How to find a planet s orbital period
[DOC File]Teacher Guide - Adventures with Science - Home
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Activity C – Students find the relationship between a planet’s orbital radius and period. Suggested Lesson Sequence. Pre-Gizmo activity: Solar System Explorer ( 45 – 60 minutes) Use the Solar System Explorer Gizmo to introduce students to the geometry of planetary orbits.
[DOC File]UC Observatories
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A) the planet's size. B) the planet's mass. C) the planet's density. D) the orbital period of the planet. E) the orbital eccentricity of the planet. Answer: E. 24) The depth of the dip in a star's brightness due to the transit of a planet depends most directly on . A) the planet's mass. B) the planet's density. C) the planet's size. D) the size ...
[DOCX File]All Bottled up: The Perfect Ecosystem
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Orbital period (period of revolution) Rotational period. Number of satellites. Surface temperature (°C) Make sure students use the same units. Also, have students on opposite teams confer with each other to ensure they are using the same data for the same planets (e.g., make sure both Mercury posters use an orbital period of 88 days).
[DOC File]Part 1: Masses and Springs
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Understand Kepler’s Laws of orbital motion. Discover how does the distance and planet’s tangential speed affect the shape of the orbit. Measure the change in orbital period as distance is increased. Apply concepts relating to Kepler’s Laws to speculate conditions that lead to a stable planet …
[DOC File]Kepler's Laws of Planetary Motion
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(One planet's sidereal period/another planet's sidereal period)2 = (one planet's average distance from Sun/another planet's average distance from Sun)3. If you compare the planets to the Earth (with an orbital period = 1 year and a distance = 1 A.U.), then you get a very simple relation: (a planet's sidereal period in years)2 = (semimajor axis ...
[DOC File]PT3 Lesson Plan Rubric - ARRL - Home
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Kepler’s 3rd law states that the semi-major axis of a planet’s orbit (average distance to the sun in A. U.’s) is related to the planet’s orbit period (in Earth-years) by the equation: p2 = a3. Where p = orbital period in Earth years and a = distance from sun in A.U.’s.
[DOC File]TAP303-0: Orbital motion
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The square of the period of a planet’s orbit is directly proportional to the cube of its mean distance from the Sun. These laws apply for all satellite motions (not just for the planets around the Sun). Remember that circular orbits are just a special case of elliptical orbits.
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