Wikipedia:Featured article candidates/243 Ida/archive1
Tools
Actions
General
Print/export
In other projects
Appearance
From Wikipedia, the free encyclopedia
- The following is an archived discussion of a featured article nomination. Please do not modify it. Subsequent comments should be made on the article's talk page or in Wikipedia talk:Featured article candidates. No further edits should be made to this page.
The article was promoted by Karanacs 18:32, 12 May 2009 [1].
Toolbox |
---|
I am nominating this for featured article because Reyk and I have significantly improved it and would like an independent assessment. This was previously assessed as a good article by OhanaUnited and later received a thorough peer review by Chzz and several other editors. 243 Ida is one of the few asteroids imaged by a space probe. Wronkiew (talk) 01:35, 16 April 2009 (UTC)[reply]
- Wronkiew and I have extensively rewritten this article and improved it a lot. The suggestions and concerns raised at the Good Article review and the Peer Review have, I think, been addressed and have further improved the article. I think it is now good enough that it meets, or at least is very close to meeting, all of the featured article criteria. Reyk YO! 01:44, 16 April 2009 (UTC)[reply]
- Tech. Review
- There are no disambiguation nor dead external links found with dab finder tool and the links checker tool, respectively.
The following ref is used more than once, and appears more than once in the ref section, use the ref name already used before.
{{harvnb|Greeley|Sullivan|Pappalardo|Veverka|1994|p=469}}--Truco 02:56, 16 April 2009 (UTC)[reply]
- Fixed. Reyk YO! 03:02, 16 April 2009 (UTC)[reply]
- I have to say, while going through GAN, I'm very impressed with its current condition and its thoroughness. This is one of those few GAs that are ready to go for FA at any time. OhanaUnitedTalk page 03:03, 16 April 2009 (UTC)[reply]
- Comments - sources look okay, links checked out with the link checker tool. Ealdgyth - Talk 14:22, 16 April 2009 (UTC)[reply]
CommentsHey mate! I believe I owe you some review work. Oppose for now. Lots of ambiguities and fuzzy patches. --Cryptic C62 · Talk 18:27, 17 April 2009 (UTC)[reply]
|
- "Prior to the flyby" Erm, what flyby? The lead previously mentioned that the asteroid was visited. Do "visit" and "flyby" refer to the same thing?
- Clarified so it reads " Galileo flyby ". Reyk YO! 00:39, 17 April 2009 (UTC)[reply]
- What I meant was that "visit" implies that something actually landed on the asteroid, so it's not clear that Galileo's "visit" and "flyby" are the same thing. --Cryptic C62 · Talk 01:41, 17 April 2009 (UTC)[reply]
- I have to disagree there; I don't think the word "visit" implies an actual landing. The featured article Jupiter, for instance, uses the word "visit" to describe the New Horizons probe flying past it. Reyk YO! 05:50, 17 April 2009 (UTC)[reply]
- Likewise, I am not at all confused by the mixed terms. Wronkiew (talk) 04:18, 18 April 2009 (UTC)[reply]
- That is probably because you wrote the article. I suppose, however, that it is not the mixed terminology that concerns me, but the fact that "visit" appears before the first instance of "flyby". Without any hint up to that point as to whether or not Galileo actually landed, it is entirely up to the reader to guess. --Cryptic C62 · Talk 04:56, 19 April 2009 (UTC)[reply]
- What I meant was that "visit" implies that something actually landed on the asteroid, so it's not clear that Galileo's "visit" and "flyby" are the same thing. --Cryptic C62 · Talk 01:41, 17 April 2009 (UTC)[reply]
- Clarified so it reads " Galileo flyby ". Reyk YO! 00:39, 17 April 2009 (UTC)[reply]
"Ida's irregular shape is responsible for the asteroid's highly uneven gravitational field. The surface gravity is lowest at the extremities due to the fast rotation, and near the minimum radius due to less mass being present interior to that location" Why is this in a separate paragraph? It doesn't really make sense to discuss the gravitational field in two different paragraphs, though I see that this information should follow the paragraph about Ida's shape. Consider merging this paragraph into the astronaut rock chucking paragraph, then moving that paragraph to after the shape paragraph.Also, this little paragraph makes total sense up until the final clause about the interior location radius birthday present. I had to read that at least 3 times, and I'm still not entirely sure what it means.- Merged the paragraphs as you suggested. Reyk YO! 22:02, 17 April 2009 (UTC)[reply]
- Good, but the part about the interior mass gravity thingo is still confusing. --Cryptic C62 · Talk 22:50, 20 April 2009 (UTC)[reply]
- Rewritten. Wronkiew (talk) 04:44, 22 April 2009 (UTC)[reply]
- I understand what you're trying to communicate with this statement, and I've been wracking my brain trying to come up with a clear, concise way to explain it, and it looks like you guys have been too. I think splitting it off from the extremities sentence definitely helps. I think the best thing to do would be to fully explain the characteristics of the "waist" when you first introduce it earlier in this paragraph. That will allow you to explain the differences in the gravitational field like this: "The gravitational field is also weaker at the "waist" because it encompasses less mass than the main body of the asteroid." That's not exactly a perfect sentence either, but eh. I definitely think giving more info about the waist earlier on will help. --Cryptic C62 · Talk 17:47, 22 April 2009 (UTC)[reply]
- Rewritten. Wronkiew (talk) 04:44, 22 April 2009 (UTC)[reply]
- Good, but the part about the interior mass gravity thingo is still confusing. --Cryptic C62 · Talk 22:50, 20 April 2009 (UTC)[reply]
- Merged the paragraphs as you suggested. Reyk YO! 22:02, 17 April 2009 (UTC)[reply]
- "Some grooves are related to major impact events" Perhaps this sentence should include "though" or "however" as it contrasts the sentence before it.
- It does not contrast. The only seismic waves on an asteroid are caused by impact events, and I think that's knowledge we can expect readers to start with. Wronkiew (talk) 05:40, 27 April 2009 (UTC)[reply]
- Clearly not! I, too, am a reader, and I had no idea that that was the case! --Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]
- I attempted to explain the association between impact events and seismic waves, but the resulting prose had so many "might be"s and "appear to"s that I decided to drop it entirely. Wronkiew (talk) 16:46, 28 April 2009 (UTC)[reply]
- Cool. Also, what does it mean to be "related to" impact events? "Caused by" seems more logical. --Cryptic C62 · Talk 03:22, 29 April 2009 (UTC)[reply]
- I attempted to explain the association between impact events and seismic waves, but the resulting prose had so many "might be"s and "appear to"s that I decided to drop it entirely. Wronkiew (talk) 16:46, 28 April 2009 (UTC)[reply]
- Clearly not! I, too, am a reader, and I had no idea that that was the case! --Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]
- It does not contrast. The only seismic waves on an asteroid are caused by impact events, and I think that's knowledge we can expect readers to start with. Wronkiew (talk) 05:40, 27 April 2009 (UTC)[reply]
- "and range in age from fresh to very old" Yikes. This sentence is totally useless without some hard numbers. Even rough estimates would be better than "fresh" and "very old".
- The next sentence defines "very old" as comparable in age to Ida itself. Wronkiew (talk) 06:29, 27 April 2009 (UTC)[reply]
- ...Which isn't discussed until section 7. If, by chance, the reader reads through the article backwards and gets a sense of the age of Ida by the time s/he gets to this section, "How old is very old?" will have been answered, but "How fresh is fresh?" will remain. --Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]
- Clarified. Reyk YO! 00:26, 29 April 2009 (UTC)[reply]
- I think the "range" has lost its meaning entirely at this point. Why not just shorten it to "and some are as old as Ida itself."? --Cryptic C62 · Talk 03:22, 29 April 2009 (UTC)[reply]
- Clarified. Reyk YO! 00:26, 29 April 2009 (UTC)[reply]
- ...Which isn't discussed until section 7. If, by chance, the reader reads through the article backwards and gets a sense of the age of Ida by the time s/he gets to this section, "How old is very old?" will have been answered, but "How fresh is fresh?" will remain. --Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]
- The next sentence defines "very old" as comparable in age to Ida itself. Wronkiew (talk) 06:29, 27 April 2009 (UTC)[reply]
- "Region 2 contains nearly all of the craters larger than 6 km (3.7 mi) in diameter, but Region 1 has no large craters at all. Some craters are arranged in chains" Cool stuff. Any conclusions that can be drawn from these statements?
- I believe we have hit the best parts of the available literature. Wronkiew (talk) 06:29, 27 April 2009 (UTC)[reply]
- Well, I had a look for myself, and found this sentence: "Crater chains may result from low-velocity impact of ejecta from a primary crater (although no crater chain can yet be linked to a larger primary) or from a string of original impactors".
Also, this source was published in March 1994 and is based on images taken in August 1993. The author makes reference to new images that would be made available during that spring, as well as the increased accuracy in identifying features that such images would provide. Has any attempt been made to find an analysis of these images?--Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]- Chapman 1996 and Sullivan et al. 1996 seem to be the most detailed analyses of the full set of images. I have not seen a better analysis of the crater chains, and the one in Greeley et al. 1994 is not specific to Ida. Wronkiew (talk) 00:52, 29 April 2009 (UTC)[reply]
- Well, I had a look for myself, and found this sentence: "Crater chains may result from low-velocity impact of ejecta from a primary crater (although no crater chain can yet be linked to a larger primary) or from a string of original impactors".
- I believe we have hit the best parts of the available literature. Wronkiew (talk) 06:29, 27 April 2009 (UTC)[reply]
- "Another significant crater is Afon, which marks the prime meridian" You've linked to prime meridian, but that is an article that is devoted almost entirely to discussion of the prime meridian on Earth. Did you mean to link to a subsection? --Cryptic C62 · Talk 14:27, 27 April 2009 (UTC)[reply]
- Prime meridian does emphasize the prime meridian on Earth, but the lead section contains a useful definition of the term which applies to all bodies. Wronkiew (talk) 00:40, 28 April 2009 (UTC)[reply]
- Are we reading the same article? Nothing in the lead of prime meridian gives any indication of its use on other bodies. Perhaps linking to the woefully inadequate subsection on other planetary bodies would help. --Cryptic C62 · Talk 03:22, 29 April 2009 (UTC)[reply]
- We are. The lead section contains the important information that the prime meridian is arbitrary and that it corresponds to the International Date Line on the Earth. The other planetary bodies section contains no useful information whatsoever in the context of Ida's prime meridian. Wronkiew (talk) 00:39, 30 April 2009 (UTC)[reply]
- Bah. Why don't you just say something like "marks Ida's prime meridian" rather than "marks the prime meridian" ? --Cryptic C62 · Talk 21:47, 30 April 2009 (UTC)[reply]
- Done. Wronkiew (talk) 16:49, 12 May 2009 (UTC)[reply]
- Bah. Why don't you just say something like "marks Ida's prime meridian" rather than "marks the prime meridian" ? --Cryptic C62 · Talk 21:47, 30 April 2009 (UTC)[reply]
- We are. The lead section contains the important information that the prime meridian is arbitrary and that it corresponds to the International Date Line on the Earth. The other planetary bodies section contains no useful information whatsoever in the context of Ida's prime meridian. Wronkiew (talk) 00:39, 30 April 2009 (UTC)[reply]
- Are we reading the same article? Nothing in the lead of prime meridian gives any indication of its use on other bodies. Perhaps linking to the woefully inadequate subsection on other planetary bodies would help. --Cryptic C62 · Talk 03:22, 29 April 2009 (UTC)[reply]
- Prime meridian does emphasize the prime meridian on Earth, but the lead section contains a useful definition of the term which applies to all bodies. Wronkiew (talk) 00:40, 28 April 2009 (UTC)[reply]
- "Olivine and pyroxene were detected by Galileo" This sentence should include "Ida" in it somewhere.
- Done. Wronkiew (talk) 05:41, 28 April 2009 (UTC)[reply]
- Argh, now the sentence reads quite awkwardly: "Olivine and pyroxene were detected on Ida by Galileo." How about something like this: "During its flyby, Galileo detected the presence of both olivine and pyroxene on Ida's surface." --Cryptic C62 · Talk 21:47, 30 April 2009 (UTC)[reply]
- Done. Wronkiew (talk) 05:41, 28 April 2009 (UTC)[reply]
- "interior voids have been predicted by simulations and observed on other Solar System objects" Shouldn't this be in other objects? Also, "simulations" is a tad vague.
- Removed. Wronkiew (talk) 04:23, 30 April 2009 (UTC)[reply]
- "the asteroid's spin indicates an even density." This sentence seems to conflict with the final paragraph in this section. How can an object with interior voids and a layer of megaregolith have a consistent density?
- "Interior voids" removed, as it was general to all asteroids and not Ida in particular. I don't see a conflict beteen the roughly consistent density and the fractured rock throughout. Wronkiew (talk) 04:23, 30 April 2009 (UTC)[reply]
- Alright, perhaps I'm envisioning "fractured rock" differently than I should. However, the conflict still remains with the interior voids, though it seems you've swept that under the rug, something I'm not really a fan of. You said there were simulations which predicted voids. I said your description of said simulation was vague. Vagueness and the fact that the content "was general to all asteroids" is not an excuse to eliminate relevant conflicting content. --Cryptic C62 · Talk 21:47, 30 April 2009 (UTC)[reply]
- Not really "swept under the rug". I can explain the discrepancy, but it's just not worth going into that much detail about scientists' theories about what Ida's structure might be. If you think this information is vital to the article, I can add it back with a better explanation, otherwise I'd rather stick to more solid facts if possible. Wronkiew (talk) 04:44, 1 May 2009 (UTC)[reply]
- Why don't you just explain it to me here so we can discuss it in greater detail? --Cryptic C62 · Talk 19:34, 3 May 2009 (UTC)[reply]
- Sure. What we really know about Ida's internal density variations is that it is roughly consistent in terms of angular momentum. This would imply a homogeneous interior only if Ida were shaped like a perfect, tasty doughnut. Since it is a three-dimensional, irregularly shaped object, it could have extreme variations in density and coincidentally look like it had a consistent density. For example, Ida could be made of styrofoam in the northern hemisphere and lead in the southern hemisphere, and it would move the same way that Galileo observed. However, this is considered unlikely based on our understanding of how asteroids are formed. The nature of this measurement also leaves open the possiblity of large internal voids inside Ida, because if they are distributed evenly throughout it, they would be undetectable. What this all really means is that the two halves of Ida do not differ in bulk density to a measurable degree. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- Why don't you just explain it to me here so we can discuss it in greater detail? --Cryptic C62 · Talk 19:34, 3 May 2009 (UTC)[reply]
- Not really "swept under the rug". I can explain the discrepancy, but it's just not worth going into that much detail about scientists' theories about what Ida's structure might be. If you think this information is vital to the article, I can add it back with a better explanation, otherwise I'd rather stick to more solid facts if possible. Wronkiew (talk) 04:44, 1 May 2009 (UTC)[reply]
- Alright, perhaps I'm envisioning "fractured rock" differently than I should. However, the conflict still remains with the interior voids, though it seems you've swept that under the rug, something I'm not really a fan of. You said there were simulations which predicted voids. I said your description of said simulation was vague. Vagueness and the fact that the content "was general to all asteroids" is not an excuse to eliminate relevant conflicting content. --Cryptic C62 · Talk 21:47, 30 April 2009 (UTC)[reply]
- "Interior voids" removed, as it was general to all asteroids and not Ida in particular. I don't see a conflict beteen the roughly consistent density and the fractured rock throughout. Wronkiew (talk) 04:23, 30 April 2009 (UTC)[reply]
- "The calculated maximum moment of inertia of a uniformly dense object the same shape as Ida coincides with the spin axis of the asteroid." Um, what? "Coincides" implies that these two values are comparable, which is mathematically unsound. This is like saying "The maximum number of employees at Big City Construction coincides with Eric Bobrow, the foreman." Yes, the two are related, but in no way do they "coincide". My guess is that you meant to say something like this: "For an object with the same shape as Ida, the maximum possible moment of inertia is achieved when the object is uniformly dense and has a certain axis of rotation (INSERT DESCRIPTION OF AXIS HERE). Ida's axis of rotation (SUMMARIZE DESCRIPTION OF AXIS HERE), implying that it is uniformly dense." That isn't perfectly logical either, but at least it provides all of the steps required for the comparison to make sense to the reader.
- "Ida's axis of rotation precesses with a period of 77,000 years" Another mention of the axis of rotation, but still no description of such an axis!
- Not sure what you're looking for here. The direction of Ida's axis is defined in the infobox. We don't have any additional information on where Ida's spin axis is located, except at +90 and -90 degrees latitude. Wronkiew (talk) 05:11, 1 May 2009 (UTC)[reply]
- The whole time I've been reading this article, I've had no idea how the latitude-longitude coordinate system works. It totally makes sense on the lovely spherical Earth on which we live, but I don't understand how it applies to asteroids. Perhaps this is something that those in the field of astronomy would consider "common knowledge", but not all of our readers are astronomers. What I'm trying to get at here is that some sort of of physical landmark would be incredibly useful in helping users to visualize this. Does the spin axis go through the waist?
- Ida and Earth both rotate around a single axis, marked by the poles. The midpoint between the north and south poles, in spherical coordinates, is the equator, or zero degrees latitude. The equator does not coincide with the waist, and no one has planted a flag on its north pole yet. You might want to watch the Galileo approach animation for a better sense of Ida's rotation. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- *headdesk* Perhaps I'm not making it clear what I'm asking for. The animation is helpful, but not precise. My question is this: Where (physically where, don't tell me 90° north latitude) is Ida's spin axis? The article repeatedly abuses the coordinate system without ever making it clear how it is defined on this asteroid. Something like this would help: "The spin axis runs perpendicular to the asteroid's longest dimension and passes through the asteroid approximately 20 meters from the waist." Do you see what I'm getting at? Physical landmarks. Not flags. Not mumbo jumbo. --Cryptic C62 · Talk 05:15, 7 May 2009 (UTC)[reply]
- Ida and Earth both rotate around a single axis, marked by the poles. The midpoint between the north and south poles, in spherical coordinates, is the equator, or zero degrees latitude. The equator does not coincide with the waist, and no one has planted a flag on its north pole yet. You might want to watch the Galileo approach animation for a better sense of Ida's rotation. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- The whole time I've been reading this article, I've had no idea how the latitude-longitude coordinate system works. It totally makes sense on the lovely spherical Earth on which we live, but I don't understand how it applies to asteroids. Perhaps this is something that those in the field of astronomy would consider "common knowledge", but not all of our readers are astronomers. What I'm trying to get at here is that some sort of of physical landmark would be incredibly useful in helping users to visualize this. Does the spin axis go through the waist?
- Not sure what you're looking for here. The direction of Ida's axis is defined in the infobox. We don't have any additional information on where Ida's spin axis is located, except at +90 and -90 degrees latitude. Wronkiew (talk) 05:11, 1 May 2009 (UTC)[reply]
There is a section labeled "Orbit and rotation". It contains no information about the orbit. It does, however, contain totally irrelevant historical information that should probably be moved to "Origin".- Discovery information moved to "Discovery and observations", added more detail about Ida's orbit. Wronkiew (talk) 05:11, 1 May 2009 (UTC)[reply]
- Much better, though I think this paragraph would benefit from some more numbers. What is Ida's orbital speed relative to the sun? You say it orbits at an average distance of 2.862 AU. Any mention of what the variation is? --Cryptic C62 · Talk 19:34, 3 May 2009 (UTC)[reply]
- More detail about Ida's orbit can be found in the infobox, where it belongs. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- Unfortunately for the entire non-astronomy-obsessed English-speaking Wikipedia-browsing population of the Earth, the infobox uses terms that go way over our heads. This section gives you an opportunity to explain some of the more interesting orbital characteristics in full sentences. --Cryptic C62 · Talk 05:15, 7 May 2009 (UTC)[reply]
- More detail about Ida's orbit can be found in the infobox, where it belongs. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- Much better, though I think this paragraph would benefit from some more numbers. What is Ida's orbital speed relative to the sun? You say it orbits at an average distance of 2.862 AU. Any mention of what the variation is? --Cryptic C62 · Talk 19:34, 3 May 2009 (UTC)[reply]
- Discovery information moved to "Discovery and observations", added more detail about Ida's orbit. Wronkiew (talk) 05:11, 1 May 2009 (UTC)[reply]
- "However, this is inconsistent with the estimated age of the Ida–Dactyl system of less than 100 million years; it is unlikely that Dactyl, due to its small size, could have escaped being destroyed in a major collision for longer" Yikes, very awkwardly arranged. How about: "However, it is unlikely that Dactyl, due to its small size, could have avoided being destroyed in a collision for more than 100 million years."
- I think the first version is clearer, if a little verbose. Wronkiew (talk) 06:45, 9 May 2009 (UTC)[reply]
- "The difference in age estimates may be explained by an increased rate of cratering from the debris of the Koronis parent body's destruction" Not entirely certain what this sentence means. My understanding is thus: At some point, the Koronis parent body was destroyed entirely, and the resulting debris created craters on Ida's surface much faster than before. This discrepancy in the rate of cratering affected the accuracy of the age estimate, yes?
- "A small satellite named Dactyl" Is there something to which we could link "satellite"? Some of the less nerdy readers might not be aware that "satellites" are not necessarily man-made.
- Done. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- "Dactyl was initially designated 1993 (243) 1" Was this meant to be a placeholder name like ununoctium?
- This is explained in the wikilinked article. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- "Dactyl is an "egg-shaped", but "remarkably spherical" object measuring 1.6 × 1.4 × 1.2 km (0.99 × 0.87 × 0.75 mi). It was oriented with its longest axis pointing towards Ida" Why the random switch from present to past tense?
- It's safe to say that it did not change shape in the past 15 years, but we've no idea if it is still oriented the same way. Wronkiew (talk) 04:52, 7 May 2009 (UTC)[reply]
- "These features, and Dactyl's spheroidal shape, imply that the moon is gravitationally controlled despite its small size" This strikes me as being a bit odd. Why would the size of an object be relevant to whether or not it is gravitationally controlled?
- "roughly 10–20 times smaller than Ida" I've never understood how something can be "10 times smaller" than something else. Does this mean Dactyl is 1/10th to 1/20th the size of Ida? Or that Ida is 10 to 20 times larger than Dactyl? Both of these mean the same thing and are clearer than the phrasing currently employed.
- Removed. Wronkiew (talk) 06:45, 9 May 2009 (UTC)[reply]
- "the Hubble Space Telescope observed Ida for eight hours and was unable to spot Dactyl" Bolded for emphasis. Not particularly scientific.
- We now seem to have the opposite problem here: Dactyl's rotation and orbit section has no information about its rotation!
- Renamed the section. Wronkiew (talk) 16:47, 12 May 2009 (UTC)[reply]
- "It is extremely unlikely that it was captured by Ida" Because...
- I recommend that instead of giving Dactyl four subsections (which are confusingly similar to those about Ida), you split Dactyl off into a separate article.
- This has come up before. In my opinion, we do not know enough about Dactyl to make a decent standalone article. Wronkiew (talk) 16:47, 12 May 2009 (UTC)[reply]
- Backtracking: "Ida's rotation period is 4.63 hours, making it one of the fastest rotating known asteroids. It is in the top 10% of measured asteroids by spin." Yuck. How about: "Ida's rotation period is 4.63 hours, making it one of the fastest rotating asteroids yet discovered." the second sentence is useless trivia.
- Done. Wronkiew (talk) 16:47, 12 May 2009 (UTC)[reply]
- "Prior to the flyby" Erm, what flyby? The lead previously mentioned that the asteroid was visited. Do "visit" and "flyby" refer to the same thing?
- This concludes my read-through. Good work so far. --Cryptic C62 · Talk 17:02, 7 May 2009 (UTC)[reply]
- Cryptic, do you mind if we move the struck comments to a collapsed section? Wronkiew (talk) 04:18, 18 April 2009 (UTC)[reply]
- I would have no problem with it, but my understanding is that the use of collapse templates is discouraged because it borks WP:FAC. I suppose you can make the struck comments small, if you like. --Cryptic C62 · Talk 05:11, 18 April 2009 (UTC)[reply]
- Discouraged only if it causes the page to run into transclusion limits. Wronkiew (talk) 04:19, 25 April 2009 (UTC)[reply]
- I would have no problem with it, but my understanding is that the use of collapse templates is discouraged because it borks WP:FAC. I suppose you can make the struck comments small, if you like. --Cryptic C62 · Talk 05:11, 18 April 2009 (UTC)[reply]
- Cryptic, do you mind if we move the struck comments to a collapsed section? Wronkiew (talk) 04:18, 18 April 2009 (UTC)[reply]
- "Physical characteristics" is used as a header twice; please change it up per WP:MSH. Dabomb87 (talk) 00:49, 19 April 2009 (UTC)[reply]
- Fixed. Thanks for catching that. Wronkiew (talk) 04:31, 19 April 2009 (UTC)[reply]
- I think a better solution would be to call the section about Ida "Physical characteristics" and the section about Dactyl "Physical characteristics of Dactyl". This seems more logical, and I seem to remember reading something about avoiding using the name of the article in its sections. --Cryptic C62 · Talk 22:18, 25 April 2009 (UTC)[reply]
- Done. Wronkiew (talk) 06:29, 27 April 2009 (UTC)[reply]
- I think a better solution would be to call the section about Ida "Physical characteristics" and the section about Dactyl "Physical characteristics of Dactyl". This seems more logical, and I seem to remember reading something about avoiding using the name of the article in its sections. --Cryptic C62 · Talk 22:18, 25 April 2009 (UTC)[reply]
- Fixed. Thanks for catching that. Wronkiew (talk) 04:31, 19 April 2009 (UTC)[reply]
Tentativesupport—It's good overall,with only a couple of nits to pick:"...Ida is one of the larger asteroids in the main belt." Unfortunately this doesn't really say anything. A JPL Small-Body Database query finds 1,735 known MBAs with a diameter of 15 km or larger. So you could potentially say something more definitive, such as it is among the 2,000 largest known MBAs.- I couldn't find a reliable source that has a size distribution of main belt asteroids, so I removed the comparison. Also, the diameter is 31.4 km, according to the source cited in the infobox, so I fixed that as well. Wronkiew (talk) 04:38, 21 April 2009 (UTC)[reply]
"Estimates of Ida's density are constrained to less than 3.2 g/cm3 ... This low density rules out the presence of significant quantities of metal..." Please clarify whether you mean iron here. Note that the the density of aluminum is 2.7 g/cm3 and the density of silicon is 2.33 g/cm3, which are both lower than this value and the latter implies there is a non-trivial proportion of denser elements. Also, wouldn't a maximum porosity of 42% indicate a much higher density for the solid parts?- I reworked the sentence with information from a new source. Wronkiew (talk) 06:47, 21 April 2009 (UTC)[reply]
- Thank you.—RJH (talk) 19:29, 20 April 2009 (UTC)[reply]
- Conditional support on addressing Cryptic C62's points. Looks pretty good otherwise. --mav (talk) 21:01, 26 April 2009 (UTC)[reply]
Image review as follows:
- File:Ejecta block on 243 Ida.svg: how did you obtain the image from http://pds-imaging.jpl.nasa.gov/cgi-bin/Nav/GLL_search.pl? Why is it an SVG?
- SVG is the native format for this diagram. It could be converted to JPEG, but it would lose some information. The ID 202562313 is the time stamp for the image, which you can search for in the database with the start and end time fields. Wronkiew (talk) 15:19, 28 April 2009 (UTC)[reply]
- See below for comments regarding the format. I am still rather confused on how to obtain the image. The PDS brings up a field of checkboxes, tabs, and fields. I keyed the ID in the OBSERVATION_ID and clicked on SUBMIT, but the next screen stated the image cannot be found. Jappalang (talk) 01:16, 29 April 2009 (UTC)[reply]
- You need to enter the ID in both the Min and Max fields of SPACECRAFT_CLOCK_START_COUNT. The database does not allow direct links to the images. Wronkiew (talk) 05:52, 29 April 2009 (UTC)[reply]
- See below for comments regarding the format. I am still rather confused on how to obtain the image. The PDS brings up a field of checkboxes, tabs, and fields. I keyed the ID in the OBSERVATION_ID and clicked on SUBMIT, but the next screen stated the image cannot be found. Jappalang (talk) 01:16, 29 April 2009 (UTC)[reply]
- SVG is the native format for this diagram. It could be converted to JPEG, but it would lose some information. The ID 202562313 is the time stamp for the image, which you can search for in the database with the start and end time fields. Wronkiew (talk) 15:19, 28 April 2009 (UTC)[reply]
- File:Fingal on 243 Ida.svg: why is this an SVG?
- Same as above. Neither of these images have a particularly large file size. Wronkiew (talk) 15:19, 28 April 2009 (UTC)[reply]
- That does not quite answer the question. Inproper format comes into play here. SVGs are containers of vectors; they are scripts of lines (text), not data. The two images are not rendered in terms of vectors; rather, their bitmaps are pasted in the scripts as arrays of raw data, which would not benefit from the scaling that vectors give and may result in larger file sizes than JPGs. No benefit is derived from them as SVGs. I have constructed File:Fingal on 243 Ida.jpg from the large image. Is this acceptable (as inserted in the article)? Jappalang (talk) 01:16, 29 April 2009 (UTC)[reply]
- I would prefer that the SVG version be placed in the article. The Fingal image in particular contains a rather high-resolution overview which is lost in the JPEG version. The SVG version is also not much larger than the file sizes of its included images. The overview image by itself, in JPEG format, takes up 238 KB. The SVG is 245 KB. A rasterization of this diagram at full resolution in JPEG format would take many times that amount. In my view, this is an entirely appropriate use of the SVG format, and, on top of that, it's in an editable format, so labels and other elements can be added later with no loss in quality. As for WP:IUP, it says diagrams should be in SVG format, while photos should be in JPEG format. We obviously disagree over whether these images are diagrams or photos, but, in any case, these recommendations are subject to common sense. There is no reason to degrade the quality of these images as displayed in the article just to follow the policy. Wronkiew (talk) 05:52, 29 April 2009 (UTC)[reply]
- I still fail to see the purpose of it stuffed in SVGs. The "rather high-resolution overview" is of no use; no one would get to see its full resolution unless they open it in an SVG editor and zoomed in. The overview is simply a reduced size File:243_Ida_large.jpg with an orange box to denote the zoomed in area. There is no degradation of image quality as far as I am concerned. It also does not answer why the above image (Ejecta) is in SVG; it has no high resolution texture stuffed in it. Diagrams, as definitions go, are plans, sketches, drawings, or outlines. While I do not disagree that this definition could be narrow in the sense that marked photos serve pretty well as illustrated guides, there could be reasons why such wording is used. SVGs are advocated for diagrams, mainly (in my opinion) because text and fine lines will not be lost when rescaled; I doubt it is to stuff high resolution textures into small size images. Jappalang (talk) 12:36, 29 April 2009 (UTC)[reply]
- I posted a comparison of the two images at 800x800 on the talk page. 320x320 is just the preview resolution for the SVG. Wronkiew (talk) 16:01, 29 April 2009 (UTC)[reply]
- I still fail to see the purpose of it stuffed in SVGs. The "rather high-resolution overview" is of no use; no one would get to see its full resolution unless they open it in an SVG editor and zoomed in. The overview is simply a reduced size File:243_Ida_large.jpg with an orange box to denote the zoomed in area. There is no degradation of image quality as far as I am concerned. It also does not answer why the above image (Ejecta) is in SVG; it has no high resolution texture stuffed in it. Diagrams, as definitions go, are plans, sketches, drawings, or outlines. While I do not disagree that this definition could be narrow in the sense that marked photos serve pretty well as illustrated guides, there could be reasons why such wording is used. SVGs are advocated for diagrams, mainly (in my opinion) because text and fine lines will not be lost when rescaled; I doubt it is to stuff high resolution textures into small size images. Jappalang (talk) 12:36, 29 April 2009 (UTC)[reply]
- I would prefer that the SVG version be placed in the article. The Fingal image in particular contains a rather high-resolution overview which is lost in the JPEG version. The SVG version is also not much larger than the file sizes of its included images. The overview image by itself, in JPEG format, takes up 238 KB. The SVG is 245 KB. A rasterization of this diagram at full resolution in JPEG format would take many times that amount. In my view, this is an entirely appropriate use of the SVG format, and, on top of that, it's in an editable format, so labels and other elements can be added later with no loss in quality. As for WP:IUP, it says diagrams should be in SVG format, while photos should be in JPEG format. We obviously disagree over whether these images are diagrams or photos, but, in any case, these recommendations are subject to common sense. There is no reason to degrade the quality of these images as displayed in the article just to follow the policy. Wronkiew (talk) 05:52, 29 April 2009 (UTC)[reply]
- That does not quite answer the question. Inproper format comes into play here. SVGs are containers of vectors; they are scripts of lines (text), not data. The two images are not rendered in terms of vectors; rather, their bitmaps are pasted in the scripts as arrays of raw data, which would not benefit from the scaling that vectors give and may result in larger file sizes than JPGs. No benefit is derived from them as SVGs. I have constructed File:Fingal on 243 Ida.jpg from the large image. Is this acceptable (as inserted in the article)? Jappalang (talk) 01:16, 29 April 2009 (UTC)[reply]
- Same as above. Neither of these images have a particularly large file size. Wronkiew (talk) 15:19, 28 April 2009 (UTC)[reply]
WP:IUP would ask for the two above images to be JPGs. All other images are verifiably in public domain or appropriately licensed. Jappalang (talk) 07:05, 28 April 2009 (UTC)[reply]
- Support — I'm not at all familiar with asteroids or space objects, but this article was written well enough and included enough information for me to understand the subject and grasp its significance. Nice work by everyone who contributed. I've got just one criticism — commas aren't being used correctly in spots throughout the article. In the last sentence of the first paragraph: "It was the second asteroid to be visited by a spacecraft, and the first found to possess a satellite.", you shouldn't use the comma before "and". This is because the second clause — "the first found to possess a satellite" — can't stand alone as a sentence. If you'd said "It was the second asteroid to be visited by a spacecraft, and it was the first found to possess a satellite.", the comma would be needed. But since the subject isn't restated, you shouldn't use a comma before the conjunction. I found a handful of examples of this throughout the article. But as I said, this is a minor thing and doesn't affect the ability of a reader to understand the article. Nice work. JKBrooks85 (talk) 08:16, 10 May 2009 (UTC)[reply]
- Support some minor prose-flow issues but tricky to reword. No deal-breakers left. Casliber (talk · contribs) 10:14, 10 May 2009 (UTC)[reply]
- The above discussion is preserved as an archive. Please do not modify it. No further edits should be made to this page.