https://sol24.net/data/html/SOHO/C3/96H/VIDEO/
Because Mercury passes behind the Sun frequently, several observations are now possible.
The Earth and Mercury are on opposite sides of the Sun in our respective orbits when the faster-moving planet moves from right to left while our world travels in the opposite direction on the other side of the Sun.
The frequency allows for variable orbital speeds to be observed with each different pass, and currently, Mercury appears to pass slower from right to left than at other times.
When Mercury passes between the Earth and the Sun, it moves considerably faster, just as watching cars passing at a closer distance across the frame of a window will appear quicker than cars at a distance crossing the same window frame.
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