what are the 3 keplers law
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Kepler's laws are also called as Kepler's laws of planetary motion
KEPLERS FIRST LAW :
" All planets move around the sun in elliptical orbits with the sun situated at one of its focci " .This is also called as law of orbits .
Where the closest point P is called as perhilion and the farthest point A is called as Apehilion
a is called as semi major axis and b is called as semi minor axis
KEPLERS SECOND LAW :
" The line that joins the sun and any planet sweeps equal area in intervals of time " This is also called as law of areas
KEPLER'S THIRD LAW :
" The square of the time period of revolution of a planet is proportional to the cube of the semi major axis of the elliptical orbit "
This law is also called as law of periods T^2 proportional to R ^3
here's the pics of first and second laws of KEPLER
hope ull get the answer to the given question and mark as brainliest one.....
Kepler's laws are also called as Kepler's laws of planetary motion
KEPLERS FIRST LAW :
" All planets move around the sun in elliptical orbits with the sun situated at one of its focci " .This is also called as law of orbits .
Where the closest point P is called as perhilion and the farthest point A is called as Apehilion
a is called as semi major axis and b is called as semi minor axis
KEPLERS SECOND LAW :
" The line that joins the sun and any planet sweeps equal area in intervals of time " This is also called as law of areas
KEPLER'S THIRD LAW :
" The square of the time period of revolution of a planet is proportional to the cube of the semi major axis of the elliptical orbit "
This law is also called as law of periods T^2 proportional to R ^3
here's the pics of first and second laws of KEPLER
hope ull get the answer to the given question and mark as brainliest one.....
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Answer:
KEPLER'S 3 LAW
Explanation:
KEPLER'S 1 LAW
planetary orbit are elliptical of the sun at a focus .
KEPLER'S 2ND LAW
the radius vector from the sun to planet sweeps equal areas to equal form.
KEPLER'S 3RD LAW
a planet orbital period of proportional to size of the orbit .
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