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the moon, earths closest celestial neighbor, formed approximately 4.5 billion years ago through a series of dramatic events. the process began when a mars - sized object, often referred to as theia, collided with the early earth. this massive impact ejected a tremendous amount of debris into space, marking the first step in the moons creation. the collision was so powerful that it altered earths composition, scattering molten material into orbit. following the impact, the ejected debris started to coalesce due to gravitational forces. over thousands of years, these fragments clumped together, gradually forming a larger body. this accretion process was slow but steady, as smaller pieces merged into bigger ones. by this stage, the proto - moon was taking shape, orbiting earth in a chaotic dance of rock and dust. finally, the newly formed moon stabilized in its orbit, settling into the position we observe today. over millions of years, it cooled and developed its familiar features, such as craters and maria. this sequential process, from collision to stabilization, explains how the moon became earths constant companion, influencing tides and lighting up the night sky. text structures what type of text structure is used in the article? sequence compare & contrast problem & solution
The text describes the moon's formation in a step - by - step manner. It starts with the collision (first step), then the coalescing of debris (second step), and finally the stabilization (last step). This is characteristic of a sequence text structure where events are presented in the order they occurred.
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