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Sylvia Else wrote:
David Bromage wrote: Sylvia Else wrote: BTW, right at the beginning I was annoyed at the apparent assertion that in the normal way of things, a planet could not be in orbit about a black hole. There's no reason a planet cannot be. Provided the planet is outside the event horizon and was captured after the black hole was formed. The star's original planets would have been destroyed when it went supernova. Even if a planet was captured its orbit would certainly not be stable. I take your point about surviving the supernova event (or perhaps neutron star collision) that created tbe black hole. Given the absence of existing planets, capture of one is problematic. I suppose it would require a rather coincidental meeting of two objects in the vicinity of the black hole. One is ejected or falls into the hole, and the other ends up in orbit. However, provided the object's orbit (which is hardly likely to be circular) doesn't take it close to the black hole, I cannot see why its orbit would be any less stable than that of an object in orbit around an ordinary star of similar mass to the black hole. And if it was far enough away not to be sucked it, it would be far enough away to retain an atmosphere. That's it if retained one whereever it was orginally created. If Mercury were ejected from the solar system (by a freak event involving a large mass) and then captured in orbit about by a black hole (by another freak event involving a large mass) then it wouldn't have an atmosphere. However this does rather suggest that the chances of finding a planet in orbit about a black hole are pretty slim. Sylvia. It's certainly very unusual, but I like the reasoning! The problem isn't just one of origin, although that makes it really unlikely. It's tidal force, bit of a misnomer as there's no such force, just the observation off the back of this planet's oceans that gravity pulls slightly more on the forward side of a facing object. When dealing with gravity of this order this translates into a lot of disproportionate pull. Astronomers were amazed to find a planet in orbit around a neutron star, so the Doctor's reaction that this system is "impossible" is justifiable hyperbole. Martin... -- http://sfsa.org.au/, the South Australian Doctor Who Fan Club, Inc. |
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Martin Dunne wrote:
It's certainly very unusual, but I like the reasoning! The problem isn't just one of origin, although that makes it really unlikely. It's tidal force, bit of a misnomer as there's no such force, just the observation off the back of this planet's oceans that gravity pulls slightly more on the forward side of a facing object. When dealing with gravity of this order this translates into a lot of disproportionate pull. And not on the ocean (there wasn't any) but on the rock, such that the planet would be distorted to the extent that a Mt Everest could be pulled up on the side closest to the black hole every rotation. The friction alone would guarantee that there would be little if any solid crust and the surface of the planet would be akin to our mantle. Also the orbital period of a planet that close would be measured in hours rather than days, weeks or months. Cheers David |
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David Bromage wrote:
Martin Dunne wrote: It's certainly very unusual, but I like the reasoning! The problem isn't just one of origin, although that makes it really unlikely. It's tidal force, bit of a misnomer as there's no such force, just the observation off the back of this planet's oceans that gravity pulls slightly more on the forward side of a facing object. When dealing with gravity of this order this translates into a lot of disproportionate pull. And not on the ocean (there wasn't any) but on the rock, such that the planet would be distorted to the extent that a Mt Everest could be pulled up on the side closest to the black hole every rotation. The friction alone would guarantee that there would be little if any solid crust and the surface of the planet would be akin to our mantle. Also the orbital period of a planet that close would be measured in hours rather than days, weeks or months. Did the program ever say how close the planet was. Also, it seems to me that if the tidal effects were enough to melt the surface of the planet, then by the same token the planet's rotation would be reducing rapidly. It would end up in tidal lock and cool down. Sylvia. Cheers David |
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On Wed, 13 Sep 2006 14:30:18 +1000, Sylvia Else
wrote: Also, it seems to me that if the tidal effects were enough to melt the surface of the planet, then by the same token the planet's rotation would be reducing rapidly. It would end up in tidal lock and cool down. Jesus. Fracking, H. Christ. ....Kids, this is Doctor Who. This isn't Star Trek, or even Babylon 5. Hell, it ain't even Lost in Space. It's *supposed* to have all disbelieve put not only on suspension, but in total escrow awaiting Supreme Court judiciary disposition. Just sit back, enjoy the ride, and quit being anal-retentive pedantics. This is the *one* show you're supposed to just let go and don't worry about whether or not it could really happen. [shakes head at those obviously still living in their parents' basement] OM -- ]=====================================[ ] OMBlog - http://www.io.com/~o_m/omworld [ ] Let's face it: Sometimes you *need* [ ] an obnoxious opinion in your day! [ ]=====================================[ |
#5
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![]() "OM" wrote in message ... ...Kids, this is Doctor Who. OM- try decafe. |
#6
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David Bromage wrote in
: Martin Dunne wrote: It's certainly very unusual, but I like the reasoning! The problem isn't just one of origin, although that makes it really unlikely. It's tidal force, bit of a misnomer as there's no such force, just the observation off the back of this planet's oceans that gravity pulls slightly more on the forward side of a facing object. When dealing with gravity of this order this translates into a lot of disproportionate pull. And not on the ocean (there wasn't any) but on the rock, such that the planet would be distorted to the extent that a Mt Everest could be pulled up on the side closest to the black hole every rotation. The friction alone would guarantee that there would be little if any solid crust and the surface of the planet would be akin to our mantle. Also the orbital period of a planet that close would be measured in hours rather than days, weeks or months. Doesn't Jupiter's moon Io has active volcanoes because of tidal forces from Jupiter's gravity? If that's case, how would a planet around a black hole survive for long? Or at least, it may be able to have a solid surface. |
#7
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The Doctor wrote:
David Bromage wrote in : Martin Dunne wrote: It's certainly very unusual, but I like the reasoning! The problem isn't just one of origin, although that makes it really unlikely. It's tidal force, bit of a misnomer as there's no such force, just the observation off the back of this planet's oceans that gravity pulls slightly more on the forward side of a facing object. When dealing with gravity of this order this translates into a lot of disproportionate pull. And not on the ocean (there wasn't any) but on the rock, such that the planet would be distorted to the extent that a Mt Everest could be pulled up on the side closest to the black hole every rotation. The friction alone would guarantee that there would be little if any solid crust and the surface of the planet would be akin to our mantle. Also the orbital period of a planet that close would be measured in hours rather than days, weeks or months. Doesn't Jupiter's moon Io has active volcanoes because of tidal forces from Jupiter's gravity? If that's case, how would a planet around a black hole survive for long? Or at least, it may be able to have a solid surface. It's all a question of distance. If the planet is suitably far from the black hole, then it will not suffer such disruptive tidal effects. People often seem under the impression that a black hole has a specially high gravitational field. It doesn't. It has exactly the same gravitational field as any other object of the same mass. The mass of the black hole does not have to be particularly high by stellar standards. It's a bad idea to get close to a black hole, but then it's a bad idea to get close to any massive object. Sylvia. |
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![]() Sylvia Else wrote: It's all a question of distance. If the planet is suitably far from the black hole, then it will not suffer such disruptive tidal effects. Also, the mass of the black hole- the larger the mass, the less intense the tidal gravity gradient will be for a planet orbiting it at a distance to have the same orbital period, assuming the planet's diameter and mass are kept the same. Pat |
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