The partial eclipse looks as if a bite has been taken out of the Sun. The annular looks like an orange ring around the blackened Moon. The total looks like wisps of white around the blackened Moon.

Get ready for the April 2024 total solar eclipse. Learn about the science behind solar eclipses, how to watch safely, and how to engage students in NASA science.


On April 8, 2024, a total solar eclipse will be visible across much of the central and northeastern United States, as well as parts of Mexico and Canada.

Whether you are traveling to the path of the total eclipse or will be able to step outside and watch the eclipse where you live, here's everything you need to know, including what to expect, how to watch safely, and how to engage in scientific observations and discovery with NASA.

What Are Solar Eclipses?

Solar eclipses occur when the Sun, the Moon, and Earth align. For this alignment to happen, two things need to be true. First, the Moon needs to be in the new moon phase, which is when the Moon’s orbit brings it between Earth and the Sun. Second, eclipses can only happen during eclipse seasons, which last about 34 days and occur just shy of every six months. An eclipse season is the time period when the Sun, the Moon, and Earth can line up on the same plane as Earth's orbit during a new or full moon. If a new moon happens during an eclipse season, the shadow cast by the Moon will land on Earth, resulting in a solar eclipse. Most of the time, because the Moon’s orbit is slightly tilted, the Moon’s shadow falls above or below Earth, and we don't get a solar eclipse.

Not all solar eclipses look the same. The distance between the Sun, the Moon, and Earth plays an important role in what we see during a solar eclipse. Even though the Moon is much smaller than the Sun (about 400 times smaller in diameter), the Sun and Moon look about the same size from Earth. This is because the Sun is about 400 times farther away than the Moon. But as the Moon travels its elliptical orbit around Earth, its size appears slightly larger when it is closer to Earth and slightly smaller when it is farther from Earth. This contributes to the different kinds of solar eclipses you might have heard about. For example:

  • During a total solar eclipse, the Moon is closer to Earth in its orbit and appears larger, completely blocking the Sun's disk. This allows viewers in the path of totality to see the Sun’s corona, which is usually obscured by the bright light of the Sun’s surface.
  • Whisps of white haze flare out around the blackened disk of the Moon, which completely covers the Sun's disk

    This image of a total solar eclipse was captured on Aug. 21, 2017 from Madras, Oregon. Image credit: NASA/Aubrey Gemignani | › Full image and caption

  • An annular solar eclipse occurs when the Sun, Moon, and Earth are properly aligned, but the Moon is farther away in its orbit, so it does not completely cover the Sun's disk from our perspective. Annular eclipses are notable for the "ring of fire," a thin ring of the Sun’s disk that's still visible around the Moon during annularity. The name annular eclipse comes from the world of mathematics, where a ring shape is known as an annulus.
  • The bubbling surface of the Sun's disk and the surrounding haze of orange and yellow light can be seen as a ring around the blackened disk of the Moon.

    On Jan. 4, 2017, the Hinode satellite captured these breathtaking images of an annular solar eclipse. Image credit: Hinode/XRT | › Full image and caption

  • Partial eclipses can happen for two reasons. First, viewers outside the path of totality during a total solar eclipse – or the path of annularity during an annular eclipse – will see only part of the Sun’s surface covered by the Moon. The other time a partial eclipse can occur is when the Moon is nearly above or below Earth in its orbit so only part of the Moon’s shadow falls on Earth. In this case, only part of the Sun’s surface will appear covered by the Moon.
  • The Sun appears to have a small bite taken out of the top of its yellow-orange disk. The bite grows in size in this sequence of three images.

    The Sun appears partially eclipsed in this series of photos taken from NASA’s Johnson Space Center in Houston on Aug. 21, 2017. Image credit: NASA/Noah Moran | › Full image and caption

How to Watch the Upcoming Solar Eclipse

First, an important safety note: Do not look directly at the Sun or view any part of the partial solar eclipse without certified eclipse glasses or a solar filter. Read more below about when you can safely view the total solar eclipse without eclipse glasses or a solar filter. Visit the NASA Eclipse website for more information on safe eclipse viewing.

When following proper safety guidelines, witnessing an eclipse is an unparalleled experience. Many “eclipse chasers” have been known to travel the world to see solar eclipses. Here's what to expect on April 8, 2024:

Map of where the October 14 annular eclipse will be visible. Refer to caption for list of locations.

The April 8 total solar eclipse will be visible across much of the central and northeastern United States, as well as Mexico and Canada. Meanwhile, viewers in all of the continental United States, Hawaii, Mexico, Central America, Greenland, Iceland, Ireland, Cook Islands, French Polynesia, the Azores, and parts of Alaska and the United Kingdom will be able to see a partial eclipse. (Note that in some areas, the eclipse will begin before sunrise or end after sunset). | › Full image and caption

The start time and visibility of the eclipse will depend on your location. You can use this map to find detailed eclipse information, including the start time, by clicking on your location.

The eclipse begins when the edge of the Moon first crosses in front of the disk of the Sun. This is called a partial eclipse and might look as if a bite has been taken out of the Sun.

It is important to keep your eclipse glasses on during all parts of the partial solar eclipse. The visible part of the Sun is tens of thousands of times brighter than what you see during totality. You can also use a pinhole camera to view the eclipse.

An approximately 115-mile-wide strip known as the path of totality is where the shadow of the Moon, or umbra, will fall on Earth. Inside this path, totality will be visible starting about 65 to 75 minutes after the eclipse begins.

If you are in the path of totality, it is safe to take off your eclipse glasses and look at the total eclipse only during totality. Be sure to put your glasses back on before the total phase ends and the surface of the Sun becomes visible again. Your viewing location during the eclipse will determine how long you can see the eclipse in totality. In the U.S., viewers can expect to see 3.5 to 5.5 minutes of totality.

After totality ends, a partial eclipse will continue for 60 to 80 minutes, ending when the edge of the Moon moves off of the disk of the Sun.

For more information about the start of the partial eclipse, the start and duration of totality, and the percentage of the Sun eclipsed outside the path of totality, find your location on this eclipse map.

On April 8, NASA Television will host a live broadcast featuring views from telescopes along the path of totality.

What Solar Eclipses Mean for Science

Solar eclipses provide a unique opportunity for scientists to study the Sun and Earth from land, air, and space, plus allow the public to engage in citizen science!

A solid red circle with a smaller white-outlined circle inside it is centered over the disk of the Sun. Streams of yellow, red, and orange shoot out from the Sun, all around the solid circle, while a large solar flare bursts out of the upper left portion of the circle. A time stamp in the corner reads 2000/02/27.

NASA’s Solar and Heliospheric Observatory, or SOHO, constantly observes the outer regions of the Sun’s corona using a coronagraph. Image credit: ESA/NASA/SOHO | + Expand image

Scientists measure incoming solar radiation, also known as insolation, to better understand Earth’s radiation budget – the energy emitted, reflected, and absorbed by our planet. Just as clouds block sunlight and reduce insolation, eclipses create a similar phenomenon, providing a great opportunity to study how increased cloud cover can impact weather and climate.

Solar eclipses can also help scientists study solar radiation in general and the structure of the Sun. On a typical day, the bright surface of the Sun, called the photosphere, is the only part of the Sun we can see. During a total solar eclipse, the photosphere is completely blocked by the Moon, leaving the outer atmosphere of the Sun (corona) and the thin lower atmosphere (chromosphere) visible. Studying these regions of the Sun’s atmosphere can help scientists understand solar radiation, why the corona is hotter than the photosphere, and the process by which the Sun sends a steady stream of material and radiation into space. Annular solar eclipses provide opportunities for scientists to practice their observation methods so that they'll be ready when a total solar eclipse comes around.

Citizen scientists can get involved in collecting data and participating in the scientific process during the eclipse through NASA’s GLOBE program. Anyone in the path of the eclipse and in partial eclipse areas can act as citizen scientists by measuring temperature and cloud cover data and report it using the GLOBE Observer app to help further the study of how eclipses affect Earth’s atmosphere.

Visit NASA's Eclipse Science page to learn more about the many ways scientists are using the eclipse to improve their understanding of Earth, the Moon, and the Sun.

Taking Eclipse Science Farther

Eclipses also make a great jumping-off point to concepts and techniques used in astrophysics and our search for planets beyond our solar system.

Similar to a solar eclipse, a transit occurs when a planet crosses in front of the face of a star. From Earth, the planets Venus and Mercury can occasionally be seen transiting in front of the Sun, appearing as small, dark dots. Transits are also useful for detecting exoplanets – distant planets around other stars. When an exoplanet passes in between its star and Earth, we can measure tiny dips in the star's brightness that tell scientists a planet is there even when it’s too small to see.

Another way that eclipse concepts are used for astrophysics is with coronagraphs, mechanisms inside telescopes that block the light from a star. By creating a sort of artificial eclipse, coronagraphs help scientists search for exoplanets by making much dimmer planets orbiting a star easier to see. For example, NASA’s Nancy Grace Roman Telescope, slated for launch later this decade, will use an advanced coronagraph to analyze and directly image planets that orbit other stars. Learn more about the astrophysics involved in eclipses, including the use of gravitational lensing to study background objects, from NASA’s Universe of Learning.

Learn how the coronagraph instrument on the Nancy Grace Roman Telescope will allow the spacecraft to peer at the universe through some of the most sophisticated sunglasses ever designed. | Watch on YouTube

Solar Eclipse Lessons and Projects

Use these standards-aligned lessons, plus related activities and resources, to get your students excited about the eclipse and the science that will be conducted during the eclipse.

Explore More

Eclipse Info

Eclipse Safety

Interactives

Citizen Science

Facts & Figures


NASA's Universe of Learning materials are based upon work supported by NASA under award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and the Jet Propulsion Laboratory.

TAGS: Solar Eclipse, Eclipse, Annular Eclipse, K-12 Education, Lessons, Classroom Resources, STEM Resources

  • Lyle Tavernier
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Update – Sept. 20, 2017: Due to the number of requests we have received, this bulletin board registration is now closed. In the event more materials become available, an update will be posted here. All materials are also available to download at the links below. 


This year has been full of exciting discoveries at NASA as we learn more about our solar system as well as star systems light years away.

Want a cool way to share these missions and discoveries with your classroom? Sign up online to receive the latest classroom bulletin board set from the Educator Resource Center at NASA’s Jet Propulsion Laboratory.

Note:

  • Bulletin board mailers are limited to teachers at U.S.-based institutions.
  • Available while supplies last.
  • Requests will be fulfilled in the order they are received.

Here’s what’s included:


Exoplanet Space Tourism Posters

Exoplanet Space Tourism Posters

NASA’s Kepler space telescope, which has already discovered more than 1,000 planets beyond our solar system, continues to identify more and more of these so-called exoplanets – some of which have features similar to Earth. (Learn more about these worlds on NASA's Exoplanet Exploration website.) This popular poster set imagines what life would be like on these distant worlds.

Note: The bulletin board materials will include a small sample of the full set, which can be downloaded here.


Reading, Writing and Rings Activities

Reading, Writing and Rings

Closer to home, September 15 will mark the end of the Cassini mission, which has spent nearly 13 years orbiting the ringed giant Saturn. Images and science from Cassini have shaped our understanding of Saturn and its mysterious moons, and continue to provide wonder to students. This collection of activities will get students using reading and writing to explore the Cassini mission’s science at Saturn.

Find out more about the Cassini mission and its Grand Finale on Sept. 15, 2017.


Saturn Postcards

Saturn Postcards

Take in some of Cassini’s best views of Saturn with these NASA postcards featuring images from the mission!

Explore more images from the Cassini mission at Saturn.


Visit our educator resources page for more downloads and online resources.

TAGS: materials, educator resources, educator resource center, classroom resources, bulletin board, teaching materials

  • NASA/JPL Edu
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