Very first image of a black hole
The bright, lopsided ring in the new images offers visual confirmation of these effects: The material headed toward our vantage point as it rotates around appears brighter than the other side.įrom these images, theorists and modelers on the team have determined that the black hole is about 6.5 billion times as massive as our sun. Relativity predicts that the immense gravitational field will cause light to bend around the black hole, forming a bright ring around its silhouette, and will also cause the surrounding material to orbit around the object at close to light speed. But if a black hole is surrounded by light-emitting material such as plasma, Einstein’s equations predict that some of this material should create a “shadow,” or an outline of the black hole and its boundary, also known as its event horizon.īased on the new images of M87, the scientists believe they are seeing a black hole’s shadow for the first time, in the form of the dark region at the center of each image. By definition, black holes are invisible.
#VERY FIRST IMAGE OF A BLACK HOLE SERIES#
In a series of papers published today in a special issue of Astrophysical Journal Letters, the team has revealed four images of the supermassive black hole at the heart of Messier 87, or M87, a galaxy within the Virgo galaxy cluster, 55 million light years from Earth.Īll four images show a central dark region surrounded by a ring of light that appears lopsided - brighter on one side than the other.Īlbert Einstein, in his theory of general relativity, predicted the existence of black holes, in the form of infinitely dense, compact regions in space, where gravity is so extreme that nothing, not even light, can escape from within. They accomplished this remarkable feat by coordinating the power of eight major radio observatories on four continents, to work together as a virtual, Earth-sized telescope.
They were then painstakingly converted into an image using novel computational tools developed by the collaboration.Īn international team of over 200 astronomers, including scientists from MIT’s Haystack Observatory, has captured the first direct images of a black hole. These data were flown to highly specialised supercomputers - known as correlators - at the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory to be combined. Each telescope of the EHT produced enormous amounts of data – roughly 350 terabytes per day – which was stored on high-performance helium-filled hard drives. These observations were collected at a wavelength of 1.3 mm during a 2017 global campaign. While this may sound large, this ring is only about 40 microarcseconds across - equivalent to measuring the length of a credit card on the surface of the Moon.Īlthough the telescopes making up the EHT are not physically connected, they are able to synchronize their recorded data with atomic clocks - hydrogen masers - which precisely time their observations. The black hole’s boundary - the event horizon from which the EHT takes its name - is around 2.5 times smaller than the shadow it casts and measures just under 40 billion km across. The shadow of a black hole seen here is the closest we can come to an image of the black hole itself, a completely dark object from which light cannot escape. In coordinated press conferences across the globe, EHT researchers revealed that they succeeded, unveiling the first direct visual evidence of the supermassive black hole in the centre of Messier 87 and its shadow. The Event Horizon Telescope (EHT) - a planet-scale array of eight ground-based radio telescopes forged through international collaboration - was designed to capture images of a black hole.