What happens to the body when it is thrown upwards @ 11.5km/s?
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The escape velocity on the earth surface is about 11.2 km/s.
When a body is projected from the surface of a planet with a velocity equal to or higher than the escape velocity, it escapes from the gravitational influence of that planet.
As in this case, the velocity of the body(11.5 km/s) is higher than the escape velocity(11.2 km/s) on the earth, the body escapes from the earth's gravitational influence, when projected upwards.
When a body is projected from the surface of a planet with a velocity equal to or higher than the escape velocity, it escapes from the gravitational influence of that planet.
As in this case, the velocity of the body(11.5 km/s) is higher than the escape velocity(11.2 km/s) on the earth, the body escapes from the earth's gravitational influence, when projected upwards.
Angella:
The Escape velocity is independent of mass of the body.
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Let v be the velocity of projection of the body from Earth.
![Total\ mechanical\ energy\ of\ the\ body\ on\ Surface\ of\ Earth\\\\ E= \frac{1}{2}mv^2-\frac{GM_em}{R_e},\ \ m=mass\ of\ the\ body,\ \ M_e=mass\ of\ Earth\\\\.\ \ \ \ \ \ R_e=Radius\ of\ Earth,\ \ G=Unversal\Gravitational\ Constant\\\\ Total\ mechanical\ energy\ of\ the\ body\ on\ Surface\ of\ Earth\\\\ E= \frac{1}{2}mv^2-\frac{GM_em}{R_e},\ \ m=mass\ of\ the\ body,\ \ M_e=mass\ of\ Earth\\\\.\ \ \ \ \ \ R_e=Radius\ of\ Earth,\ \ G=Unversal\Gravitational\ Constant\\\\](https://tex.z-dn.net/?f=Total%5C+mechanical%5C+energy%5C+of%5C+the%5C+body%5C+on%5C+Surface%5C+of%5C+Earth%5C%5C%5C%5C+E%3D+%5Cfrac%7B1%7D%7B2%7Dmv%5E2-%5Cfrac%7BGM_em%7D%7BR_e%7D%2C%5C+%5C+m%3Dmass%5C+of%5C+the%5C+body%2C%5C+%5C+M_e%3Dmass%5C+of%5C+Earth%5C%5C%5C%5C.%5C+%5C+%5C+%5C+%5C+%5C+R_e%3DRadius%5C+of%5C+Earth%2C%5C+%5C+G%3DUnversal%5CGravitational%5C+Constant%5C%5C%5C%5C)
Since the total mechanical energy is conserved by the gravitational force, the energy at a distance d from the center of Earth is given by:
![E=\frac{1}{2}mv_d^2-\frac{GM_em}{d}=\frac{1}{2}mv^2-\frac{GM_em}{R_e}\\\\For\ d=>\infty,\ and\ v_{\infty}=nearly\ 0,\ minimum\ velocity\ v_e\ needed:\\\\ \frac{1}{2}mv_e^2=\frac{GM_em}{R}\\\\v_e=\sqrt{\frac{2GM_e}{R_e}}\\ E=\frac{1}{2}mv_d^2-\frac{GM_em}{d}=\frac{1}{2}mv^2-\frac{GM_em}{R_e}\\\\For\ d=>\infty,\ and\ v_{\infty}=nearly\ 0,\ minimum\ velocity\ v_e\ needed:\\\\ \frac{1}{2}mv_e^2=\frac{GM_em}{R}\\\\v_e=\sqrt{\frac{2GM_e}{R_e}}\\](https://tex.z-dn.net/?f=E%3D%5Cfrac%7B1%7D%7B2%7Dmv_d%5E2-%5Cfrac%7BGM_em%7D%7Bd%7D%3D%5Cfrac%7B1%7D%7B2%7Dmv%5E2-%5Cfrac%7BGM_em%7D%7BR_e%7D%5C%5C%5C%5CFor%5C+d%3D%26gt%3B%5Cinfty%2C%5C+and%5C+v_%7B%5Cinfty%7D%3Dnearly%5C+0%2C%5C+minimum%5C+velocity%5C+v_e%5C+needed%3A%5C%5C%5C%5C+%5Cfrac%7B1%7D%7B2%7Dmv_e%5E2%3D%5Cfrac%7BGM_em%7D%7BR%7D%5C%5C%5C%5Cv_e%3D%5Csqrt%7B%5Cfrac%7B2GM_e%7D%7BR_e%7D%7D%5C%5C)
It is called the escape velocity of Earth, as a body projected with this velocity away into the space, just manages to travel to infinite distance. Substituting the values numerically and calculating, ,we find![v_e=11.2\ km/sec.\\\\ v_e=11.2\ km/sec.\\\\](https://tex.z-dn.net/?f=v_e%3D11.2%5C+km%2Fsec.%5C%5C%5C%5C)
If a body is projected with a velocity 11.5 km/sec., then the body escapes from the gravitational field of Earth and it will have some kinetic energy still. After that it will move at uniform velocity:
![v_{\infty}=\sqrt{11.5^2-11.2^2}=2.61\ km/sec.\\ v_{\infty}=\sqrt{11.5^2-11.2^2}=2.61\ km/sec.\\](https://tex.z-dn.net/?f=v_%7B%5Cinfty%7D%3D%5Csqrt%7B11.5%5E2-11.2%5E2%7D%3D2.61%5C+km%2Fsec.%5C%5C)
Perhaps the body will get into gravitational field of another planet in space.
Since the total mechanical energy is conserved by the gravitational force, the energy at a distance d from the center of Earth is given by:
It is called the escape velocity of Earth, as a body projected with this velocity away into the space, just manages to travel to infinite distance. Substituting the values numerically and calculating, ,we find
If a body is projected with a velocity 11.5 km/sec., then the body escapes from the gravitational field of Earth and it will have some kinetic energy still. After that it will move at uniform velocity:
Perhaps the body will get into gravitational field of another planet in space.
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