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zero. The x-component  of acceleration can be found from the data of
                  the velocity  acquired in a given time. Since the forces  are constant , the
                  x-acceleration is constant therefore we have the next  equation
                                                                      m
                                                                   4
                                                        v   v 0      s        m
                                                        a                2
                                                   x
                                                           t        2s        s 2
                  The resultant of the forces is
                                                                         
                                                       F   F   F   m g   N ,
                                                               fr
                                                        x
                                                           
                  where   F    frictional force ,   N    - supporting force
                               fr
                                     
                  So that  gm       N   in component form

                                                      F   F   F .
                                                              fr
                                                       x
                  Hence  we can apply Newton's second  law to the block
                                                    F   F  fr    ma .
                                                x
                                                                x
                  When the block is in motion on the horizontal surface
                                                     F  fr     mg .

                  Then
                                    F       mg    ma   x     F     m  (a     ) g 
                                      x
                                                                    x
                                                 m                m
                                     10kg    2 (      , 0  05 10  )   25N   ..
                                                s  2              s 2
                                                                4   GRAVITATION

                        4.1 Newton's law of  Universal  Gravitation. Kepler's laws .

                          Gravitation,  or  gravity,  is  a  natural  phenomenon  by  which
                  physical  bodies  attract  with  a  force  proportional  to  their  masses.

                  Gravitation is most known  as the agent that gives weight to objects with
                  mass  and  makes    them    fall  to  the ground  when dropped.  Gravitation
                  causes  dispersed  matter  to  coalesce,  and  coalesced  matter  to  remain

                  intact, thus accounting for the existence of the Earth, the Sun, and most
                  of the macroscopic objects in the Universe.
                         Gravitation is responsible for keeping the Earth and the other
                  planets in their orbits around the Sun; for keeping the Moon in its orbit

                  around the Earth; for the formation of tides; for natural convection, by
                  which fluid flows occur under the influence of a gravity; for heating the
                  interiors of forming stars and planets to very high temperatures; and for

                  various other phenomena observed on the Earth.




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