The Moon
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The most widely accepted theory for how the Moon formed is the 'giant-impact hypothesis'. This theory suggests that a Mars-sized object called Theia, collided with the early Earth billions of years ago. The debris that was ejected out from this tremendous impact, a mix of material (gas, dust and rock) from both Earth and Theia, went into a circular orbit around Earth. The material collided and coalesced (came together) in orbit around Earth to form the Moon.Â
Our Moon is a natural object that orbits around the Earth. When we look at it with our own eyes, we see brighter spots and darker patches.Â
Rocks collected from the Moon show that these darker patches are ancient lava beds (maria), created when our Moon was still forming and made mostly of liquid rock. This shows the Moon was once molten and covered in lava, but was also made of material that is similar, yet different from Earth.
Click on this link to access the interactive on a new tab: https://bit.ly/3HSDd7ZÂ
On the left-hand menu, click on Projections > select "Lunar Globe (3D)"
Try and find as many features from the "Moon Features You Can See From Earth" poster above. You may need to use the search function at the top of left hand corner (directly under the ACT Lunar/LROC logo).
Like other moons and planets, our moon does not give off any of its own light or heat, so it can only be seen when it is being lit up by the Sun. This reflected light can then shine down onto our planet and affect how wildlife behave at night.Â
Although the Moon receives a similar amount of sunlight as Earth, it has no atmosphere and so there is no weather to even out the temperatures. So the part of the Moon that faces the Sun can reach as high as 127°C, but the part that is facing away from the Sun can get as cold as -173°C.Â
Instead, the Moon has a very thin exosphere that has a density vastly lower than Earth's atmosphere and contains elements like helium, neon and argon.
Click on this link to access the interactive on a new tab: https://science.nasa.gov/moon/composition/?intent=021. Explore the Tools panel on the right hand side.Â
Tools > Data: Explore the digital elevation map, gravity map, surface slope, hydrogen abundance and surface roughness. What does this tell you about the conditions on Mars?
When rocks or other objects crash into the Moon, they create craters, hole-like structures in the surface. Craters have been found in many sizes on the Moon from 300km across down to a fraction of a millimetre in diameter. We see far fewer craters on Earth because our weather causes them to be covered in dirt, water, or ice, and they can also be worn away by wind and weather. The Moon has no atmosphere to slow down the rocks nor create the weather needed to cover / wear away the craters.Â
Linne crater (simple crater) - small, bowl-shaped with round floors.
Aristarchus crater (complex crater) - central peaks, terraces and flat floors.
Impact basins are massive craters (spanning more than 300 km in diameter) formed by large asteroids or meteorites. The impact is so great that the impact site rebounds, melts and cracks.Â
Magma comes up through the cracks in the crust, flows as lava and cools as dark igneous rock. These dark areas we see on the Moon's surface are called maria (singular = mare).Â
Over a long period of time, all of the moons and planets in the solar system are hit by rocks, meteors and other objects that are floating in space.Â
Even though the Earth has craters, our planet doesn't seem to have nearly as many as the Moon.Â
Why do you think this is?
atmosphere: The layer of gases that surrounds a planet or moon.
crater: A bowl-shaped hole on the surface of a planet or moon, formed by the impact of a meteorite or asteroid.
diameter: The distance from one side of a circle or sphere, straight across to the other side, passing through the centre.
exosphere: The outermost layer of a planet’s or moon’s atmosphere, where the air is very thin.
impact: When a large object hits another object, like a meteor striking the Moon, forming a crater.
mare (maria = plural): A large, dark area on the Moon’s surface, formed by ancient lava flows.Â
reflect: To bounce light, sound, or heat off a surface instead of absorbing it.