A solar eclipse is when the Moon lines up between Earth and the Sun such that the Moon either partially or completely blocks out the Sun.
Eclipses occur about 2-3 times a year, but only part of the world gets to see it in-person. The next Annular Solar Eclipse will be visible in parts of the United States, Mexico, and several Central American and South American countries on October 14, 2023 at 15:03 UTC. Stay tuned for details! In the meantime, check out some of the recent eclipses…
Photo Credits: Fred Espenak (L) / Stephan Heinsius (R)
IT’S ALL ABOUT THE MOON
While the sun is the main focus of a solar eclipse, our moon plays the most crucial role in creating this unique event.
This video tutorial explains what happens during a total solar eclipse and a partial eclipse and how often they both occur. It also explains how a solar eclipse differs from a lunar eclipse, and gives a helpful tip on how to remember the difference. In addition, the video examines how the two parts of the moon’s shadow, the umbra and penumbra, affect how we see an eclipse on the Earth, and illustrates the surprising true shape of the umbra. The video concludes by highlighting how data from NASA’s Lunar Reconnaissance Orbiter has helped us better map a solar eclipse’s path of totality. Visualizations included in this piece showcase the August 21, 2017 total solar eclipse happening in the United States.
This video explains how our moon creates a solar eclipse, why it’s such a rare event to see, and how data from NASA’s Lunar Reconnaissance Orbiter has enhanced our ability to map an eclipse’s path of totality.Credit: NASA, Music Provided By Killer Tracks: “Bring Me Up” – Kampe Wikstrom
ECLIPSE & TRANSIT FACTS
- A solar eclipse occurs when the moon passes between the Sun and the Earth, and the moon fully or partially blocks the Sun as viewed from a location on Earth.
- The longest duration for a total solar eclipse is 7.5 minutes.
- The shortest total solar eclipse in the 21st Century will be 1:06 on May 31, 2068, visible in New Zealand and Australia.
- Eclipse shadows travel at 1,100 miles per hour at the equator and up to 5,000 miles per hour near the poles.
- The maximum number of solar eclipses (partial, annular, or total) is 5 per year.
- A total eclipse can only happen during a new moon.
- The shortest total lunar eclipse in recorded history was in 1529 and lasted only 1 minute and 41 seconds.
- Nearly identical eclipses (total, annual, or partial) occur after 18 years and 11 days, or every 6,585.32 days (Saros Cycle).
- A total solar eclipse is not noticeable until the Sun is more than 90 percent covered by the Moon. At 99 percent coverage, daytime lighting resembles local twilight.
- The width of the Moon’s shadow is at most 170 miles wide.
- There are at least 2 solar eclipses per year somewhere on the Earth. However, since the Earth is mostly water, and weather (or a single cloud) can block your view, it is still a rare event—especially to see a total solar eclipse.
- Total solar eclipses happen about once every year or two.
- The Sun’s corona (“crown”) can ONLY be seen from the Earth’s surface during a total eclipse.
- One can see the corona or atmosphere of the Sun safely with naked eyes only during a total solar eclipse.
- Gemini 12 witnessed a total solar eclipse in 1966 and the International Space Station, in 2006.
- The alignment of Sun, Venus, and Earth comes in pairs that are eight years apart but separated by over a century.
- There will be 36 solar eclipses from 2001-2025, of which 15 will be total eclipses on some part of Earth’s surface – a little less than the average of one a year.
- Transits and eclipses are rare celestial events but the Transit of Venus is the rarest.
- A transit of Venus occurs when Venus passes directly between the Sun and the Earth.
- The most recent pair was in June 2004 and June 2012.
- The last transit of Venus pair before 2012 happened in December 1874 and December 1882.
- After 2012, subsequent Transit of Venus pairs will be in December 2117 and December 2125.
- Transits of Venus allow astronomers to calculate more accurately the distance of Venus from the Sun, and subsequently the distances of other planets.
- The Hubble Space Telescope will be aimed at the moon to detect dips in brightness during the 2012 transit of Venus.
- The Solar Dynamic Observatory captured the Sun and Venus during the 2012 transit in unprecedented detail.
Annular Solar Eclipses
An annular eclipse happens when the moon is farthest from Earth.
Because the moon is farther away from Earth, it seems smaller and does not block the entire view of the sun.
Photo Credit: Stefan Seip
Partial Solar Eclipses
When the Sun is completely blocked out we called it a total solar eclipse, and often this is what people think of with an eclipse. But a partial eclipse can be just as exciting.
When the Moon comes just shy of completely blocking out the Sun a bright ring or annulus is visible.
This is a special kind of partial eclipse, an annular eclipse.
This composite image of seven pictures shows the progression of a partial solar eclipse near from Ross Lake, Northern Cascades National Park, Washington on Monday, Aug. 21, 2017. The second to the last frame shows the International Space Station, with a crew of six onboard, in silhouette as it transits the Sun at roughly five miles per second. A total solar eclipse swept across a narrow portion of the contiguous United States from Lincoln Beach, Oregon to Charleston, South Carolina. A partial solar eclipse was visible across the entire North American continent along with parts of South America, Africa, and Europe. Photo Credit: (NASA/Bill Ingalls)
During a lunar eclipse, Earth gets in the way of the sun’s light hitting the moon. That means that during the night, a full moon fades away as Earth’s shadow covers it up.
The moon can also look reddish because Earth’s atmosphere absorbs the other colors while it bends some sunlight toward the moon. Sunlight bending through the atmosphere and absorbing other colors is also why sunsets are orange and red. During a total lunar eclipse, the moon is shining from all the sunrises and sunsets occurring on Earth!
NASA TV provided coverage of Super Blue Moon Lunar Eclipse on Jan. 31. The full moon was the third in a series of “supermoons,” when the Moon is closer to Earth in its orbit — known as perigee — and about 14 percent brighter than usual. It was also the second full moon of the month, commonly known as a “blue moon.” As the super blue moon passed through Earth’s shadow, viewers in some locations experienced a total lunar eclipse. While in Earth’s shadow, the moon also took on a reddish tint – which is sometimes referred to as a “blood moon.” Credit: NASA
ECLIPSES HELP US STUDY THE SUN
Studying the Sun during total solar eclipses helps scientists understand the source and behavior of solar radiation that drives space weather near Earth, which can affect the health of astronauts in space and the durability of materials used to build spacecraft.
Similar data will be important in planning NASA’s return of astronauts to the Moon in 2024 and eventual crewed missions to Mars.
Eclipses also set the stage for historic science.
NASA took advantage of the Aug. 21, 2017 eclipse by funding 11 ground-based scientific studies. As our scientists prepare their experiments for next week, we’re looking back to an historic 1860 total solar eclipse, which many think gave humanity our first glimpse of solar storms — called coronal mass ejections — 100 years before scientists first understood what they were.
Scientists observed these eruptions in the 1970s during the beginning of the modern satellite era, when satellites in space were able to capture thousands of images of solar activity that had never been seen before. But in hindsight, scientists realized their satellite images might not be the first record of these solar storms. Hand-drawn records of an 1860 total solar eclipse bore surprising resemblance to these groundbreaking satellite images.
CREDITS: NASA’s Goddard Space Flight Center • Music credits: ‘Electricity Wave’ by Jean-François Berger [SACEM] and ‘Solar Winds’ by Ben Niblett [PRS], Jon Cotton [PRS]
|Calendar Date||Type ||Geographic Region of Eclipse Visibility |
|2021 May 26||Total Lunar||e Asia, Australia, Pacific, Americas|
|2021 Jun 10||Annular Solar||n North America, Europe, Asia
[Annular: n Canada, Greenland, Russia]
|2021 Nov 19||Partial Lunar||Americas, n Europe, e Asia, Australia, Pacific|
|2021 Dec 04||Total Solar||Antarctica, South Africa, s Atlantic
|2022 Apr 30||Partial Solar||se Pacific, s South America|
|2022 May 16||Total Lunar||Americas, Europe, Africa|
|2022 Oct 25||Partial Solar||Europe, ne Africa, Mid East, w Asia|
|2022 Nov 08||Total Lunar||Asia, Australia, Pacific, Americas|
|2023 Apr 20||Hybrid Solar||se Asia, East Indies, Australia, Philippines, New Zealand
[Hybrid: Indonesia, Australia, Papua New Guinea]
|2023 May 05||Penumbral Lunar||Africa, Asia, Australia|
|2023 Oct 14||Annular Solar||North America, Central America, South America
[Annular: w US, Central America, Colombia, Brazil]
|2023 Oct 28||Partial Lunar||e Americas, Europe, Africa, Asia, Australia|
|2024 Mar 25||Penumbral Lunar||Americas|
|2024 Apr 08||Total Solar||North America, Central America
[Total: Mexico, c US, e Canada]
|2024 Sep 18||Partial Lunar||Americas, Europe, Africa|
|2024 Oct 02||Annular Solar||Pacific, s South America
[Annular: s Chile, s Argentina]
|2025 Mar 14||Total Lunar||Pacific, Americas, w Europe, w Africa|
|2025 Mar 29||Partial Solar||nw Africa, Europe, n Russia|
|2025 Sep 07||Total Lunar||Europe, Africa, Asia, Australia|
|2025 Sep 21||Partial Solar||s Pacific, New Zealand, Antarctica|
|2026 Feb 17||Annular Solar||s Argentina & Chile, s Africa, Antarctica
|2026 Mar 03||Total Lunar||e Asia, Australia, Pacific, Americas|
|2026 Aug 12||Total Solar||n North America, w Africa, Europe
[Total: Arctic, Greenland, Iceland, Spain]
|2026 Aug 28||Partial Lunar||e Pacific, Americas, Europe, Africa|
-  Hybrid eclipses are also known as annular/total eclipses. Such an eclipse is both total and annular along different sections of its umbral path.
-  “Geographic Region of Eclipse Visibility” is the portion of Earth’s surface where a partial eclipse can be seen. The central path of a total or annular eclipse covers a much smaller region of Earth and is described in brackets .