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<p><b>Very-long-baseline interferometry</b> (<b>VLBI</b>) is a type of <a href="page.php?w=astronomical_interferometer">astronomical interferometry</a> used in <a href="page.php?w=radio_astronomy">radio astronomy</a>. In VLBI a signal from an <a href="page.php?w=astronomical_radio_source">astronomical radio source</a>, such as a <a href="page.php?w=quasar">quasar</a>, is collected at multiple radio telescopes on Earth or in space. The distance between the radio telescopes is then calculated using the time difference between the arrivals of the radio</p><p>
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