Newton’s conclusion unified the motion of celestial bodies and objects on Earth under a single universal law of gravitation.
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The evidence is the observed orbital motion of planets around the Sun, which implies a gravitational force maintaining these orbits.
Newton extended the idea by arguing that the same force causing an apple to fall to Earth and the Moon to orbit Earth also governs the motion of planets around the Sun.
Newton concluded that all objects in the universe attract each other with a force called gravitational force.
The motion of the Earth due to the Moon’s gravitational pull can be observed through precise measurements and the study of the Earth-Moon system’s dynamics. For instance, the Earth and Moon actually orbit around their common center of mass (the ...
Yes, the gravitational attraction between the Earth and the Moon causes observable effects such as ocean tides. The gravitational pull of the Moon creates tidal bulges in the Earth’s oceans, leading to high and low tides.
The mass of the Earth is about 81 times greater than the mass of the Moon. Due to this large mass difference, the acceleration of the Earth towards the Moon is extremely small compared to the acceleration of the Moon ...
Newton’s second law states that acceleration is inversely proportional to the mass of an object when subjected to a given force. Because the mass of the Earth is much greater than the mass of the Moon, the acceleration of the ...
Newton’s third law states that for every action, there is an equal and opposite reaction. Thus, when the Earth exerts a gravitational force on the Moon, the Moon exerts an equal and opposite gravitational force on the Earth.
The force of attraction of the Earth provides the centripetal force that keeps the moon in orbit around it.