Abstract

The high sensitivity of a planet's gravity assist (GA) to changes in test-body impact parameter prompts a space experiment that tests the nature of gravitational fields in the solar system. The Sun, Earth, and Venus can serve as a space-borne laboratory with a primitive space probe (“space ball”) as a test body moving on a ballistic trajectory from Earth to Venus, producing GA, and backward to Earth's orbit. We show that in Newton and Einstein (Schwarzschild) gravity, the probe's final positions, which are reached concurrently, may differ markedly, and an Earth-based observer can definitively measure that difference.

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