Stability of the Solar System essentially the distance from sun to earth). These are now known as the Kirkwood gaps. Some asteroids were later discovered to orbit in these gaps, but their orbits are unstable and they will eventually break out of the resonance due to close encounters with a major planet. Another common form of resonance in the Solar System is spin–orbit resonance, where the period of spin (the time it takes the planet or moon to rotate once about its axis) has a simple numerical relationship with its orbital period. An example is our own Moon, which is in a 1:1 spin–orbit resonance
Orchestral Suite in G minor, BWV 1070 minor is heavy-treaded and the central trio is in the bright G major (the tonic major). The concluding movement is a bustling piece written in a learned imitative style. J. S. Bach: Orchestral Suites Nos. 1 ~ 4, BWV 1066 ~ 1069 Orchestral Suite in G minor, BWV 1070 The Orchestral Suite in G minor, BWV 1070 is a work by an unknown composer. It is part of the Bach-Werke-Verzeichnis catalogue (BWV catalogue) of the works of J. S. Bach, and sometimes called the "Orchestral Suite No. 5", but was almost certainly not composed by him. It is more likely