Measuring Rotational Speed of Io w/Doppler & Relative Velocity to Jupiter

AI Thread Summary
To measure Io's rotational speed using a spectrograph and the Doppler formula, it's essential to consider its velocity relative to Jupiter. The angle of observation affects the measurement, as Io does not rotate at a right angle to the observer. The solution involves calculating the dot product of Io's velocity vector with the unit observation vector. This calculation yields the radial velocity, which translates into red or blueshift according to the Doppler effect. A larger radial velocity is achieved when Io's motion is parallel to the observation vector.
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I want to measure the rotational speed of Io using a spectrograph, using the doppler formula. Since it is rotating around Jupiter, i have to take the velocity relative to jupiter, but I wonder tough how this is possible when Io is not rotating at an right angle to my observation point. Is there some mathematical way to solve this?
 
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Link said:
I want to measure the rotational speed of Io using a spectrograph, using the doppler formula. Since it is rotating around Jupiter, i have to take the velocity relative to jupiter, but I wonder tough how this is possible when Io is not rotating at an right angle to my observation point. Is there some mathematical way to solve this?

You'll want to take the dot product of Io's velocity vector with your unit observation vector (a magnitude 1 vector pointing towards Io):

v_r = \vec{v}_{total} \cdot \hat{u}

This translates into red or blueshift in the usual way:

\frac{\Delta \lambda}{\lambda}=\frac{v_r}{c}

Note that you'll want it to be moving parallel to your observation vector if you want a large radial velocity.
 
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