Estimating the area swept out by the orbit

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Reference no: EM133361933

Prove Keplers second law (numerically)

Use JPL Horizons Web app to retrieve some position data about an object orbiting the sun. Try to show Kepler's 2nd law by numerically estimating the area swept out by the orbit during a short time duration and comparing that area to an equal time duration at another location along the orbit.

You can pick your own object but it needs to have an eccentricity value greater than 0.1 (and less than 1.0) (Many comets are in this range)

You'll want to pick the right output values in your JPL Horizons query. The Observer range & range-rate and True Anomaly Angle are your best bets here. (Though you could do it will several others as well.)

Explain your process and the geometry you did.

Make a plot showing the orbit of the object you chose as well as the orbit of the Earth around the sun for a comparison/reference.

Reference no: EM133361933

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