Estimating the temperature of a star

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  • เผยแพร่เมื่อ 12 ต.ค. 2024
  • A quick energy-based method to estimate the temperature of a star given only its mass and radius. Although based on a simple model, the equation we derive shows surprisingly good agreement with the temperature of the Sun!
    To support the channel: ko-fi.com/beny...
    About me: I studied Physics at the University of Cambridge, then stayed on to get a PhD in Astronomy. During my PhD, I also spent four years teaching Physics undergraduates at the university. Now, I'm working as a private tutor, teaching Physics & Maths up to A Level standard.
    My website: benyelverton.com/
    #physics #mathematics #stars #temperature #gravity #energy #equipartitiontheorem #boltzmannconstant #density #integration #calculus #sphere #thermalenergy #potential #mass #gravitationalpotentialenergy #star #conservationofenergy #hydrogen #atoms #thermalphysics #ionisation #physicsproblems #maths #math #science #education

ความคิดเห็น • 21

  • @logician1234
    @logician1234 3 วันที่ผ่านมา +10

    Prof takes a break and then the first video he posts is calculating temperature of the star 💀

    • @DrBenYelverton
      @DrBenYelverton  2 วันที่ผ่านมา +3

      I had to think of something impressive for my return!

  • @shrivatsa8604
    @shrivatsa8604 3 วันที่ผ่านมา +4

    Great to have you back, sir. I had previously worked with the same problem, which after solving yielded the same result. And then tried to solve it in a non-classical, relativistic way .my initial goal was to find the potential energy of the entire system using relativistic way calculating energy (Swartzchild interior solution) , which was complicated. Based on your expertise in this field, I believe working on relativistic physics in your upcoming videos will be very brilliant and intresting like this one.

    • @DrBenYelverton
      @DrBenYelverton  2 วันที่ผ่านมา +3

      Thanks for your support. Solving this one relativistically certainly sounds complicated!

  • @yahavhazut
    @yahavhazut 2 วันที่ผ่านมา +1

    Great video that shows the power of estimation theory!
    Thanks!

    • @DrBenYelverton
      @DrBenYelverton  วันที่ผ่านมา +2

      Thank you - it's amazing how well simple models work sometimes!

  • @mohsenrezaei5965
    @mohsenrezaei5965 2 วันที่ผ่านมา +1

    brilliant! your work in this channel is priceless, thank you

    • @DrBenYelverton
      @DrBenYelverton  วันที่ผ่านมา

      Thanks for your kind words! Glad you are enjoying the videos.

  • @paxshild4924
    @paxshild4924 22 ชั่วโมงที่ผ่านมา

    Hey Dr. Ben, it's great to see you back! I really enjoyed your recent video on the temperature of a star, especially after such a lon break. Your content always brings out some of the most interesting problems in physics!
    I was thinking, as a follow-up to this thermodynamics topic, what if you did a video exploring how temperature changes over time for an object in a completely empty vacuum? Specifically, if we consider an object with a certain initial temperature in an ideal vacuum (with no surrounding objects), how does its temperature evolve over time as it radiates heat away? I've been trying to come up with a satisfying equation for this, but it seems like Newton's law of cooling might not fully apply in this scenario. I feel like this could be a really fascinating continuation of your recent video.
    Also, I wanted to say that I'm deeply sorry for your loss, and I admire your resilience in continuing to share such amazing content. Looking forward to more thought-provoking problems from you!

    • @umylten4142
      @umylten4142 11 ชั่วโมงที่ผ่านมา +1

      Just for fun (as almost all assumptions are incorrect), assume:
      - constant density r
      - constant specific heat capacity c
      - uniform temperature T(t)
      - black body radiation
      Then, thermal energy is (up to a constant) r•c•V•T(t) (where V is the volume) and radiated power is s•A•T(t)⁴ (where s is Stephan-Bolzmann constant and A is the area of the object).
      Equating the loss of thermal energy with the radiated power:
      r•c•V•(dT/dt) = -s•A•T⁴
      This is a simple differential equation which provides T(t) :^) If I didn't mess up, the result is
      T(t) = T(0)/[(1 + bt)^(1/3)]
      where b = 3•s•A•T(0)³/(r•c•V).

    • @paxshild4924
      @paxshild4924 2 ชั่วโมงที่ผ่านมา

      @@umylten4142 I tried to solve it a long time ago with the approach similar to yours which kinda worked but I'm not sure of it's accuracy hence I wanted to ask a professional

  • @Herogamergaming59
    @Herogamergaming59 วันที่ผ่านมา

    Sir after doing some analysis using the Stefan-Boltzmann law I found out that this model suggests that the intensity released by a star is proportional to the mass of the star raised to the power of 4 ! I find that quite interesting

    • @DrBenYelverton
      @DrBenYelverton  วันที่ผ่านมา

      Apparently, that is actually a pretty good approximation for Sun-like stars! See e.g. en.wikipedia.org/wiki/Mass%E2%80%93luminosity_relation

  • @mxminecraft9410
    @mxminecraft9410 3 วันที่ผ่านมา +3

    Sir I have been doing a lot of physics problems some of them are very hard where can I share the problems with you?

    • @DrBenYelverton
      @DrBenYelverton  2 วันที่ผ่านมา +1

      Feel free to email me at ben.yelverton@cantab.net!

    • @mxminecraft9410
      @mxminecraft9410 2 วันที่ผ่านมา +1

      @@DrBenYelverton ok

    • @mxminecraft9410
      @mxminecraft9410 2 วันที่ผ่านมา +3

      @@DrBenYelverton question sent

    • @DrBenYelverton
      @DrBenYelverton  2 วันที่ผ่านมา +1

      @@mxminecraft9410 Got it, looks interesting! I will have a go at solving it when I get the chance.

    • @mxminecraft9410
      @mxminecraft9410 2 วันที่ผ่านมา +3

      @@DrBenYelverton ok can you also upload a solution too?

  • @drscott1
    @drscott1 3 วันที่ผ่านมา +2

    👍🏼