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Yes. What makes you think it would be a problem? The laws of physics are the same a light year out as they are at 1 au. The gravitational atraction is smaller, so the tangential velocities are smaller, but as long as an object is in a location where the force of Sol is greater than the force of any other object, it is possible for that object to orbit Sol. I don't know the exact crossover distance, but in the direction of Alpha Centauri, it should be something like 1.5 lightyears. The system of 3 Centauri stars has roughly twice the mass of Sol, so I am guestimating the crossover is about 1/3 the distance from Sol. There may be other factors involved.
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dirty_g,
As Tony said in his reply to me, comets in the Oort cloud are not so much in circular orbits as in orbits which have perihelion far enough from the Sun that they don't grow visible comas and tails, and so are never noticed. Aphelion might be a light-year from the Sun, while perihelion might be inside the orbit of Neptune. Any nearby star so dim that it isn't immediately obvious from Earth is too dim to change icy asteroids into comets with comas and tails. Even if a comet did have a full-blown tail, the star would not be bright enough to illuminate it. Even if such a comet were illuminated as brightly as one near the Sun, at a distance of a light-year it would almost certainly be invisible. -- Jeff, in Minneapolis
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http://www.FreeMars.org/jeff/ "I find astronomy very interesting, but I wouldn't if I thought we were just going to sit here and look." -- "Van Rijn" "The other planets? Well, they just happen to be there, but the point of rockets is to explore them!" -- Kai Yeves |
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The slow motions of such distanct comets are the main obsticle in detecting them. Consider Iris (Xena). It's the 4th brightest KBO, but over 500 KBOs were discovered before it. That's because it moved too slow for the detection schemes to pick it up.
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Wasn't it Gould who called it the "Shiva Hypothesis" because he, too, recognized the apparent periodicity that is so hotly contested?
Binary Research Institute highlights what some consider evidence. And then I myself include astronomers like Murray, Matese, Whitmire, Brown and a few others who've suggested such a perturber in the Oort cloud can not be ruled out. In my mind, the perturbed highly elliptical and elongated orbits of various recently discovered outer system bodies, coupled with the sheer edge of the kuiper belt, the facts that not only are binaries more prevalent in the observable universe (brown drawfs too?) and planets have been found to be stable in these systems... these and various other puzzles in our system all constitute evidence for such a body. I'd suggest we've not found it simply because it is a dim brown dwarf moving slowly and inclined to the ecliptic, generally toward the galactic center. I suspect we'll discover it soon.
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"Where the telescope ends, the microscope begins. Which of the two has the greater view?" - Hugo "Men occasionally stumble over the truth, but most pick themselves up and hurry off as if nothing had happened." - Churchill |
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It seems to me that the periodicity should be shakey at best. If Nemesis exists in a wide orbit, it is likely that nearby stars would be perturbing its orbit. I doubt it would trace the same orbit over and over again. Its period each orbit would likely be different.
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seems the Nemesis theory is gaining support recently. Still I am sure it has equal opposition. I suppose though that if you say it is a brown dwarf then that is an easy way of getting out of detecting it as it would be so hard to see.
With regards to the orrt cloud I still do not see why there has to be a cloud of them together?? Maybe im just being silly but why can't the comments all just orbit the solar system on long period orbits instead? Understand im not rguing with you all here I just am really interested as to why a cloud of them would group together?? Oh and if a Brown Dwarf was hiding behind them all (the apparent Nemesis) then wouldnt it of sent them all heading off towards us by now?? |
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When designing interstellar missions, one has to consider the likelyhood that an Oort cloud-like environment exists between each of the stellar systems (occupies all of interstellar space within the MW) with density falling off towards the mid-point between stellar systems. Such material would provide both hazards and a source for propellant for interstellar ships. Has anyone computed how much mass could be contributed to that of the MW by such material and not have been detected either by visual observation or by its gravitational interaction with the observable objects?
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For those inclined to oppose human meddling with the structure of the universe or the composition and configuration of objects and groups of objects within the universe, consider: Whether there is a limit to the magnitude of a modulation of chaos below which order remains invariant? Or, is order but a fiction invented by perspectives applied over finite, however large, time intervals? |