![<span class="mw-page-title-main">Solar eclipse of March 29, 2006</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/3/35/Diamondring-eclipse-March03-29-2006.jpg/320px-Diamondring-eclipse-March03-29-2006.jpg)
A total solar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, March 29, 2006, with a magnitude of 1.0515. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.1 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of August 1, 2008</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/6/6b/Corona.jpg/320px-Corona.jpg)
A total solar eclipse occurred at the Moon's descending node of orbit on Friday, August 1, 2008, with a magnitude of 1.0394. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.4 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of July 11, 1991</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/8/8b/Eclipse_CR_1991_a_zoom.jpg)
A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, July 11, 1991, with a magnitude of 1.08. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 8 hours after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of March 9, 2016</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ec/Total_Solar_Eclipse%2C_9_March_2016%2C_from_Balikpapan%2C_East_Kalimantan%2C_Indonesia.JPG/320px-Total_Solar_Eclipse%2C_9_March_2016%2C_from_Balikpapan%2C_East_Kalimantan%2C_Indonesia.JPG)
A total solar eclipse occurred at the Moon's descending node of orbit between Tuesday, March 8 and Wednesday, March 9, 2016, with a magnitude of 1.045. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.25 days before perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of July 2, 2019</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/8/89/20190702_Totality_LaSerena_Chile.jpg/320px-20190702_Totality_LaSerena_Chile.jpg)
A total solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, July 2, 2019, with a magnitude of 1.0459. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.4 days before perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of July 10, 1972</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/7/77/SE1972Jul10T.png/320px-SE1972Jul10T.png)
A total solar eclipse occurred at the Moon's descending node of orbit between Monday, July 10 and Tuesday, July 11, 1972, with a magnitude of 1.0379. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.8 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of June 30, 1954</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/0/05/SE1954Jun30T.png/320px-SE1954Jun30T.png)
A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, June 30, 1954, with a magnitude of 1.0357. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 3.1 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of February 26, 1998</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/2/29/Ecl002-2_%284321047401%29.jpg/320px-Ecl002-2_%284321047401%29.jpg)
A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, February 26, 1998, with a magnitude of 1.0441. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.1 days before perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of February 15, 1961</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/8/8e/1961_Total_Solar_Eclipse.jpg/320px-1961_Total_Solar_Eclipse.jpg)
A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, February 15, 1961, with a magnitude of 1.036. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 21 hours after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of August 23, 2044</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d6/SE2044Aug23T.png/320px-SE2044Aug23T.png)
A total solar eclipse will occur at the Moon's descending node of orbit between Monday, August 22 and Tuesday, August 23, 2044, with a magnitude of 1.0364. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.1 days after perigee, the Moon's apparent diameter will be larger.
![<span class="mw-page-title-main">Solar eclipse of August 2, 2027</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d4/SE2027Aug02T.png/320px-SE2027Aug02T.png)
A total solar eclipse will occur at the Moon's descending node of orbit on Monday, August 2, 2027, with a magnitude of 1.079. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.5 hours before perigee, the Moon's apparent diameter will be larger.
![<span class="mw-page-title-main">Solar eclipse of May 11, 2078</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/5/56/SE2078May11T.png/320px-SE2078May11T.png)
A total solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, May 11, 2078, with a magnitude of 1.0701. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 16 hours after perigee, the Moon's apparent diameter will be larger.
![<span class="mw-page-title-main">Solar eclipse of March 7, 1970</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/6/63/C72pct_%284321372614%29.jpg/320px-C72pct_%284321372614%29.jpg)
A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, March 7, 1970, with a magnitude of 1.0414. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days after perigee, this eclipse occurred when the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of June 29, 1927</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/5/5c/SE1927Jun29T.png/320px-SE1927Jun29T.png)
A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, June 28 and Wednesday, June 29, 1927, with a magnitude of 1.0128. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 20 hours after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of June 8, 1918</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/5/56/SE1918Jun08T.png/320px-SE1918Jun08T.png)
A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, June 8 and Sunday, June 9, 1918, with a magnitude of 1.0292. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring 3.7 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of February 4, 1943</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/a/aa/SE1943Feb04T.png/320px-SE1943Feb04T.png)
A total solar eclipse occurred at the Moon's descending node of orbit between Thursday, February 4 and Friday, February 5, 1943, with a magnitude of 1.0331. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 22 hours after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of May 1, 2079</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/2/26/SE2079May01T.png/320px-SE2079May01T.png)
A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, May 1, 2079, with a magnitude of 1.0512. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.2 days before perigee, the Moon's apparent diameter will be larger.
![<span class="mw-page-title-main">Solar eclipse of May 28, 1900</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/2/28/Thomas_Smillie_-_Smithsonian_Institution_-_Corona_of_the_Sun_during_a_Solar_Eclipse_%28pd%29.jpg/320px-Thomas_Smillie_-_Smithsonian_Institution_-_Corona_of_the_Sun_during_a_Solar_Eclipse_%28pd%29.jpg)
A total solar eclipse occurred at the Moon's descending node of orbit on Monday, May 28, 1900, with a magnitude of 1.0249. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 3.9 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of July 9, 1945</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/d/df/1945Jul09T.png/320px-1945Jul09T.png)
A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, July 9, 1945, with a magnitude of 1.018. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 4.4 days after perigee, the Moon's apparent diameter was larger.
![<span class="mw-page-title-main">Solar eclipse of April 28, 1930</span> Total eclipse](https://upload.wikimedia.org/wikipedia/commons/thumb/8/88/SE1930Apr28H.png/320px-SE1930Apr28H.png)
A total solar eclipse occurred at the Moon's ascending node of orbit on Monday, April 28, 1930, with a magnitude of 1.0003. It was a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The Moon's apparent diameter was near the average diameter because it occurred 7.2 days after apogee and 6 days before perigee.