Orbits of Planets
and Satellites
Orbits
An orbit is a repeating path that one object in space takes around another one:
An object in an orbit is called a satellite: it can be natural (Earth and moon) or man-made (machine that is launched into space).
Kepler’s Law
Kepler’s laws describe the motion of planets:
Although we usually apply the laws to planets orbiting the Sun, they hold equally well for satellites orbiting Earth or any other massive central body.
Kepler’s Law
1st Law of Orbit: All planets move in elliptical orbits, with the Sun at one focus.
The eccentricity of Earth’s orbit is only 0.0167.
The Sun is at one of the two focal points.
Kepler’s Law
2nd Law of Areas: The radial vector from the sun to a given planet sweeps out equal areas in equal time intervals.
Kepler’s Law
3rd Law of Areas: The square of the period of any planet is proportional to the cube of the semimajor axis of its orbit.
If the orbit is circular:
Orbit speed:
Kepler’s Law
3rd Law of Areas: The square of the period of any planet is proportional to the cube of the semimajor axis of its orbit.
If the orbit is circular:
and
Ex: Given the elliptical planetary orbit shown above, identify the interval during which the planet travels with the highest speed?
(A) Interval P1 to P2
(B) Interval P3 to P4
(C) They are the same.
The planet travels a greater distance from P1 to P2 in the same time interval.
Ex: A satellite orbits a planet in an elliptical path as shown. Specific positions of the satellite are noted on the diagram as A, B, C, and D.
Rank from highest to lowest the following characteristics of the satellite at each position:
I) Speed
II) Gravitational Potential Energy
III) Total Mechanical Energy
A
B
C
D
Same (energy conservation)
Ex: A student is asked to determine the mass of Jupiter. Knowing which of the
following about Jupiter and one of its moons will allow the determination to be made?
I. The time it takes for Jupiter to orbit the Sun
II. The time it takes for the moon to orbit Jupiter
III. The average distance between the moon and Jupiter
(A) I only
(B) II only
(C) III only
(D) I and II
(E) II and III
Kepler’s third law
distance between the moon and Jupiter
time it takes for the moon to orbit Jupiter
Escape Speed
It’s the speed required for an object to completely escape the influence of gravity.
Escape Speed
It’s the speed required for an object to completely escape the influence of gravity.
By Conservation of Energy:
The gravitational pull by Jupiter provides the centripetal force on its moon:
Conservation of Angular Momentum
Consider a satellite that rotates around a planet in a elliptical orbit:
Angular momentum of a system is conserved if there is no net external torque acting on the system.
Conservation of Angular Momentum
Angular momentum of a system is conserved if there is no net external torque acting on the system.
Consider a satellite that rotates around a planet in a elliptical orbit:
a) What is the total energy of the asteroid?
Sun
Orbit of asteroid
Perihelion
aphelion
The total energy of the asteroid is equal to:
semimajor axis
Sun
Orbit of asteroid
Perihelion
aphelion
Applying Conservation of Angular Momentum:
At aphelion:
At perihelion:
c) What is the time necessary for the asteroid to make a complete orbit around the Sun?
Sun
Orbit of asteroid
Perihelion
aphelion