PETALING JAYA: Astronomers from Universiti Malaya (UM) were part of the international team that made the first images of a black hole a reality.
The images were captured using the Event Horizon Telescope (EHT) — a planet-scale array of eight ground-based radio telescopes forged through international collaboration designed to capture the images of a black hole.
"UM contributed to the project," said Dr Juan Carlos Algaba, a VLBI (Very Long Baseline Interferometry) expert of the Radio Cosmology Laboratory in the Department of Physics, Faculty of Science in UM.
“We are at the edge of a new era where we can directly see black holes, objects for science fiction and popular imagination just a few years ago, ”
UM Faculty of Science Department of Physics Radio Cosmology Laboratory head and investigator Dr Zamri Zainal Abidin, said this would definitely boost the role of Malaysian astronomy.
In coordinated press conferences across the globe on Wednesday, EHT researchers reveal that they had succeeded and unveiled the first direct visual evidence of a supermassive black hole and its shadow.
This breakthrough was announced on Wednesday in a series of six papers published in a special issue of the Astrophysical Journal Letters.
The image reveals the black hole at the centre of Messier 87, a massive galaxy in the nearby Virgo galaxy cluster. This black hole resides 55 million light-years from Earth and has a mass 6.5-billion times that of the Sun.
The EHT links telescopes around the globe to form an Earth-sized virtual telescope with unprecedented sensitivity and resolution.
The EHT is the result of years of international collaboration and offers scientists a new way to study the most extreme objects in the universe predicted by Einstein’s general relativity during the centennial year of the historic experiment that first confirmed the theory.
"We have taken the first picture of a black hole," said EHT project director Sheperd S. Doeleman of the Center for Astrophysics, Harvard & Smithsonian.
"This is an extraordinary scientific feat accomplished by a team of more than 200 researchers."
Black holes are extraordinary cosmic objects with enormous masses but extremely compact sizes.
The presence of these objects affects their environment in extreme ways, warping spacetime and super-heating any surrounding material.
"If immersed in a bright region, like a disc of glowing gas, we expect a black hole to create a dark region similar to a shadow — something predicted by Einstein’s general relativity that we’ve never seen before," explained chair of the EHT Science Council Heino Falcke of Radboud University, the Netherlands.
"This shadow, caused by the gravitational bending and capture of light by the event horizon, reveals a lot about the nature of these fascinating objects and allowed us to measure the enormous mass of M87’s black hole," he added.
Multiple calibration and imaging methods have revealed a ring-like structure with a dark central region — the black hole’s shadow — that persisted over multiple independent EHT observations.
"Once we were sure we had imaged the shadow, we could compare our observations to extensive computer models that include the physics of warped space, superheated matter and strong magnetic fields.
"Many of the features of the observed image match our theoretical understanding surprisingly well," said Paul T.P. Ho, EHT Board member and Director of the East Asian Observatory.
"This makes us confident about the interpretation of our observations, including our estimation of the black hole’s mass."
Creating the EHT was a formidable challenge which required upgrading and connecting a worldwide network of eight pre-existing telescopes deployed at a variety of challenging high-altitude sites.
These locations included volcanoes in Hawaii and Mexico, mountains in Arizona and the Spanish Sierra Nevada, the Chilean Atacama Desert and Antarctica.
The EHT observations use a technique called VLBI, which synchronises telescope facilities around the world and exploits the rotation of our planet to form one huge, Earth-size telescope observing at a wavelength of 1.3mm.
VLBI allows the EHT to achieve an angular resolution of 20 micro-arcseconds — enough to read a newspaper in New York from a sidewalk café in Paris.
The telescopes contributing to this result were ALMA, APEX, the IRAM 30m telescope, the James Clerk Maxwell Telescope, the Large Millimeter Telescope Alfonso Serrano, the Submillimeter Array, the Submillimeter Telescope, and the South Pole Telescope.
Petabytes of raw data from the telescopes were combined by highly specialised supercomputers hosted by the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory.
The construction of the EHT and the observations announced represent the culmination of decades of observational, technical, and theoretical work.
This example of global teamwork required close collaboration by researchers from around the world.
Thirteen partner institutions worked together to create the EHT, using both pre-existing infrastructure and support from a variety of agencies.
Key funding was provided by the US National Science Foundation (NSF), the EU's European Research Council (ERC), and funding agencies in East Asia.
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