Recent content by redbaldyhead

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    The determination of frequency v from Planck's formula

    Homework Statement B=10^-7Wm^-2Hz^-1sr^-1;T=10^4K h=6.6x10^-34J.s k=1.4x10-23JK^-1 c=3.0x10^8m^-1 Homework Equations Calculate v fom Bv(T)=(2hv^3)/(c^2)x1/(exp(hv/kT)-1) The Attempt at a Solution I have managed to obtain a LHS= (Bc^2/2h)xexp(h/kT) but RHS is posing a problem...
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    Dealing with an exponentially debilitating problem

    Actually =Bc^2 exp(h.kT)/2h I think I correctly calculated the exp(h/kT) bit but I just can't figure out the rest of the equation on the RHS Thanks for looking
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    Dealing with an exponentially debilitating problem

    Sorry for the delay in responding! No it is the RHS of Planck's equation for B(v)T The LHS as I have reduced it to =Bc^2/2H
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    Dealing with an exponentially debilitating problem

    I can't resolve v(cubed)/exp(v)-1 which is the RHS of an equation that has been sorted out of the left! I am rather hoping that this becomes v(cubed)/v which simplifies to v^2. Thanks
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    Calculating Absolute Magnitude of a Star - Red's Help

    Can anyone help me get my head around this one? A star with a parallax angle of pi = 10 millisecs and has apparent magnitude of V= 10.2 How can I determine absolute magnitude: I have the formula M=v -5logd -5 +A which can be ignored. d=1/pi but I am always determining d which is less than...
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    Thick as a planck and making a spectra of myself

    Thanks to all you good guys! Is the Planck function mentioned above, valid for high frequency range where v>>kt/h? What would a graph look like; v against kt/h?...an exponential rising upwards and rapidly from 0. How would the range on the y-axis appear 10^-1 to 10^-10 for example or the...
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    Thick as a planck and making a spectra of myself

    Thanks 82 I actually thought that the result would be of little consequence; I'll look closely at the differentiation! Obviously now that I see it, with h=constant and K=constant, any overall increase over 1 must mean the value of v increases against T which I assume doesn't change either...
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    Thick as a planck and making a spectra of myself

    Thanks for looking; I have been looking at Rayleigh Jeans Formula and I need to understand what happens for hv>>kT
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    Thick as a planck and making a spectra of myself

    for hv>>kT how does exp(hv/kT) compare to 1? I understand hv >>KT leads to an exponential fall in brightness but why did Planck introduce 1 in his equation. and only for values hv<<kT can this exponential be expanded! Thanks for any help!
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