ºÝºÝߣshows by User: AlokKumar1221 / http://www.slideshare.net/images/logo.gif ºÝºÝߣshows by User: AlokKumar1221 / Mon, 19 Oct 2020 05:44:23 GMT ºÝºÝߣShare feed for ºÝºÝߣshows by User: AlokKumar1221 Keplers laws of planetry motion /slideshow/keplers-laws-of-planetry-motion/238910075 keplerslawsofplanetrymotion-201019054423
Kepler’s laws of planetary motion (1) the orbit of each planet is an ellipse with the Sun atone focus. the first law consequence of the conservation of energy of a planet orbiting the Sun under the effect of a central attraction that varies as the inverse square of distance. (2) the orbital radius of a planet sweeps out equal areasin equal intervals of time. The second law describing the rate of motion of the planet around its orbit follows directly from the conservation of angular momentum of the planet. (3) the ratio of the square of a planet’s period (T2) to the cube of the semi-major axis of its orbit (a3) is a constant for all the planets, including the Earth. The third law results from the balance between the force of gravitation attracting the planet towards the Sun and the centrifugal force away from the Sun due to its orbital speed. The third law is easily proved for circular orbits ]]>
Kepler’s laws of planetary motion (1) the orbit of each planet is an ellipse with the Sun atone focus. the first law consequence of the conservation of energy of a planet orbiting the Sun under the effect of a central attraction that varies as the inverse square of distance. (2) the orbital radius of a planet sweeps out equal areasin equal intervals of time. The second law describing the rate of motion of the planet around its orbit follows directly from the conservation of angular momentum of the planet. (3) the ratio of the square of a planet’s period (T2) to the cube of the semi-major axis of its orbit (a3) is a constant for all the planets, including the Earth. The third law results from the balance between the force of gravitation attracting the planet towards the Sun and the centrifugal force away from the Sun due to its orbital speed. The third law is easily proved for circular orbits ]]> Mon, 19 Oct 2020 05:44:23 GMT /slideshow/keplers-laws-of-planetry-motion/238910075 AlokKumar1221@slideshare.net(AlokKumar1221) Keplers laws of planetry motion AlokKumar1221 Kepler’s laws of planetary motion (1) the orbit of each planet is an ellipse with the Sun at�one focus. the first law consequence of the conservation of energy of a planet orbiting the Sun under the effect of a central attraction that varies as the inverse square of distance. �(2) the orbital radius of a planet sweeps out equal areas�in equal intervals of time. The second law describing the rate of motion of the planet around its orbit follows directly from the conservation of angular momentum of the planet. �(3) the ratio of the square of a planet’s period (T2) to the cube of the semi-major axis of its orbit (a3) is a constant for all the planets, including the Earth. The third law results from the balance between the force of gravitation attracting the planet towards the Sun and the centrifugal force away from the Sun due to its orbital speed. The third law is easily proved for circular orbits <img style="border:1px solid #C3E6D8;float:right;" alt="" src="https://cdn.slidesharecdn.com/ss_thumbnails/keplerslawsofplanetrymotion-201019054423-thumbnail.jpg?width=120&amp;height=120&amp;fit=bounds" /><br> Kepler’s laws of planetary motion (1) the orbit of each planet is an ellipse with the Sun at�one focus. the first law consequence of the conservation of energy of a planet orbiting the Sun under the effect of a central attraction that varies as the inverse square of distance. �(2) the orbital radius of a planet sweeps out equal areas�in equal intervals of time. The second law describing the rate of motion of the planet around its orbit follows directly from the conservation of angular momentum of the planet. �(3) the ratio of the square of a planet’s period (T2) to the cube of the semi-major axis of its orbit (a3) is a constant for all the planets, including the Earth. The third law results from the balance between the force of gravitation attracting the planet towards the Sun and the centrifugal force away from the Sun due to its orbital speed. The third law is easily proved for circular orbits
Keplers laws of planetry motion from AlokKumar1221
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