Event Horizon Telescope

Event Horizon Telescope
The Event Horizon Telescope and Global mm-VLBI Array on the Earth.jpg
Event Horizon Telescope.svg
Alternative namesEHT Edit this on Wikidata
Websiteeventhorizontelescope.org Edit this at Wikidata
TelescopesAtacama Large Millimeter Array
Atacama Pathfinder Experiment
Heinrich Hertz Submillimeter Telescope
IRAM 30m telescope
James Clerk Maxwell Telescope
Large Millimeter Telescope
South Pole Telescope
Submillimeter Array Edit this on Wikidata
Commons page Related media on Wikimedia Commons

The Event Horizon Telescope (EHT) is a large telescope array consisting of a global network of radio telescopes. The EHT project combines data from several very-long-baseline interferometry (VLBI) stations around Earth with angular resolution sufficient to observe objects the size of a supermassive black hole's event horizon. The project's observational targets include the two black holes with the largest angular diameter as observed from Earth: the black hole at the center of the supergiant elliptical galaxy Messier 87 (M87), and Sagittarius A* (Sgr A*) at the center of the Milky Way.[1][2][3]

The Event Horizon Telescope project is an international collaboration launched in 2009[1] after a long period of theoretical and technical developments. On the theory side, work on the photon orbit[4] and first simulations of what a black hole would look like[5] progressed to predictions of VLBI imaging for the Galactic Center black hole, Sgr A*.[6] Technical advances in radio observing moved from the first detection of Sgr A*,[7] through VLBI at progressively shorter wavelengths, ultimately leading to detection of horizon scale structure in both Sgr A* and M87.[8] The collaboration now comprises over 200 members, 60 institutions, working over 20 countries and regions.[3]

The first image of a black hole, at the center of galaxy Messier 87, was published by the EHT Collaboration on April 10, 2019, in a series of six scientific publications.[9] The array made this observation at a wavelength of 1.3 mm and with a theoretical diffraction-limited resolution of 25 microarcseconds. Future plans involve improving the array's resolution by adding new telescopes and by taking shorter-wavelength observations.[2][10]

Telescope array

Soft X-ray image of Sagittarius A* (center) and two light echoes from a recent explosion (circled)

The EHT is composed of many radio observatories or radio telescope facilities around the world, working together to produce a high-sensitivity, high-angular-resolution telescope. Through the technique of very-long-baseline interferometry (VLBI), many independent radio antennas separated by hundreds or thousands of kilometres can act as a phased array, a virtual telescope which can be pointed electronically, with an effective aperture which is the diameter of the entire planet.[11] The effort includes development and deployment of submillimeter dual polarization receivers, highly stable frequency standards to enable very-long-baseline interferometry at 230–450 GHz, higher-bandwidth VLBI backends and recorders, as well as commissioning of new submillimeter VLBI sites.[12]

Each year since its first data capture in 2006, the EHT array has moved to add more observatories to its global network of radio telescopes. The first image of the Milky Way's supermassive black hole, Sagittarius A*, was expected to be produced in April 2017,[13][14] but because the South Pole Telescope is closed during winter (April to October), the data shipment delayed the processing to December 2017 when the shipment arrived.[15]

Data collected on hard drives are transported by commercial freight airplanes[16] (a so-called sneakernet) from the various telescopes to the MIT Haystack Observatory and the Max Planck Institute for Radio Astronomy, where the data are cross-correlated and analyzed on a grid computer made from about 800 CPUs all connected through a 40 Gbit/s network.[17]

Other Languages
Bahasa Indonesia: Event Horizon Telescope