Hi ltcmmdr,
Everything we see in the nightsky are stars. We call them stars because they are very bright and very heavy.. Planets do not emit light (well not visible anyway) and they are generally a lot less heavy than their stars.
That's what makes it so difficult to detect a planet around a star, simply because the star itself is so bright, we cannot see the planet revolving around it.
There are different methods thast can be used to detect planets:
A simple and uneffective method:
Planets orbit their stars, so everytime a planet moves in front of side of the star we see the star's brightness fade just this tiny little bit.
If the brigthness is then plotted as a function of the time, you can clearly see the "dimming" of everytime the planet moves in front of the star. That way we can determine the number of hours/days/weeks/.. it takes for the planet to complete one orbit.
The currently used method:
Large planets pull the actual star from its rest position because of gravitational interaction. This causes the star to change from position all the time (since the planet orbits the star, the star is dragged along in a circle). By measuring the doppler shifts in the light we receive from the star, we can tell whether there's something dragging the star or not.
Bye!
Crisp
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"The best thing you can become in life is yourself" -- M. Eyskens.
[This message has been edited by Crisp (edited December 20, 1999).]