Perhaps astrologers will deem this portentous, but the rest of us can simply marvel at the natural spectacle.
On the night of 2007 MAR 03/04 (Saturday/Sunday) the Full Moon will enter the Earth’s shadow and become totally eclipsed. The maximum magnitude will be 1.227, meaning the lunar limb will be separated from the edge of the umbra (dark central shadow) by 0.227 lunar diameters. It will be visible from the eastern half of North America and east across the Atlantic and most of Eurasia to India.
For most eastern North Americans the Moon will rise while in total eclipse. Those along the New England coast will witness the Moon entering the umbra shortly after it rises. Europeans will witness the entire event. Indians will see almost all of it except the final penumbral stage.
Below are my calculated event timings in Universal Time using the French Rule for shadow sizes. Unlike virtually all other sources, I also take into account the oblate shape of the Earth.
20:18 UT Penumbral Phase Begins (penumbra is light fringe shadow)
21:31 UT Partial Phase Begins (enters umbra)
22:45 UT Totality Begins (fully in umbra)
23:21 UT Maximum Eclipse
23:57 UT Totality Ends
01:11 UT Partial Phase Ends
02:23 UT Penumbral Phase Ends
I’ve created graphics that demonstrate the stages of the eclipse as observed from several cities. More will be added as the event nears. To see them, click:
http://www.curtrenz.com/astronomical.html
The graphics may be removed soon after the event occurs.
On the night of 2007 MAR 03/04 (Saturday/Sunday) the Full Moon will enter the Earth’s shadow and become totally eclipsed. The maximum magnitude will be 1.227, meaning the lunar limb will be separated from the edge of the umbra (dark central shadow) by 0.227 lunar diameters. It will be visible from the eastern half of North America and east across the Atlantic and most of Eurasia to India.
For most eastern North Americans the Moon will rise while in total eclipse. Those along the New England coast will witness the Moon entering the umbra shortly after it rises. Europeans will witness the entire event. Indians will see almost all of it except the final penumbral stage.
Below are my calculated event timings in Universal Time using the French Rule for shadow sizes. Unlike virtually all other sources, I also take into account the oblate shape of the Earth.
20:18 UT Penumbral Phase Begins (penumbra is light fringe shadow)
21:31 UT Partial Phase Begins (enters umbra)
22:45 UT Totality Begins (fully in umbra)
23:21 UT Maximum Eclipse
23:57 UT Totality Ends
01:11 UT Partial Phase Ends
02:23 UT Penumbral Phase Ends
I’ve created graphics that demonstrate the stages of the eclipse as observed from several cities. More will be added as the event nears. To see them, click:
http://www.curtrenz.com/astronomical.html
The graphics may be removed soon after the event occurs.
