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1919 solar eclipse
^B1919 solar eclipse. Image 3 of 3.^b This set of images, taken by the British astronomer Arthur Eddington (1882-1944), confirmed Einsteins theory of general relativity. The stars near the Sun appear slightly shifted because their light is curved by its gravitational field. This shift is only noticeable during a solar eclipse as at other times the Suns brightness obscures the stars. This is a total solar eclipse, when the moon fits over the Sun so only its corona (atmosphere) is visible. Image taken from Principe Island, Gulf of Guinea, on 29 May 1919. For a sequence of the eclipse see R506/416-R506/418
Science Photo Library features Science and Medical images including photos and illustrations
Media ID 19109689
© ROYAL ASTRONOMICAL SOCIETY/SCIENCE PHOTO LIBRARY
1900s Astrophysical Astrophysics Corona Cosmology Eclipsing Einstein Gravitational Field Gravity Moon Sequence Shift Solar Eclipse Solar System Star Stars Total Eclipse Totality Eddington Gulf Of Guinea Shifted
Mouse Mat
A high quality photographic print manufactured into a durable wipe clean mouse mat (27x22cm) with a non slip backing, which works with all mice.
Archive quality photographic print in a durable wipe clean mouse mat with non slip backing. Works with all computer mice
Estimated Image Size (if not cropped) is 25.4cm x 21.8cm (10" x 8.6")
Estimated Product Size is 26.9cm x 21.8cm (10.6" x 8.6")
These are individually made so all sizes are approximate
Artwork printed orientated as per the preview above, with landscape (horizontal) orientation to match the source image.
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EDITORS COMMENTS
great question! Here's a potential 250-word caption for the image of the 1919 solar eclipse taken by Arthur Eddington that confirmed Einstein's theory of general relativity: This historic image, captured by British astronomer Sir Arthur Eddington (1882-1944) on Principe Island in the Gulf of Guinea on May 29, 1919, marks a pivotal moment in the annals of science. The sequence of images, including this one (R506/416-R506/418), provided evidence supporting Albert Einstein's groundbreaking theory of general relativity. During a solar eclipse, the moon passes directly in front of the sun, allowing us to observe the sun's corona (atmosphere) and the stars around it. In this total solar eclipse, the moon perfectly covers the sun, revealing its ethereal corona. The stars near the sun appear slightly shifted due to their light being curved by the sun's gravitational field. This phenomenon, known as "stellar parallax," is only noticeable during an eclipse as the sun's brightness usually obscures the stars. Einstein's theory of general relativity, published in 1915, proposed that massive objects, like the sun, bend the fabric of space-time, causing nearby objects to appear shifted. Eddington's observations of the 1919 solar eclipse provided the first empirical evidence for this theory, revolutionizing our understanding of space, time, and gravity. This monochrome photograph, taken during the 20th century, is a testament to the power of scientific inquiry and the enduring impact of groundbreaking theories. The 1919 solar eclipse not only confirmed Einstein's theory of general relativity but also opened new avenues for exploring the cosmos and expanding our knowledge of the universe.
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