Because of the size of the moon and the distance of the sun, the moon can only cover the sun for a very short time. Because the moon is much closer to Earth and Earth is much bigger than the moon, it casts a big shadow, larger than the size of the moon itself, so it takes it longer to pass through it.
Because the Earth is much larger relative to the Moon than the Moon is relative to the Sun. In a total solar eclipse the Moon will only just cover the Sun so a slight change in position means that you will only see a partial eclipse whereas the Earth will cause a much larger shadow relative to the Moon so a difference in location will not affect it so much.
There are not more solar eclipses than lunar eclipses; in the long run, they are balanced pretty evenly.
because of our location on earth so depending on where we are on earth you can see a total or partial solar and lunar eclipses
There were no total solar eclipses during 2007. There was one total lunar eclipse, one partial lunar eclipse, and two partial solar eclipses.
There are two main types of eclipses: solar and lunar. Lunar eclipses occur every 6 months. Solar eclipses occur 2-5 times per year. Eclipses can be partial or total. Partial eclipse covers only part of the sun or moon, while total covers the full entity.
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 was 2 lunar eclipses in 2008.
because of our location on earth so depending on where we are on earth you can see a total or partial solar and lunar eclipses
There were no total solar eclipses during 2007. There was one total lunar eclipse, one partial lunar eclipse, and two partial solar eclipses.
There are, on average, two solar eclipses and two lunar eclipses each year. In 1999, there was an annular solar eclipse on February 16, and a total solar eclipse on August 11. For lunar eclipses, there was a penumbral lunar eclipse on January 21 and a partial lunar eclipse on July 16. You can look up all eclipses from 2000 BC to 3000 AD on the NASA Eclipse web page.
There are two main types of eclipses: solar and lunar. Lunar eclipses occur every 6 months. Solar eclipses occur 2-5 times per year. Eclipses can be partial or total. Partial eclipse covers only part of the sun or moon, while total covers the full entity.
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.
Actually solar eclipses are slightly more common, but a solar eclipse, and especially the total phase, can only be seen in a relatively narrow strip of Earth.
There was 2 lunar eclipses in 2008.
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.
There are two general types of Eclipse. They are Solar(Sun) and Lunar(Moon). Each of these eclipses can then be further classified into Total or Partial. Total is where the obscuring body completely blocks light from the third body. Partial is where the obscuring body only covers part of the third body.
About two per year, since the Moon formed. So, around 4000 solar eclipses (and 4000 lunar eclipses) since the year 1. You can check the list of all eclipses since the year 2000 BC on the NASA Eclipse Web Page at the link below.
No. About 50% of all lunar eclipses are total; the remainder are partial or penumbral.
During the 100 years of the 20th Century, there were 228 solar eclipses and 229 lunar ones. So over the long term, you can figure on equal numbers, at the rate of around 7 of each every 3 years.