sobota, 6 września 2008

I Law of Kepler

The first law of Kepler states that every planet of the solar system will move around the Sun on the ellipse, in which he is one of bonfires Sun.
He results from the property of the ellipse, that for two locations of the planet, P1 and P2, is fulfilled
where O it Sun
It results from the law of mechanics that this law correctly is describing the movement of the planet in the agreement connected with the Sun. In the inertial arrangement both planet as well as alone Słońce are making a move after ellipses having one shared bonfire. This bonfire is coinciding with the centre of mass of the arrangement.
It is possible to circumscribe the ellipse to a lot of ways, in astronomy ellipses are most often circumscribed giving their large semi-axis (a) and eccentric (e) which the step of flattening the ellipse is describing (for them oh closer for nought, the closer ellipse is it for circle). When we know the length of the c segment between the middle, but one of bonfires we can write the pattern to the eccentric of the ellipse "e" equal:
e= c/a
Kopernik building one's model of the system heliocentycznego based sie still on the idea of combining uniform motions all over the district. It made it keep in the model several dozen small epicykli. Only Kepler exchanging these districts for ellipses got rid koniecznosci of leading epicykli.
Orbits of planets in our arrangement are largely little. Outside Mercury for which the eccentric exceeds 0.2 value a little bit, ellipses of orbits of remaining planets are below value 0.1.

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