An international scientific team on Wednesday announced a milestone in astrophysics – the first-ever photo of a black hole – using a global network of telescopes to gain insight into celestial objects with gravitational fields so strong no matter or light can escape.
The team’s observations of the black hole at the center of Messier 87, a massive galaxy in the nearby Virgo galaxy cluster, lend strong support to the theory of general relativity put forward in 1915 by physicist Albert Einstein to explain the laws of gravity and their relation to other natural forces.
The research was conducted by the Event Horizon Telescope (EHT) project, an international collaboration begun in 2012 to try to directly observe the immediate environment of a blackhole using a global network of Earth-based telescopes. The announcement was made in simultaneous news conferences in Washington, Brussels, Santiago, Shanghai, Taipei and Tokyo.
WATCH: First image released of a giant black hole in a distant galaxy
The team includes Avery Broderick, an astrophysicist at the Perimeter Institute in Waterloo, Ont., which contributes to the EHT project.
“We have achieved something presumed to be impossible just a generation ago,” said astrophysicist Sheperd Doeleman, director of the Event Horizon Telescope at the Center for Astrophysics, Harvard & Smithsonian.
This black hole resides about 54 million light-years from Earth. A light year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km).
Black holes, phenomenally dense celestial entities, are extraordinarily difficult to observe despite their great mass. A black hole‘s event horizon is the point of no return beyond which anything – stars, planets, gas, dust and all forms of electromagnetic radiation – gets swallowed into oblivion.
“This is a huge day in astrophysics,” said U.S. National Science Foundation Director France Córdova. “We’re seeing the unseeable.”
The fact that black holes do not allow light to escape makes viewing them difficult. The scientists look for a ring of light – disrupted matter and radiation circling at tremendous speed at the edge of the event horizon – around a region of darkness representing the actual black hole. This is known as the black hole‘s shadow or silhouette.
One of the black holes – Sagittarius A* – is situated at the center of our own Milky Way galaxy, possessing 4 million times the mass of our sun and located 26,000 light years from Earth. A light year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km).
The second one – M87 – inhabits the center of the neighboring Virgo A galaxy, boasting a mass 3.5 billion times that of the sun and located 54 million light-years away from Earth. Streaming away from M87 at nearly the speed of light is a humongous jet of subatomic particles.
Black holes, which come in different sizes, are formed when very massive stars collapse at the end of their life cycle. Supermassive black holes are the largest kind, growing in mass as they devour matter and radiation and perhaps merging with other black holes.
The project’s researchers obtained the first data in April 2017 using telescopes in the U.S. states of Arizona and Hawaii as well as Mexico, Chile, Spain and Antarctica. Since then, telescopes in France and Greenland have been added to the global network. The global network of telescopes has essentially created a planet-sized observational dish.
*with a file from the Canadian Press