A solar eclipse occurs when the Earth, moon and sun are all in the same plane and the moon completely covers the sun.
Regardless of how much of the sun gets covered by the moon's shadow, you should never look directly at a solar eclipse.
During this time, one must use protective equipment to view the sun, according to William Teets, director of the Vanderbilt Dyer Observatory. That could include glasses, telescopes, binoculars, or a projection method.
Solar eclipses can be total, partial, and hybrid.
The solar eclipse is a happy accident of nature. According to NASA, the sun is 400 times bigger than the moon, which is just over 3,500 km in diameter. The moon is about 400 times closer to Earth than the sun is, and this is due to the fact that the sun and moon are elliptical. On average, a total solar eclipse is visible somewhere on Earth every 18 months.
The moon casts two types of shadows during a solar eclipse. The dark part of the shadow is called the umbra. The umbra is shaped like a cone. It is surrounded by the penumbra, a shadow that partially obscures sunlight.
You need to be located in the direct path of the umbra, which can sweep a third of the way around the planet in just a few hours, in order to view a total solar eclipse. The sun's disk would diminish into a crescent as the moon's dark shadow moved across the landscape.
Don't look directly at the sun.
If you look directly at the sun, even if it is partially covered by the moon, it can cause serious eye damage or blindness. Don't look at a partial solar eclipse if you don't have proper eye protection.
The corona is revealed when the sun is completely covered. A solar eclipse usually lasts for a few minutes, according to a NASA solar astronomer. According to NASA, the longest solar eclipse on June 15, 743 B.C., lasted 7 minutes and 28 seconds.
When the sun is completely obscured by the moon, total eclipses are rare because they are only visible along a narrow path on Earth.
The next solar eclipse will take place on April 30, 2022, and will be visible in South/West South America, the Atlantic and Pacific Ocean, and parts of Antarctica.
The next total solar eclipse will be visible in South/East Asia, Australia, the Pacific and Indian Ocean, and Antarctica, where viewers can see at least a partial sun covering. The Great North American Eclipse will occur on April 8, 2024. Timeanddate.com reported that the path of totality will go through Mexico, the U.S., and Canada.
During a partial solar eclipse, the moon passes between the Earth and the sun. During the eclipse, a part of the sun remains in view. Depending on the circumstances, how much of the sun remains in view depends.
Sometimes the penumbra gives a glancing blow to the planet over the polar regions, but in other 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. A partial solar eclipse can be seen if you are positioned within a couple thousand miles of the path of the total eclipse.
The closer you are to the path of totality, the greater the solar obscuration. If you are positioned outside of the path of the eclipse, you will be able to see the sun diminish to a narrow crescent as the shadow passes by.
A total eclipse is not the same as an annular eclipse. Since so much of the sun still shows, the sky will be dark. A partial not total eclipse is called the annular eclipse. There is a maximum duration for an eclipse.
The next solar eclipse will take place on October 14, 2023. Millions of people will be able to see the eclipse in parts of the US, Mexico, and South America.
A solar eclipse is similar to a total eclipse in that the moon passes across the sun. The difference is due to the moon's position, which causes it to be too small to cover the disk of the sun completely. The moon's distance from Earth can be as much as 356,400 miles. The dark shadow cone of the moon is less than the average distance from Earth.
The tip of the umbra does not reach Earth if the moon is at a greater distance. During an eclipse, the antumbra, a theoretical continuation of the umbra, reaches the ground, and anyone located within it can look up past either side of the umbra and see a ring of fire around the moon. A penny is the moon and a nickel is the sun.
These are called eclipses. This type of eclipse occurs when the moon is close to the umbra. 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.
Eclipses that are only partial are called partial eclipses, while eclipses that are total are called total eclipses.
Only 5% of solar eclipses are hybrid. On April 20, 2023, there will be a total solar eclipse in some areas.
Date | Type of solar eclipse | Visibility |
---|---|---|
April 30, 2022 | Partial | Southeast Pacific, South America |
Oct. 25, 2022 | Partial | Europe, parts of Africa, Middle East, parts of Asia |
April 20, 2023 | Total | South/East Asia, Australia, Pacific, Indian Ocean, Antarctica |
Oct. 14, 2023 | Annular | Parts of Africa, N. America, S. America, Pacific & Atlantic, and Arctic |
April 18, 2024 | Total | Totality: Parts of Mexico, U.S. and Canada |
Oct. 2, 2024 | Annular | Parts of South America, Pacific & Atlantic, and Antarctica |
Do not look directly at the sun without protective equipment.
This equipment could be approved for solar eclipse glasses or a properly filter telescope or pair of binoculars.
The skywatcher should never put on solar eclipse glasses and use them to look through a telescope or pair of binoculars, as the light from the eclipse will burn through the glasses and blinding you as well.
You can also use a projection method to view a solar eclipse, if you choose to. To project the image onto a sheet of paper, you need to remove the eyepiece from the telescope. According to Sky and Telescope, you can find the spot with the most focused image by moving the sheet of paper back and forth.
Sky and Telescope states that a pinhole camera is used to create an image of the sun on a screen that is about 1 meter behind the opening. A magnified image of the sun can be projected onto a white card using a small telescope or binoculars. The larger the image, the closer it is to the card. Look for sun spots. The sun appears to be a bit darker around the edge. If you remember not to look through the binoculars or telescope when they are pointed toward the sun, this method of solar viewing is safe.
The pinhole mirror is a variation on the pinhole theme and is a pocket mirror that has a quarter-inch hole punched in it. If you want to see a disk of light on the far wall inside, place the covered mirror on the sunlit sill. The disk of light is a representation of the sun. Sky and Telescope states that the image will be 1 inch across for every 9 feet or 3 centimeters from the mirror. The mirror can be held in place by modeling clay. Try different holes in the paper. A large hole makes the image bright, but fuzzy, and a small hole makes it dim. The room should be dark as much as possible. To make sure the mirror is good enough to project a clean, round image, be sure to try this out before you buy it. Don't let anyone look at the sun in the mirror.
The shadow cast by leafy trees during the partial phases can be seen. What do you see? Is it worth taking a picture of? You can see the suns through the gaps between the leaves. Diffusion is a property of light. The light rays do not shoot straight by the rim of the gaps, but bend around the edge, according to an optical physicist at the NASA Marshall Space Flight Center. The wave effect creates rings that look like a bull's eye.
Aluminized Mylar is one of the acceptable filters for visual solar observations. Mylar filters are specially designed for solar observing. shade 14 arcs-welder's glass is available for a few dollars at welding supply shops. It is always a good idea to test your observing techniques before the eclipse.
Unacceptable filters include sunglasses, old color film negatives, black-and-white film that contains no silver, photographic neutral-density filters and polarizing filters. These materials have very low visible-light transmittance levels, but they transmit an unacceptably high level of near-infrared radiation that can burn your retinas. The fact that the sun appears dim or that you don't mind looking at the sun through these types of filters is not a guarantee that your eyes are safe.
Sunspots are patches of the sun that are relatively cool. They will look like black spots on the sun's disk. The spots are too small to see through your solar eclipse glasses.
You might catch a glimpse of more than sunspots if you use ahydrogen-alpha solar telescope. The second layer of the sun's atmosphere is called the chromoosphere, and you should be able to see it with this gear.
There are clouds of material lofted up from the sun, and they sometimes look like flames on the edge of the sun.
You could see what might be gems dancing around the outer disk of the sun with that same specialized telescope. The lower atmosphere of the sun is about a million times less dense than the atmosphere on Earth, according to the University Corporation for Atmospheric Research. UCAR said that the light from this atmospheric layer is drowned out by the brighter photoosphere underneath it.
There is a time when you can look directly at the sun during a total eclipse. During those few seconds or minutes, the outer atmosphere that lies just above the chromoosphere shines in all its glory like a halo around the sun.
It is different in size and pattern from eclipse to eclipse. It is faint and delicate, with a sheen like a pale Aurora. Sometimes the corona appears as a soft continuous structure; at other times, long rays of it shoot out in three or four directions. The corona can be seen in the streamers and filmy petals. When the sun begins to emerge into view again, the corona disappears and you need to protect your eyes again.
There are a lot of sun and solar eclipse resources at UCAR.
If you want to take a photo of an eclipse, this guide will show you how to do it.
Some of the oldest records of solar eclipses can be found in this NASA resource.