1) [tex]-3.19\cdot 10^9 J[/tex]
2) 7909 m/s
Explanation:
1)
The potential energy of a system consisting of the Earth and an object in orbit around the Earth is given by
[tex]U=-\frac{GMm}{r}[/tex]
where
G is the gravitational constant
M is the Earth's mass
m is the mass of the object
r is the distance between the object and the Earth's centre
Here we have:
[tex]M=5.98\cdot 10^{24} kg[/tex]
m = 102 kg is the mass of the object
r = 2R is the distance of the object from the Earth's centre, where
[tex]R=6.37\cdot 10^6 m[/tex] is the Earth's radius
Substituting,
[tex]U=-\frac{(6.67\cdot 10^{-11})(5.98\cdot 10^{24})(102)}{2(6.37\cdot 10^6)}=-3.19\cdot 10^9 J[/tex]
2)
The total mechanical energy of the object is the sum of its potential energy and its kinetic energy:
[tex]E=U+K[/tex]
where
E is the mechanical energy
U is the potential energy
K is the kinetic energy
Here we want the object to have zero energy, so
E = 0
This means that the kinetic energy is
[tex]K=-U=3.19\cdot 10^9 J[/tex]
The kinetic energy of the object can be rewritten as
[tex]K=\frac{1}{2}mv^2[/tex]
where
m = 102 kg is the mass
v is the speed of the object
And solving for v, we find:
[tex]v=\sqrt{\frac{2K}{m}}=\sqrt{\frac{2(3.19\cdot 10^9)}{102}}=7909 m/s[/tex]