Meteoroids are lumps of rock or iron that orbit the sun, just as planets, asteroids, and comets do. Meteoroids, especially the tiny particles called micrometeoroids, are extremely common throughout the solar system. They orbit the sun among the rocky inner planets, as well as the gas giants that make up the outer planets. Meteoroids are even found on the edge of the solar system, in regions called the Kuiper belt and the Oort cloud.
Different meteoroids travel around the sun at different speeds and in different orbits. The fastest meteoroids travel through the solar system at a speed of around 42 kilometers (26 miles) per second.
Many meteoroids are formed from the collision of asteroids, which orbit the sun between the paths of Mars and Jupiter in a region called the asteroid belt. As asteroids smash into each other, they produce crumbly debris—meteoroids. The force of the asteroid collision can throw the meteoroid debris—and sometimes the asteroids themselves—out of their regular orbit. This can put the meteoroids on a collision course with a planet or moon. Continue reading from National Geographic
A meteor is the streak of light that you see in the sky when a small piece of cometary or asteroidal material enters the atmosphere at high speed and burns up because of the frictional heating from the piece’s collision with the atoms and molecules in the atmosphere. Before the small bit of comet or asteroid enters Earth’s atmosphere, it floats through interplanetary space and is called a meteoroid.
Most meteoroids that enter the atmosphere burn up completely as meteors. In some cases, however, the meteoroid does not completely burn up, and the object actually makes it to Earth’s surface. The chunk that has survived its fiery journey is called a meteorite. A small body starts its life as a meteoroid floating through space between the planets until it makes a bright streak of light in Earth’s atmosphere as a meteor and then, if it isn’t consumed by frictional heating, finally lands on the ground as a meteorite. Continue reading from Britannica
Our solar system formed about 4.5 billion years ago from a dense cloud of interstellar gas and dust. The cloud collapsed, possibly due to the shockwave of a nearby exploding star, called a supernova. When this dust cloud collapsed, it formed a solar nebula—a spinning, swirling disk of material.
At the center, gravity pulled more and more material in. Eventually the pressure in the core was so great that hydrogen atoms began to combine and form helium, releasing a tremendous amount of energy. With that, our Sun was born, and it eventually amassed more than 99 percent of the available matter. Continue reading from NASA
