When.com Web Search

Search results

  1. Results From The WOW.Com Content Network
  2. State of matter - Wikipedia

    en.wikipedia.org/wiki/State_of_matter

    Normally free neutrons outside an atomic nucleus will decay with a half life of approximately 10 minutes, but in a neutron star, the decay is overtaken by inverse decay. Cold degenerate matter is also present in planets such as Jupiter and in the even more massive brown dwarfs, which are expected to have a core with metallic hydrogen. Because ...

  3. Gravitational collapse - Wikipedia

    en.wikipedia.org/wiki/Gravitational_collapse

    The compression caused by the collapse raises the temperature until thermonuclear fusion occurs at the center of the star, at which point the collapse gradually comes to a halt as the outward thermal pressure balances the gravitational forces. The star then exists in a state of dynamic equilibrium. During the star's evolution a star might ...

  4. Stellar core - Wikipedia

    en.wikipedia.org/wiki/Stellar_core

    Once a star has converted all the hydrogen in its core into helium, the core is no longer able to support itself and begins to collapse. It heats up and becomes hot enough for hydrogen in a shell outside the core to start fusion. The core continues to collapse and the outer layers of the star expand. At this stage, the star is a subgiant. Very ...

  5. Frost line (astrophysics) - Wikipedia

    en.wikipedia.org/wiki/Frost_line_(astrophysics)

    In astronomy or planetary science, the frost line, also known as the snow line or ice line, is the minimum distance from the central protostar of a solar nebula where the temperature is low enough for volatile compounds such as water, ammonia, methane, carbon dioxide and carbon monoxide to condense into solid grains, which will allow their accretion into planetesimals.

  6. Star formation - Wikipedia

    en.wikipedia.org/wiki/Star_formation

    Westerhout 51 nebula in Aquila - one of the largest star factories in the Milky Way (August 25, 2020). Star formation is the process by which dense regions within molecular clouds in interstellar space—sometimes referred to as "stellar nurseries" or "star-forming regions"—collapse and form stars. [1]

  7. Unique white dwarf will help clarify what happens to dying stars

    www.aol.com/news/2016-04-01-zombie-white-dwarf...

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

  8. Phlogiston theory - Wikipedia

    en.wikipedia.org/wiki/Phlogiston_theory

    When the oxide was heated with a substance rich in phlogiston, such as charcoal, the calx again took up phlogiston and regenerated the metal. Phlogiston was a definite substance, the same in all its combinations. [10] Stahl's first definition of phlogiston first appeared in his Zymotechnia fundamentalis, published in 1697.

  9. Unpacking The Truth About Starbucks' Legendary Cold-Curing Drink

    www.aol.com/unpacking-truth-starbucks-legendary...

    A Medicine Ball isn't a cure-all for a cold. But just like with chicken soup and other sick-day staples, its warmth and comforting flavors make it a great treat to enjoy while you wait for your ...