The point at which the gravitational pull of the Sun balances that of the Earth is known as the Lagrange point L1. For the Earth-Sun system, L1 is approximately 1.5 million kilometers from Earth, directly between the Earth and the Sun. At this point, the gravitational forces from the Earth and the Sun counterbalance, allowing objects to remain relatively stable in that position.
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The point at which the gravitational pull of the Sun balances that of the Earth is known as the Lagrange point L1. For the Earth-Sun system, L1 is approximately 1.5 million kilometers from Earth, directly between the Earth and the Sun. At this point, the gravitational forces from the Earth and the Sun counterbalance, allowing objects to remain relatively stable in that position.