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  2. Convection - Wikipedia

    en.wikipedia.org/wiki/Convection

    Mantle convection occurs at rates of centimeters per year, and it takes on the order of hundreds of millions of years to complete a cycle of convection. Neutrino flux measurements from the Earth's core (see kamLAND) show the source of about two-thirds of the heat in the inner core is the radioactive decay of 40 K, uranium and thorium.

  3. Heat transfer - Wikipedia

    en.wikipedia.org/wiki/Heat_transfer

    Another form of convection is forced convection. In this case, the fluid is forced to flow by using a pump, fan, or other mechanical means. Convective heat transfer , or simply, convection, is the transfer of heat from one place to another by the movement of fluids , a process that is essentially the transfer of heat via mass transfer .

  4. Light-year - Wikipedia

    en.wikipedia.org/wiki/Light-year

    The product of Simon Newcomb's J1900.0 mean tropical year of 31 556 925.9747 ephemeris seconds and a speed of light of 299 792.5 km/s produced a light-year of 9.460 530 × 10 15 m (rounded to the seven significant digits in the speed of light) found in several modern sources [10] [11] [12] was probably derived from an old source such as C. W ...

  5. Sun - Wikipedia

    en.wikipedia.org/wiki/Sun

    Multiple other interstellar clouds exist in the region within 300 light-years of the Sun, known as the Local Bubble. [160] The latter feature is an hourglass-shaped cavity or superbubble in the interstellar medium roughly 300 light-years across. The bubble is suffused with high-temperature plasma, suggesting that it may be the product of ...

  6. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    This core convection occurs in stars where the CNO cycle contributes more than 20% of the total energy. As the star ages and the core temperature increases, the region occupied by the convection zone slowly shrinks from 20% of the mass down to the inner 8% of the mass. [25] The Sun produces on the order of 1% of its energy from the CNO cycle.

  7. 50 Of The Most Fascinating, Stunning And Dangerous Natural ...

    www.aol.com/100-most-incredible-stunning-strange...

    Moist convection and ice formation can also contribute to the phenomenon, sometimes occurring even without ice crystals in the cloud. ... and spans roughly 100,000 light-years in diameter. The ...

  8. Unusual Martian mounds could help solve one of the red planet ...

    www.aol.com/news/unusual-martian-mounds-could...

    Convection, or the transfer of heat from one spot to another, likely took place in the mantle, or inner layer, of Mars billions of years ago, the study authors said. The mantle is located between ...

  9. Stellar core - Wikipedia

    en.wikipedia.org/wiki/Stellar_core

    Once stars with the mass of the Sun form, the core region reaches thermal equilibrium after about 100 million (10 8) [2] [verification needed] years and becomes radiative. [3] This means the generated energy is transported out of the core via radiation and conduction rather than through mass transport in the form of convection.