The first image of a black hole at the center of the Messier 87 galaxy published this week is amazing. The technology developed to create it is just as amazing. The Event Horizon Telescope (EHT) project brought together a network of 10 telescopes across the globe to see, as project director Sheered Doeleman put it, “what we thought was un-seeable”.
Einstein first theorized the existence of black holes 100 years ago while developing his theory of general relativity. Since then, there has been a lot of evidence supporting the existence of back holes, and simulations of what they might look like, because one had not been directly observed.
So what took so long? Why haven’t we used something like the Hubble Space Telescope (HST) to take this photo?
While the black hole in M87 is as wide as our solar system, it’s also 55 million light years away, which makes it very, very small in our sky. Each pixel in HST’s WFC3 camera is about 1,250 times wider than the black hole. A telescope as big as the Earth was needed, so one was created, virtually.
Radio telescopes in Hawaii, Arizona, Spain, Mexico, Chile, and Antarctica were linked together in a process called Very Long Baseline Interferometry to create a single virtual telescope effectively as big as Earth, producing five petabytes of data. That is about the size of the Library of Congress’s digital collection or the equivalent of 190 continuous years of streaming Netflix in high definition.
This isn’t just an achievement in astronomy, it’s an achievement in data science, particularly data reduction and image construction from sparse data.
Read more : First ever black hole image released
Even with so much data and all that processing, there were still a lot of gaps. This is like putting together a puzzle where 90 percent of the pieces are missing and you don’t even know what the final image is supposed to look like. So where does the confidence come from that the image published this week is accurate? The answer lies in data science.
Petabytes were reduced to terra-bytes through correlation of observations between the radio telescopes which take into account things like Earth’s rotation during the observations and the amount of water vapor in the atmosphere above each telescope. The dry conditions in the Atacama Desert of northern Chile, where one of the telescopes is located, helped make this easier. This step also helps pull useful data out of the noise, a common problem in data science.
The EHT broke into teams which independently built algorithms to further reduce that data down into an image, still trying to put together a puzzle with infinite possibilities, with missing pieces and no box with a picture to refer to. Each built algorithms that reduced those infinite possibilities down to just those that made sense physically. They came back together last July to share their work and they knew they had solved the problem when the teams produced strikingly similar results.
The techniques and resulting image processing libraries developed by the team could have far-reaching applications in fields which need to build useful images from sparse data like medical imaging and self-driving vehicles.
This black hole also now has a name, Pōwehi, meaning “embellished dark source of unending creation”. The name was sourced from the Kumulipo, the primordial chant describing the creation of the Hawaiian universe, reflecting the role of the Mauna Kea Observatories in creating the image.
Hawaiian Astronomers on the project consulted with Larry Kimura, of the University of Hawaii at Hilo’s College of Hawaiian Language. Hawaii’s governor David Ige declared April 10 “Powehi Day.”
You can see Pōwehi, or at least where it is in the southeastern sky, after sunset. Look for the backward question mark that makes up the front of the constellation Leo the Lion, look below for the bright star Spica in the constellation Virgo. The M87 galaxy and Pōwehi are about 1/3 of the way between Virgo’s left shoulder and Leo’s tail.