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Leave it to the Hubble Space Telescope to prove Albert Einstein wrong. Or at least, unnecessarily pessimistic.
Recently, Hubble spied a dead star about 18 light-years away warping the light of a more distant star that appeared to pass behind it. Einstein predicted this effect would happen based on his general theory of relativity, but he then claimed scientists had no hope of actually seeing it.
Of course, he wrote that dour phrase nearly 60 years before humans launched a rather impressive piece of hardware into Earths orbit.
The star-crossed effect, called gravitational microlensing, has been observed before using a much closer starour own sunas a lens. Most notably, during the total solar eclipse of 1919, Arthur Eddington measured the positions of stars situated near the edge of the darkened sun. He saw that our home stars gravity was tweaking that distant starlight, demonstrating that Einstein was onto something with his work on relativity.
Astronomers have used similar techniques to detect exoplanets and clumps of otherwise invisible dark matter, which bend light coming from background objects, and they have used entire clusters of galaxies as lenses to watch faraway stars explode over and over again.
But until now, no one had caught one small star in the act of bending light from another. Thats the scenario Einstein laid out in a 1936 paper also published in Science, which he suggested would be near impossible to see.
Turns out, Einstein only published this paper because a buddy suggested he do so: Some time ago, R. W. Mandl paid me a visit and asked me to publish the results of a little calculation, which I had made at his request, he wrote. This note complies with his wish.
Another article:
A team led by Kailash Sahu, an astronomer at the Space Telescope Science Institute in Baltimore, Maryland, watched the position of a distant star jiggle slightly, as its light bent around a white dwarf in the line of sight of observers on Earth. The amount of distortion allowed the researchers to directly calculate the white dwarfs mass 67% that of the Sun.
Sahus team studied a white dwarf known as Stein 2051 B, in the constellation Camelopardalis. At 5 parsecs (17 light years) from Earth, it is the sixth-nearest white dwarf.
Because it is so close, it appears to move quickly across the sky compared with more-distant stars. Sahu and his colleagues realized that during 2014 it would pass directly in front of a background star that lies around 1,500 parsecs, or 5,000 light-years, away. They signed up for time on Hubble to watch the event.
In eight observations between October 2013 and October 2015, the background star seemed to shift back and forth slightly. The shift was so small it was equivalent to a person in London watching an ant crawl across a coin in Moscow, but it was enough to confirm that the gravity of Stein 2051 B was bending the light of the background star.
In 1919, British astronomer Arthur Eddington and his team watched light bending around the Sun during a total solar eclipse, confirming Einsteins theory. Researchers have since seen light from distant galaxies bending around the gravity of intervening galaxies, but the new work is the first time anyone has observed a single object the white dwarf seemingly cause a background star to shift.