The data has been taken, collected, and analyzed. So where is the first image of an event horizon, already?
Across multiple continents, including Antarctica, an array of radio telescopes observe the galactic center.
A view of the different telescopes contributing to the Event Horizon Telescope’s imaging capabilities from one of Earth’s hemispheres. The data taken from 2011 to 2017 should enable us to now construct an image of Sagittarius A*. (APEX, IRAM, G. Narayanan, J. McMahon, JCMT/JAC, S. Hostler, D. Harvey, ESO/C. Malin)
The most-visualized black hole of all, as illustrated in the movie Interstellar, shows a predicted event horizon fairly accurately for a very specific class of rotating black holes. (Interstellar / R. Hurt / Caltech)
Of all the black holes visible from Earth, the largest is at the galactic center: 37 μas.
This multiwavelength view of the Milky Way’s galactic center goes from the X-ray through the optical and into the infrared, showcasing Sagittarius A* and the intragalactic medium located some 25,000 light years away. Using radio data, the EHT will resolve the event horizon of the central black hole. (X-ray: NASA/CXC/UMass/D. Wang et al.; Optical: NASA/ESA/STScI/D.Wang et al.; IR: NASA/JPL-Caltech/SSC/S.Stolovy)
With a theoretical resolution of 15 μas, the EHT should resolve it.
A plot of the coverage in space of the area around the galactic center’s black hole from the telescopes whose data has been brought together so far. Additional telescopes will further constrain the black hole’s size, shape and orientation. (R.-S. Lu et al, ApJ 859, 1)
They found evidence for an asymmetric source, about 3 Schwarzschild radii large: consistent with Einstein’s prediction of 2.5.
Two of the possible models that can successfully fit the Event Horizon Telescope data thus far. Both show an off-center, asymmetric event horizon that’s enlarged versus the Schwarzschild radius, consistent with the predictions of Einstein’s General Relativity. (R.-S. Lu et al, ApJ 859, 1)
The South Pole Telescope, a 10 meter radio telescope located at the South Pole, will be the most important addition to the EHT as far as resolving the central black hole goes. (Daniel Michalik/South Pole Telescope)
Earth’s atmospheric turbulence, instrumentation noise, and spurious signals require identification, obtainable through additional imaging.
A map of the 7 million second exposure of the Chandra Deep Field-South. This region shows hundreds of supermassive black holes, each one in a galaxy far beyond our own. There should be hundreds of thousands of times as many stellar-mass black holes; we’re just waiting for the capability of detecting them. (NASA/CXC/B. Luo et al., 2017, ApJS, 228, 2)
Although the data has been combined, novel algorithms must be developed to process them into an image.
Five different simulations in general relativity, using a magnetohydrodynamic model of the black hole’s accretion disk, and how the radio signal will look as a result. Note the clear signature of the event horizon in all the expected results. (GRMHD simulations of visibility amplitude variability for Event Horizon Telescope images of Sgr A*, L. Medeiros et al., arXiv:1601.06799)
Only two black holes, Sagittarius A* and M87, could have event horizon “silhouettes” imaged.
The second-largest black hole as seen from Earth, the one at the center of the galaxy M87, is shown in three views here. Despite its mass of 6.6 billion Suns, it is over 2000 times farther away than Sagittarius A*. It may not be resolvable by the EHT. (Top, optical, Hubble Space Telescope / NASA / Wikisky; lower left, radio, NRAO / Very Large Array (VLA); lower right, X-ray, NASA / Chandra X-ray telescope)
New data will be taken annually, improving the future, overall pictures through subsequent analysis.
The locations of the radio dishes that are planned be part of the Event Horizon Telescope array. Each new data set taken by each telescope can stack with the previous data, improving our picture as time goes on. (Event Horizon Telescope / University of Arizona)
Over the coming months, preliminary images will show the:
size,
shape,
changes,
and surrounding environment,
of our first directly-observed black holes.
Some of the possible profile signals of the black hole’s event horizon as simulations of the Event Horizon Telescope indicate. (High-Angular-Resolution and High-Sensitivity Science Enabled by Beamformed ALMA, V. Fish et al., arXiv:1309.3519)
Mostly Mute Monday tells the astronomical story of an object, technique, or phenomenon in the Universe in visuals, images, and no more than 200 words. Talk less, smile more.
