👉 The term "pfeffernuss" is a term used in physics and astronomy to describe an object's gravitational field. It is named after Wilhelm Pfeffermann, who first described it in 1879. The gravitational field of a celestial body can be described using the formula:
F = G
(m1
m2) / r^2
where F is the force acting on an object, G is the universal gravitational constant, m1 and m2 are
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