The
discovery of the elliptical orbit concept propelled me towards
another simple but important conclusion. Again, using Brahe's
observational data coupled with my own study, I determined that the line from
the sun to a given planet sweeps out equal areas of the ellipse of its orbit
during equal time intervals. As shown below, at the aphelion the planet
covers less distance along its orbital path, while more
distance is covered along its orbital path when rounding the perihelion. This relationship holds because when planets are further from the sun they move at slower orbital rates than when they are closer to the sun. In turn, the two shaded areas are in fact equal!
This concept has gone down in the history books as my "Second Law of Planetary Motion." More importantly, in my opinion, this analysis led me to ponder the relationship between the size of a given planet's orbit and the amount of time it takes said planet to make one complete revolution about this orbit, and therefore, one complete revolution around the sun (call this time period, P).
P2 = a3
Here is an example that should inspire the reader's belief, if in fact it is lacking. For simplicity, let's assign a value of 1 astronomical unit (AU) to the length of earth's semi-major axis, a. Also, let P = 1 earth year. Given these values of course the equality holds: (1)2 = (1)3 . Keep in mind that one earth year is equal to 365 24-hour periods we conventionally call "days." Trust me when I tell you that Brahe's observational data provides us with the length of Mars' semi-major axis with relation to the earth's, a value of 1.524 AU's (a = 1.524). Cubing this value yields 3.54. By our equation, recall that this equals, P2 . In order to solve for P we must take the square root of 3.54; it is 1.88. In other words, the time it should take Mars to orbit the sun is equivalent to 1.88 earth years. You now know by much more rigorous observational data and measurements than I was ever privy to that Mars makes one complete orbit about the sun every 687 earth days, which is precisely equal to 1.88 earth years! See the steps below of the aforementioned mathematical operations:
1) P2 = a3
2) a = 1.524 AU, so a3 = (1.524)3 = 3.54
3) Therefore P2 = 3.54.
4) Take the square root of both sides (or raise both sides to the 1/2 power) to solve for P.
5) (3.54)(1/2) = 1.88 earth years ~ 687 earth days!
So therein lies the third and final planetary motion law that I derived in my lifetime. Note that if we wish to use another type of measure such as kilometers rather than the simple units of earth years and astronomical units, I did in fact derive the appropriate constant that would allow us to do so (go here for more information), which still yields the same proportional relationship.
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Thank you for indulging this humble, hind-sighted look at my planetary motion laws. I am proud and so thankful to God that he enabled me to do all of this work and that it seems to have paid off for the good of humanity and His creation. As I said when I started, it would not have been possible without Him, or without those who came before me. What's even more rewarding than having my name attached to these laws in the history books is the view I've gotten from up here as others have continued to build on my work. As a matter of fact, as I write this, one Sir Isaac Newton is close to proving that these laws hold not just in our solar system, but anytime one object moves under the influence of another object's pulling force - something he calls gravity. That is to say, these laws may very well hold as general universal principles - who would've thought! Sir Isaac, I suppose...
For kicks, I'll leave you with a picture that I found of myself. Someone photo-shopped me over a pic of our solar system, as if I created it or something. A little presumptuous but it certainly gave me a good laugh! Anyway, take care for now and God bless.
Sources:
1. http://oneminuteastronomer.com/8626/keplers-laws/
2. https://en.wikipedia.org/wiki/Semi-major_and_semi-minor_axes
3. http://www.windows2universe.org/the_universe/uts/kepler3.html
4. https://www.youtube.com/watch?v=KbXVpdlmYZo
5. http://whoisbiography.com/johannes-kepler-biography/
3. http://www.windows2universe.org/the_universe/uts/kepler3.html
4. https://www.youtube.com/watch?v=KbXVpdlmYZo
5. http://whoisbiography.com/johannes-kepler-biography/
