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Lunar eclipse, 28 / 08 / 2007

Lunar eclipse, 28  /  08  /  2007


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Lunar eclipse, 28 / 08 / 2007

Lunar eclipse. Totality during a lunar eclipse. A lunar eclipse occurs as the Moon passes into the Earths shadow. The red light is due to shorter wavelengths, such as blue light, being scattered more in the atmosphere than longer wavelengths such as red light. Lunar eclipses occur only at full Moon, and then only when the Earth and Moon are correctly aligned (about 2-3 times a year). Photographed from the northern hemisphere on 28 August 2007

Science Photo Library features Science and Medical images including photos and illustrations

Media ID 6426037

© JOHN SANFORD/SCIENCE PHOTO LIBRARY

2007 August Circle Circular Crater Craters Full Moon Lunar Lunar Eclipse Mare Maria Moon Night Sky Northern Hemisphere Optical Optics Orange Refracted Refraction Round Scattered Scattering Solar System Telescope Total Totality


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