"\\nu = \\nu_0 \\frac{\\sqrt{1-\\frac{v^2}{c^2}}}{1-\\frac{v}{c}cos\\theta}"
where "v" is a velocity of source relative to the observer, "\\theta" is the angle between directions of source and observer. When source is behind the observer, "\\theta=0"; when the source will be ahead, "\\theta=\\pi".
To find relative velocity, we use relativistic velocity-addition formula:
"v = \\frac{u_2-u_1}{1-\\frac{u_1u_2}{c^2}}= \\frac{c\/2-c\/3}{1-1\/6}= \\frac{c}{5}"
Before the moment of meeting (source is coming closer):
"\\nu = \\nu_0 \\frac{\\sqrt{1-\\frac{1}{5^2}}}{1-\\frac{1}{5}}= \\nu_0 \\frac{\\sqrt{24}}{5}\\frac{5}{4} = 1.225 \\nu_0"
After the moment of meeting (source becomes more and more distant from the observer):
"\\nu = \\nu_0 \\frac{\\sqrt{1-\\frac{1}{5^2}}}{1+\\frac{1}{5}}= \\nu_0 \\frac{\\sqrt{24}}{5}\\frac{5}{6} = 0.816\\nu_0"
Comments
Leave a comment