 12 km radius, the nuclear pasta layer in the crust can be about 100 m thick and have a mass of about 0.01 M ☉. In terms of mass, this is a significant portion of the crust of a neutron star. [9] [10]

  4. Magnetar - Wikipedia

    en.wikipedia.org/wiki/Magnetar

    Like other neutron stars, magnetars are around 20 kilometres (12 mi) in diameter, and have a mass of about 1.4 solar masses. They are formed by the collapse of a star with a mass 10–25 times that of the Sun. The density of the interior of a magnetar is such that a tablespoon of its substance would have a mass of over 100 million tons. [2]

  5. Nuclear matter - Wikipedia

    en.wikipedia.org/wiki/Nuclear_matter

    Densities are in terms of ρ 0 the saturation nuclear matter density, where nucleons begin to touch. Patterned after Haensel et al. , [ 7 ] page 12 Some authors use "nuclear matter" in a broader sense, and refer to the model described above as "infinite nuclear matter", [ 1 ] and consider it as a "toy model", a testing ground for analytical ...

  6. Nuclear density - Wikipedia

    en.wikipedia.org/wiki/Nuclear_density

    Its size is approximately 10 −15 meters and its density 10 18 kg/m 3. The descriptive term nuclear density is also applied to situations where similarly high densities occur, such as within neutron stars. Using deep inelastic scattering, it has been estimated that the "size" of an electron, if it is not a point particle, must be less than 10 ...

  7. Nuclear drip line - Wikipedia

    en.wikipedia.org/wiki/Nuclear_drip_line

    As we go deeper into the neutron star the free neutron density increases, and as the Fermi momentum increases with increasing density, the Fermi energy increases, so that energy levels lower than the top level reach neutron drip and more and more neutrons drip out of nuclei so that we get nuclei in a neutron fluid. Eventually all the neutrons ...

  8. 25 Best Dessert Recipes For People With Diabetes, According ...

    www.aol.com/25-best-dessert-recipes-people...

    A crustless pie, using a sugar substitute like Truvia and slashing the peach filling in half reduces the carb and sugar count, Dr. Mohr says. Get the easy peach galette recipe 13.

  9. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    Neutron stars are expected to have a skin or "atmosphere" of normal matter on the order of a millimeter thick, underneath which they are composed almost entirely of closely packed neutrons called neutron matter [5] with a slight dusting of free electrons and protons mixed in. This degenerate neutron matter has a density of about 6.65 × 10 17 ...