Jump to content

Talk:Ceres (dwarf planet): Difference between revisions

Page contents not supported in other languages.
From Wikipedia, the free encyclopedia
Content deleted Content added
Line 222: Line 222:
== Multiple entries saying that this is an "Asteroid" ==
== Multiple entries saying that this is an "Asteroid" ==


On the NASA website this is stated as NOT being an asteroid. Yes, it is in the asteroid belt, but it a dwarf planet. PAGE: https://solarsystem.nasa.gov/planets/dwarf-planets/ceres/overview/ (look at No.4 on list). I believe NASA should be considered a vary valid authority. NASA tends to defer to other agencies/ organisations as well. If no one objects I can go through and remove references implying it is an asteroid. If someone beats me to it then fine. [[Special:Contributions/92.238.237.65|92.238.237.65]] ([[User talk:92.238.237.65|talk]]) 03:46, 18 February 2022 (UTC)
On the NASA website this is stated as NOT being an asteroid. Yes, it is in the asteroid belt, but it a dwarf planet. PAGE: https://solarsystem.nasa.gov/planets/dwarf-planets/ceres/overview/ (look at No.4 on list). I believe NASA should be considered a valid authority. NASA tends to defer to other agencies/ organisations as well. If no one objects I can go through and remove references implying it is an asteroid. If someone beats me to it then fine. [[Special:Contributions/92.238.237.65|92.238.237.65]] ([[User talk:92.238.237.65|talk]]) 03:46, 18 February 2022 (UTC)

Revision as of 03:48, 18 February 2022

Template:Vital article

Former featured articleCeres (dwarf planet) is a former featured article. Please see the links under Article milestones below for its original nomination page (for older articles, check the nomination archive) and why it was removed.
Good articleCeres (dwarf planet) has been listed as one of the Natural sciences good articles under the good article criteria. If you can improve it further, please do so. If it no longer meets these criteria, you can reassess it.
Main Page trophyThis article appeared on Wikipedia's Main Page as Today's featured article on January 1, 2010.
In the newsOn this day... Article milestones
DateProcessResult
August 25, 2006Good article nomineeNot listed
October 11, 2006Good article nomineeListed
November 7, 2006Featured topic candidatePromoted
September 15, 2007Peer reviewReviewed
December 13, 2007Featured article candidatePromoted
August 27, 2008Featured topic candidatePromoted
September 4, 2008Featured topic removal candidateDemoted
September 16, 2008Featured topic candidatePromoted
September 14, 2019Featured article reviewDemoted
May 4, 2020Featured topic removal candidateDemoted
May 15, 2020Good topic removal candidateDemoted
July 7, 2021Peer reviewReviewed
July 26, 2021Good article nomineeListed
September 10, 2021Peer reviewReviewed
October 1, 2021Featured article candidateNot promoted
In the news A news item involving this article was featured on Wikipedia's Main Page in the "In the news" column on March 6, 2015.
On this day... Facts from this article were featured on Wikipedia's Main Page in the "On this day..." column on January 1, 2005, January 1, 2006, January 1, 2008, January 1, 2009, January 1, 2011, January 1, 2017, and January 1, 2019.
Current status: Former featured article, current good article


Sig figs for orbital elements

I have reduced the sig figs in the infobox orbital elements from 11 to 6. Using 10 sig figs, the orbital elements change every minute. This also allows a bot to do a more appropriate conversion from AU to millions of km. These frequent changes to the orbit is also the reason the "unperturbed two-body" JPL SBDB (using epoch 2021-Jul-01) misses the time of perihelion by 1 day. -- Kheider (talk) 11:32, 26 September 2021 (UTC)[reply]

@Kheider: The semi-major varies in its 4th digit from year to year, and eccentricity in its 3rd, so even 6 would seem to be too much. I'll round off to 3 -- pls rv if you think that's too much. — kwami (talk) 19:16, 26 September 2021 (UTC)[reply]
My biggest concern with 3 sig figs is someone coming back at a later date and putting back in 10 sig figs. Another option might be 5 sig figs and use |sigfig=3 for the conversion template. -- Kheider (talk) 21:56, 26 September 2021 (UTC)[reply]
Done. That does generate an error for the Proper orbital period, though [fixed], and if I round off by hand, it still calcs out to 6 digits. — kwami (talk) 00:08, 27 September 2021 (UTC)[reply]
I was thinking something like {{Convert|2.54885|AU|e6km|abbr=unit|sigfig=3}} which outputs 2.54885 AU (381 million km). -- Kheider (talk) 00:15, 27 September 2021 (UTC)[reply]
Yeah, but that still shows more precision than is justified. And this way, if someone does put in 10 digits, it won't make any difference. — kwami (talk) 01:29, 27 September 2021 (UTC)[reply]

Requested move 2 October 2021

The following is a closed discussion of a requested move. Please do not modify it. Subsequent comments should be made in a new section on the talk page. Editors desiring to contest the closing decision should consider a move review after discussing it on the closer's talk page. No further edits should be made to this discussion.

The result of the move request was: not moved (non-admin closure) NW1223(Howl at me|My hunts) 15:01, 9 October 2021 (UTC)[reply]



– Firstly, using "dwarf planet" (DP) in the title and treating the IAU-recognised dwarf planets as fundamentally different from other minor planets seems to be based on the situation in 2006 when the IAU stated that it would start a process to recognise dwarf planets. However, it's now over 15 years later, and to date there seems to be no such process. Haumea and Makemake were named in 2008 only assuming they were DPs, because they met the absolute magnitude cutoff H < +1 (and were announced as DPs by press release). This is not actually part of the IAU definition of a DP (only a rule saying that bodies found to meet it will be named assuming that they are DPs), and no new bodies have met that since 2008. Also, we don't even know that Haumea, Makemake, and Eris truly meet the IAU definition to the letter, since that requires hydrostatic equilibrium, and to strictly find it out to the standards most scientists seem to use in papers (which excludes round Iapetus), you basically need to send a space probe. Even Ceres is noticeably not quite right, but before we sent the probe, measurements were consistent with it being in HE.

But in practice, scientists routinely call other objects DPs in their papers, whatever IAU press release recognition and the IAU definition strictly read say. It is completely normal to see the term "dwarf planet" in papers referring to the large TNOs Quaoar, Orcus, Sedna, and Gonggong. Our articles on these bodies (50000 Quaoar, 90482 Orcus, 90377 Sedna, 225088 Gonggong) already call them dwarf planets without reservation because that's what the scientific consensus seems to be, but their titles follow the minor-planet convention to have the number. To use a different naming convention here seems to imply that the IAU-recognised five are the only dwarf planets, which not even the IAU seems to believe (it calls them the five identified DPs and admits that "There may be dozens or perhaps even more than a hundred [DPs] waiting to be discovered."), and which is against common scientific usage.

Secondly, Ceres and Eris already need disambiguation, and it seems more natural disambiguation to use the minor planet number than to use parenthetical disambiguation. Especially when that's what's done for most minor planets (e.g. 2 Pallas, 4 Vesta, 10 Hygiea which in 2006 were considered as DP candidates too). Haumea and Makemake do not need disambiguation, but it is already common to use the minor planet number on WP even when it does not need disambiguation (Quaoar redirects to 50000 Quaoar, and 52246 Donaldjohanson is where it is despite Donaldjohanson being a redlink).

Pluto is not requested because it is by far the most well-known DP or minor planet and its MP number is a modern afterthought rather than contemporary with its name.

P.S. I'm aware that this move request goes against WP:NCASTRO making officially recognised DPs an exception from the minor-planet naming convention. But that was established back in 2006, where there was some reason to believe that the IAU would actually follow up on creating a process to designate which objects were DPs as they said they would. In 2021, with no process still, there is no such reason. Double sharp (talk) 07:51, 2 October 2021 (UTC)[reply]

  • Oppose for Makemake and Haumea, proposed titles are unlikely search terms for non-astrogeeks, and disambiguation isn't necessary, so the choice consistent with our naming conventions is the current title. Neutral on the others, don't care much what's type of disambiguation is used here. —Kusma (talk) 08:48, 2 October 2021 (UTC)[reply]
  • Oppose nobody would search for Makemake as 136472 Makemake, and the same is applicable for others. It's redundant level of complexity and would benefit nobody at all. And Ceres here is a lot like Pluto - it's well known by people by its name, not by a number. Artem.G (talk) 09:30, 2 October 2021 (UTC)[reply]
  • Oppose per common name. Randy Kryn (talk) 11:25, 2 October 2021 (UTC)[reply]
  • Oppose Dwarf planets are usually not referred to with their minor planet numbers, unlike most other minor planets.--Beanpickle (talk) 14:11, 2 October 2021 (UTC)[reply]
  • Comment from the OP. Many of the arguments given here so far seem equally true for large planetoids that either are not DPs or at least have not been recognised as DPs, like 2 Pallas and the similarly unmemorably numbered 225088 Gonggong. I agree that DPs often are referred to without the minor planet numbers, but it is not just them. Pallas in Google Scholar seems to lack the number quite often, too. Even when the number is present in the header and first occurrence, it is often absent afterwards. Or if we want likely-dwarf TNOs, the same's true for Gonggong. However, the already standard naming convention on WP (WP:NCASTRO#Asteroids, also see List of minor planets) gives them all the numbers in the title, and the five IAU-recognised dwarfs are the only exceptions. So given the way this seems to be going, perhaps WP:NCASTRO needs updating away from using the MP numbers in titles. Double sharp (talk) 14:35, 2 October 2021 (UTC)[reply]
  • Most articles I see refer to minor planets with their numbers in their titles, but for the rest of the article they use their name only. However dwarf planets (especially the 5 IAU ones) usually do not show their number at all.
  • Oppose as common name should win out here. I think the first 20 numbered asteroids have numbers and names that are easier to recall. As I wrote over at Talk: Pluto, "Before looking at List of minor planets: 1–1000, 19 Fortuna is the highest minor planet that I can recall the number to on any given day. I do know the numbers to 24 Themis, 52 Europa, 65 Cybele, etc, but I do not think of their numbers unless I am already thinking specifically of that asteroid." -- Kheider (talk) 15:02, 2 October 2021 (UTC)[reply]
    • @Kheider: Do you mean this oppose to apply to Ceres too, since it's in the first 20? Double sharp (talk) 09:50, 3 October 2021 (UTC)[reply]
      • Being easy to recall "1 Ceres" does not make it the common name used by the public. Since there are only 5 original (significant) dwarf planets, we should point to their common name as the general public does not care to see a MPC number in a large BOLD font leading the article title. I suspect a lot of astronomers do not care if other minor planets receive the official dwarf planet title because it will not change the science. -- Kheider (talk) 04:42, 4 October 2021 (UTC)[reply]
  • I mostly just think it should be consistent, if Pluto isn't showing it's number, the other 4 IAU dwarf planets shouldn't either, or alternatively no minor planet shows its number.Beanpickle (talk) 15:20, 2 October 2021 (UTC)[reply]
  • Though from what I see online, small minor planets are commonly referred to with their numbers, the 5 IAU dwarf planets usually don't have their numbers displayed and the non-IAU dwarf planets use varying designations.Beanpickle (talk) 02:19, 3 October 2021 (UTC)[reply]
There plenty of online sources that use "(1) Ceres" or "1 Ceres". Several of them are in the refs to this article. There are also recent print sources, such as 'Bright carbonate deposits as evidence of aqueous alteration on (1) Ceres', Nature (2016) and 'The brittle boulders of dwarf planet Ceres', Planetary Science Journal (2021): "Dwarf planet (1) Ceres maintains a position somewhat in between small bodies and the terrestrial planets." — kwami (talk) 03:08, 4 October 2021 (UTC)[reply]
  • Support for consistency with the many many similar article titles. Most of these need dabs anyway, so it's not a matter of what people would look up. If we're going to tag something as 'dwarf planet', what qualifies? Whose opinion do we follow? If Grundy, Buie et al., then down to Orcus or Salacia, but per Sterns dozens of named bodies are DPs. We shouldn't be picking a POV in an article title. Such things can be discussed in the text. Also, for Haumea, IMO a major deity that is culturally important takes precedence over a planetoid that was in the news for a short while but no longer gets much attention, so the planetoid should be moved to something.
Some of the objections above are specifically for the higher numbers. Is there any problem moving 'Ceres (dwarf planet)' to '1 Ceres'? If we're going by search criteria, the latter is easier, and is what I put in the search window. (There's also some doubt that it's actually a dwarf planet, according to the only ref to evaluate the situation that I've ever seen.) — kwami (talk) 23:03, 2 October 2021 (UTC)[reply]
I don't understand this argument, which has been made several times now. How is "Ceres (dwarf planet)" a more common name than "1 Ceres"? Should 50000 Quaoar be moved to "Quaoar (dwarf planet)"? 4 Vesta to "Vesta (asteroid)"? Without any reasoning, it doesn't make sense to me. — kwami (talk) 07:38, 6 October 2021 (UTC)[reply]
Ceres was discovered in 1801, and since then it has only been referred to as "Ceres" commonly. In most of the books you'll find this object named as only Ceres. Same is the case for Pluto. Nobody, apart from the IAU (officially), calls it "134340 Pluto". 4 Vesta and the 2002-discovered 50000 Quaoar are not known to as many people as the ones who know Ceres or Pluto. Peter Ormond 💬 09:17, 6 October 2021 (UTC)[reply]
But you're not advocating it be located at "Ceres", you want it located at "Ceres (dwarf planet)". That doesn't follow COMMONNAME. If we're going to have a dab anyway, "1 Ceres" wins out per COMMONNAME, as well as following the pattern of all other MP's but Pluto. (Pluto's unique in not being assigned a MP number until decades after discovery.) And probably about as many people know about Vesta as about Ceres, so that's not much of an argument either. If we need a dab, why should the dab for Ceres be different than the dab for all other MPs? — kwami (talk) 11:30, 6 October 2021 (UTC)[reply]
It is not at Ceres because of the deity. But more people know Ceres as a "Dwarf Planet" than as "MPC number 1". The general public does not know Quaoar from a hole in the ground. -- Kheider (talk) 11:59, 6 October 2021 (UTC)[reply]
And more people know of Vesta as an asteroid than as "MPC number 4", yet the article is still at '4 Vesta'. Then there's the problem that the only RS we have says there are 'unexplained anomalies' re. Ceres being a dwarf planet. We shouldn't be making a claim of truth in the article title about something debatable like that. — kwami (talk) 14:10, 6 October 2021 (UTC)[reply]
Wikipedia long ago decided to treat the 5 IAU dwarf planets as more special than the other 585 THOUSAND NUMBERED minor planets. Debates can be covered in the article body. -- Kheider (talk) 16:09, 6 October 2021 (UTC)[reply]
The problem is that that categorization is obsolete. There are other dwarf planets than these five, and the IAU has nothing to do with classifying them. As for debates, that's precisely my point: they should be covered in the article body and not in the title. Since there is uncertainty whether Salacia is a DP, the article shouldn't be at "Salacia (dwarf planet)". Same for Ceres. It's one thing to say in the text "the dwarf planet Ceres (BTW, we're not entirely sure it's a dwarf planet)", and another to formally declare it one in the title. — kwami (talk) 09:15, 7 October 2021 (UTC)[reply]
What you're looking for is a name which won't change if the category of the object changes. As best I can tell from the Venn diagram at Minor_planet#/media/File:Euler_diagram_of_solar_system_bodies.svg, such a universal designation doesn't exist. It used to be "minor planet", but the IAU reclassified dwarf planets to not be included in that designation. The best you could do would be "astronomical object" or "small solar system body", which would be even worse in terms of usable name. In general, I'd suggest trying to solve this problem comes under Ralph Waldo Emerson's "foolish consistency" dictum, and thus not worth pursuing. Regards, Tarl N. (discuss) 17:38, 7 October 2021 (UTC)[reply]
There are multiple solutions. "1 Ceres" is the most consistent, but it could also be "Ceres (asteroid)", "Ceres (astronomy)", or just "Ceres", making it the primary topic of the name. And it's not a matter of "if the category changes" -- Ceres is what it is. The problem is that we're not sure what it is, and claiming surety in the article title is unprofessional. — kwami (talk) 18:08, 7 October 2021 (UTC)[reply]
Comment wouldn't disagree in saying that Makemake and Haumea should remain titled as they are per WP:PRIMARYTOPIC.
As to naming: looking at the links from the current DABs Ceres and Eris, the primary topics for these names are indeed the dwarf planets due to the length of the articles and they are also rated as at least good article class. Per page views of Eris and Ceres shows both the dwarf planets have higher page views over the latest 20 days, more page watchers, larger size and are rated as higher class articles. Moving Ceres & Eris to Ceres (disambiguation) & Eris (disambiguation) respectively and Ceres (dwarf planet) & Eris (dwarf planet) to Ceres & Eris respectively could be a better alternative.
The dwarf planets article does not have any numbers visible in front of the names i.e. 90377 Sedna is just seen as Sedna. Per comment made by Beanpickle, numbers are not really well known to most people and I don't know the actual number in front of Sedna as much as the name of the dwarf planet itself. Either way, we should consider the dwarf planets to be WP:PRIMARYTOPIC as they have higher educational value and more significance than others listed on the disambiguation pages including Ceres, Eris and Sedna so I say they should be titled as Ceres and Eris and perhaps remove the 90377 from 90377 Sedna as well as numbers are obscure in this part of the Solar System. Thanks, Iggy (Swan) (Contribs) 09:58, 9 October 2021 (UTC)[reply]
Comment Since this has been suggested a couple of times here, I would support the moves Ceres (dwarf planet)Ceres and Eris (dwarf planet)Eris. Double sharp (talk) 12:19, 9 October 2021 (UTC)[reply]
Strong Nope to Ceres and Eris as primary, the figures in mythology, who the topics are named after, would intrude on that idea. Anyway, this RM is for the dwarf planet and any other naming idea would need another RM (which would likely be wasting time per the mythological figures, see this 2006 RM and this 2018 RM which tried to go the other way). Randy Kryn (talk) 12:42, 9 October 2021 (UTC)[reply]
The discussion above is closed. Please do not modify it. Subsequent comments should be made on the appropriate discussion page. No further edits should be made to this discussion.

Who approves of US missions?

The paragraph ending "Other missions to the asteroid belt were proposed in the 1980s by France, Germany, Italy, and the United States, but none were approved" reads as if the European Space Agency has dibs on missions to this place. I suspect that if the United States or rather someone in the United States were proposing a mission it would be NASA or Congress that was the decider. ϢereSpielChequers 14:44, 11 October 2021 (UTC)[reply]

Fixed I think. I can't check the soruce, since it's a book, but I assume that's what was meant. Serendipodous 15:59, 11 October 2021 (UTC)[reply]
Thanks, that works for me. ϢereSpielChequers 16:52, 11 October 2021 (UTC)[reply]

I suspect that will get deleted during copy-editing, as it's completely redundant. "Other missions" can't be read to mean "the same mission". — kwami (talk) 22:05, 11 October 2021 (UTC)[reply]

Wow. And there I was thinking you were going to say something constructive. Speaking of, what's the point of that graph? The selection of comparative objects seems completely random. Serendipodous 23:39, 11 October 2021 (UTC)[reply]
No need to be hostile. It probably will be deleted some day, because people are going to think, "of course, who else would approve of the missions?", just as the title of this thread states. It's even confusing, because the reader is going to wonder why we would say something so superfluous -- surely we meant something by it, but it's not clear what that could be. Then when they realize it doesn't mean anything, they'll delete it to clean up the article.
The selection of objects is those closest to Ceres in mass. If it were random, they wouldn't be comparable -- either they would be invisible or Ceres would. Orcus we mention in the text. — kwami (talk) 00:14, 12 October 2021 (UTC)[reply]
What's the point of comparing Ceres to a group of objects of similar mass? Surely the point of such visual comparisons is to show differences, not similarities. The real question is, given that no one outside of astronomy nut-dom has a clue what those names mean, shouldn't we use more familiar objects? As for hostility, well as it happens the guy you just said was too stupid to understand something so obvious as who would launch a space mission is a friend of mine. So yeah. Not happy. Serendipodous 01:16, 12 October 2021 (UTC)[reply]
I never said anything of the sort. You really do seem to search for things to be offended about. What I said was stupid was claiming that 33% is a "quarter". That is stupid, and if you're offended by that, too bad. As for the above, I wasn't criticizing the objection, but the awkward fix.
What's the point of comparing Ceres to other DPs? We do that in the text. In fact, you were adamant about doing that to the point of inaccuracy. What's the point of comparing it to other asteroids? We do that in the text. Personally, knowing that Ceres is about the size of Dione or Ariel, rather smaller than Charon, and midway between Orcus and Quaoar among DPs gives me a better feel for the Solar system than just a raw number for its mass. If you want to show differences, fine and good: what did you have in mind? — kwami (talk) 03:54, 12 October 2021 (UTC)[reply]

I agree with kwami that it's redundant. But I guess, if someone has wondered about what it means already, then it's better that it's redundant than slightly confusing.

I like the comparison of Ceres to the largest asteroids, but I think that there should be a few more, not just the big five, or at least a sector for "all other asteroids". Otherwise it looks a bit weird to have that pie-slice that looks like it's more like two-thirds than one-third.

The comparison to similarly-sized round objects seems quite nice to me too; it makes me understand about how big these things are. Admittedly this is because I have a feel for the planemo moons' sizes already, so maybe that's a case of "astronomy nut-dom". But outside that, what's better? Size of the Earth? That's not exactly a comparison in similar scales anymore. Size of the Moon? Better but still not much? Size of Pluto? Judging by how it's often depicted on solar system posters as comparable to Mercury (combined with Jupiter and Saturn failing to look as overwhelming as they should), I suspect the average person has a pretty wrong idea of what that is. Although at least that seems like a more reasonable comparison, of Ceres to the other DPs. Double sharp (talk) 15:27, 12 October 2021 (UTC)[reply]

I was leery of adding many more, because their masses are so uncertain. For these five, we're pretty sure that's the order they go in. But after that, any new estimate is likely to scramble the order. I agree that having them as a %age of the whole belt would be useful, even if we only have a very crude estimate for it. That's what we currently have at asteroid#Largest asteroids. That chart's already badly dated, so I should probably replace it. — kwami (talk) 23:25, 12 October 2021 (UTC)[reply]

Updated values

JPL's small body database has orbit parameter updates to a new reference epoch 2000001 1 Ceres (A801 AA) epoch=2022-01-21.0 e=0.0785 a=2.76 q=2.549 i=10.59 om=80.27 w=73.64 ma=291.38. 112.119.158.212 (talk) 07:42, 12 December 2021 (UTC)[reply]

Updated. Little diff at 3 sig fig except for mean anomaly. — kwami (talk) 00:15, 13 December 2021 (UTC)[reply]

Multiple entries saying that this is an "Asteroid"

On the NASA website this is stated as NOT being an asteroid. Yes, it is in the asteroid belt, but it a dwarf planet. PAGE: https://solarsystem.nasa.gov/planets/dwarf-planets/ceres/overview/ (look at No.4 on list). I believe NASA should be considered a very valid authority. NASA tends to defer to other agencies/ organisations as well. If no one objects I can go through and remove references implying it is an asteroid. If someone beats me to it then fine. 92.238.237.65 (talk) 03:46, 18 February 2022 (UTC)[reply]