Editing 2133: EHT Black Hole Picture

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The image was produced from data gathered since 2006, collected by over a dozen radio telescopes around the world and combined through a process called {{w|interferometry}}.  Normally, a telescope's resolution is limited by the size of its aperture, but by recording radio signals at multiple sites, the minute differences between the signals can be digitally processed into an image with much higher resolution.  The telescopes used for the EHT are in Hawaii, North and South America, Europe, and Antarctica, and so the effective diameter of the collective EHT is almost the size of the Earth itself.  As each telescope recorded observations of the black holes, the results were written to hard drives and mailed to observatories at {{w|MIT}} and the {{w|Max Planck Institute for Radio Astronomy}} for processing.  Astronomical recordings can involve astronomical amounts of data, so the raw, original, feed from a telescope may never be stored if it is too dense -- it is instead processed live by computers to capture the information of interest, and the processed result is stored.  <!-- Should add remarks here about how many petabytes of data were processed and how much computing power and time was used, when that's announced.  -->
 
The image was produced from data gathered since 2006, collected by over a dozen radio telescopes around the world and combined through a process called {{w|interferometry}}.  Normally, a telescope's resolution is limited by the size of its aperture, but by recording radio signals at multiple sites, the minute differences between the signals can be digitally processed into an image with much higher resolution.  The telescopes used for the EHT are in Hawaii, North and South America, Europe, and Antarctica, and so the effective diameter of the collective EHT is almost the size of the Earth itself.  As each telescope recorded observations of the black holes, the results were written to hard drives and mailed to observatories at {{w|MIT}} and the {{w|Max Planck Institute for Radio Astronomy}} for processing.  Astronomical recordings can involve astronomical amounts of data, so the raw, original, feed from a telescope may never be stored if it is too dense -- it is instead processed live by computers to capture the information of interest, and the processed result is stored.  <!-- Should add remarks here about how many petabytes of data were processed and how much computing power and time was used, when that's announced.  -->
  
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The first image released by the EHT was expected to be in April 2017, but unforeseen events delayed it by two years, to April 2019.  Randall predicts this trend will continue, and makes a joke by analogy to real-world difficult experiences capturing important moments.
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The first image released by the EHT was expected to be on April 2017, but unforeseen events have so far delayed it by two years, to April 2019.  Randall predicts this trend will continue, and makes a joke by analogy to real-world difficult experiences capturing important moments.
  
 
Luckily this comic was not in any way prophetic, and five days after this comic was released [https://www.bbc.com/news/science-environment-47873592 the EHT team released a black hole picture] for the world to enjoy.
 
Luckily this comic was not in any way prophetic, and five days after this comic was released [https://www.bbc.com/news/science-environment-47873592 the EHT team released a black hole picture] for the world to enjoy.

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