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Thanks for reminding us SGT (Join to see) that March 8, 1618 Johannes Kepler discovers the third law of planetary motion which is "sometimes referred to as the law of harmonies - compares the orbital period and radius of orbit of a planet to those of other planets. The third law makes a comparison between the motion characteristics of different planets. The comparison being made is that the ratio of the squares of the periods to the cubes of their average distances from the sun is the same for every one of the planets.
Kepler discovered that the size of a planet's orbit (the semi-major axis of the ellipse) is simply related to sidereal period of the orbit. If the size of the orbit (a) is expressed in astronomical units (1 AU equals the average distance between the Earth and the Sun) and the period (P) is measured in years, then Kepler's Third Law says:
After applying Newton's Laws of Motion and Newton's Law of Gravity we find that Kepler's Third Law takes a more general form:
Image: Kepler's 3rd law equation - General Form
where M1 and M2 are the masses of the two orbiting objects in solar masses. Note that if the mass of one body, such as M1, is much larger than the other, then M1+M2 is nearly equal to M1. In our solar system M1 =1 solar mass, and this equation becomes identical to the first.
Summary
Kepler's 1st Law the law of ellipses - explains that planets are orbiting the sun in a path described as an ellipse. Kepler's first law is rather simple - all planets orbit the sun in a path that resembles an ellipse, with the sun being located at one of the foci of that ellipse.
Kepler's 2nd Law the law of equal areas - describes the speed at which any given planet will move while orbiting the sun. The speed at which any planet moves through space is constantly changing. A planet moves fastest when it is closest to the sun and slowest when it is furthest from the sun. Yet, if an imaginary line were drawn from the center of the planet to the center of the sun, that line would sweep out the same area in equal periods of time.
FYI COL Mikel J. Burroughs LTC Stephen C. LTC Orlando Illi Lt Col Charlie Brown Maj Bill Smith, Ph.D. Maj William W. 'Bill' Price CPT Jack Durish Capt Tom Brown MSG Andrew White SFC William Farrell Sgt Albert Castro SSG David Andrews Sgt Randy Wilber Sgt John H. CPL Dave Hoover SGT Mark Halmrast SPC Margaret Higgins SrA Christopher Wright
Kepler discovered that the size of a planet's orbit (the semi-major axis of the ellipse) is simply related to sidereal period of the orbit. If the size of the orbit (a) is expressed in astronomical units (1 AU equals the average distance between the Earth and the Sun) and the period (P) is measured in years, then Kepler's Third Law says:
After applying Newton's Laws of Motion and Newton's Law of Gravity we find that Kepler's Third Law takes a more general form:
Image: Kepler's 3rd law equation - General Form
where M1 and M2 are the masses of the two orbiting objects in solar masses. Note that if the mass of one body, such as M1, is much larger than the other, then M1+M2 is nearly equal to M1. In our solar system M1 =1 solar mass, and this equation becomes identical to the first.
Summary
Kepler's 1st Law the law of ellipses - explains that planets are orbiting the sun in a path described as an ellipse. Kepler's first law is rather simple - all planets orbit the sun in a path that resembles an ellipse, with the sun being located at one of the foci of that ellipse.
Kepler's 2nd Law the law of equal areas - describes the speed at which any given planet will move while orbiting the sun. The speed at which any planet moves through space is constantly changing. A planet moves fastest when it is closest to the sun and slowest when it is furthest from the sun. Yet, if an imaginary line were drawn from the center of the planet to the center of the sun, that line would sweep out the same area in equal periods of time.
FYI COL Mikel J. Burroughs LTC Stephen C. LTC Orlando Illi Lt Col Charlie Brown Maj Bill Smith, Ph.D. Maj William W. 'Bill' Price CPT Jack Durish Capt Tom Brown MSG Andrew White SFC William Farrell Sgt Albert Castro SSG David Andrews Sgt Randy Wilber Sgt John H. CPL Dave Hoover SGT Mark Halmrast SPC Margaret Higgins SrA Christopher Wright
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SGT (Join to see)
LTC Stephen F. Thanks for the great addition. I am amazed at the abilities of the men who have grasped these ideas
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An excellent read and post, SGT (Join to see). And thank you for sending me off to search for "Kepler's Witch".
https://www.goodreads.com/book/show/1021757.Kepler_s_Witch
https://www.goodreads.com/book/show/1021757.Kepler_s_Witch
Set against the backdrop of the witchcraft trial of his mother, this lively biography of Johannes Kepler – 'the Protestant Galileo' and 1...
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