Editing Talk:2816: Types of Solar Eclipse

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By the time you see the cuboid eclipse, it's already too late. Resistance is futile.  
 
By the time you see the cuboid eclipse, it's already too late. Resistance is futile.  
 
[[User:ProphetZarquon|ProphetZarquon]] ([[User talk:ProphetZarquon|talk]]) 23:52, 17 August 2023 (UTC)
 
[[User:ProphetZarquon|ProphetZarquon]] ([[User talk:ProphetZarquon|talk]]) 23:52, 17 August 2023 (UTC)
:Not for everyone. The weak will perish. -- [[User:Hkmaly|Hkmaly]] ([[User talk:Hkmaly|talk]]) 20:33, 18 August 2023 (UTC)
 
  
 
Given that [https://socratic.org/questions/why-is-earth-s-moon-spherical the moon is slightly oblate], would an oblate eclipse be possible when the angular sizes of the moon and sun are almost the same? [[User:Ehusmark|EHusmark]] ([[User talk:Ehusmark|talk]]) 09:11, 18 August 2023 (UTC)
 
Given that [https://socratic.org/questions/why-is-earth-s-moon-spherical the moon is slightly oblate], would an oblate eclipse be possible when the angular sizes of the moon and sun are almost the same? [[User:Ehusmark|EHusmark]] ([[User talk:Ehusmark|talk]]) 09:11, 18 August 2023 (UTC)
:A good question, but the diagram shows the sun as being oblate, so I don't think the intention was to reference the slight (but real) oblate nature of the moon.  Good catch, though.  [[User:Dextrous Fred|Dextrous Fred]] ([[User talk:Dextrous Fred|talk]]) 16:54, 18 August 2023 (UTC)
 
:The Moon has an equatorial diameter of ~3576.2km, polar diameter of ~3472.0km. 104ish km difference. The Sun is near-spherical, said to be less than 10km difference between equatorial and polar diameters, which projected inwards to 'Moon equivalent distance' is even more practically zero. But as it would be distorted at roughly the same angle as the Moon (spin axis of each varyies maybe +/-5 degrees, depending on what point of each orbit everything is) it would always be <105km difference so long as the Sun's oblativity weren't double that of the Moon (or prolate to any degree). Moon-'mountains' seem to be about 2.5km high, so local rim-variations won't actually add/subtract much from any oval-adjustments.
 
:Anyway, 90km in 3500km(+/-) is around a quarter of a percent of variation. And a handful of millionths of a degree, subtended to the Earth observer, if my best-/worst-case calculations that I just did are correct (roughly 1/60th of an arc-second is one of the answers I pulled out, in case anyone wants to sanity-check what I just did on the back of this 'ere envelope). [[Special:Contributions/172.69.79.153|172.69.79.153]] 18:56, 18 August 2023 (UTC)
 
 
"A normal Sun-Moon-Earth eclipse seen from the Moon would either be ineffectual or perfectly normal 'night-time'" -- The shadow on the Earth should be visible from the dark side, probably with the naked eye but certainly with modest optics.  Perhaps it's not dramatic but it would still be interesting.[[Special:Contributions/162.158.159.80|162.158.159.80]] 03:16, 19 August 2023 (UTC)
 
:Yes, here's an example: [https://www.nasa.gov/audience/forstudents/k-4/stories/moons-shadow NASA picture of Moon's shadow during solar eclipse] [[User:AdmiralMemo|Admiral Memo]] ([[User talk:AdmiralMemo|talk]]) 05:53, 19 August 2023 (UTC)
 
:As the author of the phrase, to clarify that I was refering mostly to: 1) ineffectual because you're sunlit on the far side and can't see the Earth at all, or 2) 'normal night-time' (ok, not ''perfectly'', but nearly so) because you have a 99.9999...% "full-Earth" amount of earthshine illuminating you. As opposed to Earth-viewed eclipses where all (direct/reflected) illumination is conspicuously absent for a number of minutes. (Or much, for partial(solar/lunar) or annular(solar).)
 
:Being on the Moon for a lunar-eclipse (even partial, if you're somewhere on the right bit) is far more significant. Unless you're on the far-side, in which case it's an extreme non-event just as being there during the solar eclipse is (but 'essentially normal night' instead of 'essentially normal day').
 
:Perhaps some fun could be had by being out on the limbs/poles of the lunar surface, raised high enough against the local surface to have significant 'both sides' experience (''become'' an actual bailey's bead/miniscule gap between them? ...not that it would be personally so obvious as such). Just remember to account for libration, when you choose your spot! ;) [[Special:Contributions/172.71.242.193|172.71.242.193]] 09:49, 19 August 2023 (UTC)
 

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