It's because of the relative sizes of the Sun, moon and Earth. the moon - being the smallest of the three - casts a small shadow - and thus a solar eclipse rarely lasts more than a few minutes. The shadow cast by the Earth in a lunar eclipse is much larger - and thus the lunar eclipse lasts much longer.
Sometimes there can be more solar eclipses or more lunar eclipses in a given year, but they're pretty even on average. However, because a solar eclipse is only visible along a narrow track on the Earth's surface, whereas a lunar eclipse is visible from anywhere the Moon is visible, it is much more common to SEE a lunar eclipse. ======================================= During the 100 years from 1901 to 2000, there were 228 solar eclipses and 229 lunar ones, for an average rate of about 2.3 of each per year.
Lunar eclipse: Visible to everyone who can see the moon in their sky . . . roughly half of the earth's surface.Solar eclipse: Visible only to the people within a narrow strip on the earth's surface ...a few thousand miles long, but only a few hundred miles wide.
You need to look up the dates of the next eclipses in your location and then be ready to look out for them. Eclipses of the moon are more frequent at any one place, because every eclipse is seen from the whole dark hemisphere of the Earth. Solar eclipses on the other hand are seen from a much smaller area because the Moon is much smaller than the Earth.
A solar eclipse is when the moon blocks the suns light coming to the earth... a lunar eclipse is when the light from the sun is blocked and so you can't see it but it is there...
All eclipses are shadows. A solar eclipse is the Moon's shadow on the Earth. A lunar eclipse is the Earth's shadow on the Moon.
There are generally two lunar eclipses and two solar eclipses each year. Sometimes you will see two partial eclipses instead of one total eclipse; in 2011, there will be four partial solar eclipses, and no total or annular solar eclipses. Since lunar eclipses happen on the Moon, they are visible from the entire night half of the Earth. Solar eclipses, when the Moon's shadow hits the Earth, affect very small areas of the Earth, and so they seem to be more rare. The next total lunar eclipse will happen on December 21, 2010, and will be visible from any point in North America.
There are eclipses of the sun (solar), and eclipses of the moon (lunar). At different places on the Earth, each of those may be total or partial. Sometimes only a partial eclipse is visible anywhere.
Lunar eclipses are visible from the entire night half of the Earth, and on average, every person on Earth can view a total lunar eclipse from home about every two years. Solar eclipses cover much smaller paths across the Earth, and are widely scattered. The NASA Eclipse web page offers a catalog of every eclipse from the year 2000 BCE to 3000 AD.Check the maps at the links below.
A solar eclipse occurs when the Moon passes between the Earth and the Sun, blocking sunlight and casting a shadow on the Earth, while a lunar eclipse happens when the Earth passes between the Sun and the Moon, causing the Earth's shadow to cover the Moon. Solar eclipses are visible only from specific areas on Earth, whereas lunar eclipses can be seen from anywhere on the night side of the Earth. Additionally, solar eclipses are relatively brief events, lasting only a few minutes, while lunar eclipses can last several hours.
Lunar eclipses and solar eclipses happen EQUALLY often; about two of each kind per year. However, solar eclipses are visible only across a small path on the Earth, while lunar eclipses are visible from the entire nighttime hemisphere of the planet.
No. during the 100 years from 1901 to 2000, there were 228 solar eclipses and 229 lunar ones ... an average of about 2.3 of each every year. If you stay in one place, though, you see lunar eclipses more frequently. That's because a solar eclipse is visible from only a small area on earth, whereas a lunar eclipse is visible from wherever the moon is visible ... the entire night-time half of the earth.
There are generally two solar eclipses and two lunar eclipses each year. Of the lunar eclipses, about 40% are "total"; the remainder are partial or penumbral. A lunar eclipse is visible from one-half of the Earth's surface. So on average, and weather permitting, you will see a total lunar eclipse about every third year.