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  2. Steam rocket - Wikipedia

    en.wikipedia.org/wiki/Steam_rocket

    Water, while under pressure, is heated up to a high temperature (approx. 250–500 °C). As the hot water goes through the nozzle (usually a de Laval nozzle) and the pressure reduces, the water flashes to steam pressing on the nozzle, and leaving at high speed. By the recoil the rocket accelerates in the opposite direction to the steam.

  3. Aeolipile - Wikipedia

    en.wikipedia.org/wiki/Aeolipile

    An illustration of Hero's aeolipile. An aeolipile, aeolipyle, or eolipile, from the Greek "Αἰόλου πύλη," lit. ' Aeolus gate ', also known as a Hero's (or Heron's) engine, is a simple, bladeless radial steam turbine which spins when the central water container is heated.

  4. Molecules in stars - Wikipedia

    en.wikipedia.org/wiki/Molecules_in_stars

    Although the Sun is a star, its photosphere has a low enough temperature of 6,000 K (5,730 °C; 10,340 °F), and therefore molecules can form. Water has been found on the Sun, and there is evidence of H 2 in white dwarf stellar atmospheres. [2] [4] Cooler stars include absorption band spectra that are characteristic of molecules.

  5. Steam - Wikipedia

    en.wikipedia.org/wiki/Steam

    Boiling water creating steam in an electric kettle. Steam's capacity to transfer heat is also used in the home: for cooking vegetables, steam cleaning of fabric, carpets and flooring, and for heating buildings. In each case, water is heated in a boiler, and the steam carries the energy to a target object.

  6. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    Typical boundary conditions set the values of the observable parameters appropriately at the surface (=) and center (=) of the star: () =, meaning the pressure at the surface of the star is zero; () =, there is no mass inside the center of the star, as required if the mass density remains finite; () =, the total mass of the star is the star's ...

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

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

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  8. 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 ...

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