This means that, as seen from Earth, the Moon’s diameter is 95.2 percent as large as the Sun’s diameter. The shadow will have stayed on Earth’s surface for 5 hours 51 minutes 29 seconds. EDT, about 220 miles (350 km) northeast of the Brazilian capital of Brasília. The last remnants of the Moon’s shadow disappear into the night over northeastern Brazil at 4:55 p.m. EDT in the Caribbean Sea, 60 miles (97 km) from the coast of Nicaragua. EDT about 360 miles (580 km) off the coast of Brazil. The annular part of the eclipse begins at 12:10 p.m. That happens nearly 970 miles (1,560 kilometers) south of Ketchikan, Alaska, in the North Pacific Ocean. The eclipse starts when the Moon’s penumbra (its lighter, outer shadow where a partial eclipse occurs) touches Earth at 11:04 a.m. The shot was taken from Monument Valley, Utah. For each of the 1/250-second shots in this composite, the imager used a Nikon D300 DSLR and 400mm Nikon lens at f/8 with a 2x extender, giving an effective focal length of 600mm. This means over your eyes, your camera, and your binoculars or telescope - NO EXCEPTIONS! Photographers produced many different images of the May 2012 annular eclipse.
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Please note that because part of our star’s surface is always visible, you must use an approved solar filter (one that meets the ISO 12312–2 international safety standard) during the entire eclipse.
Anyone within the path will see a ring of the Sun’s surface surrounding the darkened Moon. So, only the antumbra, where the Moon appears completely within the disk of the Sun, touches the surface of Earth.
In this case, however, either the Sun is too close or the Moon is too far from Earth for the Moon to completely cover the solar disk. Like during a total eclipse, an annular eclipse occurs when the Sun, the Moon, and Earth line up. The number seeing the main part of the eclipse is low because only two big cities, Albuquerque and San Antonio, lie in the path. Several hundred million more will see a partial eclipse, weather permitting. In the U.S., approximately 6.6 million people lie in the path of annularity. Afterward, it will touch nine additional countries: Mexico, Belize, Guatemala, Honduras, Nicaragua, Costa Rica, Panama, Colombia, and Brazil. 14, an annular eclipse will cross the western U.S. “We’ve already started planning here at the Michigan Science Center for that one,” Epstein says.The photographer combined 30 images of Horseshoe Bend in the Glen Canyon National Recreation Area with 18 images of the Sun to produce this stunning composite of the May 20, 2012, annular eclipse. The moon will obscure 99% of the sun over the rest of metro Detroit. Toledo, Cleveland and Sandusky, Ohio will be in the path of totality, along with Leamington and Point Pelee, Ontario. The next total solar eclipse visible from Michigan will occur on April 8, 2024, but it will touch only a very small corner of Monroe County. “We’ll only be able to see just a little bit of it here in Detroit as the sun is rising, but it’ll still be pretty cool,” she says. Epstein says the visible part of the sun will look like a “ring of fire.” The moon will pass in front of the sun, but will not totally obscure it. While much of North America will experience a partial solar eclipse, a portion of Canada and the Arctic will be treated to an annular eclipse.
“If anybody has those solar eclipse glasses left over from 2017, make sure the expiration date has not passed,” she says. Epstein says eyewear designed specifically for solar eclipses might also be OK. Obviously, no one should ever look directly into the sun - especially during an eclipse - without adequate eye protection, such as level 14 welding glass.
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