However, a Counter-Earth would nevertheless be visible from Earth because the gravitational forces of the other planets on it would make its own orbit unstable. Venus has 82% of the mass of Earth and would come within 0.3 AU of the location of a Counter-Earth every 20 months, providing considerable gravitational pull that over the years would move its orbit into sight of observers on Earth. If a Counter-Earth was much smaller than Earth, its location at the "Sun–Earth L3" Lagrangian point (see diagram) would mean the combined gravitational pull of the two large masses of Earth and Sun would provide "precisely the centripetal force required to orbit with them". But a small planet would be even more influenced by the orbit of Venus, Mars and Jupiter, making it even more unstable.