This interaction does two things: it creates friction that slows Earth’s own rotation, and creates forces that change the Moon’s orbital speed, causing it to fall farther away into space. Earth’s bulging oceans don’t exactly match up with the position of the Moon, they’re always a little out of sync because it takes time for all that water to shift and pile up. The energy propelling it away comes primarily from Earth’s oceans, which both bulge out in response to the Moon’s gravity and exert a gravitational pull of their own on the Moon. The Moon continues to move away from Earth at a rate of about an inch-and-a-half (4 cm) per year, its drift slowing as it goes. Credit: Vi Nguyen, NASA Goddard Space Flight Center Motions in this animation are exaggerated to highlight the changes. At the same time, the moon continuously drifts away. As energy leaves the system, the moon’s rotation very quickly synchronizes with its orbit around its host planet. This animation illustrates how the Moon becomes tidally locked after its formation. In this state, the bulge on the Moon was no longer shifting relative to the Earth, therefore no more energy needed to be dissipated by this particular process, and the spin rate stopped changing. As the energy dissipated, the Moon’s rotation slowed until a single spin on its axis took the same amount of time as one trip around Earth. As the Moon bent and fluxed in this tug of war, energy was released in the form of heat. This means the Moon’s bulge was always a little out of alignment with Earth, yet always being pulled toward alignment by gravity. The part of the Moon that was pulled toward Earth would have shifted as the Moon spun, but always at a delay, since it takes time for so much material to rise and then later fall. Earth’s gravitational pull distorts the Moon into a slight football shape even today, but this distortion would have been much more dramatic when the Moon was both closer to Earth and less solid. The hot, molten object that coalesced from the ejected material would have been spinning wildly, with its shape changing as it was pulled at by Earth’s gravity. Earth’s Moon is thought to have formed when a massive object collided with Earth early in its history, splattering some of our planet into space. Tidal locking is common, but its dynamics are complex. A smiling face has been added to make it easier to see the Moon’s rotation. This should allow it to see plenty as it goes about completing its mission and searching for ice on the Moon.Each time that the Moon completes a turn, it also orbits the Earth once, keeping its far side perpetually hidden. This should allow it to come within nine miles of the lunar South Pole at its closest and 43,000 miles at its farthest. To make sure it can get close enough to the Moon, the small satellite will use a near-rectilinear halo orbit that is designed for energy efficiency. Now, with this plan to search for ice on the Moon, NASA is hoping to learn more about our lunar satellite before sending humans back to it. Just last month, NASA launched its Artemis I mission, which carried the Orion space capsule in an orbit around the Moon before returning to Earth just last week for a successful splashdown. During that time, it will use a reflectometer equipped with four lasers, all of which emit near-infrared light in wavelengths that should be easily absorbed by surface water ice on the Moon. Like some that have come before it, the Lunar Flashlight will continue its life orbiting the Moon until it either runs out of power or is decommissioned. This satellite will never return to Earth, either.
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