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Radio Telescopes were officially discovered and invented by Karl G. Jansky in 1931. His radio telescope was a series of arms that spun around with the intention of detecting radio frequency interference during a thunder storm. However, as time progressed he realized that his "radio telescope" was detecting static which he could not account for. He also discovered that each day the static peaked four minutes earlier, ruling out his original explanation as the source being the sun. Astronomers refer to a stellar day (which is typically four minutes shorter than a solar day) as a sidereal day. Not being an astronomer himself, it took Jansky a while to surmise that the source of his static was in fact of Extraterrestrial origin. With further study he discovered the source to be the milky way galaxy and in 1933 published his findings in a scientific journal. However his research was largely ignored by the scientific community until in 1937 when Grobe Reber picked up where Jansky left off and built the prototype of what we now know to be a radio telescope in his back yard in Wheaton, Illinois. At first he began looking for radio waves at shorter wavelengths, with little to no success. He later increased his target wavelengths to 1.87 meters where he located strong radio emissions along the Milky Way. Reber continued his research up until 1944, when he published his own scientific findings. Despite this, it wasn't until after World War 2 that Radio Waves were explored in depth, since the Allies had discovered radio interference from the sun on their radars.

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