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#51
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In article . com,
wrote: "Purely historical. Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto are planets. Nothing else in the solar system is a planet. This definition is definitely historically valid, but fails miserably under scientific meaning. What if a new object larger than Pluto is found? What is it? Why is Pluto a planet but an object 3/4 its size, like Sedna, is not? This definition, completely lacking in scientific motivation, makes the word 'planet' meaningless as a scientific description." Does it matter that the term planet is "meaningless as a scientific description"? Are scientists suffering from any confusion as a result? Is research being held back? It seems to me that if there were a need for a precisely defined term, it would be clear what the required definition was. The fact that there is no consensus on a definition suggests that we have no real need for one. -- Richard |
#52
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Richard Tobin wrote:
It seems to me that if there were a need for a precisely defined term, it would be clear what the required definition was. The fact that there is no consensus on a definition suggests that we have no real need for one. I think you are correct that there is no technical need. I suggest that there is a public relations need. Maybe it can be obviated by consistent avoidance of the term, but I'm doubtful of that. -- Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.html |
#53
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![]() steve wrote: With this set to be finalised fairly soon in September 2006 I think it is essential that a few sensible parameters are added. 1) A body in orbit around a star. The definition of a star? 2) Size must be larger than Pluto ( or another agreed specified size and mass) to give a minimum size UNLESS extra-terrestial life is found on the planet when a much smaller size would be allowed. Why should the existence of life be a criterion? Might not life also exist on moons? 3) If the size of a moon is similar (to a stated percentage e.g. 80%) to the larger body in its group it to can be called a planet if it meets (1) and (2) Thus it is possibe to have binary planets. 4) It would probably be necessary to specify a maximum distance from the star in which the planet is in orbit to dis-allow wandering rocks. Double-A |
#54
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#56
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![]() Brian Tung wrote: Double-A wrote: The definition of a star? People often say "fusor": that is, an object that fuses hydrogen for energy (or did, previously, if it's a "dead" fusor). Sometimes a distinction is made between stars like our Sun that fuse ordinary hydrogen, as opposed to brown dwarfs that fuse only deuterium. Since deuterium is much scarcer than ordinary hydrogen, a brown dwarf's supply of it doesn't last very long. -- Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.html Saying that a star is a current or former fusor certainly covers most bases. But I can still think of some exceptions. For instance, if Jupiter were adrift in space, would its satellites be called moons or planets? Double-A |
#57
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Double-A wrote:
Saying that a star is a current or former fusor certainly covers most bases. But I can still think of some exceptions. For instance, if Jupiter were adrift in space, would its satellites be called moons or planets? That is a reasonable question, but the answer has nothing to do with the definition of a star; Jupiter is far too small to fuse even deuterium. A body with the composition of Jupiter would have to be on the order of 13 times as massive to begin deuterium fusion. Approximately 80 Jovian masses are needed to start the fusion of ordinary hydrogen. If Jupiter were free-floating with its satellites, I think they would just be called satellites (as they are now); the bigger question is what we would call Jupiter. They are sufficiently exotic (in terms of public awareness, not in terms of their physics) that I think one could get away with calling them free-floating non-fusors, or something like that. -- Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.html |
#58
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In article .com,
Double-A wrote: Brian Tung wrote: Double-A wrote: The definition of a star? People often say "fusor": that is, an object that fuses hydrogen for energy (or did, previously, if it's a "dead" fusor). Sometimes a distinction is made between stars like our Sun that fuse ordinary hydrogen, as opposed to brown dwarfs that fuse only deuterium. Since deuterium is much scarcer than ordinary hydrogen, a brown dwarf's supply of it doesn't last very long. -- Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.html Saying that a star is a current or former fusor certainly covers most bases. But I can still think of some exceptions. For instance, if Jupiter were adrift in space, would its satellites be called moons or planets? Double-A The definition of a star we were given involved spherical symmetry, thermal equilibirum, fusion, hydrostatic equilibirum, constant mass yadda yadda with the proviso that many of these could be not relevant in certain cases. I like - "Big shiny thing" myself. -- The greatest enemy of science is pseudoscience. Jaffa cakes. Sweet delicious orangey jaffa goodness, and an abject lesson why parroting information from the web will not teach you cosmology. Official emperor of sci.physics. Please pay no attention to my butt poking forward, it is expanding. |
#59
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![]() The definition of a star we were given involved spherical symmetry, thermal equilibirum, fusion, hydrostatic equilibirum, constant mass yadda yadda with the proviso that many of these could be not relevant in certain cases. I like - "Big shiny thing" myself. How big? How shiny? How thing? Greg |
#60
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In article . com,
wrote: The definition of a star we were given involved spherical symmetry, thermal equilibirum, fusion, hydrostatic equilibirum, constant mass yadda yadda with the proviso that many of these could be not relevant in certain cases. I like - "Big shiny thing" myself. How big? How shiny? How thing? Why must it always be about size? Any choice on size by itself is always going to be completely arbitrary. Even the "spherical compaction" idea, while at least vaguely more interesting, is still arbitrary: these two objects are identical in all respects, except this one had enough mass to become quite spherical, whereas this other one is so very lumpy. But if they are, in their formation, composition, and general dynamics, the same, why would you bother distinguishing between them on an otherwise unimportant feature? The definition of stars and planets should tell us something about how they formed, and how they act. Not how big they are. Who cares how big a star is. What does is fuse now? What did it fuse when it was born? What was it born from? What composition? Same for planets. How did they form? Early or late? Close in, or far out? What are they composed of? Of course, the big problem here is, what is the purpose of defining a planet? Is it a purely scientific purpose, or a popular (educational) purpose, or both? Ideally, we want a definition that is scientifically meaningful, and at the same time useful for elementary school astronomy. A definition of planet that results in Jupiter, Earth, Mercury, Pluto, "Xena", and Ceres all being called planets is not useful to scientists. And when we get up to 15 or 20 planets that way, it stops being useful in elementary school also. So I'm not sure exactly what the definition should be, but I'm pretty sure that eight planets is more useful, both scientifically, and pedagogically, than 15-20. tom |
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