Tuesday, December 2, 2008

Unilateral Orchiectomy

Isaac Newton e la sua legge della gravità


" Any object Universe attracts every other object with a force directed along the line joining the centers of gravity of the two objects , intensity directly proportional to the product of their masses and inversely proportional to the square of their distance " .



click here to read the full article gravity on Wikipedia




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la forza di gravità e le leggi di Keplero

The law of gravity



Gravity is one of the four fundamental interactions governing the entire universe . In classical mechanics gravity turns out to be a conservative force that occurs between bodies with mass , and therefore has a ' gravitational potential energy , in theory Ria of general relativity gravity is instead linked to the geometry (non-Euclidean) space-time of and deviates from the straight course, including massless particles, such as the foton .




Kepler's Laws



The three laws of planetary motion are the main contribution of Johannes Kepler, Kepler said, to ' astronomy and mechanics . Kepler derived in part by studying the observations of Tycho Brahe . Isaac Newton was later verified the validity of these laws in light of theory of universal gravitation .



FIRST LAW
L ' orbit described by a planet is an ellipse , whose Sun occupies one of two fires .


SECOND LAW
The radius vector joining the center of the Sun with the center of the planet describes areas in equal times equal.


THIRD LAW
The squares of revolution periods of planets are directly proportional to the cubic and semi-major axes of their orbits.








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Monday, December 1, 2008

Add A Toolbox To Matlab

KEPLERO E NEWTON

PROF. RIGOLI G.

HELLO, BOYS!
we are studying Kepler's laws?
EVEN IF YOU DID NOT GET STARTED NOW.
and insert images that explains how to MOVE The planet around the sun.
Next: Gravity '
AND THE LAW OF NEWTON.



The orbits of the planets are ellitticheGiovanni Kepler (1571-1630), astronomo tedesco, derivò le tre leggi del moto dei pianeti che successivamente influenzarono le idee di Newton quando ricavò le leggi della gravitazione universale. Nel 1597 Keplero pubblicò il Mysterium cosmographicum che lo fece conoscere al grande astronomo Tycho Brahe e a Galileo Galilei.Durante il suo soggiorno a Praga, tra il 1600 e il 1611, egli calcolò l'orbita di Marte e ricavò le prime due leggi del moto dei pianeti.Nel 1619, Keplero pubblicò la terza legge che assieme alle prime due furono descritte nella sua opera maggiore, l'Epitome astronomiae copernicanae, edita in sette libri dal 1618 al 1621. L'opera di Keplero ebbe una grande influenza nell'astronomia del Seicento.