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The first paragraph refers to the "discovery of Algol." Algol is a second or third magnitude star with a declination of about +40°. No one in the northern hemisphere or the tropics "discovered" it--it was easily visible.
Presumably the intention is to refer to the "discovery of Algol's periodic variability."
I am hesitant to simply make the change, as I am a very infrequent editor and this article has obviously generated a lot of back and forth conversation. SarahLawrence Scott (talk) 21:46, 1 December 2024 (UTC)
Algol Ab (C) or it's the primary pair (Aa1 and Aa2) in either 680 or 681 days - the article gives both numbers in adjacent sections. Which is correct? Mastakos (talk) 12:42, 19 March 2025 (UTC)
The use of Aa1/Aa2/Ab vs. A/B/C is inconsistent in the article, making it confusing. even the summary table at the front uses Aa1/Aa2 for the primary orbital characteristics, but then uses A/B for the secondary. this occurs later as well. someone knowledgeable should clean this up so us non-astronomers don't get confused. Especially since the two possible companions might be B and C or D and E depending on nomenclature used
also, nowhere does it seem to give the individual masses of the three confirmed stars - only a mass ratio! (For that matter, the possibility of 2 additional stars B and C is mentioned once, then ignored completely. What are their characteristics, do they co-move or not?) Mastakos (talk) 13:13, 19 March 2025 (UTC)
Algol A is said to have accreted mass from the once more massive Algol B; should Algol A be then considered a blue straggler as it accreted (or at least removed) enough mass for Algol B to become the secondary? Pancakes321 (talk) 07:02, 19 September 2025 (UTC)
The table with Algol minima times in 2025 is wrong, the times are off.
https://skyandtelescope.org/observing/the-minima-of-algol/ — Preceding unsigned comment added by 2A05:4F46:417:9100:B991:7BD1:B423:C493 (talk) 06:31, 30 September 2025 (UTC)
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