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Telescope illuminated in red light.
Photo Credit: Daniel Luong-Van/Antarctic Photo Library
The South Pole Telescope has been involved in investigating some of the greatest mysteries of the universe. Now the powerful instrument in Antarctica will be used to form an Earth-sized telescope to study a black hole in the center of the Milky Way Galaxy.

Joining together

South Pole Telescope to be used to form Earth-sized instrument to study black hole

The South Pole Telescope (SPT) External Non-U.S. government site has been involved in investigating some of the greatest mysteries of the universe, from the enigmatic force known as dark energy External U.S. government site to the exponential expansion of the universe as it first exploded into existence, a period of time called inflation External U.S. government site.

Now the powerful astrophysics instrument, located at the National Science Foundation’s Amundsen-Scott South Pole Station External U.S. government site, will be used to form an Earth-sized telescope to study a black hole External U.S. government site in the center of the Milky Way Galaxy.

It sounds like the plot of a science fiction movie. In fact, the analogy that Christopher Greer External Non-U.S. government site uses to explain the concept of combining a half-dozen radio telescopes around the world into one super-telescope draws upon a 1980s cartoon series called Voltron: Defender of the Universe, in which a fleet of smaller, lion-like robots combine into a powerful, giant robot called Voltron.

In the case of the Event Horizon Telescope External Non-U.S. government site, or EHT, the goal isn’t to fight some intergalactic evil but to get a better picture of a very distant and small object – like viewing something the size of a softball on the surface of the moon – by eventually joining the observing power of telescopes in the United States, Europe, the Pacific Ocean, Mexico, Chile and Antarctica.

“The bigger your telescope, the smaller the thing you can see,” explained Greer, a postdoctoral researcher at Steward Observatory External Non-U.S. government site at the University of Arizona External Non-U.S. government site in Tucson, one of the primary institutions involved in the EHT project, which is partly supported by the National Science Foundation (NSF).

View of buildings surrounded by trees.
Photo Credit: University of Arizona
The Steward Observatory at the University of Arizona is one of the key players in the Event Horizon Telescope project.

Daniel Marrone External Non-U.S. government site, an assistant professor at the University of Arizona’s Steward Observatory is the principal investigator (PI) on an NSF grant from the Division of Astronomical Sciences External U.S. government site to build an instrument that will allow the SPT to join the EHT network. John Carlstrom External Non-U.S. government site, SPT PI at the University of Chicago External Non-U.S. government site, and Shepherd Doeleman External Non-U.S. government site, assistant director at MIT's Haystack Observatory External Non-U.S. government site in Massachusetts and head of the EHT project, are co-PIs.

Despite the name, black holes are anything but empty. Just the opposite: Black holes are so densely packed with matter that not even light can escape their gravitational pull.

Predicted by physicist Albert Einstein’s general theory of relativity – the handbook for gravity and its effects on the universe – black holes are by definition nearly unobservable. Instead, scientists must rely on indirect observations to detect and study them.

Such was the case with the supermassive black hole at the center of the Milky Way Galaxy in a region referred to as Sagittarius A* (pronounced “Sagittarius A-star”) near the border of the constellations Sagittarius and Scorpius, about 26,000 light years away.

Observations from instruments that scan different parts of the electromagnetic spectrum, which is the range of electromagnetic radiation from radio waves to visible light to gamma rays, found Sagittarius A* to be a very bright radio source. The eccentric orbit of the star S2 around Sagittarius A* – observations made in the infrared spectrum by the Keck telescopes External Non-U.S. government site in Hawaii and the Very Large Telescope (VLT) External Non-U.S. government site in Chile – also implied the object was extremely dense with a powerful gravitational force.

Instrument sized against a penny for scale.
Photo Courtesy: Christopher Greer
Digital instrumentation to be installed on the South Pole Telescope will make it possible to receive and record progressively higher bandwidths, which increases sensitivity levels for the EHT array.

Calculations of S2’s orbit pegged the object of its attraction at four million times the mass of the Earth’s sun. If indeed it is a black hole, as astronomers believe, it would inhabit a space much smaller than the orbit of Mercury, according to Greer.

“There are very few things in astronomers’ minds that could be so massive in such a small space. We’re really getting into black hole territory,” he said. “The EHT is the first experiment that really has the chance to image something this small directly.”

The term “event horizon” in Event Horizon Telescope refers to a theorized boundary around a black hole that marks the gravitational “point of no return” from which matter or energy falling into the black hole cannot escape. Gas in the region will circle the black hole, like water going down a drain, emitting signals in a variety of wavelengths, as it is drawn into the black hole. The event horizon should then cast a “shadow” on that bright emission.

It’s that shadow that the scientists using the EHT hope to map employing a technique called very long baseline interferometry (VLBI), which involves capturing a signal from an astronomical radio source, such as Sagittarius A*, at multiple locations on Earth.

The distance between the radio telescopes is calculated using the time difference between the arrivals of the radio signal at different telescopes using. This allows observations of an object that are made simultaneously by many radio telescopes to be combined. Extremely accurate atomic clocks are employed to “freeze” the light at each telescope for later comparison.

As Doeleman explained the VLMI process to Space.com in a 2013 article about the EHT experiment: “In a typical telescope, light bounces off a precisely curved surface and all the light gets focused into a focal plane. The way VLBI works is we have to freeze the light, capture it, record it perfectly faithfully on the recording system, then shift the data back to a central supercomputer, which compares the light from California and Hawaii and the other locations, and synthesizes it. The lens becomes a supercomputer here at MIT.”

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Curator: Peter Rejcek, Antarctic Support Contract | NSF Official: Winifred Reuning, Division of Polar Programs