Kepler s third law calculator

    • [DOCX File]

      Now, let’s look at Kepler’s third law, which compares the time that different planets take to go around. the Sun. Kepler’s original formulation of the third law says that . (orbital period ) 2 (length of long axis ) 3 = constant .This means that if you calculate this fraction for …

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    • [DOC File]Lick Observatory

      44) Each of the following lists two facts. Which pair can be used with Newton's version of Kepler's third law to determine the mass of the Sun? A) Mercury is 0.387 AU from the Sun, and Earth is 1 AU from the Sun. B) The mass of Earth is 6 × 1024 kg, and Earth orbits the Sun in 1 year. C) Earth rotates in 1 day and orbits the Sun in 1 year.

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    • [DOC File]The Physics Classroom

      Calculator; the provided table of planetary data. Description of Procedure: Students receive data for the period of the planets and the mean distance from the sun. The data is analyzed in order to develop the evidence for Kepler's third law of planetary motion. Alternative Materials and Procedure:

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    • [DOC File]Astro 18 - Planets and Planetary Systems - Winter 2002

      2) Testing Kepler's third law: We can test Kepler's third law, p2/a3 = constant, for the classical planets and dwarf planets in our own Solar System. Use Appendix E in Bennett (page A-14), or use one of the planetary science web links listed on our class web page, to fill in the second, third, and fourth columns of the following Table.

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    • [DOC File]

      Calculator; the provided table of data for Jupiter's moons. Description of Procedure: Students receive data for the period of the moons orbiting Jupiter and their mean distance from the Jupiter. The data is analyzed in order to determine if there is any evidence the moons of Jupiter follow Kepler's third law. Alternative Materials and Procedure:

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    • [DOC File]ASTR 1050: Survey of Astronomy

      Assume that you have a circular, edge on orbit and the mass of 55 Cancri is 0.95 times that of our sun or 1.9 x 1030 kg. 1. From Kepler's third law, obtain the orbital radius R. Remember to convert the period to seconds (there are 86400 seconds in a day). 2.

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    • [DOC File]PHYSICS CHAPTER 8 : Universal Gravitation

      When you use Kepler's third law to find the radius of the orbit of a planet or satellite, first solve for the cube of the radius, then take the cube root. This is easier to do if your calculator has a cube-root key. On TI-83 push math:4, then put in number, and press enter.

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    • [DOC File]Student Exploration Sheet: Growing Plants

      Kepler’s first law, one of three laws discovered by the German astronomer Johannes Kepler (1571–1630). Kepler’s first law states that planets travel around the Sun in elliptical orbits with the Sun at one focus of the ellipse. (Activity A continued on next page) Activity A (continued from previous page)

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    • [DOC File]The Revolution of the Moons of Jupiter

      You now have all the information you need to use Kepler’s Third Law to find the mass of Jupiter. But note that values you obtained from the graphs have units of days for p, and J.D. for a. In order to use Kepler’s Third Law, you need to convert the period into years by dividing by the number of days in a year (365), and the orbital radius ...

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    • [DOC File]Science RWLO Template Title Placeholder

      online access, printer, calculator, pencil and paper. Prerequisites: Students should have knowledge of Kepler’s third Law. Implementation: This RWLO can be used as a laboratory project or as a homework assignment. Students can work individually or in groups of up to two. 1.

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