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  2. Characteristic energy - Wikipedia

    en.wikipedia.org/wiki/Characteristic_energy

    The characteristic energy with respect to Sun was negative, and MAVEN – instead of heading to infinity – entered an elliptical orbit around the Sun. But the maximal velocity on the new orbit could be approximated to 33.5 km/s by assuming that it reached practical "infinity" at 3.5 km/s and that such Earth-bound "infinity" also moves with ...

  3. Vacuum energy - Wikipedia

    en.wikipedia.org/wiki/Vacuum_energy

    Using the upper limit of the cosmological constant, the vacuum energy of free space has been estimated to be 10 −9 joules (10 −2 ergs), or ~5 GeV per cubic meter. [3] However, in quantum electrodynamics , consistency with the principle of Lorentz covariance and with the magnitude of the Planck constant suggests a much larger value of 10 113 ...

  4. Energy - Wikipedia

    en.wikipedia.org/wiki/Energy

    The energy industry provides the energy required for human civilization to function, which it obtains from energy resources such as fossil fuels, nuclear fuel, and renewable energy. Forms In a typical lightning strike, 500 megajoules of electric potential energy is converted into the same amount of energy in other forms, mostly light energy ...

  5. Outline of energy - Wikipedia

    en.wikipedia.org/wiki/Outline_of_energy

    Radiant energy – (≥0), energy of electromagnetic radiation including light and of gravitational radiation; Renewable energyenergy from renewable natural resources that are replenished on a human timescale; Rest energy – (≥0) given by E = mc 2, where m is an object's rest mass; Solar energy; Surface energy; Sustainable energy

  6. Cosmic ray - Wikipedia

    en.wikipedia.org/wiki/Cosmic_ray

    The magnitude of the energy of cosmic ray flux in interstellar space is very comparable to that of other deep space energies: cosmic ray energy density averages about one electron-volt per cubic centimetre of interstellar space, or ≈1 eV/cm 3, which is comparable to the energy density of visible starlight at 0.3 eV/cm 3, the galactic magnetic ...

  7. HZE ion - Wikipedia

    en.wikipedia.org/wiki/HZE_ion

    Space radiation is composed mostly of high-energy protons, helium nuclei, and high-Z high-energy ions (HZE ions). The ionization patterns in molecules , cells , tissues , and the resulting biological harm are distinct from high-energy photon radiation: X-rays and gamma rays , which produce low- linear energy transfer (low-LET) radiation from ...

  8. Radiation - Wikipedia

    en.wikipedia.org/wiki/Radiation

    [clarification needed] The international symbol for types and levels of ionizing radiation (radioactivity) that are unsafe for unshielded humans. Radiation, in general, exists throughout nature, such as in light and sound. In physics, radiation is the emission or transmission of energy in the form of waves or particles through space or a ...

  9. Potential energy - Wikipedia

    en.wikipedia.org/wiki/Potential_energy

    There are various types of potential energy, each associated with a particular type of force. For example, the work of an elastic force is called elastic potential energy; work of the gravitational force is called gravitational potential energy; work of the Coulomb force is called electric potential energy; work of the strong nuclear force or weak nuclear force acting on the baryon charge is ...