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Planet X
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The following statement appearing under [[Pluto#Planet X?]] is somewhat inaccurate:
The following statement appearing under [[Pluto#Planet X?]] is somewhat inaccurate:
<blockquote><nowiki>When Pluto was discovered in 1930, H.P. Lovecraft wrote a short story ("The Whisperer in Darkness") which proposed that Pluto was a base of invading extraterrestrials known as the Mi-go, who called it Yuggoth.</nowiki></blockquote>According to [[S. T. Joshi]] and David E. Schultz (''An H. P. Lovecraft Encyclopedia'' ISBN 0-3133-1578-7) this is not true: "It cannot be said that the discovery of Pluto inspired the writing of ["The Whisperer in Darkness"] (p. 298). Lovecraft began writing the story February 24, 1930, but the discovery of Pluto was not officially announced until March 14. Lovecraft was already aware that a trans-Neptunian planet might exist and had alluded to such a possibility in previous writings. Thus, the discovery of Pluto and the writing of the tale are simply coincidences.<br><small>_,-~</small>[[User:RlyehRising|<small><sup>R<big>'lyeh<big>R</big>isin</big >g</sup></small>]]<small>~-,_</small>&nbsp;&nbsp;<font color=blue><small>02:58, 2 June 2006 (UTC)</small></font>
<blockquote><nowiki>When Pluto was discovered in 1930, H.P. Lovecraft wrote a short story ("The Whisperer in Darkness") which proposed that Pluto was a base of invading extraterrestrials known as the Mi-go, who called it Yuggoth.</nowiki></blockquote>According to [[S. T. Joshi]] and David E. Schultz (''An H. P. Lovecraft Encyclopedia'' ISBN 0-3133-1578-7) this is not true: "It cannot be said that the discovery of Pluto inspired the writing of ['The Whisperer in Darkness']" (p. 298). Lovecraft began writing the story February 24, 1930, but the discovery of Pluto was not officially announced until March 14. Lovecraft was already aware that a trans-Neptunian planet might exist and had alluded to such a possibility in previous writings. Thus, the discovery of Pluto and the writing of the tale are simply coincidences.<br><small>_,-~</small>[[User:RlyehRising|<small><sup>R<big>'lyeh<big>R</big>isin</big >g</sup></small>]]<small>~-,_</small>&nbsp;&nbsp;<font color=blue><small>02:58, 2 June 2006 (UTC)</small></font>

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Template:FAOL Template:V0.5

Prior discussion has been moved to Talk:Pluto_(planet)/Archive1

Diameter

I changed the diameter back to 2390 per the NASA factsheet that is linked at the bottom of the Pluto page. This also matches the given volume. If NASA doesn't have it right, who would? The "most sources" referred to by the previous poster cannot be relied on. If someone has other numbers from a major astonomical org. then please post here. I also checked the diameter in miles, corrected the diameter in Earths per the NASA factsheet, checked the volume against the NASA number, and verified the area by calulation from the NASA number. - --Enon 19:45, 24 September 2005 (UTC)[reply]

Changed the diameter from 2390 km to 2274 km. Most sources say around 2300 km, only Wikipedia had 2390 km, which seems wrong.

On Template:March 19 selected anniversaries

Pluto: American planet, European Kuiper belt object?

Sorry, but in the light of recent discoveries it appears more than obvious that Pluto is nothing but a (huge) object belonging to the Kuiper belt. Its status as a planet, therefore, has to be considered a whimsical anachronism, and it's rather funny to read through the (more or less) scientific debate on both sides of the Atlantic. In the 1930s, Pluto's classification as a planet was based on insufficient knowledge about the outer Solar System (being understood as its outer edge, rather than the inner edge of the - then unknown - Kuiper Belt). Fair enough, but what is it based on today? American patriotism? 80.145.233.192 00:47, 11 February 2006 (UTC)-[reply]

Wikiproject Echo

Template:FAOL

There are many similarities between the French and English articles, including numerous passages which are translations of one another. It seems that borrowing of content has already happened. As it stands, it does not seem that there is any additional content in the French article that could be added to the English article. -- Curps 14:52, 6 August 2005 (UTC)[reply]

Orbital period?

I've seen Pluto's orbital period listed as 247.7 or as 248.54 Earth years. Converting from Julian to Gregorian won't account for this discrepancy, or with the value 248.09 Julian years in the article's table. Can somebody clarify?--192.35.35.35 20:52, 14 Feb 2005 (UTC)

Well, I checked out JPL Horizons, and it turns out that Pluto's orbital elements are considerably affected by perturbations. The instantaneous orbital elements (what they would be if no further perturbations were ever received) show the following orbital periods at different times:
  • 1920: 91438 d
  • 1980: 91828 d
  • 2005: 91115 d
  • 2040: 90210 d
  • 2100: 90065 d
The variation here is almost 3 1/2 years. So maybe the figures quoted represent some kind of average... but I wouldn't be surprised if that average also varies slowly over time. -- Curps 02:35, 15 Feb 2005 (UTC)
Then what is the value 90,613.3058 d in the table? Genuine result of a careful computation, or wildly unjustified precision? Do we really know the period down to the nearest 10 seconds, or only within ± 2 years?--192.35.35.34 18:00, 15 Feb 2005 (UTC)
At any given time, we know Pluto's orbit with extremely high accuracy, it's just that that orbit changes over time as a result of perturbations (but again, we can predict those perturbations with extremely high accuracy). So I'm sure this figure represents a valid result and the digits after the decimal point represent the actual precision... I'm just not sure what result it represents. -- Curps 19:36, 15 Feb 2005 (UTC)
Let's see. The JPL data tables give the semi-major axis with ten digits of precision, and we know the heliocentric gravitational constant and the value of the AU to twelve digits. Nine digits of precision on the period (more accurately, the instantaneous mean orbit for J2000) is what the error bars give.
Urhixidur 01:32, 2005 Feb 16 (UTC)
The upshot I get, then, is that these superprecise results are not actual real world orbital periods, but extrapolations fraught with uncertainty over what the actual perturbations will be in the long long run. I, too, can apply Kepler's law and get 9 decimal places, but I'm ignorant of what 240-some years of perturbations do to the final orbital period or the accuracy with which it is known.--192.35.35.36 15:43, 2 Mar 2005 (UTC)
Not quite. The instantaneous orbit is very well known, and so is its future evolution over a fairly large time span, since we know the masses of all main objects quite well, down to the larger asteroids. Uncertainty creeps in, but before it can make a detectable difference probably takes on the order of a million years or more. Note that an orbit may also vary "chaotically" but within very well-defined bounds. Search the ADS, there may be some papers on the long-term orbit of Pluto already in there.
Urhixidur 23:04, 2005 Mar 2 (UTC)

Other symbols

See Symbols.com

On Pluto's Name

The article mentions that the grandfather sent the idea for Pluto's name to a former Astronomer Royal. Does this refer to Frank Dyson, as he was the only retired Astronomer Royal at the time?

Numerous sources say that it was Herbert Hall Turner who cabled his colleagues in America with Venetia Burney's suggestion (see [1], [2], [3]). He was not, however, a former Astronomer Royal. I have edited the article accordingly. -- Curps 00:19, 7 August 2005 (UTC)[reply]

Also, and by the way, you've got to be kidding me when you state that an 11-year old by the name of Venetia Phair (nee Burney) knew all the deep facts about Roman and Greek mythology.

The real reason she suggested "Pluto" was because that was her favourite cartoon character. Yes, the lovable dog courtesy Disney.

Please allow me to kill this rumor once and for all. Pluto first appeared in The Chain Gang, released 18 August 1930, though he did not receive the name "Pluto" until a few cartoons later. The name for the planet Pluto was announced 1 May 1930. May comes before August. (And in the future, sign your contributions with 4 ~s, which will turn into a signature and timestamp.) DenisMoskowitz 15:35, 23 February 2006 (UTC)[reply]
Right, the dog was named after the planet.--Jyril 17:02, 23 February 2006 (UTC)[reply]

Pluto's composition

Is there any more information available about Pluto's surface/interior composition? Right now it just mentions nitrogen and carbon monoxide ice. Surely there's more information than that. Kaldari 18:28, 23 May 2005 (UTC)[reply]

This page may be helpful if someone wants to write up a new section. Kaldari 18:46, 23 May 2005 (UTC)[reply]

Poorly written section

"there may *now* be many other such objects beyond Neptune -- the foremost of these being Fred L. Whipple"

Heheh!

Requested Move

This article has been renamed after the result of a move request.

Atmosphere

I removed the following sentence from the article:

It is thought by some that Pluto shares its atmosphere with its moon.

It struck me as misleading. I think the intention of the author (and the closest thing I found to the sense of this) is that some of the atmosphere escapes when it is at its hottest and somehow interacts with Charon. The sentence as it was implies that that an extremely thin atmosphere could be shared across 20000km, or that it's believed Charon has an atmosphere. Both of these seem unlikely to me, but if anyone knows what this is about, please put it back. Moogsi 13:18, 16 September 2005 (UTC)[reply]

Besides, it's clearly a disco ball. lysdexia 00:52, 9 October 2005 (UTC)[reply]

There is contradictory information about the atmosphere. In the box area, atmosphere of Pluto is nitrogen and methane. In the written section, the atmosphere is nitrogen and carbon monoxide. Which is it?

Planetoid Pluto

I'm just another guy who is clueless when it comes to Astronomy, but there are scientists who believe that since Pluto is smaller than half of Saturn’s or Jupiter’s moons that it's not a planet at all. The Astronomers who support objects smaller than moons aren't planets apply here. They suggest that there is only 8 planets in the Sol planetary system and 1 enormous planetoid.

NASA is on the verge of confirming this too. It's about people excepting the truth it's not a planet that's a problem. There is a lot of denial here — Preceding unsigned comment added by Renegadeviking (talkcontribs)

It isn't up to NASA, but a decision by the International Astronomical Union (IAU) which is currently studying the situation to determine a precise definition of a planet. Currently, the IAU considers Pluto to be a planet.Shsilver 19:51, 21 September 2005 (UTC)[reply]
  • The planetology articles in En. wikipedia are in the verge of useless and disinformative articles, full of POV on this subject about planethood. This article about Pluto is dreadful, and it focuses on useless things about planets, namely theories that some wikipedians like a lot, like that planetoid or asteroid thing. It is really sad. In every article where Pluto comes along comes this theory that Pluto is not a planet. What a stupid idea to define a planet by the size of the moons of Saturn, what kinds of scientists are those, some wikipedians? I don't believe that real scientists said that. Very nice scientific definition! A planet is an object bigger than the moons of Saturn. OMG. "An enormous planetoid"?! Oh jesus... -Pedro 23:22, 28 October 2005 (UTC)[reply]
Don't worry, it's just a matter of time and the IAU will sort it all out. Frankly, any object orbiting the Sun, that isn't in resonance with a larger object with an overlap in the range (q ,Q ), is >95% of the mass orbiting near that semimajor axis, and is rendered spherical due to its mass, will someday be the "official definition". Due to Pluto being locked in a 3:2 dance with the more massive Neptune, that is what will sink Pluto. Resonance also will sink Xena, Orcus, and many other TNO's. And the mass fraction will sink Quaoar. Sedna might skate by: but as soon as a second Sedna-class object of similar mass is found (and it will be, surely) it loses planethood, too. As for Pluto not being a planet: not a problem, although minor planet number 10000 is gone (as is 100000 as of October 2005), the elegant solution is to use 0. 0 Pluto does have quite a ring to it. --Sturmde 02:43, 29 October 2005 (UTC)[reply]
I agree with this point of view. Currently it would seem to me at least that Sedna has a greater claim on planethood than Pluto, given the uniqueness of its orbital location. I particularly agree with your last point there on classifying Pluto with Minor Planet number 0. I actually suggested that to Brian Marsden of the Minor Planet Centre about 7 years ago when the whole debate about classifying it as 10000 was floating about, and he indicated he had a favourable view of that solution.
You make a claim about what will "someday be the 'official definition'" of a planet. One, Wikipedia is not a crystal ball, so claims about what will be are out-of-place here. On the assumption that some currently argue those criteria should be the official definition of a planet, can you please cite your source? Thanks. --DragonHawk 14:49, 2 January 2006 (UTC)[reply]
Excuse me, but you're confusing articles, with discussion about articles. I haven't edited the article to reflect my comments above. THAT would be what you're bogusly claiming has been done. It is not an assumption that there is currently debate. There IS current debate. See the IAU page at[4], and you'll note that the final determination will be in September 2006. What I have provided above is the shared opinion of a number of actual astronomers and physicists (such as me) who have interests in Solar System dynamics. Pluto is in "trouble" because it's in a 3:2 lock with Neptune; and it isn't the preponderance of matter contained in the range (qPluto,QPluto). Its only argument is that it is rendered spherical by its gravity. Providing an informed scientific observation in the DISCUSSION about an article is entirely appropriate. You may of course choose to ignore anything in discussions at your own leisure. Were these observations expressed in the article, then that would be different. --Sturmde 20:57, 15 March 2006 (UTC)[reply]

This is just a comment I will add at the bottom of this topic. If the "planet" Pluto should be found to be on the inside of the orbit of the exterior asteroid belt Kupor Belt (I believe thats how its spelled) then as long as the orbit is a respectible distance from the belt wouldn't it make sense to classify it as a planet. Given that it could be an asteroid from the Kupor Belt that was somehow pulled into orbit, but the fact that it does indeed have another object that orbits it as a moon and the fact it is profoundly more rounded then an asteroid would classify it as a planet. As we further leave the forces of gravity induced by the sun we have to take such things into consideration, don't we? As we go out of the suns influence obviously certain conditions would change and therefore the orbits and appearance of such planets that can be found there. -Comment by Just another guy on November 1 2005

  • I think we all have different perpectives of what's a planet, on a common view and a planetologist view it is a planet. But to those people who looks at the orbit it isnt. But Lets see... Titan is a moon of Saturn and it has a denser atmosphere than Earth. So, Earth is not a planet, but a planetoid. And, what if we discover something bigger than Earth in the Kuiper Belt? Certainling we will also question Earth position as a planet in the future, the same for the other planets. It is acceptable too see the smaller KBO's and Ceres as planetoids, but something bigger than Pluto should be named a planet, and the limit is already big anough cause a planet should be every round object that "doesnt shine by itself" (in a simplist view). We can have terrestial planet, gas planets, ice planets and planets that dont orbit any star. -Pedro 19:25, 3 November 2005 (UTC)[reply]

If Pluto is considered a planet for "planetologist" reasons, then so are dozens of other objects. Pluto would never be called a planet if it were discovered today. "The planet Pluto" is a mistake and an embarrassment. I am mystified by people who are emotionally attached to a nine-member planet list that happens to be wrong. 216.99.217.92 05:36, 16 November 2005 (UTC)[reply]

I'm checking out this article and this talk section for the first time. While it's clear that there is some question on Pluto's status, we need to keep in mind the Wikipedia policy of verifiability. Regardless of what any of us believe is the right classification for Pluto, we need to keep in mind that Wikipedia's purpose is not to establish correctness, but to summarize the work of others. So, when making claims about Pluto's status one way or the other, please cite your sources. This is not a place for unverified claims. --DragonHawk 14:29, 2 January 2006 (UTC)[reply]

Blah. Note tab at top: "discussion". Not "article". Your lecture is inappropriate and condescending.
  • If some dimwitted scientists think Pluto isn't a planet because it's smaller than a moon, I've got news for you: MERCURY ISN'T A PLANET, EITHER. That's right, it's smaller than both Ganymede, Titan, and is just barely larger than Callisto. Pluto is a planet, live with that. It orbits the sun, has an atmosphere, 3 moons, is a sphere, and has weather. Can Mercury say that? It orbits the sun, but has no atmosphere, weather, or moons. It's some piece of brown rock with a bunch of craters. In 4 million years or so it will burn up instantaeneously when the Sun becomes a Red Giant, and I can't wait for that to happen! Pluto has been a planet since 1930, society accepts that, I accept that, and the IAU accepts that. I can't wait to see you naysayers get slapped in the face when September rolls around and Pluto is STILL a planet. How many planets are in our solar system, teacher? 9. What's the NINTH planet agian? PLUTO.

As this review shows, Camelot 30K occurs on "1999 ZX", "a celestial body between comet and planet, out in the Kuiper belt at 35 AU from the Sun". It turns out that designation is "safe", since no minor planet can have Z as it first letter (see Provisional designation of asteroids or New- And Old-Style Minor Planet Designations) —Z would be the half-month after December 31... Urhixidur 23:03, 4 October 2005 (UTC)[reply]

article introduction

Pluto is a small celestial body in the outer solar system. 
Discovered in 1930 and originally classified as a planet, its 
status is currently under dispute.

Someone added this "small celestial body". It is in dispute by some, but its status is that it is a planet. It seems that wikipedia as taken a position, against what is the common sence and the official designation by the IAU.

The problem is that "common sense" is _opposed_ to the official designation by the IAU, which was approved a long time ago based on data which turned out to be wrong. Common sense says Kuiper belt objects orbiting in resonance with Neptune aren't planets. If Pluto is a planet, then so are all the rest of them. Either way the "nine planet story" we remember from grade school is bullshit. 216.99.217.92 05:42, 16 November 2005 (UTC)[reply]

THE STATUS OF PLUTO: A CLARIFICATION IAU Press release.

Besides, what size is small? what is celestial body a star? I've said previously this article focus little on the planet, but is foccus to much on controversy over what humans on Earth call it.

surely, It needs a POV tag. -Pedro 21:52, 9 November 2005 (UTC)[reply]

"what is celestial body a star?" What the hell are you talking about? 216.99.217.92 05:42, 16 November 2005 (UTC)[reply]
Dropped small. Not small compared to its neighbourhood. Does not need a POV tag unless we claim A not B. Come up with a sentence briefly explaining the debate. Marskell 22:32, 9 November 2005 (UTC)[reply]
I changed 'originally classified as a planet' to 'officially classified as a planet', to stress that it hasn't changed (yet). The Singing Badger 22:36, 9 November 2005 (UTC)[reply]

Pluto is not a real planet. Latest scientific research proves this. Pluto the dog was such a faker.

I recently changed the article herein to false information. I apologize. Please return it to normal.

Pluto's albedo is wrong in the article.

This article lists Pluto's albedo a 0.30. It is considerably more reflective than that; the estimate used by Mike Brown at Caltech in his article on the "New Planet",:

http://www.gps.caltech.edu/~mbrown/planetlila/index.html#hack

lists the ablbedo at 0.60. That's actually at the low range of albedo estimates that I have read over the years. Similarly, the albedo of Triton is listed at 0.76. The last I heard, which was around the time of the Voyager flyby, was 0.90.

No absolute magnitude is listed for Pluto, Triton, Charon, or several other objects. I stumbled onto this error because I wanted the absolute magnitude to compare to other absolute magnitudes listed by the Minor Planet Center. Also, there is some dispute about the diameter. As a result, I am calling for help on this rather than editing it directly. Thank you. Mike Emmert 19:41, 21 December 2005 (UTC)Michael C. Emmert[reply]

Yeah, albedo of 0.3 is way too low for Pluto. I replaced it with a value of 0.5 – 0.7 from NSSDC's Pluto fact sheet[5]. I wonder if this wide range represents uncertainty or albedo differences, because Pluto's surface has highly contrasting lighter and darker regions.--Jyril 01:35, 30 December 2005 (UTC)[reply]

Dark King Star - Kanji

Can someone insert the Kanji characters into the article for Pluto like we have for the other planets? WilliamKF 03:23, 15 January 2006 (UTC)[reply]

Okay I found on wiktionary: 冥王星 WilliamKF 03:34, 15 January 2006 (UTC)[reply]

Retrograde rotation

I believe Pluto rotates retrogradely? At least my physics books and a couple of google's says so. Anyway, I don't know how to edit those Infoboxes - can't find any button for it.

-josteinaj 20/01/06 20:15

Pluto's axial tilt is over 90° (122.54°), which means its rotation is indeed retrograde. However, the difference is small enough that it is better to say Pluto orbits on its side than it orbits backwards. Uranus has similar situation, whereas Venus rotates clearly in retrograde motion.
Fixed; the minus sign denoting the retrograde motion was missing before the rotation period.
You can't edit infoboxes directly, instead you must edit the infobox template, which in the case of Pluto is Template:Planet_Infobox/Pluto.--Jyril 20:09, 20 January 2006 (UTC)[reply]

Is Pluto a Planet?

I found this article http://www.smh.com.au/articles/2003/03/09/1047144868646.html if anyone wants to add information from it please do. there are many more articles like this one.

  • Yes, Pluto is a planet. Always has been, always will.

new horizons

non-sequitur

'Constance Lowell, Percival's widow who had delayed the search through her lawsuit,...' what lawsuit? Has something been removed here or have I missed something?Badgerpatrol 22:37, 5 February 2006 (UTC)[reply]

CJKV name

In Vietnamese, Pluto is called Diêm Vương Tinh or Sao Diêm Vương, named after Yama (閻王), not Minh Vương Tinh (冥王星) as in the CJK languages. At the time of Pluto's discovery, the Chinese grip on Vietnamese culture isn't as strong as before and Vietnamese had already started to be written in quoc ngu. Writing 冥 in quoc ngu would become Minh, which is easily misinterpreted as "bright" (since that is the much more common meaning of minh), and I suspect that's the reason it wasn't named that. DHN 18:04, 9 March 2006 (UTC)[reply]

Actually, like in Vietnamese, 冥 and bright (明) share the same pronunciation in Chinese, too. — Yaohua2000 09:06, 11 March 2006 (UTC)[reply]

NPOV concerns

Some editors are getting caught up on the amount of controversy surrounding the classification of pluto as a planet. I find that the addition of qualifiers, such as "some controversy" and "sometimes under controversy" marginalize debate over pluto's classification, and so violate the standards at WP:NPOV. Ihe amount of controversy isn't as important as the fact that there is controversy. shaggy 02:57, 14 March 2006 (UTC)[reply]

First Photograph?

On the front page today, it is said that Pluto was photographed for the first time on March 19, 1915. The article indicates the same thing with no additional information. It this a reference to photos taken at Lowell Observatory on March 19 and April 17, 1915 with the 9-inch camera from Swarthmore College, or to some other photograph(s)?

In any case, does anyone have information about when these prediscovery images were discovered, and when the positions derived from them were incorporated into a determination of Pluto's orbit? As most hanging around here will know, prediscovery observations of minor planets have been of great significance to orbit determination in the past, and I'm curious whether this was the case with Pluto. A fifteen-year prediscovery arc in the first years of Pluto's observation could have been significant.

I've done some checking in the references I have, and am turning up empty-handed on both questions. --Jeff Medkeff | Talk 01:06, 19 March 2006 (UTC)[reply]

Most of the prediscovery observations were found within a year or so of the discovery in 1930, although I don't recall about those specific ones (I'll check my source tonight). I have a list of them if people are interested in it being posted. CFLeon 21:47, 5 April 2006 (UTC)[reply]


Second Largest

I reverted a edit that said that Pluto was the second largest. I assume in reference to 2003 UB313, which is already mentiond in the article, This link http://www.gps.caltech.edu/~mbrown/planetlila/ says 2003 UB313 is a Kuiper belt object, is there some doubt about this? Should we change it back to Second largest object? Orangutan 18:33, 30 March 2006 (UTC)[reply]

It's a scattered KBO, like Chiron. It has an inclination of 39°, compared to Pluto's 12°. The Scattered disc is usually considered apart from the Kuiper Belt, just as with the Main Belt, but that's a matter of definition. kwami 19:29, 30 March 2006 (UTC)[reply]
Thanks Kwami, That's what I love about Wikipedia, I'm always learning new stuff.Orangutan 14:35, 31 March 2006 (UTC)[reply]

100 Planets?

The problem with classifying Pluto as a planet is that: suppose we find a hundred objects that size out beyond Neptune? Or 200? or 1000? Do we WANT a hundred planetary bodies to memorize? It's basically the same problem that the 19th Centurians faced with the bodies between Mars and Jupiter, except their's was easier- it was quickly apparent that none of the objects was even the size of Luna, let alone Mercury. So they came up with 'minor planets', and that worked fine. Our problem is rather more complicated by Pluto being the only one known for over 60 years. We need to consider what is the MOST USEFUL definition. It certainly is useful to have names for the type of movement: primary vs secondary revolution around a star ('planet' vs 'moon')in rather low eccentric orbits to distinguish from comets (but aren't there some comets with lower eccentricies than Pluto?). So, using that, Pluto is a planet (but so is Ceres, Juno, Eros, Chiron, etc.). However, that can be carried TOO far, with all the tens of thousands of bodies just over a km!!! So, there NEEDS to be a size limit, 'major planets' vs 'minor planets' ('planets' vs 'planetoids'?; although I propose 'planetoid' as being very fitting for the loose interstellar bodies not orbiting a star). The POOREST choice is probably what the entertainment industry and some PR people for NASA do already and letting size ALONE being the factor and upgrading the major moons to 'planets'. There's ALREADY a word for large spherical bodies with atmospheres, no matter if they're revolving around a star or a planet: 'worlds'. As I see it, our BEST solution is to keep it at 8 planets (I know, what if we find an Earth-sized body out there? or even another Jupiter or larger?), and 2 'minor planet belts' (we can work on the exact term) typified by Ceres and Pluto. Perhaps a new term: I like 'plutinos', but it's become restricted to a particular type of orbit; and I think 'cubinos' and such, while useful for destinguishing between different types is too restricting to use as a general term. How about a contest like they did with picking Pluto's name? For a dollar (or equivalent currency), you can make an entry to pick the generic name of the trans-neptunians? Set up some basic rules (limited to 3 syllables, NO living people, no businees intests represented, that sort of thing), run the contest for a year or two, and have the winner picked by the IAU? All proceeds go to fund research on TNOs. Just give me credit for the idea! CFLeon 21:47, 5 April 2006 (UTC)[reply]

I'm not sure what kind of a response you're looking for, but this page is meant for discussing the Wikipedia article on Pluto, not the IAU policies on Pluto, so your idea won't get much exposure here. This same debate has been going on for decades, and is also occurring on Talk:Planet if you're interested. --P3d0 20:12, 27 April 2006 (UTC)[reply]

Barycenter; Inclination

  • Could someone trace the source of the statement that the barycenter lies above the planet's surface, please? New data from (Bluie, Grundy et al. 2006 do not seem to support that (mass ratio: 0.1165±0.0055)
  • Does someone know the source of the inclination data for the moons (Charon's infobox)? Again, they are at odds with the source quoted above (~96 degrees to the ecliptic). Thank you. Eurocommuter 16:26, 27 April 2006 (UTC)[reply]

P1 and P2 Names

Any idea when the names for P1 and 2 will be out? Aeon 18:31, 30 April 2006 (UTC)[reply]

Research

If anyone is needing info on Pluto, I wrote a paper about it last year. User:The_stuart/Is_Pluto_a_Planet --The_stuart 01:36, 9 May 2006 (UTC)[reply]

I think you meant nuclear fusion in your article. --P3d0 20:04, 9 May 2006 (UTC)[reply]

What the hell is that thing used for a pictur of pluto at the top of the page?That doesnt even look like pluto.--Killswitch Engage 16:17, 25 May 2006 (UTC)Killswitch Engage[reply]

That is an image taken with I believe the Hubble. As of now no images other tahn a few low res pics have been taken. Other images are drawn or created by people. Aeon 22:17, 25 May 2006 (UTC)[reply]
If you know what Pluto looks like, feel free to tell us. Otherwise we have to wait until 2015 when New Horizons gets there. The title image is created from data collected from the mutual eclipses of Pluto and Charon which occurred between 1985 and 1990. Maps created from Hubble data are less detailed, but unlike this they cover whole Pluto except for the south polar region.--JyriL talk 05:44, 26 May 2006 (UTC)[reply]


orbit

i came here wanted to know how many years it takes for pluto to complete its orbit. this should be in the orbit section. thanks. --MateoP 20:47, 27 May 2006 (UTC)[reply]

Planet X

The following statement appearing under Pluto#Planet X? is somewhat inaccurate:

When Pluto was discovered in 1930, H.P. Lovecraft wrote a short story ("The Whisperer in Darkness") which proposed that Pluto was a base of invading extraterrestrials known as the Mi-go, who called it Yuggoth.

According to S. T. Joshi and David E. Schultz (An H. P. Lovecraft Encyclopedia ISBN 0-3133-1578-7) this is not true: "It cannot be said that the discovery of Pluto inspired the writing of ['The Whisperer in Darkness']" (p. 298). Lovecraft began writing the story February 24, 1930, but the discovery of Pluto was not officially announced until March 14. Lovecraft was already aware that a trans-Neptunian planet might exist and had alluded to such a possibility in previous writings. Thus, the discovery of Pluto and the writing of the tale are simply coincidences.
_,-~R'lyehRising~-,_  02:58, 2 June 2006 (UTC)[reply]