How long eclipse last

By Melissa Chan. Related Stories. Already a print subscriber? Go here to link your subscription. Need help? The umbra takes the shape of a dark, slender cone. It is surrounded by the penumbra , a lighter, funnel-shaped shadow from which sunlight is partially obscured. During a total solar eclipse, the moon casts its umbra upon Earth's surface; that shadow can sweep a third of the way around the planet in just a few hours.

Those who are fortunate enough to be positioned in the direct path of the umbra will see the sun's disk diminish into a crescent as the moon's dark shadow rushes toward them across the landscape. During the brief period of totality, when the sun is completely covered, the beautiful corona — the tenuous outer atmosphere of the sun — is revealed.

Totality may last as long as 7 minutes 31 seconds, though most total eclipses are usually much shorter. A partial solar eclipse occurs when only the penumbra the partial shadow passes over you. In these cases, a part of the sun always remains in view during the eclipse. How much of the sun remains in view depends on the specific circumstances. Usually the penumbra gives just a glancing blow to our planet over the polar regions; in such cases, places far away from the poles but still within the zone of the penumbra might not see much more than a small scallop of the sun hidden by the moon.

In a different scenario, those who are positioned within a couple of thousand miles of the path of a total eclipse will see a partial eclipse. The closer you are to the path of totality, the greater the solar obscuration. If, for instance, you are positioned just outside of the path of the total eclipse, you will see the sun wane to a narrow crescent, then thicken up again as the shadow passes by. An annular eclipse, though a rare and amazing sight, is far different from a total one.

The sky will darken The annular eclipse is a subspecies of a partial eclipse, not total. The maximum duration for an annular eclipse is 12 minutes 30 seconds. However, an annular solar eclipse is similar to a total eclipse in that the moon appears to pass centrally across the sun.

The difference is, the moon is too small to cover the disk of the sun completely. Because the moon circles Earth in an elliptical orbit, its distance from Earth can vary from , miles to , miles. But the dark shadow cone of the moon's umbra can extend out for no longer than , miles; that's less than the moon's average distance from Earth.

So if the moon is at some greater distance, the tip of the umbra does not reach Earth. During such an eclipse, the antumbra , a theoretical continuation of the umbra, reaches the ground, and anyone situated within it can look up past either side of the umbra and see an annulus, or "ring of fire" around the moon.

A good analogy is putting a penny atop a nickel, the penny being the moon, the nickel being the sun. These are also called annular-total "A-T" eclipses. This special type of eclipse occurs when the moon's distance is near its limit for the umbra to reach Earth. In most cases, an A-T eclipse starts as an annular eclipse because the tip of the umbra falls just short of making contact with Earth; then it becomes total, because the roundness of the planet reaches up and intercepts the shadow tip near the middle of the path, then finally it returns to annular toward the end of the path.

Because the moon appears to pass directly in front of the sun, total, annular and hybrid eclipses are also called "central" eclipses to distinguish them from eclipses that are merely partial.

Eclipses do not happen at every new moon, of course. This is because the moon's orbit is tilted just over 5 degrees relative to Earth's orbit around the sun. For this reason, the moon's shadow usually passes either above or below Earth, so a solar eclipse doesn't occur. But as a rule, at least twice each year and sometimes as many as five times in a year , a new moon will align itself in just such a way to eclipse the sun.

That alignment point is called a node. Depending on how closely the new moon approaches a node will determine whether a particular eclipse is central or partial. Western Kentucky University. Apply Visit More Info. The Great American Eclipse took place in August This is an archived website. The point closest to Earth is called the perigee and the side farthest from Earth is known as the apogee. Earth's orbit around the Sun is also elliptical, with the Sun closest at perihelion , and farthest away at aphelion.

It also means that from Earth, the Sun's and Moon's apparent sizes change during the year. When the Moon is about times closer to Earth than the Sun, the Moon's and the Sun's apparent sizes roughly match. Because of this, total eclipses of the Sun can only occur when the Moon is near perigee—it is the only time when the disk of the Moon looks big enough to cover the entire disk of the Sun.

What if the Moon is near apogee? A total solar eclipse can last for several hours and totality can range from a few seconds to 7. The longest total solar eclipse of the 21st century took place on July 22, , when totality lasted 6 minutes and 39 seconds! More details about upcoming Eclipses.

Topics: Astronomy , Eclipses , Moon , Sun. Sign in.