Universal gravitation worksheet answer

    • [DOCX File]Gravity Force Simulation Activity.docx

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      Explain why the Earth orbits the Sun (you must use both the terms gravity and inertia in your answer). Earth is an object in motion so according to newton the Earth would keep travelling forward forever until it runs into another object or is disturbed by an unbalanced force. The Sun’ gravity provides that unbalanced force.

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    • [DOC File]1 - Portland Community College

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      The Universal Gravitation Constant (G) is 6.67x10-11 N.m2/kg2. a. Use Newton’s Universal Law of Gravitation to calculate the gravitational force (weight) for a 70 kg person standing on the surface of the Moon. b. What is the gravitational acceleration on the surface of the Moon? Use you answer to . Part A. to find this value. c.

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    • [DOC File]Unit 2: Universal Motion

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      Unit 2: Universal Motion – Review Worksheet. Directions: Answer the following questions. 1: Kepler’s Laws. Describe an ellipse. Label the parts of an ellipse. The eccentricity of an ellipse measures _____ _____. Explain Kepler’s 1st Law.

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    • [DOCX File]POGIL:

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      is a constant of proportionality, called the Universal Gravitational Constant, equal to 6.67×10−11 N-m2/kg2. This equation is known as Newton’s Law of Universal Gravitation. It was discovered by the same Newton who gave us our trusty three laws of motion. The diagram below shows a 10 kg mass and a 70 kg mass separated by a distance of 1 m. 1 m

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    • [DOCX File]WORKSHEET -- UNIVERSAL GRAVITATION

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      WORKSHEET – Universal Law of Gravitation For an object to have weight, it must interact with another object. In other words, weight is dependent upon the surroundings. Any two masses will exert a mutual, attractive force, upon each other, called the gravitational force.

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    • [DOC File]WORKSHEET -- UNIVERSAL GRAVITATION

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      WORKSHEET – Law of Universal Gravitation. mass of: radius of: Earth ( 5.98 x 1024 kg Earth ( 6.38 x 106 m. Jupiter ( 1.91 x 1027 kg Jupiter ( 7.14 x 107 m . Mars ( 6.43 x 1023 kg Mars ( 3.40 x 106 m. Mercury ( 3.32 x 1023 kg Mercury ( 2.44 x 106 m. moon ( …

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    • [DOC File]Lesson 1 | Gravity and Friction

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      Key Concept What is the law of universal gravitation? This diagram represents a star orbited by two planets—planet A and planet B. The star is also orbited by a mysterious object, object X, that entered into the star’s gravitational field. Directions: Use the diagram to answer each question or respond to each statement. 1.

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    • [DOC File]Universal Gravitation - St. Louis Public Schools

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      Universal Gravitation PhET Lab. ... Conclusion Questions and Calculation: (½-point each) – circle the correct answer in 1-6. Show all work for problems 7-16. Attach a separate sheet of notebook paper if necessary. Gravitational force is always attractive / repulsive.

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    • [DOC File]Section 3 - Tredyffrin/Easttown School District

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      Newton’s Law of Universal Gravitation states that the gravitational force between two masses (say, the earth and the moon), m and M, is equal to their product divided by the square of the distance r between them. Mathematically, where G is the Universal Gravitational Constant .

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    • [DOCX File]Newton’s Law of Universal Gravitation

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      Universal Gravitation Practice Problems. Universal Gravitation: F G = G m 1 m 2 r 2 , G = 6.67 x10-11. Nm. 2 /kg. 2. Class Work. Two spherical objects have masses of 200 kg and 500 kg. Their centers are separated by a distance of 25 m. Find the gravitational attraction between them. Two spherical objects have masses of 1.5 x 105 kg and 8.5 x ...

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