Rick Fienberg, Project Manager, Solar Eclipse Task Force, American Astronomical Society
+1 857-891-5649, [email protected]

Diana Hannikainen, Observing Editor, Sky & Telescope
+1 617-500-6793 ×22100, [email protected]

Susanna Kohler, Communications Manager and Press Officer, American Astronomical Society
+1 202-328-2010 ×127, [email protected]

Note to Editors/Producers: This release is accompanied by high-quality graphics; see the end of this release for the images and links to download.

One year from now, on Monday, April 8, 2024, the Moon will pass directly between Earth and the Sun, creating a total solar eclipse like the one that crossed the United States from coast to coast on August 21, 2017. As it did that day, the new Moon will fully block the Sun’s bright face, turning day into night for several minutes and revealing the magnificent solar corona, our star’s wispy outer atmosphere. Our natural satellite’s dark shadow, about 115 miles wide, will cross Mexico, sweep from Texas to Maine, and then darken parts of Eastern Canada. Outside this narrow path, nearly everyone in North America will get a chance to witness a partial solar eclipse.

Remarkably, we’ll have had another major solar eclipse just six months earlier. But on Saturday, October 14, 2023, when the Moon is centered in front of the Sun, it will cover only 90% of the brilliant solar disk. The remaining 10% will appear as a blazing “ring of fire” around the Moon’s black silhouette. This annular (Latin for ring-shaped) solar eclipse will be visible within a roughly 125-mile-wide path from Oregon to Texas and on into Mexico, Central America, and northern South America. Again, most North Americans outside the path will experience a partial solar eclipse.

Where and How to See Them

From beginning to end, a solar eclipse lasts up to about 3 hours. For most of that time, the Moon slowly covers the Sun, then uncovers it; these are the eclipse’s beginning and ending partial phases. The real excitement comes in the middle, but only for those within the narrow path of the Moon’s dark shadow, and only for a few fleeting minutes.

April 8, 2024: The Moon’s shadow will pass over more big cities than in 2017 and give at least 30 million Americans a shot at seeing the solar corona without having to travel. But there’s a catch: In early April much of the country is still in winter’s grip. Clear skies are most likely across Mexico and Texas Hill Country, and these places also happen to be where totality — the brief total phase of the eclipse — lasts longest, nearly 4½ minutes. Many diehard eclipse enthusiasts have already made plans to visit Mexico or Texas next April.

October 14, 2023: Weather prospects for the annular eclipse look most promising in parts of Utah, New Mexico, and Texas, where the “ring of fire” lasts about 5 minutes. Sky & Telescope offers package tours to the best places to see both eclipses.

During partial and annular solar eclipses, the Sun remains dangerously bright at all times and must never be looked at directly except through special-purpose “eclipse glasses” or handheld viewers that meet the requirements of the ISO 12312-2 international standard. See our safety guidelines for advice on where to get safe solar filters and on indirect viewing methods. During totality you can safely view the eclipsed Sun without eye protection.

“If you can get yourself into the path of the Moon’s shadow for a total solar eclipse, it’s definitely worth the effort,” says Rick Fienberg, Project Manager of the American Astronomical Society (AAS) Solar Eclipse Task Force and Senior Contributing Editor of Sky & Telescope. “A 99% partial solar eclipse doesn’t get you 99% of the experience of a total solar eclipse — the last 1% is literally the difference between night and day. As the Moon blots out the thinning arc of the bright Sun in the final minute before totality, daylight fades by up to 1,000 times. And the solar corona surrounding the Moon’s velvety black silhouette is one of the most glorious sights in all of nature!”

During a total solar eclipse you’ll experience many other noteworthy phenomena, including a drop in air temperature, changes in wind speed and direction, bright planets and stars shining in deep twilight, ruby-red solar prominences (eruptions of hot gas protruding beyond the limb, or edge, of the Sun’s hidden disk), pastel sunrise/sunset colors around the horizon, and plants and animals behaving as if the Sun has set. Another total solar eclipse won’t cross the U.S. until August 12, 2045, so the April 2024 event is your best chance to catch totality for a generation.

Getting Organized

The AAS Solar Eclipse Task Force, partnering with the outreach team for NASA’s PUNCH (Polarimeter to UNify the Corona and Heliosphere) mission, is holding a hybrid (in-person + virtual) planning workshop Friday–Saturday, June 9–10, 2023, at the New Mexico Museum of Natural History & Science, 1801 Mountain Rd. NW, Albuquerque, NM 87104, on the heels of the AAS summer meeting in the same city.

This workshop is for everyone involved (or wanting to become involved) in preparing their community for the upcoming North American solar eclipses, whether on or off the eclipse path(s). Attendees will include amateur and professional astronomers; formal and informal educators; local, state, and national government officials; representatives from the tourism and hospitality industries; professionals in health, safety, transportation, and emergency management; local, state, and national park rangers; and artists, filmmakers, science writers, and event planners.

Links to essential eclipse resources for a wide variety of stakeholders can be found on the task force’s website and resources page.

Eclipse Geometry

We get solar eclipses because, by an amazing cosmic coincidence, the Sun and Moon appear almost exactly the same size in our sky. The Sun’s diameter is really about 400 times bigger than the Moon’s, but the Sun is also about 400 times farther away. Because Earth’s orbit around the Sun and the Moon’s orbit around Earth are both ellipses rather than circles, the apparent sizes of the Sun and Moon vary a little during the year (Sun) and during each month (Moon).

Our planet is closest to the Sun (perihelion) in early January and farthest (aphelion) in early July, and the Sun appears about 3% wider in January than in July — not that you’d notice. When the Moon is closest to Earth (perigee), its apparent diameter can be up to 14% larger than when it’s farthest (apogee); again, this effect is not too noticeable. When the Moon is closer than average and the Sun farther away than average, as will be the case on April 8, 2024, the Moon can easily cover the entire solar disk and unveil the ethereal corona. But when the opposite is true, as will happen on October 14, 2023, the Moon is too small to fully cover the Sun’s face, so at mideclipse a brilliant annulus (ring) of sunlight encircles the lunar silhouette.

You might wonder why we don’t have a solar eclipse at every new Moon. This is because the Moon’s orbit around Earth is tipped by about 5° to Earth’s orbit around the Sun (which, from our perspective, is the Sun’s annual path through the zodiacal constellations). At new Moon, our natural satellite usually passes above or below the Sun. But twice each year, currently in April and October, the new Moon does pass in front of the Sun, so we get solar eclipses — including one in Australia and Indonesia on April 20th this year. Whether a solar eclipse is partial, annular, or total depends on how precisely the Sun, Moon, and Earth align and on the distances of the Moon and Sun from Earth.

More Information

For more information about the October 2023 annular eclipse, see “Solar and Lunar Eclipses in 2023” on Sky & Telescope’s website. A thorough preview of the April 2024 total solar eclipse appears in the April 2023 issue of Sky & Telescope magazine, now on newsstands.

You can get local circumstances of upcoming solar (and lunar) eclipses for cities worldwide on’s Eclipses page.

Sky & Telescope is making the illustrations below available to editors and producers. Permission is granted for nonexclusive use in print and broadcast media, as long as appropriate credits (as noted) are included. Web publication must include a link to

April 2024 Total Solar Eclipse
Over the April 8, 2024, eclipse’s total duration of 3 hours 15 minutes, the Moon’s shadow travels along a 9,200-mile strip that extends from the Pacific Ocean, across North America, to the Atlantic Ocean. At the point of greatest eclipse totality lasts nearly 4½ minutes. Blue percentage lines refer to eclipse magnitude, the fraction of the Sun’s diameter covered by the Moon at maximum eclipse. Within the green path, that fraction exceeds 100%. Red lines indicate when maximum eclipse occurs in Universal Time, which is 4 hours ahead of Eastern Daylight Time (7 hours ahead of Pacific Daylight Time) in the United States. Click on the image or here for a larger version.
Sky & Telescope illustration; source: Fred Espenak
October 2023 Annular Eclipse

The October 14, 2023, annular solar eclipse can be witnessed in the United States along a narrow strip from Oregon through Texas. After that, the Moon’s shadow crosses the Yucatán Peninsula, Central America, Colombia, and Brazil. Annularity lasts longest, about 5¼ minutes, just off the coast of the Nicaragua–Costa Rica border. Blue percentage lines refer to eclipse magnitude, the fraction of the Sun’s diameter covered by the Moon at maximum eclipse. Within the green path, that fraction is about 95%. Red lines indicate when maximum eclipse occurs in Universal Time, which is 4 hours ahead of Eastern Daylight Time (7 hours ahead of Pacific Daylight Time) in the United States. Click on the image or here for a larger version.
Sky & Telescope illustration; source: Fred Espenak
Total Solar Eclipse Madras, Oregon
The total solar eclipse of August 21, 2017, as seen from Madras, Oregon. This is a composite of short, medium, and long exposures. No single exposure can capture the huge range of brightness exhibited by the solar corona, which is sculpted by the Sun’s magnetic field. Several red solar prominences (eruptions of glowing hydrogen gas) are visible, as are a couple of stars. No filter was used for the exposures, as totality is about as bright as the full Moon and just as safe to look at. At all other times, though, a safe solar filter is required to observe or photograph the Sun. Click on the image or here for a larger version.
Photo by Rick Fienberg, processing by Sean Walker; courtesy TravelQuest International and Sky & Telescope
The annular solar eclipse of May 10, 1994, as seen from Ogunquit, Maine. The sky appears black because the photograph was made through a safe solar filter, which blocks all but 1 part in 100,000 of the incident light. This photo and the one above, of a total solar eclipse, are at the same scale. Click on the image or here for a larger version.
Photo by Richard Tresch Fienberg; courtesy Sky & Telescope and the American Astronomical Society.

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The American Astronomical Society (AAS), established in 1899, is a major international organization of professional astronomers, astronomy educators, and amateur astronomers. Its membership of approximately 8,000 also includes physicists, geologists, engineers, and others whose interests lie within the broad spectrum of subjects now comprising the astronomical sciences. The mission of the AAS is to enhance and share humanity’s scientific understanding of the universe as a diverse and inclusive astronomical community, which it achieves through publishing, meetings, science advocacy, education and outreach, and training and professional development.


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