Full Moon

Everyone talks about a full moon and how it affects a person. Now since we know there is no such thing as a full moonpeople that say they are afected by the full moon only use that as an excuse. Do the research.


We could then say that the Moon is officially "full" for only one minute. The Full Moon of Feb. 6, for instance, occurred at 3:14 a.m. EST. In the very strictest sense, one minute before that time, the phase of the Moon was a waxing gibbous; one minute after that time, it was a waning gibbous phase.
But the mechanics of the celestial alignment -- the Sun, Earth and Moon all in a line -- adds a twist to the idea of fullness.
The disk of the Moon can appear 100 percent sunlit from Earth only if it is diametrically opposite to the Sun in the sky. But at that moment the Moon would be positioned in the middle of Earths shadow -- and in total eclipse. So in any month when there is no eclipse, there is an ever-so-slight sliver of darkness somewhere on the lunar limb throughout those hours -- or that moment -- when the Moon is passing through "full" phase.
So why isn't there an eclipse every month?
Because the plane of the Moon's orbit is inclined 5 percent with respect to the plane of Earth's orbit around the Sun. Only once every few months does a Full Moon occur when the orbits are lined up just right to create an eclipse.
People often refer to the Moon as being full a day or two before or after the actual date of fullness. Yet, close inspection will usually reveal that the Moon is not fully illuminated on these prior or subsequent days, but is indeed gibbous or slightly out of roundness.
So, just how long is the interval during which the full Moon seems to appear perfectly round? And when can this effect first be noted with binoculars or the unaided eye?
In the course of one hour, the Moon appears to move eastward against the background stars at roughly its own apparent diameter, or about half a degree. As a consequence, the lunar phase angle the angle of illumination that the Moon makes with the Sun changes, but very slowly. On the Moons surface, this corresponds to only about 10 miles each hour. So the change from a disk that appears fully illuminated, to one that shows a slight out of roundness can be rather subtle.
This test can be made Saturday night, March 6, when full Moon occurs at 23:14 U.T., or 6:14 p.m. EST. For Europeans, the Moon will be high in the south-southeast sky. For North Americans, the Moon will either have just risen, or moonrise will be, at most, less than a few hours away.
When the Moon sets about seven hours later for Europeans, will it still appear perfectly round for them, or ever so slightly out of shape? At about that same time the Moon will be approaching its highest point in the sky over North America.
After about another six or seven hours or at least a half a day after the time that the Moon turned full the Moon will be getting ready to set over North America. By then, anyone looking carefully enough with binoculars should be able to detect a slight sliver of darkness (astronomers call this the terminator) along the western, or right edge of the Moon.