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Our Solar System Consists of:
Sun Eight planets and their moons The dwarf planets The planets are all unique and differ in terms of their: Size (volume) Surface temperature Chemical elements (e.g. H2, He, O2 and C) Gravitational field strength (surface gravity)
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The planets orbit the sun in the following order: M V E M J S U N P
“My very elderly mother just sent us nine pizzas”
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The Inner (Terrestrial) Planets
The four planets closest to the sun are: Mercury, Venus, Earth and Mars Characteristically they are: Small High in density Mainly composed of rocks/metals
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The Inner (Terrestrial) Planets
Venus Mercury Earth Mars
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The Outer Planets (Gas Giants)
The four planets farthest from the sun are: Jupiter, Saturn, Uranus & Neptune Characteristically they are: Large Low in density Mainly composed of gases such as hydrogen and helium Separated from the inner planets by the asteroid belt.
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The Outer (Gas Giant) Planets
Jupiter Saturn Uranus Neptune
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Dwarf Planets The big difference between a dwarf planet and a regular planet is that: A dwarf planet’s path around the sun is full of other objects like asteroids and comets whereas a regular planet has a clear path Pluto Due to its strange orbit and tiny size astronomers questioned whether it should be considered a planet. A decision was made to reclassify Pluto to a dwarf planet in 2006.
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Ceres, Eris, MakeMake & Haumea
The Dwarf Planets Ceres, Eris, MakeMake & Haumea Ceres (formally an asteroid and still found in the asteroid belt), Eris, MakeMake & Haumea are also dwarf planets. They are different from planets because they are not big enough to clear their orbits and thus orbit with a lot of other debris. Eris Ceres Pluto
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