The last total lunar eclipse of 2011 will appear in the western sky Saturday morning just before dawn in the west coast of the U.S.
Saturday's show will be the last chance to catch a total lunar eclipse for another three years, according to the Associated Press.The eclipse will begin at 4:45 a.m. PST when a red shadow starts to cover the moon. Those in western North America will have the best views well before dawn, but can still catch the eclipse until as late as 6:05 a.m. PST, according to NASA Science Cast.
How to Catch lunar eclipse of 2011
Clear skies and geographical location permitting, Saturday will be your last chance to spy a total lunar eclipse until 2014. Here's what you need to know to catch a glimpse before it's gone.
For the majority of the Western Hemisphere, the eclipse will be most noticeable early Saturday morning in the hours right before dawn.
A lunar eclipse occurs when the sun and moon are aligned with the Earth in between them. Earth then casts a temporary shadow on the moon as it blocks the suns rays. As opposed to a partial eclipse, total eclipses entail a perfect alignment of the three bodies.
Saturday's show will be the last chance to catch a total lunar eclipse for another three years, according to the Associated Press.The eclipse will begin at 4:45 a.m. PST when a red shadow starts to cover the moon. Those in western North America will have the best views well before dawn, but can still catch the eclipse until as late as 6:05 a.m. PST, according to NASA Science Cast.
How to Catch lunar eclipse of 2011
Clear skies and geographical location permitting, Saturday will be your last chance to spy a total lunar eclipse until 2014. Here's what you need to know to catch a glimpse before it's gone.
For the majority of the Western Hemisphere, the eclipse will be most noticeable early Saturday morning in the hours right before dawn.
A lunar eclipse occurs when the sun and moon are aligned with the Earth in between them. Earth then casts a temporary shadow on the moon as it blocks the suns rays. As opposed to a partial eclipse, total eclipses entail a perfect alignment of the three bodies.