Our solar system consists of a sun, eight planets, and their moons. All of these objects orbit around the sun. If we stood on a stationary object, we would see that the earth makes a shadow. That is evidence that the Earth is moving around the sun. We can also observe this movement by looking at constellations. These groups of stars are known as constellations. They form recognizable shapes.
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The Sun is the source of the solar wind, which is a stream of charged particles flowing outward from the Sun. This solar wind creates a bubble-like region in the interstellar medium called the heliosphere. The pressure of the solar wind equals the pressure of the interstellar medium at this distance, known as the heliopause. Long-period comets are thought to be created in this cloud. In fact, it may exist at a distance of 1,000 times farther than the heliosphere. The Solar System is approximately 26,000 light-years from the center of the Milky Way galaxy. Most of the stars that we see are in the Orion Arm.
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The distance between us and other bodies in our solar system is not the only reason we cannot see them. The vast distance between us and other stars in the universe causes the signal to degrade. A 305-meter radio dish would lose all its AM signal before reaching Mars. In the same way, UHF television receivers would emit static when passing Jupiter, while FM radio stations would fade away before reaching Saturn.
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