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An astronomy assignment focusing on deriving the transformations between cartesian, spherical polar, equatorial (ra/dec or α/δ), and ecliptic (lat/long or β/λ) coordinates. Students are required to complete the derivation started in class, calculate the locations of planets in both systems, and follow specific grading guidelines.
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Astr 345 Assignment 2: equatorial and ecliptic coordinates
Due before midnight Fri, Sep 5, 2008 (full credit), before midnight Fri Sep 12, 2008 (half credit)
x = R cos ψ cos φ y = R cos ψ sin φ z = R sin ψ
NOTE the non-standard definition: r represents the distance from the origin, ψ represents the latitude, i.e., the angle from the xy plane, and φ represents the azimuthal angle, i.e., the angle in the xy plane from the x axis measured counterclockwise.
cos δ sin α = cos β sin λ cos − sin β sin sin δ = sin β cos + cos β sin λ sin cos β sin λ = cos δ sin α cos + sin δ sin sin β = sin δ cos − cos δ sin α sin cos δ cos α = cos β cos λ
Grading: