When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  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. Orders of magnitude (mass) - Wikipedia

    en.wikipedia.org/wiki/Orders_of_magnitude_(mass)

    Operational empty weight of a Boeing 747-300: 1.8 ... A teaspoon (5 ml) of neutron star material (5000 million tonnes) [117] 10 13: 1 ...

  5. Astronomers capture gravitational landmine in neutron star ...

    www.aol.com/article/news/2017/10/16/astronomers...

    For premium support please call: 800-290-4726 more ways to reach us

  6. Neutronium - Wikipedia

    en.wikipedia.org/wiki/Neutronium

    Neutronium (or neutrium, [1] neutrite, [2] or element zero) is a hypothetical substance made purely of neutrons.The word was coined by scientist Andreas von Antropoff in 1926 (before the 1932 discovery of the neutron) for the hypothetical "element of atomic number zero" (with no protons in its nucleus) that he placed at the head of the periodic table (denoted by -).

  7. List of most massive neutron stars - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive...

    This page was last edited on 29 October 2024, at 23:12 (UTC).; Text is available under the Creative Commons Attribution-ShareAlike 4.0 License; additional terms may apply.

  8. Compact object - Wikipedia

    en.wikipedia.org/wiki/Compact_object

    They realized that because neutron stars are so dense, the collapse of an ordinary star to a neutron star would liberate a large amount of gravitational potential energy, providing a possible explanation for supernovae. [8] [9] [10] This is the explanation for supernovae of types Ib, Ic, and II. Such supernovae occur when the iron core of a ...

  9. Magnetar - Wikipedia

    en.wikipedia.org/wiki/Magnetar

    Artist's conception of a powerful magnetar in a star cluster. A magnetar is a type of neutron star with an extremely powerful magnetic field (~10 9 to 10 11 T, ~10 13 to 10 15 G). [1] The magnetic-field decay powers the emission of high-energy electromagnetic radiation, particularly X-rays and gamma rays. [2]