Talk:(307261) 2002 MS4

Diameter

Where did the old diameter of ~1386 come from? Now that I check the history logs I see that User:Michaelbusch kept re-instating it in place of wild guesses. User_talk:68.186.106.251 was the 1st to insert it on 11 Sept 2006 :-) Kheider 06:48, 8 November 2006 (UTC)

With abs mag (H)=3.8, even assuming an albedo of 0.04 in 2006 would have resulted in a diameter of only 1150. -- Kheider (talk) 18:52, 6 January 2010 (UTC)

Image

Needs an image (even though it will just be a dot!)Fig (talk) 13:33, 14 March 2015 (UTC)

External links modified

Hello fellow Wikipedians,

I have just modified one external link on (307261) 2002 MS4. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:

• Added archive https://web.archive.org/web/20111018154917/http://www.gps.caltech.edu/~mbrown/dps.html to http://www.gps.caltech.edu/~mbrown/dps.html

When you have finished reviewing my changes, please set the checked parameter below to true or failed to let others know (documentation at {{Sourcecheck}}).

This message was posted before February 2018. After February 2018, "External links modified" talk page sections are no longer generated or monitored by InternetArchiveBot. No special action is required regarding these talk page notices, other than regular verification using the archive tool instructions below. Editors have permission to delete these "External links modified" talk page sections if they want to de-clutter talk pages, but see the RfC before doing mass systematic removals. This message is updated dynamically through the template {{source check}} (last update: 18 January 2022).

• If you have discovered URLs which were erroneously considered dead by the bot, you can report them with this tool.
• If you found an error with any archives or the URLs themselves, you can fix them with this tool.

Cheers.—InternetArchiveBot (Report bug) 23:13, 3 September 2016 (UTC)

External links modified (January 2018)

Hello fellow Wikipedians,

I have just modified one external link on (307261) 2002 MS4. Please take a moment to review my edit. If you have any questions, or need the bot to ignore the links, or the page altogether, please visit this simple FaQ for additional information. I made the following changes:

• Added archive https://web.archive.org/web/20110604033434/http://www.boulder.swri.edu/~buie/kbo/astrom/02MS4.html to http://www.boulder.swri.edu/~buie/kbo/astrom/02MS4.html

When you have finished reviewing my changes, you may follow the instructions on the template below to fix any issues with the URLs.

This message was posted before February 2018. After February 2018, "External links modified" talk page sections are no longer generated or monitored by InternetArchiveBot. No special action is required regarding these talk page notices, other than regular verification using the archive tool instructions below. Editors have permission to delete these "External links modified" talk page sections if they want to de-clutter talk pages, but see the RfC before doing mass systematic removals. This message is updated dynamically through the template {{source check}} (last update: 18 January 2022).

• If you have discovered URLs which were erroneously considered dead by the bot, you can report them with this tool.
• If you found an error with any archives or the URLs themselves, you can fix them with this tool.

Cheers.—InternetArchiveBot (Report bug) 21:59, 25 January 2018 (UTC)

Occultation size estimate

@Nrco0e: Regarding your addition Calculated from the projected elliptical dimension of 842 × 688 km, or triaxial dimension of 842 × 842 × 688 km. The mean diameter of 787 km is derived from the cube root of the product of the given triaxial dimensions., I wonder where you take the information about the triaxial dimensions from. The occultation does not give triaxial dimensions; it gives an elliptical cross section $a\cdot b$, which may be assumed to be from a triaxial object with volume $a\cdot b\cdot b$ (it almost certainly isn't, but whatever). It is almost never $a\cdot a\cdot b$ for large bodies, even though this is possible. Do you have any source for why it should be the rare one (or the not-so-rare one, for that matter)? If not, I suggest to completely remove all of this, including the mean diameter. The source just doesn't give this information, and a lot of the assumptions must be WP:OR. Renerpho (talk) 04:43, 16 November 2019 (UTC)

There is one more mathematical quirk here: The fit 842 × 688 km is done with just two chords (four points), which is not enough to define an ellipse (even assuming that the two chords had perfect accuracy, which they don't).[1] So, those numbers must come with considerable uncertainty (hundreds of km's in each axis, if I should guess; the uncertainty is not specified). Having a mean diameter based on a triaxial shape based on those numbers is questionable. Renerpho (talk) 04:48, 16 November 2019 (UTC)

Occultation of 26 July 2020

Successful observation of a stellar occultation tonight, which was actually streamed live via Youtube. The occultation is starting near the 39:43 minute mark, and took about 23 seconds. The prediction details can be found here. Note that this is the first of three occultations by 2002 MS4 this summer, the other two coming up on August 8th and August 12th. Renerpho (talk) 01:26, 28 July 2020 (UTC)

Cool! We're getting a lot of occultation data, so hopefully we'll see tighter numbers. — kwami (talk) 06:14, 21 June 2022 (UTC)

Ceres

Isn't Ceres the largest known planetoid without a moon? This google search says that it is just another term for asteroid and Ceres is the largest known asteroid. (I don't think 2002 MS₄ is an asteroid)108.46.173.109 (talk) 12:38, 1 May 2021 (UTC)

'Planetoid' is synonymous with 'minor planet'. Ruslik_Zero 17:36, 1 May 2021 (UTC)

3-sigma uncertainty

We are giving a 3-sigma uncertainty of abt. 14 days for the perihelion date. This may be a sensible thing to do, but right now the article doesn't say what that reason is. The reference gives dtp=4.6936 days (1-sigma), and there has to be a good reason not to follow that. We could point here for why 3-sigma is a reasonable choice for some data, although I still don't see why we don't just give the 1-sigma value from the source.Renerpho (talk) 05:39, 21 June 2022 (UTC)

Uncertainties are generally assumed to be 1 sigma unless stated otherwise. We don't state otherwise, so I changed it to 1 sigma. If there's a reason for 3 sigma, that can be restored with the reason added. — kwami (talk) 06:11, 21 June 2022 (UTC)

Potential names?

Is it known if there are any yet suggested? I don't even know where you'd start to look, but it seems odd that there aren't even any proposed ones from some time in the last 21 years. Or might it just be left as a number forever, as a deliberate piece of astronomical weirdness, seeing as it's now been so long? (How long did Albion run before being named, again?) 51.219.168.15 (talk) 13:31, 9 May 2023 (UTC)

There's always going to be a largest unnamed object, so in that sense it doesn't matter. Often ppl will hold off naming an object until they know enough about it to decide on an appropriate (as opposed to arbitrary) name, or until someone has something or someone to commemorate. There's a whole string of small, unremarkable asteroids named after students who won an annual science competition, but there are more stringent guidelines for these objects. If someone discovers something notable about MS4, we might get a name then. — kwami (talk) 04:47, 10 May 2023 (UTC)

Albion took just over 25 years to get a real name. Double sharp (talk) 16:07, 10 May 2023 (UTC)

Naming a common dwarf planet (as there are hundreds if not thousands of them) is not really a high priority or of scientific value. As I have known many of these objects by their "license plate numbers" for numerous years, I often find them getting a name making it more difficult to remember which one someone is talking about. -- Kheider (talk) 08:44, 11 May 2023 (UTC)

Too bad we can't find mythological names like 'Orten' or 'Emsephor'. — kwami (talk) 10:54, 11 May 2023 (UTC)

No, but already in the first thousand some of the final names alluded to the provisional designation. Consider 572 Rebekka = 1905 RB, 573 Recha = 1905 RC, 574 Reginhild = 1905 RD, 575 Renate = 1905 RE. Double sharp (talk) 16:37, 11 May 2023 (UTC)

Exactly what I was thinking, but harder to do that within the naming reqs of the IAU. — kwami (talk) 08:27, 12 May 2023 (UTC)

Salacia and Varda got named, so naming similarly-sized MS4 and AW197 isn't really that unreasonable in my opinion. Especially since they were discovered so early. Double sharp (talk) 16:54, 11 May 2023 (UTC)

The discoverers had no naming interest in it, probably. I would like to propose the name Jingwei.Chinese goddess.± — Preceding unsigned comment added by 文爻林夕 (talk • contribs) 11:11, 15 June 2023 (UTC)

GA Review

The following discussion 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.

---

This review is transcluded from Talk:(307261) 2002 MS4/GA1. The edit link for this section can be used to add comments to the review.

Reviewer: CactiStaccingCrane (talk · contribs) 02:28, 17 December 2023 (UTC)

Very interesting asteroid. I am not an expert about asteroids in general so I will focus more on formatting and copyediting, though I will review the sources to the best of my ability. CactiStaccingCrane (talk) 02:28, 17 December 2023 (UTC)

P.S. No quid pro quo here, but could you also help reviewing Mars Society GAN? That article is really short and I would be very grateful if you do so. CactiStaccingCrane (talk) 02:31, 17 December 2023 (UTC)

Sorry, I'm too busy to help review other GANs. Plus, I'm going on a 4-day vacation tomorrow so I won't be available to respond if you happen to finish your GA review of this article during that time. Nrco0e (talk) 02:07, 24 December 2023 (UTC)

Hi @CactiStaccingCrane, it's been a while. Have you gotten around to reviewing this article yet? No rush of course. Nrco0e (talk) 17:41, 5 January 2024 (UTC)

I am very sorry that I have been too busy IRL lately. I will try to get the review done today. CactiStaccingCrane (talk) 01:30, 6 January 2024 (UTC)

Actually, I think I might not be the best person for verifying citations. I will ask for 2nd opinion for reviewing more technical aspects of the article. CactiStaccingCrane (talk) 01:35, 6 January 2024 (UTC)

---

Review

• "in the Kuiper belt, a region of" -> "in the Kuiper belt, which is a region of" (for clarity)
• "2002 MS4 has a diameter close to 800 km (500 mi), which approximately ties it with 2002 AW197 and 2013 FY27 (to within measurement uncertainties) as the largest unnamed object in the Solar System." -> "To within measurement uncertainties, 2002 MS4, 2002 AW197 and 2013 FY27 has a diameter close to 800 km (500 mi) and thus are the largest unnamed object in the Solar System." (again, for clarity)
• "significantly improved 2002 MS4's orbit" -> "significantly reduced the uncertainty of 2002 MS4's orbit" (I assume here 'improved' as in a better estimation)
• "Despite this, researchers do not consider 2002 MS4 to be in resonance with Neptune" – could you please clarify what exactly caused astronomers to think so? Is it because of insufficient evidence or the fact that its resonance is intermittent?

Comment: It's simply because astronomers don't classify 2002 MS₄ as a resonant TNO. Every paper (except for that one claiming the resonance) I could find about 2002 MS₄ calls it a classical Kuiper belt object. I'm not sure why it's only this paper that mentions 2002 MS₄ is resonant—there's no formal refutation to this claim, so I do not know if this is still correct or not. Nrco0e (talk) 03:57, 6 January 2024 (UTC)

• "can make Earth-based observations" -> "can make observations" (space telescopes also have this issue, I think)
• "it is approximately tied with" -> "it tied with" (redundancy)
• "which would have made mass estimates possible" -> "otherwise estimation of its mass would have been possible" (avoid ambiguity of 'which' – is it referring to the minor planet or its moons?)
• "for an assumed single-peaked light curve due to a spheroidal body with albedo variations" (might be worthwhile to explain this further in lay terms, as you have excellently done with other parts of this article)

Comment: I've decided to remove this part of the sentence since I don't think there's a need to distinguish the "single-peaked" nature of 7.33/10.44 hour period in the article, when the reference used for it does not discuss alternative possible rotation periods that are not single-peaked. For such a minor detail, I figured it would be better to explain it in a footnote instead. Nrco0e (talk) 03:57, 6 January 2024 (UTC)

I think that's a good idea too. CactiStaccingCrane (talk) 07:43, 6 January 2024 (UTC)

Overall, the article is very well written! I will try to review the citations as soon as possible, but because I am not an expert about this topic, I have asked for a second opinion for reviewing this article. CactiStaccingCrane (talk) 02:01, 6 January 2024 (UTC)

@CactiStaccingCrane: Thanks, I appreciate it. Nrco0e (talk) 03:58, 6 January 2024 (UTC)

2O on citations

Because of time: @CactiStaccingCrane:, @Nrco0e:.

I am no astronomer, but I do edit in the general natural-sciences area. To my eye, all of the citations used are scientific papers (definitely acceptable) or publications by either the Jet Propulsion Laboratory or the Minor Planet Center, which I assume are considered reliable astronomy sources. My only concern is that [8] and [9] are theses, which are not necessarily acceptable sources. Nrco0e, please justify their use. Happy editing, SilverTiger12 (talk) 20:02, 25 January 2024 (UTC)

@SilverTiger12: So you're talking about the theses of Peng and Thirouin? I assure you they're reliable. Peng works with researchers from the New Horizons mission (thesis supervised by JJ Kavelaars) and has co-authored one refereed paper, Verbiscer et al. 2022. They've been working on New Horizons observations of 2002 MS₄ since 2020. For Thirouin, she is an active researcher in minor planets and has over 50 refereed publications. Although some figures from her PhD thesis (i.e. rotation period of 2002 MS₄) weren't formally published as standalone papers, I would consider it reputable since several papers have cited the 2002 MS₄ rotation period directly from her thesis. For example, ADS says 10 papers have cited Thirouin's thesis--such papers include Verbiscer et al. 2022 on New Horizons observations and Rommel et al. 2023 on 2002 MS₄ occultation. Nrco0e (talk) 20:23, 25 January 2024 (UTC)

Thank you, those are good arguments for including them. I'd give this article a pass on citations. SilverTiger12 (talk) 20:36, 25 January 2024 (UTC)

@CactiStaccingCrane:? SilverTiger12 (talk) 21:31, 2 February 2024 (UTC)

I think the article meet ga standards for me as well. Since I don't have PC access today, feel free to self close this nomination @Nrco0e. CactiStaccingCrane (talk) 07:18, 3 February 2024 (UTC)

@CactiStaccingCrane: Done. Thank you and @SilverTiger12: for the review! Nrco0e (talk) 19:59, 3 February 2024 (UTC)

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.