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Eclipse Today
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You are invited to post links, comments and questions on today's eclipse here.
http:// www.spa ce.com/ 19195-n ight-sk y-plane ts-aste roids-w ebcasts .html
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Interactive map here - http:// xjubier .free.f r/en/si te_page s/solar _eclips es/HSE_ 2013_Go ogleMap Full.ht ml
Interactive map here - http://
As the Earth is roughly spherical greatest eclipse generally coincides with where the Moon's shadow crosses the local meridian. The ratio between Sun/Moon distance from the centre of the Earth can vary significantly throughout the duration of an eclipse so that in rare cases the eclipse begins/ends as an annular/total or vice versa, while in this particular hybrid eclipse I believe it was annular, at both ends . . . not that there's anything wrong with that!
For a limited time only (the page changes by the day) try
http:// spacewe ather.c om/
There's a photo taken from an aircraft with a neat story to it.
I struggled to understand :-
"The ratio between Sun/Moon distance from the centre of the Earth can vary significantly throughout the duration of an eclipse"
because I couldn't help but think this was talking about the orbital distance of the moon from earth and couldn't see that changing on such a short timescale.
However, by picturing an imaginary cone, representing the moon's shadow, being wiped across the surface of a globe, I think I get it. Annular at the sunrise and sunset extremities but the moon is bigger in the sky at the midpoint, because the shadow hits the surface one earth-radius closer to the moon than it does at the E and W horizons.
http://
There's a photo taken from an aircraft with a neat story to it.
I struggled to understand :-
"The ratio between Sun/Moon distance from the centre of the Earth can vary significantly throughout the duration of an eclipse"
because I couldn't help but think this was talking about the orbital distance of the moon from earth and couldn't see that changing on such a short timescale.
However, by picturing an imaginary cone, representing the moon's shadow, being wiped across the surface of a globe, I think I get it. Annular at the sunrise and sunset extremities but the moon is bigger in the sky at the midpoint, because the shadow hits the surface one earth-radius closer to the moon than it does at the E and W horizons.
//I struggled to understand :-
"The ratio between Sun/Moon distance from the centre of the Earth can vary significantly throughout the duration of an eclipse"
because I couldn't help but think this was talking about the orbital distance of the moon from earth and couldn't see that changing on such a short timescale.//
The timescale I had in mind was the several hours from the onset of the eclipse (in this case the west Atlantic) until the eclipse ends (the east coast of Africa). In that time frame the relative distances between Earth, Moon, and Sun can change enough for an eclipse to begin as an annular and end as a total, or vise versa.
"The ratio between Sun/Moon distance from the centre of the Earth can vary significantly throughout the duration of an eclipse"
because I couldn't help but think this was talking about the orbital distance of the moon from earth and couldn't see that changing on such a short timescale.//
The timescale I had in mind was the several hours from the onset of the eclipse (in this case the west Atlantic) until the eclipse ends (the east coast of Africa). In that time frame the relative distances between Earth, Moon, and Sun can change enough for an eclipse to begin as an annular and end as a total, or vise versa.
According to the "Five Millennium Catalog of Asymetric Hybrid Solar Eclipses" This was a 'Class 3' Hybrid eclipse beginning as an annular and ending as a total eclipse. Asymetric hybrid solar eclipses (Class 2 or 3) occur with a frequency (on average) of about once per century.
http:// eclipse .gsfc.n asa.gov /SEcat5 /SEhybr id5a.ht ml
http://