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Dyson, A.

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Eddington, and C. Davidson public domain. For precisely years, as of today, Albert Einstein has been a proven genius. His incredible general theory of relativity has since been fundamental to our understanding of the nature of reality, specifically of how the cosmos works. The decisive factor?

Black hole that 'rings' like a bell shows Einstein was right

An ultra-long total solar eclipse, the solar siblings of which still wow eclipse-chasers and solar scientists today. On May 29, , astronomers from Britain traveled to Africa and Brazil to measure the exact position of stars in the Hyades star cluster in the constellation of Taurus.

If the latter, science would have proof that the Sun and, therefore, all stars and planets curved space-time. Until May 29, , Isaac Newton's law of universal gravity had been regarded as accurate.

Einstein Was Right… Again! Successful Test of General Relativity Near a Supermassive Black Hole

However, Einstein's general theory of relativity, published in during the Great War, predicted that starlight should appear to bend around a massive object, such as out Sun, because it was traveling in a straight line through curved space-time. As the British scientists themselves put it: what effect, if any, is produced by a gravitational field on the path of a ray of light traversing it?

There is no need to get into equations to understand the basics of Einstein's general theory of relativity. It says that 'gravity' as a natural force does not exist. In this respect, Einstein has been proven right once again, using one the most extreme laboratory to date!

First ever Black Hole image revealed LIVE! Einstein was right!

In the near future, another relativistic test will be possible as S2 moves away from the black hole. This is known as a Schwarzschild precession, where the star is expected to experience a small rotation in its orbit. It was a huge challenge to develop the uniquely powerful instruments needed to make these very delicate measurements and to deploy them at the VLT in Paranal.

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The discovery announced today is the very exciting result of a remarkable partnership. Weather got in the way of a test during a eclipse; two years later, plans for another test were scuttled by the outbreak of the First World War. But in May of , the war was over and astronomers were hopeful that at last they would be able to see if Einstein was right.

“Through cloud. Hopeful.”

For more than two centuries, gravity had been viewed the way Isaac Newton viewed it — as an attractive force between objects. But in Einstein had offered a new explanation for gravity, describing it not as a force but as a curvature of space caused by the presence of massive objects, including stars and planets. Any mass — a bowling ball, a mountain, the Earth — will bend a beam of light.

But the astronomers knew that the deflection of light is proportional to the the mass of the object causing the deflection. To measure the tiny deflection, they needed something truly, colossally massive — something like our sun. Imagine a beam of light speeding our way from a distant star, passing the sun on its path to Earth.

Making such a measurement is tricky.