QUESTION 2 Official names and orbital information for solar system objects Planet Perihelion - Aphelion (AU) PLANET Orbital Eccentricity Mercury 0.307 - 0.466 0.205 Venus 0.718 - 0.728 0.007 Sun (Focus) Earth 0.983 - 1.016 0.016 Mars 1.381 - 1.665 0.093 Jupiter Saturn 4.951 - 5.455 0.048 9.020 - 10.053 0.054 Aphellion Uranus 18.286 - 20.096 0.047 Perihelion Neptune 29.810 – 30.327 0.008 Using the perihelion and aphelion measurements, as well as the eccentricity value, find the polar equation that defines an elliptical orbit of the planet that you selected. Upload your work and an equation. Attach File Browse My Computer QUESTION 3 Using the perihelion and aphelion measurements (from the table from part 2) of your planet, find the polar equation for an ovular orbit, as defined by Cassini. Upload your work and an equation. Attach File Browse My Computer QUESTION 4 Using the polar equation (of the elliptical orbit) that you found in part 2 of this lab, and what you learned in this chapter, estimate the distance traveled in one complete orbit around the Sun. Upload your work and answer. Attach File Browse My Computer

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Vertices Of An Ellipse

In the study of the conic section of the geometry, An ellipse is a plane curve surrounding two focal points, or foci where the set of all locus of points in the plane has their sum of the distances to the two foci is constant. On the ellipse curve, it is the intersection point of the main axis. In an ellipse graph, the center of the axis is the midpoint of the line segment connecting the foci. The major axis is the line section that runs through the ellipse's foci, while the minor axis runs through the middle and is perpendicular to the major axis.. The ellipse has two endpoints on the major axis which are known as the vertices (in plural), vertex in the singular. The equation of the major axis is 2a, the equation of the minor is 2b and the distance between the major axis and minor axis is 2c. The semi-major axis has a length of a and the semi-minor axis has a length of b. The ellipse's vertices are determined by the elliptical orbit's equation and graph.