Period of rotation formula

    • [DOC File]THE PERIOD OF ROTATION OF THE SUN

      https://info.5y1.org/period-of-rotation-formula_1_c14c93.html

      The simple formula you use to calculate the length of the Astronomical Unit A in km is: A= B • (Des - Dev) • 206265. πm• Dev• Des. CAUTION: Be sure your units are correct before you plug into this formula. B is in km, Dev and Des are both in AU, and πm is in arc seconds!

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    • [DOC File]Asteroid Rotation Periods

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      Asteroid Rotation Period Determination. The aim here is to measure the rotation period of an asteroid by means of photometry. For most asteroids the brightness variations are due to their non-spherical, elongated shape that is similar to a three-dimensional ellipsoid –ie something like a rugby ball.

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    • [DOC File]THE PERIOD OF ROTATION OF THE SUN

      https://info.5y1.org/period-of-rotation-formula_1_f98084.html

      The “true” rotation period of the Sun, known as the sidereal period of rotation, is the time it takes for a point on the Sun to rotate once with respect to the distant stars. In the time that it takes a point on the Sun to turn 360 degrees with respect to the stars, the Earth will have moved ahead in its orbit.

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    • [DOCX File]THE PERIOD OF ROTATION OF THE SUN

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      Once you have the synodic period, use the formula from page 6 to calculate the sidereal rotation period of the Sun, P[days]= (S * 365.25) / (S + 365.25) Show your work for sunspot A here, and then fill in Analysis Table 2 for each spot:

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    • [DOCX File]THE PERIOD OF ROTATION OF THE SUN

      https://info.5y1.org/period-of-rotation-formula_1_88452c.html

      Once you have the synodic period, use the formula from page 6 to calculate the sidereal rotation period of the Sun, P [days] = (S * 365. 25) / (S + 365. 25) Show your work for sunspot A here, and then fill in Analysis Table 2 for each spot: Analysis Table 2: Sidereal and Synodic Rotation …

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    • [DOC File]THE PERIOD OF ROTATION OF THE SUN

      https://info.5y1.org/period-of-rotation-formula_1_517bfa.html

      The distance modulus can be used to determine the distance of the cluster using the following formula: Log D = ((m-M)/5) +1 ANALYZING THE HR DIAGRAMS OF STAR CLUSTERS. USING THE VIRTUAL EDUCATIONAL OBSERVATORY, VIREO. Starting the Program. ... THE PERIOD OF ROTATION …

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