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To: e_engineer
Imagine a Jupiter mass planet in a circular orbit with perihelion = 1 AU. If you could change it's ellipticity (sp?) but keep the perihelion (closest approach) at 1 AU, does it become easier or harder to detect based on the stars radial velocity?

Hmmm.... Think of it this way. If the planet is highly elliptical, the star will also exibit a elliptical motion around the center of mass (greater wobble). If the orbit plane is exactly in line with our line of sight of the star, I agree detection would be much more difficult. However, if we are looking at it face on, the motions of the star becomes much more apparent.

331 posted on 07/04/2003 12:13:42 PM PDT by RadioAstronomer
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To: ThinkPlease
Sorry, did not add you to my ping. Anything you would like to add? Have I "stuffed" up my explanation?
332 posted on 07/04/2003 12:14:54 PM PDT by RadioAstronomer
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