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The Planets SPACE
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Learning Goals To be able to describe the planets of our solar system
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Classifying a Planet To be considered a planet, a celestial object must: 1. Orbit a star (such as the Sun) and no other celestial object 2. Contain enough mass so that its gravity pulls it into a round or spherical shape 3. Be able to clear other celestial objects out of its orbit
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Planetary Motion - Revolution All of the planets revolve, or travel around the Sun The orbits are elliptical, or oval-shaped Earth completes one revolution around the Sun in about 365 days, which we call 1 year The other planets take different amounts of time to complete one revolution (Mercury – 88 days; Neptune – 164 years)
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Discovered in 1930
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Planetary Motion - Rotation Planets also rotate, or spin or turn on an axis An axis is an imaginary line around which an object rotates Earth’s axis runs from pole to pole Most planets rotate in a west-to-east direction, similar to Earth Venus rotates in the opposite direction
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Planetary Motion - Rotation Earth’s rotation causes our day and night Earth completes one rotation every 24 hours, which is one day The amount of time a planet takes to rotate is equal to the length of one day on that planet
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Mercury
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Closest to the Sun Hot days ( 430 °C ); Cold nights ( -170 °C ) Mercury is 0.38 AU from the Sun Revolution of 88 days (= 1 year) Rotates once every 59 days (= 1 day) No moons Temperatures range from -170 °C at night to 430 °C during the day Mariner 10 first visited in 1974 & 1975, Messenger began orbiting in 2011
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Venus
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Volcanoes (toxic atmosphere) Brightest in night sky after Moon Hottest planet (450 °C, max 480 °C) Venus is 0.72 AU from the Sun Revolution of 224.7 days Rotation of 243 days Diameter is 0.95 times Earth’s No moons Opposite rotation to Earth
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Earth
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Liquid water Sustains life Earth is 1 AU from the Sun Revolution of 365 days Rotation of 24 hours Diameter is 12, 740 km 1 moon (the Moon) Temperatures range from -85 °C to 65 °C
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Mars
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Red soil ( red planet ) Most studied planet Evidence of water, volcanoes, glaciers in the past Mars is 1.52 AU from the Sun Revolution – 687 days (1.88 years); Rotation 24.6 hours Diameter is 0.53 times Earth’s 2 moons (Phobos and Deimos) Temperatures range from -133 °C to 27 °C Mariner 4 flyby in 1965, 2 Viking landers in 1976, Mars Pathfinder in 1997, Mars Surveyor (2000’s), Mars Science Laboratory (2012)
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Terrestrial Planets Relative Sizes
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Jupiter
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Largest planet Great Red Spot – giant hurricane 63 known moons (Io, Europa, Ganymede, Callisto) Jupiter is 5.20 AU from the Sun Revolution of 11.9 years Rotation of 9.9 hours Diameter is 11.0 times Earth’s Temperature around -153 °C
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Jupiter Visited by Pioneer 10 in 1973, then Pioneer 11, Voyager 1 and 2, Ulysses, Cassini-Huygens, and Galileo orbited it for 8 years 1994, comet Shoemaker-Levy 9 was torn apart and pieces crashed into Jupiter
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Saturn
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Over 1000 rings 62 known moons (Titan) Saturn is 9.5 AU from the Sun Revolution of 29.46 years Rotation of 10.2 hours Diameter is 9.4 times Earth’s Temperature around -185 °C Visited by Pioneer 11 (1979), Voyager 1 and 2, Cassini (recent)
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Uranus
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Rotates on its side Strong winds Uranus is 19.2 AU from the Sun Revolution of 83.75 years Rotation of 17.2 hours Diameter is 4 times Earth’s 27 moons and some rings (1977) Temperature around -210 °C Visited by Voyager 2 in 1986 Discovered as a planet in 1781
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Neptune
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Predicted and then discovered in 1846 Neptune is 30 AU from the Sun Revolution of 164.8 years Rotation of 16.1 hours Diameter is 3.9 times Earth’s 13 Moons and some rings Temperature around -220 °C Visited by Voyager 2 in 1989
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Relative Size of Jovian Planets
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Distances from Sun
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Tilt of Planets
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Dwarf Planets A dwarf planet is a celestial object that orbits the Sun and has a spherical shape, but does not clear its orbit Five recognized dwarf planets: Ceres, Pluto, Haumea, Makemake, Eris Scientists estimate another 70 000 icy objects beyond Neptune Pluto takes 248 years to orbit Sun, Eris takes twice as long
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Asteroid Belt An asteroid belt is located between the orbits of Mars and Jupiter The dwarf planet Ceres is located in the asteroid belt
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The Moon
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Earth’s only natural satellite About 384,000 km from Earth The moon revolves around Earth and rotates on its axis every 27.32 days For this reason, we always see the same side of the moon Diameter is 0.27 times Earth’s Gravity is 1/6 of Earth’s The Moon is responsible for tides on Earth
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Success Criteria I CAN describe the similarities and differences among the planets in our solar system
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