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You entered: solar eclipse
![Взгляд назад на затененную Землю](https://images.astronet.ru/pubd/2007/06/10/0001222371/eclipse99_mir.preview.jpg)
10.06.2007
Here is what the Earth looks like during a solar eclipse. The shadow of the Moon can be seen darkening part of Earth. This shadow moved across the Earth at nearly 2000 kilometers per hour.
![Силуэты Гоа](https://images.astronet.ru/pubd/2007/03/22/0001221270/pse2007mar_Schoppmeyer1_720.preview.jpg)
22.03.2007
On Moonday, March 19, shortly before the equinox, locations in Asia and the Arctic were favoured by the New Moon's shadow during a partial solar eclipse. Although the view from Goa, India found...
![Эклиптика над Новой Зеландией](https://images.astronet.ru/pubd/2010/07/14/0001246015/TaupoPlanets_tezel900h.preview.jpg)
10.07.2010
Four bright celestial beacons and a faint triangle of light follow the plane of the ecliptic as it arcs high through this southern hemisphere night skyscape. Seen on a July winter night from Lake...
![Закручивающаяся кома кометы Понса-Брукса](https://images.astronet.ru/pubd/2024/03/19/0001923410/CometPonsBrook_Vallestad_960.preview.jpg)
18.03.2024
A bright comet will be visible during next month's total solar eclipse. This very unusual coincidence occurs because Comet 12P/Pons-Brooks's return to the inner Solar System places it by chance only 25 degrees away from the Sun during Earth's April 8 total solar eclipse.
![Мимолетное затмение](https://images.astronet.ru/pubd/2003/08/14/0001192327/eclipsebird_staiger.preview.jpg)
27.08.1997
A lunar eclipse can be viewed in a leisurely fashion. Visible to anyone on the night side of planet Earth (weather permitting), totality often lasts an hour or so as the moon glides through the Earth's shadow. But a solar eclipse is more fleeting.
![Лунные игры](https://images.astronet.ru/pubd/2008/08/04/0001229006/moongames_lavederN080717_9416_c800.preview.jpg)
1.08.2008
The Moon's measured diameter is around 3,476 kilometers (2,160 miles). But apparent angular size, or the angle covered by an object, can also be important to Moon enthusiasts. Angular size depends on distance, the farther away an object is, the smaller an angle it covers.
![Корона Солнца](https://images.astronet.ru/pubd/2008/08/08/0001229068/TSE2008_luethen800.preview.jpg)
8.08.2008
During a total solar eclipse, the Sun's extensive outer atmosphere, or corona, is an inspirational sight. The subtle shades and shimmering features of the corona that engage the eye span a brightness range of over 10,000 to 1, making them notoriously difficult to capture in a single picture.
![Солнечная корона](https://images.astronet.ru/pubd/2010/07/21/0001246178/TSE2010_JLD4_900c.preview.jpg)
21.07.2010
During a total solar eclipse, the Sun's extensive outer atmosphere, or corona, is an inspirational sight. Subtle shades and shimmering features that engage the eye span a brightness range of over 10,000 to 1, making them notoriously difficult to capture in a single photograph.
![Полное солнечное затмение](https://images.astronet.ru/pubd/2003/09/08/0001192778/eclipse_js_big.preview.jpg)
11.03.1998
On February 26th, it was dark during the day. This total solar eclipse was the last visible from the Americas for this millennium. A total solar eclipse is exciting partly because it is so short.
![Затмение в Бакассе](https://images.astronet.ru/pubd/2001/07/06/0001169724/tse2001_malexander.preview.jpg)
6.07.2001
Starting at the upper left, this sequence of images follows the progress of the magnificent 21 June, 2001 solar eclipse in the clear skies over Bakasa, Zimbabwe. These pictures were recorded using a small reflecting telescope and digital camera with the approximate local time given above each frame.
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