Where is the Sun located according to Kepler's First Law of Planetary Motion regarding the ellipse?
Answer
At one of the two foci of that ellipse.
Kepler's First Law of Planetary Motion explicitly defines the orbital geometry by stating that the Sun, as the central star, is not positioned at the exact center of the orbit. Instead, the Sun occupies one of the two specific points known as the foci of the ellipse. If the Sun were positioned in the exact middle, the resulting path would be a circle, which is mathematically categorized as a degenerate form of an ellipse where both foci converge into a single central point. The placement of the Sun at one focus ensures that the planet's distance from the Sun constantly changes throughout its revolution.
#Videos
Why Are Planetary Orbits Elliptical? - YouTube
Related Questions
Where is the Sun located according to Kepler's First Law of Planetary Motion regarding the ellipse?What term quantifies the degree to which a planet's orbit deviates from being a perfect circle?What path shape results if a celestial object's eccentricity ($e$) is 1 or greater?What is defined as the longest radius of an ellipse, representing half its longest diameter?What term describes the point in an orbit where a planet moves at its maximum orbital velocity?What is the name given to the farthest point a planet reaches from the Sun during its revolution, where its speed is minimum?Which physical conservation law necessitates the variation in planetary speed between perihelion and aphelion?What orbital parameter, approximately 0.205 for Mercury, results in the highest eccentricity among major solar system planets?What did Isaac Newton provide that explained the underlying physical cause for elliptical orbits described by Kepler?How is an ellipse mathematically defined based on the sum of distances relative to its two fixed points?How do the orbital eccentricities of typical comets compare to those of major planets like Earth in terms of path stretching?