2 Men on the MoonThe Apollo space program’s objective was to land men on the moon and bring them safely back home.1st moon landing was July 20, 1969 in the Sea of TranquilityFrom 1969 through 1972, 12 men from 6 missions walked on the moon.Neil A. Armstrong, commander Michael Collins, command module pilot Edwin E. Aldrin, Jr., lunar module pilot
3 The Moon’s Characteristics Diameter: 3476km (about ¼ Earth’s)Mass: about 1/80th that of the EarthGravity: about 1/6th that of EarthAverage Distance from Earth: 363,301kmComparative sizes of the Earth and the Moon, as imaged by Deep Impact in September 2008 from 50 million km away. Credit: NASAMoon Facts:
4 The Moon’s Characteristics The surface temperature at the equator during the day is 134oC, and at night is -153o C.The moon is not round, but egg shaped with the large end pointed towards earth. The moon has no significant atmosphere or clouds.Full Moon photograph taken from Madison, AlabamaPhoto Credit: Gregory H. Revera
5 The Moon’s Structure Similar to Earth’s Iron-rich inner core with a radius of nearly 150 milesFluid, primarily liquid-iron, outer coreA partially molten boundary layer around the coreMantleCrust – 60 km thickRegolith: layer of dust, soil, and broken rock covering most of the moonRegolith layer is anywhere from 3-20m thick; formed by the impact of meteors over billions of years.
6 Features of the Moon Highlands: mountain ranges Maria (MAHR-ee-uh; singular-mare; Latin for seas): broad, smooth, lowland plains; the dark areas; vast solidified pools of ancient basaltic lava; evidence that the moon was once hot and activeNear side (left) and far side (right) of the Moon, by Lunar Reconnaissance Orbiter
7 Features of the Moon Rilles: long valleys Craters: primarily impact craters formed by the continuous bombardment of the moon by meteoritesEstimated to be about 300,000 larger than 1km acrossNamed for scholars, scientists, artists and explorers; Copernicus is an exampleNear side (left) and far side (right) of the Moon, by Lunar Reconnaissance Orbiter
8 Movements of the MoonThe Moon's orbit is inclined about 5 degrees from the Earth's ecliptic orbit around the sun.One revolution takes about 27.3 days. (The Orbital speed of the moon is 3,680 km/h.)One rotation of the moon on its axis takes about the same 27.3 days.Because a revolution and a rotation take the same time, we always see the same side of the moon.
9 Movements of the Moon The orbit of the moon is elliptical. Perigee: point closest to Earth; about 362,600 kmApogee: point farthest from Earth; about 405,400km
10 Origin of the Moon The moon is about 4.5 billions years old Formation:One Theory: The moon formed far away from the Earth and was then “captured” by the Earth’s gravity.Second Theory: The moon formed along with the Earth.Third Theory: The moon split off from the Earth due to centrifugal force.Each of these theories fails in some way to account for all the evidence we have.Theory one – would require too great and atmosphere to dissipate the energy of the passing moon to capture it; also would not account for the similarity in composition.Theory two: doesn’t explain the depletion of metallic iron in the moonTheory three would require too much initial spin for the EarthNone account for the high angular momentum of the Earth-Moon system.
11 Origin of the MoonCurrent Prevailing Theory: Soon after the Earth was formed, a Mars-sized asteroid impacted it and blasted material into orbit around the Earth. That material came together to form the moon.Recent evidence (2012) suggests that this may not be correct, as the moon’s composition appears to be exactly the same as the Earth’s, with no second contributor.
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