Answer: D by eachristenbury. Keplerâs three laws of planetary motion can be summarized as follows: Keplerâs first law: Each planet moves around the Sun in an orbit that is an ellipse, with the Sun at one focus of the ellipse. 2.6023 X 10-5N 7. Keplerâs second law: The straight line joining a planet and the Sun sweeps out equal areas in space in equal intervals of time. 54,7771.53 m (340 mi) 16. Today they are part of the history of science. 60 seconds . The orbit of a planet is an ellipse with the Sun at one of the two foci. Refer back to Figure 7.2 (a). the perihelion. Keplerâs first law of planetary motion states that the paths of the planets, which revolve around the Sun, is elliptical in shape. c) any object orbiting any other object. 1. SURVEY . Answers 1. Answer: B a. at the same speed at all times during its orbit about the Sun ... closer to the Sun during its orbit c. at slower speeds when positioned closer to the Sun during its orbit 4. b) move fastest when near the sun. 1. 5.76 X 1010m 2. Johannes Keplerâs three laws of planetary motion are described as follows. Keplerâs law â problems and solutions. ... answer choices . The Earthâs distance from the Sun is 149.6 x 10 6 km and period of Earthâs revolution is 1 year. Notice which distances are constant. Q. Kepler's laws DRAFT. ... Parabolic motion, work and kinetic energy, linear momentum, linear and angular motion â problems and solutions. Introduce your physics or astronomy class to Kepler's laws of planetary motion with this straightforward worksheet. Played 406 times. It covers the basic concepts of each and has learners answer questions to ⦠12 Using Keplerâs 3rd Law of Planetary motion, determine the distance between the center of the Earth and the center of the Sun. b) any object orbiting any star. 2. The Sun is located at the centre and acts as the focus. Tags: Question 4 . This 2 page worksheet with complete teacher's answer key makes it easy to integrate math into your astronomy lesson. the axis. 9.3416 X 10-7 N 8. Calculations Related to Keplerâs Laws of Planetary Motion Keplerâs First Law. It would be like you writing a test, and even though you did all the work on a question wrong, you somehow get the correct final answer. You wouldnât use Keplerâs laws in astronomy, in planning space missions, or in understanding how the solar system formed. the center. 9 times farther away 15. Calculate T 2 / r 3. The foci are fixed, so distance f 1 f 2 ¯ f 1 f 2 ¯ is a constant. Students put Kepler's Laws into their own words and apply simple formulas to given values for the 8 planets to test his 3rd law of planetary motion. Question 2: The ellipse to the right has an eccentricity of about … a) 0.25 b) 0.5 c) 0.75 d) 0.9 Question 3: For a planet in an elliptical orbit to âsweep out equal areas in equal amounts of timeâ it must … a) move slowest when near the sun. 3 years ago. Kepler's Laws and Planetary Motion ... 3. Although Keplerâs math was essentially wrong, the three laws he came up with were correct! Keplerâs First Law . Start studying Kepler's Laws of Planetary Motion and Universal Gravitation Law Worksheet. Learn vocabulary, terms, and more with flashcards, games, and other study tools. the Sun. A planet would move ____. Kepler's third law of planetary motion states that the ratio of ____. UNIVERSAL GRAVITY AND KEPLER'S LAWS WORKSHEET. 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