Orbital Properties of the Planets

Where are the planets now?

Solar System Live



Planetary Orbit Properties

Kepler and Newton determined the general orbital properties of bodies of the solar system:


Overview of Solar System Orbits


General Relativity and Mercury

Although all of the orbits of the planets could be described by Newtonian Mechanics, it was noticed in the mid 19th centure that the observed position of Mercury did not seem to agree with what the Newtonian model predicted. Could there be a problem with Newton's description of gravity?

Yes and Newton's theory is incomplete

Einstein to the rescue!

Description of the Mercury Problem:
Mercury's Motion through the curve spacetime near the Sun

Newton had implicitly assumed that space was flat.

This lead to a refinement of Newtonian Gravity known as Einstein's General Theory of Relativity:

General Theory of Relativity

Space communicates with matter and instructs it how to move and, in turn, matter communicates with space and instructs it how to curve.

Mercury orbits in Curved Space because it is a near a very large mass (the Sun).


The Visibility of the Planets

Viewing the planets from Earth depends on the the planet-earth-sun angle. For planets outside of Earth's orbit:

  • When this angle is 180 degrees , planet is overhead at midnight
  • When this angle is 0 degrees , the planet is up in the day time
  • When this angle is 90 degrees the planet is overhead at sunset
  • When this angle is 270 degrees the planet is overhead at sunrise

    For the Inner Planets the situation is much different as they are always relatively near the Sun. There is a time in the orbit of Mercury and Venus called greatest elongation in which Venus appears at its maximum angular separation from the Sun. This is illustrated below. Note that since there are 15 degrees in one hour of time, then the angle of 46 degrees shown below corresponds to about 3 hours of time. When Venus is at the position in its orbit shown below, it will appear in the sky either 3 hours before or after sunrise. At any other position in its orbit, Venus will appear closer in time and angular separation to the sun.