(455) HL Important gravitational field equations [IB Physics HL]
Gravitational Potential Energy (E_P)
Definition: Work done to assemble a system from infinite separation.
Equation:[ E_P = -\frac{G \cdot M_1 \cdot M_2}{R} ]
Units: Joules (J)
Key Point: Use ( R ) (not ( R^2 )) in potential energy calculations.
As ( R ) approaches infinity, ( E_P = 0 ) (asymptotic behavior).
Gravitational Potential (V)
Definition: Work done per unit mass.
Equation:[ V = -\frac{G \cdot m}{R} ]
Units: Joules per kilogram (J/kg).
Relationship: Work done is given by[ \text{Work done} = m \cdot \Delta V_g ]
Notes: To increase gravitational potential, one must move away from the mass (potential well analogy).
Gravitational Field Strength (g)
Equation:[ g = -\frac{\Delta V_g}{\Delta R} ]
Units: Newtons per kilogram (N/kg).
Equipotential Lines
Definition: Locations where gravitational potential (V_g) is constant.
Properties:
Perpendicular to gravitational field lines.
No work is done when moving along equipotential lines.
Visualization: Equipotential lines indicate the same gravitational potential at different points.