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Dear Double-A et al:
I submit that the elitist card carrying members of the French IAU who claim to have discovered these 200 extra solar "planets" have actually so far discovered exactly zero extra-solar planets. I also submit that the closest know planets to Pollux are Neptune or Pluto, depending on the time and/or the French IAU's planet definition for this week. Why? Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a planet of planetary systems. 2. The French IAU has decreed from on high that there are only 8 planets in the Universe (see Resolution 5A note 1 below). 3. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(1)(a), plus note 1 below). 4. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(1)(b) below. 5. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(1)(c). 6. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. Further, I submit that these 200 extra-solar "planets" are not even dwarf planets Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a dwarf planet of planetary systems. 2. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(2)(a)). 3. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(2)(b) below. 4. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have not cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(2)(c). 5. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. 6. The IAU has yet to provide a process for determining if borderline objects are either dwarf planets or "other" objects (see Resolution 5A note 2 below). Further, I submit that theses alleged extra-solar star wobble causing masses are in fact Small Solar-System Bodies (sub category TNOs or "other small bodies), by the process of elimination and Resolution 5A Section (3) and note 3, as proclaimed by the Universally Esteemed IAU. If I have erred in my logic, please let me know where! This discourse has caused me to ponder How many Frenchmen can't be wrong (Groucho Marx)? A. 50 million B. None Why does the IAU spell neighborhood neighbourhood? A. They're French B. They have diminished language skills C. They can't come to grips with the fact that English is the Universal language Which is the most rigorous educational regimen? A. Astronomy PhD B. Education PhD C. Antarctic Anthropology PhD D. 11th grade Calculus Are all Astronomers Law School drop-outs, as evidenced by the logic and writing skills exhibited by Resolution 5A? Do all Astronomers get their PhDs on-line from the University of Phoenix? Why is the size of one's paycheck such an accurate indicator of the combination of society's value of their vocation and their innate abilities? Wayne ------------------------------------------------------------------------------- IAU Resolution: Definition of a Planet in the Solar System Contemporary observations are changing our understanding of planetary systems, and it is important that our nomenclature for objects reflect our current understanding. This applies, in particular, to the designation "planets". The word "planet" originally described "wanderers" that were known only as moving lights in the sky. Recent discoveries lead us to create a new definition, which we can make using currently available scientific information. RESOLUTION 5A The IAU therefore resolves that "planets" and other bodies in our Solar System, except satellites, be defined into three distinct categories in the following way: (1) A "planet"1 is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit. (2) A "dwarf planet" is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape2 , (c) has not cleared the neighbourhood around its orbit, and (d) is not a satellite. (3) All other objects3 except satellites orbiting the Sun shall be referred to collectively as "Small Solar-System Bodies". 1The eight "planets" a Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. 2An IAU process will be established to assign borderline objects into either dwarf planet and other categories. 3These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies. ------------------------------------------------------------------------------------------- "Double-A" wrote in message oups.com... "A new planet with nearly three times the mass of Jupiter has been detected orbiting the bright star, Pollux, one of the Gemini twins. While the 200 extra-solar planets discovered so far have been around fairly inconspicuous stars, Pollux is the 16th brightest star in the sky and can be easily seen from all places on Earth. The discovery of planets orbiting stars other than the Sun continues at the rate of nearly one a week. The planet discovered around Pollux has the mass of 2.9 Jupiters and orbits the star in 590 days. The discovery was made independently by two teams of astronomers using the so-called Doppler method, a method of detecting the tiny wobble in the motion of the parent star caused by the planet. The Doppler method is the most successful planet detection method but because larger planets cause a bigger wobble, the method tends to find large planets in orbits relatively close to their stars. These systems may not be typical. Doppler observations need to be carried out on many stars over a period of years with a large telescope. The technology needed to measure such small stellar motions was only developed 15 years ago." http://www.nzherald.co.nz/topic/stor...ectid=10399882 Double-A |
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![]() Wayne L wrote: Dear Double-A et al: I submit that the elitist card carrying members of the French IAU The IAU is international. I also submit that the closest know planets to Pollux are Neptune or Pluto, Correct because: 3. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(1)(a), plus note 1 below). .... This discourse has caused me to ponder .... Why does the IAU spell neighborhood neighbourhood? A. They're French B. They have diminished language skills C. They can't come to grips with the fact that English is the Universal language The answer is "None of the above." The correct spelling in the English language is "neighbourhood", although "neighborhood" is a commonly seen variant in the USA. George |
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In sci.astro Wayne L wrote:
Dear Double-A et al: I submit that the elitist card carrying members of the French IAU who claim to have discovered these 200 extra solar "planets" have actually so far discovered exactly zero extra-solar planets. Hello, there, Wayne, and while I agree with the likely purport of your statement that IAU Resolution 5A might receive some refinement and revision, I would emphasize that the IAU is an international organization in which astronomers from many nations, including the USA, participate. Also, I recognize that some humor may be intended, but will try to answer some of your points since they can lead to a better understanding of the issues. I also submit that the closest know planets to Pollux are Neptune or Pluto, depending on the time and/or the French IAU's planet definition for this week. An interesting question, which has come up in other threads, is how the current Resolution 5A should be read in terms of extrasolar planets. One position I've seen suggested is that an earlier IAU document regarding extrasolar planets (2001 or so? -- actually, last revision, 2003) might still apply. Thus see: http://www.dtm.ciw.edu/boss/definition.html For a list of candidate extrasolar planets, interestingly dated 28 August 2006, or four days after the adoption of Resolution 5A, see: http://www.dtm.ciw.edu/boss/planets.html Why? Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a planet of planetary systems. Actually I'd say that they're merely establishing some official definitions, however perfectly or otherwise, for use on Planet Earth -- and that we're free to propose other usages, or revisions of the current IAU definitions. Again, I'm not sure how France plays a special role in this -- more below. 2. The French IAU has decreed from on high that there are only 8 planets in the Universe (see Resolution 5A note 1 below). I agree that Resolution 5A could have been written better and could use some revision (the next IAU General Assembly meets in Rio in 2009). However, much of the wording was borrowed from the work of astronomers in the U.S.A., for example the "has cleared the neighbourhood around its orbit" test for what could have and should have been more expressly defined as a _major_ "planet." Again, the earlier definition of extrasolar planets and the pages for I give URL's above suggest that indeed there may be more than eight planets -- "major planets," that is -- in the universe at large. 3. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(1)(a), plus note 1 below). Try, of course, and George Dishman and I have been having a lively debate on just whether and how Resolution 5A might effect extrasolar planets. I tend myself to assume that the earlier document expressly on these planets might still more or less hold. 4. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(1)(b) below. Well, depending on composition, it might be around 800 km diameter for a planet like Ceres (which evidently meets the test at around 960 km) -- and a planet with a mass of 3 jupiters, sustained by degenerate electron pressure, is rather clearly going to meet it also. 5. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(1)(c). However, papers by astronomers such as Stern and Levison (2002), Basri and Brown (2006), and Soter -- most if not all located in the USA, if I'm right -- have given the concept of "neighborhood clearing" a fairly well-understood meaning, so that it has become a "term of art," to use a legal phrase. I'd suspect that while this is a "circumstantial" test -- it depends on the location of the planet as well as absolute mass -- a superplanet with a mass of 3 jupiters is likely to meet it over a wide range of cases. 6. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. At times, as I understand, observations can indicate a _minimum_ mass only, so that sometimes one needs to ask, "Is this actually a planet, or possibly a brown dwarf at 13 or more jupiters?" More time might be required to refine one's sense of the orbit, and thus the mass. Isn't the gravitational constant assumed to follow the Cosmological Principle that certain natural laws apply uniformly in different parts of the universe? Cosmologists, is this still a reasonable assumption? Further, I submit that these 200 extra-solar "planets" are not even dwarf planets Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a dwarf planet of planetary systems. 2. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(2)(a)). What I might suspect is that the extrasolar planet definitions might be the relevant ones, because any such planet likely to be detected is going to have enough mass for self-gravity to constrain it to a spheroid shape reflecting hydrostatic equilibrium. 3. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(2)(b) below. See above -- 3 jupiters should be more than sufficient (an interesting exercise -- by how many orders of magnitude?). 4. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have not cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(2)(c). Actually, I'd say that 3 jupiters would likely make it a major planet rather than a dwarf planet -- Soter sees the concept as applicable to extrasolar planets, and discusses some possible questions that might arise. 5. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. 6. The IAU has yet to provide a process for determining if borderline objects are either dwarf planets or "other" objects (see Resolution 5A note 2 below). Again, this would only apply to objects of a mass _much_ smaller than three jupiters. Further, I submit that theses alleged extra-solar star wobble causing masses are in fact Small Solar-System Bodies (sub category TNOs or "other small bodies), by the process of elimination and Resolution 5A Section (3) and note 3, as proclaimed by the Universally Esteemed IAU. Since they aren't part of our Solar System, the scope of Resolution 5A, I'd say that some other classification would apply. Why does the IAU spell neighborhood neighbourhood? A. They're French B. They have diminished language skills C. They can't come to grips with the fact that English is the Universal language Actually, "neighbourhood" is a standard British spelling, the Queen's orthography, as it were. From this viewpoint, my own usage, "neighbhorhood," might be taken as a kind of provincialism. Again, this is not to say that IAU Resolution 5A is flawless -- only that it reflects the position of a significant group of astronomers, not least those of the U.S.A. (e.g. Brown and Soter). Your comments do point to one revision I strongly advocate: making it clear that the category "planet" in fact means "major planet," with the other two categories also defining types of planets ("dwarf planets" and Small Solar System Bodies also known as the smaller "minor planets" -- with comets, in a persuasive current view, also included as "minor planets"). Also, yes, we could use a definition applying to all planets, solar or extrasolar. |
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![]() "Margo Schulter" wrote in message ... .... I also submit that the closest know planets to Pollux are Neptune or Pluto, depending on the time and/or the French IAU's planet definition for this week. An interesting question, which has come up in other threads, is how the current Resolution 5A should be read in terms of extrasolar planets. One position I've seen suggested is that an earlier IAU document regarding extrasolar planets (2001 or so? -- actually, last revision, 2003) might still apply. Thus see: http://www.dtm.ciw.edu/boss/definition.html Curious, that means a planet ejected from a binary system ceases to be a planet and becomes a "sub-brown dwarf". Calling it a planet and qualifying that as "free-floating" would seem more logical. That said, my own suggestion (below) has the same effect. For a list of candidate extrasolar planets, interestingly dated 28 August 2006, or four days after the adoption of Resolution 5A, see: http://www.dtm.ciw.edu/boss/planets.html .... Try, of course, and George Dishman and I have been having a lively debate on just whether and how Resolution 5A might effect extrasolar planets. I tend myself to assume that the earlier document expressly on these planets might still more or less hold. I have now drafted an attempt at a more general classification scheme. I first tried to draw the current IAU version for reference though the situation of satellites is a little tricky when using the literal wording. Anyway this is what I produced: http://www.georgedishman.f2s.com/astronomy/IAU.png I then tried to adjust that minimally to add the extra-solar possibilities but it ended up with quite a bit different. I have substituted two names, "planetesimal" instead of "dwarf planet" to remove the linguistic difficulty and "asteroid or comet" instead of "small solar-system body". In hind sight it would have been better to say just "asteroid" as the intention is that is be expanded by footnote to include various types such as TNOs KBOs, QB1'os, comets, etc.. Basically everything smaller than a dwarf planet but larger than dust. Anyway, here it is: http://www.georgedishman.f2s.com/astronomy/GAD.png I would appreciate your comments. I foresee possibly contentious areas (other than name selection which I consider unimportant compared to the criteria) being the inclusion of brown dwarfs as a type of star and the use of "planemo" (which you prompted) whether the object is in orbit or not. I have restricted the use of planet to those with a stable orbit to comply with the IAU suggestion that it should have cleared its neighbourhood since that cannot be determined in say a chaotic ternary system or if the object is free-floating. best regards George |
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![]() Wayne L wrote: Dear Double-A et al: I submit that the elitist card carrying members-- I _started_ reading your article, and got this far before I clicked away. ;-) Peace, Rod Mollise Author of: Choosing and Using a Schmidt Cassegrain Telescope and The Urban Astronomer's Guide http://skywatch.brainiac.com/astroland |
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![]() Wayne L wrote: --snip-- Why does the IAU spell neighborhood neighbourhood? A. They're French That would be "voisinage." Do all Astronomers get their PhDs on-line from the University of Phoenix? Here's a bio of Guy Consolmagno, the President of the IAU Physical Study of Planets & Satellites commission. I see Harvard and MIT in there. He's also the author of Turn Left At Orion. http://clavius.as.arizona.edu/vo/R10...nsolmagno.html His notes about the IAU conference and the Pluto decision: http://homepage.mac.com/brother_guy/.Public/Br%20Guy's%20Pluto%20Opinion.pdf Greg |
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In article .com,
George Dishman wrote: Wayne L wrote: I also submit that the closest know planets to Pollux are Neptune or Pluto, Correct because: No, it's incorrect! Currently the Earth is closer to Pollux than either of Neptune or Pluto. In a century the situation will be different, but right now that's how it is. -- ---------------------------------------------------------------- Paul Schlyter, Grev Turegatan 40, SE-114 38 Stockholm, SWEDEN e-mail: pausch at stockholm dot bostream dot se WWW: http://stjarnhimlen.se/ |
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![]() "Paul Schlyter" wrote in message ... In article .com, George Dishman wrote: Wayne L wrote: I also submit that the closest know planets to Pollux are Neptune or Pluto, Correct because: No, it's incorrect! Currently the Earth is closer to Pollux than either of Neptune or Pluto. Thanks for the correction Paul, I should have been more cautious. In a century the situation will be different, but right now that's how it is. In a few months I suspect even Mercury will be closer than Earth but which is closest is another question. Thanks. George |
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![]() Margo Schulter wrote: In sci.astro Wayne L wrote: Dear Double-A et al: I submit that the elitist card carrying members of the French IAU who claim to have discovered these 200 extra solar "planets" have actually so far discovered exactly zero extra-solar planets. Hello, there, Wayne, and while I agree with the likely purport of your statement that IAU Resolution 5A might receive some refinement and revision, I would emphasize that the IAU is an international organization in which astronomers from many nations, including the USA, participate. Also, I recognize that some humor may be intended, but will try to answer some of your points since they can lead to a better understanding of the issues. I also submit that the closest know planets to Pollux are Neptune or Pluto, depending on the time and/or the French IAU's planet definition for this week. An interesting question, which has come up in other threads, is how the current Resolution 5A should be read in terms of extrasolar planets. One position I've seen suggested is that an earlier IAU document regarding extrasolar planets (2001 or so? -- actually, last revision, 2003) might still apply. Thus see: http://www.dtm.ciw.edu/boss/definition.html For a list of candidate extrasolar planets, interestingly dated 28 August 2006, or four days after the adoption of Resolution 5A, see: http://www.dtm.ciw.edu/boss/planets.html Why? Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a planet of planetary systems. Actually I'd say that they're merely establishing some official definitions, however perfectly or otherwise, for use on Planet Earth -- and that we're free to propose other usages, or revisions of the current IAU definitions. Again, I'm not sure how France plays a special role in this -- more below. 2. The French IAU has decreed from on high that there are only 8 planets in the Universe (see Resolution 5A note 1 below). I agree that Resolution 5A could have been written better and could use some revision (the next IAU General Assembly meets in Rio in 2009). However, much of the wording was borrowed from the work of astronomers in the U.S.A., for example the "has cleared the neighbourhood around its orbit" test for what could have and should have been more expressly defined as a _major_ "planet." Again, the earlier definition of extrasolar planets and the pages for I give URL's above suggest that indeed there may be more than eight planets -- "major planets," that is -- in the universe at large. 3. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(1)(a), plus note 1 below). Try, of course, and George Dishman and I have been having a lively debate on just whether and how Resolution 5A might effect extrasolar planets. I tend myself to assume that the earlier document expressly on these planets might still more or less hold. 4. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(1)(b) below. Well, depending on composition, it might be around 800 km diameter for a planet like Ceres (which evidently meets the test at around 960 km) -- and a planet with a mass of 3 jupiters, sustained by degenerate electron pressure, is rather clearly going to meet it also. 5. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(1)(c). However, papers by astronomers such as Stern and Levison (2002), Basri and Brown (2006), and Soter -- most if not all located in the USA, if I'm right -- have given the concept of "neighborhood clearing" a fairly well-understood meaning, so that it has become a "term of art," to use a legal phrase. I'd suspect that while this is a "circumstantial" test -- it depends on the location of the planet as well as absolute mass -- a superplanet with a mass of 3 jupiters is likely to meet it over a wide range of cases. 6. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. At times, as I understand, observations can indicate a _minimum_ mass only, so that sometimes one needs to ask, "Is this actually a planet, or possibly a brown dwarf at 13 or more jupiters?" More time might be required to refine one's sense of the orbit, and thus the mass. Isn't the gravitational constant assumed to follow the Cosmological Principle that certain natural laws apply uniformly in different parts of the universe? Cosmologists, is this still a reasonable assumption? Further, I submit that these 200 extra-solar "planets" are not even dwarf planets Because 1. The French IAU is the Supreme and only governing body of the Universe vested with the power to determine what is and is not a dwarf planet of planetary systems. 2. None of these alleged extra-solar star wobble causing masses are claimed to be orbiting the Sun (see Resolution 5A(2)(a)). What I might suspect is that the extrasolar planet definitions might be the relevant ones, because any such planet likely to be detected is going to have enough mass for self-gravity to constrain it to a spheroid shape reflecting hydrostatic equilibrium. 3. There has been no claim or data put forth that these alleged extra-solar star wobble causing masses have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (nearly round) shape, partly or wholly because the IAU has no definition of what is "sufficient mass" (see Resolution 5A(2)(b) below. See above -- 3 jupiters should be more than sufficient (an interesting exercise -- by how many orders of magnitude?). 4. No peer review data, nor even "bragging rights" news releases have been forthcoming showing that these alleged extra-solar star wobble causing masses have not cleared the neighbourhood around their orbits, mostly because they have no data, and partly because the IAU has provided no definition of the words "cleared", nor "neighbourhood", as used in Resolution 5A(2)(c). Actually, I'd say that 3 jupiters would likely make it a major planet rather than a dwarf planet -- Soter sees the concept as applicable to extrasolar planets, and discusses some possible questions that might arise. 5. The claimed masses of these alleged extra-solar star wobble causing masses is based on an unproved assumption that the gravitational constant is the same at their locations as it is on Earth. Einstein made no such claim. 6. The IAU has yet to provide a process for determining if borderline objects are either dwarf planets or "other" objects (see Resolution 5A note 2 below). Again, this would only apply to objects of a mass _much_ smaller than three jupiters. Further, I submit that theses alleged extra-solar star wobble causing masses are in fact Small Solar-System Bodies (sub category TNOs or "other small bodies), by the process of elimination and Resolution 5A Section (3) and note 3, as proclaimed by the Universally Esteemed IAU. Since they aren't part of our Solar System, the scope of Resolution 5A, I'd say that some other classification would apply. Why does the IAU spell neighborhood neighbourhood? A. They're French B. They have diminished language skills C. They can't come to grips with the fact that English is the Universal language Actually, "neighbourhood" is a standard British spelling, the Queen's orthography, as it were. From this viewpoint, my own usage, "neighbhorhood," might be taken as a kind of provincialism. Again, this is not to say that IAU Resolution 5A is flawless -- only that it reflects the position of a significant group of astronomers, not least those of the U.S.A. (e.g. Brown and Soter). Your comments do point to one revision I strongly advocate: making it clear that the category "planet" in fact means "major planet," with the other two categories also defining types of planets ("dwarf planets" and Small Solar System Bodies also known as the smaller "minor planets" -- with comets, in a persuasive current view, also included as "minor planets"). Also, yes, we could use a definition applying to all planets, solar or extrasolar. ayyes! 5A iff 3B9V iff P=4.594/2C [x........ P]. The Gold Dust room in Reno would be the place to settle this once and for all. |
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"WL" == Wayne L writes:
WL I submit that the elitist card carrying members of the French IAU WL who claim to have discovered these 200 extra solar "planets" have WL actually so far discovered exactly zero extra-solar planets. I WL also submit that the closest know planets to Pollux are Neptune or WL Pluto, depending on the time and/or the French IAU's planet WL definition for this week. Wow. I'm not sure whether to be impressed or amused that somebody goes to so much trouble to get themselves annoyed. In any event, ... WL Why? WL Because WL 1. The French IAU is the Supreme and only WL governing body of the Universe vested with the power to determine WL what is and is not a planet of planetary systems. WL 2. The French IAU has decreed from on high WL that there are only 8 planets in the Universe (see Resolution 5A WL note 1 below). This topic came up in the discussions at the IAU. There was considerable concern about how this definition applied to extrasolar planets. During the week, the resolution was changed to insert the words "in the Solar System" to make it clear that this definition applies *only* to objects within the solar system. There is another IAU committee still working on the definition of an extrasolar planet. -- Lt. Lazio, HTML police | e-mail: No means no, stop rape. | http://patriot.net/%7Ejlazio/ sci.astro FAQ at http://sciastro.astronomy.net/sci.astro.html |
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