The orbital velocity is 7,907 m/s and the period is 16,862 s for the circular orbit. It will take 2,827 seconds for the space station to move to the current position of the shuttle. The new elliptical orbit has a semi-major axis of 30,000 km. The space shuttle must lose 2,642 m/s of speed to achieve the new orbit. When the shuttle reaches the 12 o'clock position after one orbit, it must fire its rockets to match the velocity of the space station for docking.
To calculate the orbital velocity and period of a circular orbit, we can use the formulas:
Orbital velocity (v) = sqrt(GM/r)
Period (T) = 2πr/v
Where G is the gravitational constant (6.67 x 10^-11 N(m/kg)^2), M is the mass of Earth (5.97 x 10^24 kg), and r is the orbital radius (20,000 km).
By plugging in the values into the formulas, we get:
Orbital velocity = sqrt((6.67 x 10^-11 N(m/kg)^2)(5.97 x 10^24 kg)/(20,000,000 m)) = 7,907 m/s
Period = 2π(20,000,000 m)/(7,907 m/s) = 16,862 s
b. To calculate the time it takes for the space station to move from its current position to where the shuttle is currently, we need to find the angular distance (θ) between the two positions and use the formula:
Time (t) = θ/ω
Where ω is the angular velocity, which is equal to 2π/T.
The angle between the two positions is 30 degrees, which is equal to π/6 radians. The angular velocity is 2π/16,862 s.
By plugging in the values into the formula, we get:
Time = (π/6 radians)/(2π/16,862 s) = 2,827 s
c. The semi-major axis (a) of the new elliptical orbit can be calculated using the formula:
a = r + (Δr/2)
Where r is the original orbital radius (20,000 km) and Δr is the change in orbital radius, which is equal to the distance the space station traveled (20,000 km) minus the distance it needs to travel to reach the 12 o'clock position (0 km).
By plugging in the values into the formula, we get:
a = 20,000 km + (20,000 km/2) = 30,000 km.
d. The change in velocity (Δv) can be calculated using the equation:
Δv = √(2μ/ra - 2μ/2a)
Where μ is the gravitational parameter, which is equal to GM, G is the gravitational constant, and M is the mass of Earth.
By plugging in the values into the equation, we get:
Δv = √((2(6.67 x 10^-11 N(m/kg)^2)(5.97 x 10^24 kg))/(20,000 km) - (2(6.67 x 10^-11 N(m/kg)^2)(5.97 x 10^24 kg))/(2(30,000 km))) = 2,642 m/s.
e. To stay in the same orbit as the space station for docking, the space shuttle needs to match the velocity of the space station when it reaches the 12 o'clock position. This can be done by firing its rockets to increase its velocity to match that of the space station.