Energy Transport in the Sun

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  • čas přidán 18. 04. 2024
  • Here we learn how energy moves around in the Sun, and peek at the basic equations of stellar structure. This is part of my intro Astronomy class taught at Willam Paterson University and CUNY Hunter.
    Solar Convection Zone: en.wikipedia.org/wiki/Convect...
    Solar Radiation Zone: en.wikipedia.org/wiki/Radiati...
    Convection: en.wikipedia.org/wiki/Convect...
    Radiative Transfer: hyperphysics.phy-astr.gsu.edu/...
    Random Walk of Photons out of the Sun: physicsanduniverse.com/random-...
    Conduction: en.wikipedia.org/wiki/Thermal...
    The equations of stellar structure: en.wikipedia.org/wiki/Stellar...
    Solar Model created by Kevin France, University of Colarado: cos.colorado.edu/~kevinf/PAPE...
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Komentáře • 7

  • @FelizTheLifeguardMinion3
    @FelizTheLifeguardMinion3 Před 28 dny +2

    These videos allow me to learn and sleep at the same time. Thank you so much for making these long form awesome videos that are jam packed with goodness 😂❤🎉

  • @pbkobold
    @pbkobold Před 22 dny

    Thank you, the audio in this is so much better than the audio "What is the Cosmic Redshift?" Please continue whatever changes you have made! Thank you for the time and energy you put into these.

  • @mbird1291
    @mbird1291 Před 20 hodinami

    At 28:30 it says there is no energy produced above the core, but what about the photo sphere? I thought there was a type of fusion occurring somewhere around there, somewhere above the surface, where the solar wind is accelerated?

  • @FelizTheLifeguardMinion3

    First! 🎉

  • @HzPjtvHYom4991
    @HzPjtvHYom4991 Před 27 dny

    Um, "none of us have ever been inside the sun?" ....we were all born inside stars! Haha 😂 jokes

  • @icantseethis
    @icantseethis Před 27 dny

    bro just use metric 😂