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Old 07-09-2003, 07:39 AM   #11
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Unfortunately, the story at the link provided by Tom Sawyer doesn't give much information.

Remember, the mass of the planet discovered, assuming that it is done in the typical manner, is a lower limit. What is actually derived is M*sin(i), where i is the inclination of the planet's orbit.

So, this planet they discovered around a sun-like star is at least twice the mass of Jupiter and orbiting at almost half the Sun-Jupiter distance. I would imagine that if the planet is too massive, it may be difficult to have an earth-like planet close in because of gravitational perturbations.
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Old 07-09-2003, 07:41 AM   #12
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Quote:
Originally posted by Godless Dave
I had thought the only way they had of detecting planets outside our solar system was by observing the gravitational effects of a large planet's mass on its sun, and they can get further information from spectrometry. But I don't think there is any way yet of detecting earth-size planets. I could be wrong though.
Earth technically moves our sun, but so minorly I'm not even sure we could see it here in our system. Just not enough mass.

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Abe, I think the existences of Neptune and Pluto were postulated by orbital calculations, and confirmed with direct observation.
Correct, plus we flew by Neptune with Voyager 2, and got nice pictures.
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Old 07-09-2003, 08:01 AM   #13
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Don't most physicists now believe that the universe is not, in fact, endless? Wouldn't an infinitely large universe violate some basic precepts?
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Old 07-09-2003, 08:06 AM   #14
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Actually, Pluto's discovery was more accidental. The calculations that predicted a planet beyond the orbit of Neptune proved later to be in error. It was just plain luck that Tombaugh found Pluto where he did.
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Old 07-09-2003, 08:22 AM   #15
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Originally posted by Rhaedas
Earth technically moves our sun, but so minorly I'm not even sure we could see it here in our system. Just not enough mass.
According to Marcy & Butler's Review on the Detection of Extrasolar Giant Planets , the stellar radial velocity induced by an orbiting companion is



putting in the values for the Earth and the Sun, you get about 5 cm/s (times sin(i)).

Current technology allows us to get to about 3 m/s, maybe 1 m/s under the best conditions. So, we still need almost two orders of magnitude improvement on the current technique (or change techniques) before we can detect an Earth around a Sol.
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Old 07-09-2003, 08:34 AM   #16
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Thanks Shadowy Man for the numbers...

Plus, the inclination of the orbit has to be pointed somewhat at us. We detect the wobble by doppler changes in the star's light; if we're looking at the star system from the poles, there aren't any changes, nor would a large planet block light.
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Old 07-09-2003, 08:39 AM   #17
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Originally posted by Rhaedas

Plus, the inclination of the orbit has to be pointed somewhat at us.
Yep, that's why there's a sin(i) in there.
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Old 07-09-2003, 08:49 AM   #18
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I figured...just wanted to clarify the rareness of detection.

Or actually, due to that rareness of angle, the fact we find a lot of stuff orbiting other stars, albeit only the big ones we can see so far, it speaks to how common solar systems probably are. So given the number of stars, there has to be a lot of similiar conditions that are hospitable to self-replicating forms.
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Old 07-09-2003, 08:52 AM   #19
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So given the number of stars, there has to be a lot of similiar conditions that are hospitable to self-replicating forms.
Saying that there 'has to be' is a bit premature considering that we don't even know for certain what is needed for life to begin yet. I think it's safer to say 'it is very likely'
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Old 07-09-2003, 09:00 AM   #20
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You're correct of course...my opinion crept in there.

Would my earlier statement on finding something else in our system raise that probability to 1 though? It seems to me that the chances of having two freak abiogenesis events in one place, but nowhere else in the universe, is virtually zero.
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