Orbital period formula physics
[DOCX File]HSC PHYSICS NOTES - aceh.b-cdn.net
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Orbital Speed (Instantaneous tangential velocity) V= 2 π r T Centripetal Acceleration. Ac= v 2 r . Centripetal Force. Fc= m v 2 r . Where: r = Radius of the circle in meters . T = Period of Rotation in seconds . v = instantaneous velocity. m = mass of object in motion
[DOC File]test # 3 (unit III) – GRAVITY – “One Force To Rule Them All”
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( be able to describe (qualitatively) how the orbital period of a planet varies with distance from the Sun (or the period of one of Jupiter’s moons varies with distance from Jupiter) Sources: University of Nebraska Astronomy Apps; The Physics Classroom; learner.org
[DOC File]Physics 150 - Lawrence University
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Find an approximate expression for the force of gravity that holds a planet on an orbit about the Sun if the relationship between orbital period and orbital radius is T2 ~ r3. 10m. 30° R = 5m. 45˚ Final. Initial. 45o. m2 = 1 g. v2 = 5 m/s. m1 = 1 g. v1 = 10 m/s
[DOC File]PHYS 228 Astronomy & Astrophysics
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Orbital period Pluto-Charon system 6.4d. Motions. Orbital radius a = 39.4 AU (range 30 - 49 AU) Orbital period Porb = 249 yr. Rotation period Prot = 6.5d. Eccentricity e = 0.25. Physical Characteristics Mass M = 0.0018 M( (order magnitude less than Earth’s moon) Radius R …
[DOC File]Lick Observatory
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What (approximately) is the orbital period of this planet? Explain your answer. Answer: The orbital period of the planet would be approximately the same as that of the earth (1 year). Kepler's law considers only the sum of the object masses. In comparison with the …
[DOC File]PT3 Lesson Plan Rubric - ARRL - Home
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Where p = orbital period in Earth years and a = distance from sun in A.U.’s. In other words, p2/a3 = 1 if Kepler’s 3rd law is to hold true for all planets. Mathematically prove the accuracy of this law by computing and recording p2, a3, and the value for p2/a3 (round answers to .01) in the following table: planet. orbital period. semi-major ...
[DOC File]Physics 150 - Lawrence University
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Find an approximate expression for the force of gravity that holds a planet on an orbit about the Sun if the relationship between orbital period and orbital radius is T2 ~ r3. Consider a ramp of length 1 m and angle of incline 30 degrees. A block of mass 5 kg is released from rest from the bottom of the ramp.
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