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[Mike Brown explains orbital dominance]
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- Some years ago he advocated the criterion of orbital dominance. - About one year ago he changed to the cultural definition, found here in section "Is this object really a planet? Is Pluto a planet? What makes a planet?". - He opposed the Gingerich proposal since when it was out. - He supported the Fernandez proposal since when it was out. I hadn't (and still haven't) any doubt that, although he might have preferred the "cultural definition" for the public (I don't imply egoism here), he honestly considers the resulting resolution as scientifically sound and still better for public use than the initial proposal. There is presumably some disappointment about 2003UB313 not becoming the 10th planet (see the Requiem for Xena) and some relief about the whole uncertainty about its status, naming rules etc. being finally over. And as a teaching Professor of Planetary Astronomy he has to face some (positive) changes too. Maybe all this makes him somewhat itchy, his emotional state not yet completely settled, I don't know. But many people have to reorder their "astronomical cortex" today. ![]() |
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I still wonder how this wording was hammered together.
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"What you think you thought you saw you did not see." Agent J, MiB - Manhatten Bureau |
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Because you tried to read between the lines despite the lines providing much more insight themselves. And it was addressed at you, in the first place, and a quote is a good hint at whom I'm talking to.
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As was predicted on this board a few months ago, the IAU definition satisfies nobody and doesn't end the debate. Anyway, it's nice to see mainstream coverage of an astronomical issue that doesn't involve planetary alignments, pole shifts or comet-trailing spaceships. Granted, arguing semantics is only a small step in the right direction, but it's a start. My definition is that its a planet if I think it is a planet. Overall, I think the IAU definition is good.
Some day we will find an object that blurs the line between planet and "not a planet". If Instead of 98%, an object is found that has cleared say 71% of the mass in its vicinity, then what? I also wonder why the entire Kuiper seems to be lumped into the same "vicinity". The Kuiper belt is a volume that dwarfs the volume occupied by the inner planets. Isn't it possible that there are different regions of this volume occupied by planets?
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Time flies like an arrow. Fruit flies like a banana. |
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And, in fact, I suggested the term "dwarf planets" over a week ago for the small, Pluto-like planets that were not orbitally dominant. So I'm very satisfied! ![]() Quote:
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It's also possible that the weak 40% dominance managed by Ceres could be near the upper end before reaching this runaway point. After all, it's widely accepted that the asteroid belt has not formed into a planet because of the effect of Jupiter. If Jupiter were not so massive, then perhaps Ceres would have already cleared out it's orbital region.
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"Barbarism is the natural state of mankind. Civilization is unnatural. It is a whim of circumstance. And barbarism must always ultimately triumph" -- Conan |
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