query: Elliptical path of planets
positive_passages.docid: 2305
positive_passages.text: Why are orbits elliptical?
negative_passages.docid: 3767
negative_passages.text: Constrained stars and bars.
negative_passages.docid: 156661
negative_passages.text: Why don't we feel the subtle speed change of Earth's elliptical orbit?
negative_passages.docid: 111044
negative_passages.text: Vector path length of a hypotenuse
negative_passages.docid: 63074
negative_passages.text: The equation of a family of circles passing through two given points
negative_passages.docid: 97548
negative_passages.text: Number of normals from a point to an ellipse
negative_passages.docid: 142862
negative_passages.text: Intersection of an ellipsoid and plane in parametric form
negative_passages.docid: 120684
negative_passages.text: Calculating the number of possible paths through some squares
negative_passages.docid: 40475
negative_passages.text: Create a star system fit to conic equation
negative_passages.docid: 27531
negative_passages.text: Using map projections with astronomical data
negative_passages.docid: 7306
negative_passages.text: How is the equation of motion on an ellipse derived?
negative_passages.docid: 6001
negative_passages.text: Why are the orbits of planets in the Solar System nearly circular?
negative_passages.docid: 28840
negative_passages.text: ellipse circumference
negative_passages.docid: 118723
negative_passages.text: Finding the tangents common to two rotated ellipses?
negative_passages.docid: 442
negative_passages.text: Uniform Circular Motion
negative_passages.docid: 20775
negative_passages.text: Distribution of orbital velocities in a disk galaxy for N-body simulation?
negative_passages.docid: 15482
negative_passages.text: Paths integrals in the complex plane