my late night booty call.....
There are generally two solar eclipses each year. About half of them are partial, and the remaining ones are divided between full and annular eclipses. You can look up the catalog of all eclipses from 2000BC to 3000AD on the NASA Eclipse Web Page. We tend to think of solar eclipses as being much more rare. However, the difference is that a solar eclipse is visible only across a narrow strip across the Earth. Since the Earth is 3/4 covered by water, there is a much higher probability that the eclipse will be visible at sea. For example, the total solar eclipse of July 11, 2010 will be visible along a path across the South Pacific Ocean, including a few atolls in French Polynesia, Easter Island, and the southern tip of Chile and Argentina.
The length of the total phase in a total solar eclipse varies with the exact geometry of the eclipse; where the Sun and Moon are relative to the Earth, how far away the Moon is, and where in the path of totality you are. But it is NEVER more than 7 minutes 30 seconds, and is often much shorter. For example, for the total solar eclipse on September 21, 2968, the maximum duration of totality was 40 seconds. A duration of 4-5 minutes is typical. For total lunar eclipses, the total phase varies with the same factors, except that the maximum length of the total phase can be up to an hour and a half or more. For example, in the total lunar eclipse of June 15, 2011, the total phase will be 100 minutes, which is pretty close to the maximum.
The Moon's orbital plane is tilted about 5 degrees to the ecliptic (the Earth's orbital plane), so the Sun, the Moon and Earth do not perfectly align every new moon or full moon. We can have an eclipse only if the alignment of the three bodies happens along the intersection of the two orbital planes.
The wavelength decreases
The earth's shadow falls on the moon only during a lunar eclipse. Eclipses of the moon can have varying degrees of totality. The earth's penumbra (partial shadow) may pass over the moon, or the umbra (full shadow) may pass over some or all of the moon's surface. All of these happen only at the time of full moon. The moon's regular phases are NOT caused by earth's shadow on the moon, as is incorrectly believed by some.
The answer very much depends on the year. One calendar year has a minimum of four eclipses, which are two solar eclipses and two lunar eclipses. A year can have as many as seven eclipses. So each year is different.
On average, we can expect two lunar eclipses and two solar eclipses in any year. 2010 will have four eclipses, right on the average.
none to 3 lunar eclipses a year
There was 2 lunar eclipses in 2008.
3
2
On earth there are 2 eclipses, Lunar and Solar eclipses
alot
There are typically two lunar eclipses and two solar eclipses each year. Sometimes, depending on the precise alignment of the Sun, Earth and Moon, we'll see two "partial" or "penumbral" eclipses instead of one "total" eclipse. The NASA Eclipse Web Site lists details on all eclipses from 2000 BC to 3000 AD; you can look up all the eclipses from 2020 to 3000, and estimate how many there will be from 3000 to 3020 based on that.
No.
Probuly 2at most
i think we only have it and and all the rest have a phase