Similar tidal processes happen on the other moons in the solar system. Mercury is also in a tidal resonance with the sun. It, however is not tidally locked, but rotates exactly one and a half times for every revolution. This means that Mercury's tides are always in the same positions when the planet is closest to the Sun in its orbit, but not when it is farther away. This is as tidally locked as a planet in an elliptical orbit like Mercury's can get.
Tides are also responsible for a number of other curiosities in the solar system.
Think back to the Moon's gravity tugging on the football Earth. This addition of energy to the Moon's orbit causes the Moon to slowly migrate outwards away from the Earth, increasing its orbital radius. This has been directly measured by laser range-finding. The opposite effect happens only on Deimos, a moon of Mars. Deimos orbits Mars faster than the planet rotates, meaning that Mars's tide lags behind Deimos.