Talk:55 Pandora
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E-class?
- Recent analysis has identified Pandora as the second-largest of the E-type asteroids, after 44 Nysa.
I searched for verification of this citation-less claim, but found none. Papers since 2000 that mention the asteroid still list it as M class, as does the JPL SBDB. For this reason I removed it from the article. Praemonitus (talk) 20:17, 28 February 2020 (UTC)
- Hah! Now this (added 3 September 2008) explains the otherwise inexplicable "see also" section that I've removed today... Renerpho (talk) 00:28, 11 September 2025 (UTC)
- @Praemonitus: There are no studies that identify 55 Pandora as E-type. However, at the time when this was added (in 2008), the article gave an erroneously high albedo of 0.301 (compare this removal today); and our article about E-type asteroids, which was edited by the same user User:A.k.a. on the same day in 2008, said that E-type asteroids
have a high albedo (0.3 or better), which distinguishes them from the more common M-type asteroids
. I think the change from M- to E-type for Pandora may have come about by WP:SYNTHESIS of those two statements. See also M-type asteroid#Definition:... distinguishable only by optical albedo: P-type albedo < 0.1; M-type albedo in 0.1 ... 0.3; E-type albedo > 0.3
. No studies from the time identified Pandora as an E-type asteroid, despite its seemingly high albedo. - Now, here's the fun part: E-type asteroid is listing Pandora as one of the three largest E-type asteroid since this edit from 20 September 2012 (
only three (44 Nysa, 55 Pandora, 64 Angelina) having diameters above 50 kilometres
). This was apparently made to make this edit from 20 July 2007 (only three having diameters above 50 kilometres
) more concrete. 64 Angelina still states that 55 Pandora is the second largest E-type asteroid, and has done so since this edit from 21 February 2007. The same statement was added to the lede of 44 Nysa by the same IP on the same day, where it also survives to the present day. User:A.k.a. added it to the see also section of the Nysa article in 2008, where it also still stands. - All of the edits from 2007 were made by IP editors, none of them come with a citation, and the claim seems to be blatantly false. There are only two such asteroids, Nysa and Angelina, with the third largest 214 Aschera not even coming close. I don't understand where this came from, and how it could survive for 18½ years. It is bordering on a type 3 or type 4 hoax, and may well be worth adding to that list when this has been cleaned up. Renerpho (talk) 01:21, 11 September 2025 (UTC)
- I have now removed this from the articles where I found it (44 Nysa, 64 Angelina, E-type asteroid). Renerpho (talk) 02:13, 11 September 2025 (UTC)
- ... and added it as a type 4 (False or unreferenced and dubious statement that may or may not be a hoax as it could arguably have been added as a mistake or in good faith) to Wikipedia:List of hoaxes on Wikipedia#False statements in articles, as the 4th oldest. Renerpho (talk) 02:54, 11 September 2025 (UTC)
- I have now removed this from the articles where I found it (44 Nysa, 64 Angelina, E-type asteroid). Renerpho (talk) 02:13, 11 September 2025 (UTC)
- @Praemonitus: There are no studies that identify 55 Pandora as E-type. However, at the time when this was added (in 2008), the article gave an erroneously high albedo of 0.301 (compare this removal today); and our article about E-type asteroids, which was edited by the same user User:A.k.a. on the same day in 2008, said that E-type asteroids
- I have removed it from Wikipedia:List of hoaxes on Wikipedia#False statements in articles again, after finding a reference in the German Wikipedia article to from April 1994, which states that
The new estimate of the geometrical albedo indicates unambiguously that Pandora is an M-type asteroid, and its high albedo measured by IRAS satellite and its classification as E-asteroid are mistaken.
- Sorry for the fuzz... it turns out there actually was a study that classified it as E-type. It's just so old (, October 1986) and in such an obscure format that it's not easy to find -- unlike its refutation, which I could have found sooner. Renerpho (talk) 03:14, 11 September 2025 (UTC)
- Thank you for your in-depth investigation. Praemonitus (talk) 04:27, 11 September 2025 (UTC)

