Mercury is one of the least-studied of the solar system's planets. It was visited by only one spacecraft, [Mariner 10]?, which flew past it on three occasions in 1974 and 1975. Only 45% of the planet's surface was mapped, and it is located too near the sun for existing telescopes to conduct further mapping from Earth. Until radar observations in 1965 proved otherwise it was thought that Mercury was [tidally locked]? with the Sun, rotating once for each orbit and keeping the same face directed towards the sun at all times. Instead, Mercury is in a 3:2 resonance, rotating three times for every two revolutions around the sun. The original reason astronomers thought it was tidally locked was because whenever Mercury was best placed for observation, it was always at the same point in it's 3:2 resonance, so showing the same face, which would be also the case if it was totally locked.
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