Recent content by Thomas Smith

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    Exploring the Scale & Density of the Universe

    I thought that in regards to the number of hydrogen atoms you needed to include it
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    Exploring the Scale & Density of the Universe

    Firstly i worked out the scale factor of the universe R(t)/R(t0) = 1/1+z = 1/1+11.1 = 1/12.1 = 12.1^3 = 1/1772 The distance between the galaxies were 12.1 times less than today and the volume was 1772 times smaller than today. Then I think the average density in the universe at that time is...
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    What is the mean moleculer weight of the gas at the solar core?

    Thank you for your reply, what units is my answer in? mH ?
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    What is the mean moleculer weight of the gas at the solar core?

    Here, i have provided the description of the mean molecular weight from my course notes as well as my workings. I'm not sure about my values for X and Y. It states that X=1 if all of the hydrogen is ionised which i think the 1 represents 100% hydrogen but the core is also made up...
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    Binary System in circular orbit: Separation distance between stars

    Ah sorry, i missed out the inclination. It says the orbital plane is inclined to the plane of the sky by 90 degrees
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    Binary System in circular orbit: Separation distance between stars

    Well considering the separation of 0.04nm every 26 years, I believe the full orbit period is 52 years.
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    Binary System in circular orbit: Separation distance between stars

    Distance is d=1/0.07 = 14.3 parsecs The Doppler shift of one star is, Δλ = 512 - 512.04 = -0.04 So the radical of the velocity of the star is = (-0.04/512) x (3.00 x 10^5 km/s) = 23.4km/s which is the same for both stars because they have the same mass. This is as far as I've got.
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    What are the uncertainty values for my corrected magnitudes?

    I'm unsure about the brackets in the equation. Is this correct? ## \sqrt{((a/b)^2 + (x/y)^2)}## Or should it be ## \sqrt{(a/b)^2 + (x/y)^2}##
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    What are the uncertainty values for my corrected magnitudes?

    Homework Statement I need to work out the errors of my corrected apparent magnitudes. The Colour Excess is 0.36 with uncertainty = 0.01 The star was observed in two wavebands. r-band = 2.285 g-band = 3.303 The 2.285 and 3.303 are the ratios R_V for the SDSS (Sloan digital sky servery) r and...
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    How do I determine the uncertainty value of the star's absolute magnitude?

    I've did my calculations again and got the absolute magnitude uncertainty of 0.21. I did 0.4343 x 500/6300 ∆log(d) = 0.0345 ∆5log(d) = 0.0345 × 5 = 0.1725 ∆M = sqaureroot of (0.033030)^2 + (0.1725)^2 ∆M = 0.20553 rounded up to 0.21
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    How do I determine the uncertainty value of the star's absolute magnitude?

    Homework Statement I have a star that has an apparent magnitude of 13.73 with uncertainty of 0.03303 It's distance Modulus is 13.9967 so it's absolute magnitude is -0.26 The distance is 6300 parsecsHomework Equations [/B] The uncertainty on log10(d) is given by Δ(log10)≈0.4343 Δd/d ΔQ) =...
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