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Our telescope will start off at Earth. Its final destination is Neptune. When it is launched from Earth, the first planet it will encounter is Mars. With a gravitational pull of only 3.721 m/s², the telescope can go near it, however should maintain at least a little distance. The next planet is Jupiter. With a gravitational pull of 24.79 m/s², the telescope will need to stay very far away from Jupiter to escape its extremely strong gravitation pull. The next planet is Saturn. Saturn has a gravitational pull of 10.44 m/s², which is relatively small for its size, however, the telescope should still keep its distance to avoid being sucked in by Saturn's gravity. The final planet standing between the telescope and Neptune is Uranus. Uranus has a gravitational pull of 8.87 m/s². The telescope should try to keep a reasonable amount of distance between itself and Uranus. The telescope is now at its final destination, Neptune. Neptune has a gravitational pull of 11.15 m/s², so the telescope should try to keep a moderate amount of distance between it and Neptune. It is now at its final destination. It can now orbit the Sun with Neptune.

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We are putting a magnet inside our space telescope to protect it from during it's journey. The magnet will generate a magnetic field that will help our space telescope reach its final destination, Neptune, safely.

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Saturn's magnetic field is generated as material cycles deep within the planet's interior. Saturn's magnetic field has North and South poles and rotates with the planet. Unlike Earth's magnetic field, the magnetic poles of Saturn's magnetosphere are perfectly aligned with Saturn's geographic poles. Saturn's magnetosphere is strong enough to protect Saturn from charged solar particles.

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Earth is 1 AU / 93,000,000 miles from the Sun. Saturn is 9.5 AUs / 886,000,000 miles from the Sun. When scaling Saturn's distance from the Sun down, we decided that 1 AU will be equal to 1 foot. The scaled distance of Earth from the Sun is one foot. The scaled distance of Saturn from the Sun is 9.5 feet.

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(Saturns eclipse. Source: Envato Element)

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Since Saturn is a gas planet the planet can experience total solar eclipses. The planet has big moons and the sun appears small to the planet. However, it is impossible to stand on the planet itself and see the solar system. As seen on the image the planet is affected but the ring is untouched.

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(Saturn's rings of ice and dust. Source: Hindustan Times)

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Saturn has a mass of 5.683 x 10^26 kilograms, and it is 9.58 AU's (Astronomical Units) away from the sun.

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Saturn's diameter is 72,367 miles. When scaling Saturn we decided to scale down Saturn using the Sun, with the Sun being 500 cm when scaled and Saturn being 11.4 times smaller than the Sun. The scaled diameter of Saturn is 43.85 centimeters.

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(The tiny circles are Saturn's moons. Source: Whats-Your-Sign)

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Saturn has 82 moons. 53 of Saturn's moons are named and they are conformed to be moons. The rest are not yet named or confirmed as moons. Saturn's biggest moon is Titan. Titian is as big as Mercury. Mimas, Saturn's smallest moon has a radius of fewer than 123 miles. Saturn's moons take different times to orbit Saturn. The least is 11 hours and the most is 79 days!

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Saturn does not have any geographic features as it is a gas giant and doesn't have a solid surface. There is no evidence that Saturn has tectonic plates.

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Saturn has a tilt of 26.73 degrees and experiences seasons just like Earth due to its tilt. Each season on Saturn is more than seven Earth years long, which means that Earth experiences several seasons in the time that Saturn experiences one.

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(An artist’s rendition of what Cassini’s crash into Saturn will look like. Source: Vox)

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Saturn is mostly composed of 75% H₂ (hydrogen) and 25% He (helium). Its dense core is composed of iron and nickel surrounded by rocky material and other compounds solidified by pressure and heat.