Definition: Work done to move mass in a gravitational field.
Requires work to move mass from initial position (Ri) to final position (Rf).
Work is done against a varying gravitational force.
Graphical approach: Area under the curve in a force vs. distance graph
As mass m is lifted from Ri to Rf, this is the work done against gravity.
Reference level for GPE can be arbitrary (e.g., surface of the Earth, infinity).
GPE can be positive, negative, or zero depending on the reference level, such as for a watermelon at varying heights.
Object moved away from planet surface.
Object placed in orbit from the surface.
Object falls toward the planet under gravity without air resistance considerations.
Work required to lift objects:
If 4.00 x 10^3 kg is lifted to 3.2 x 10^5 m.
Initial position = surface, Final position = 3.2 x 10^5 m above surface.
Coordinates: Ri = 6.38 x 10^6 m, Rf = 6.70 x 10^6 m.
For a vehicle lifted to a circular orbit:
Mass = 1.60 x 10^3 kg, Height = 2.0 x 10^6 m above the Moon.
General escape velocity formula involves mass and radius of the planet.
Example question on escape velocities between Earth and Saturn, showcasing the mass and radius relationship.
Total Energy of a satellite = Gravitational Potential Energy (GPE) + Kinetic Energy (KE).
GPE can be expressed with respect to satellite characteristics and orbital mechanics.
Velocity requirements vary by location:
Escape velocities differ across celestial bodies (e.g., Earth, Mercury, Venus).
Tables of relative velocities emphasize variation in gravitational pulls.