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Published byMolly Allison Modified over 6 years ago
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“Earthrise” Apollo 8
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MINOR BODIES OF THE SOLAR SYSTEM
CHAPTER 28 THE MOON
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Sputnik Launched 1957 Initiated the space race Russian Launched 1958
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“LUNA” – Latin for Moon The Moon - A natural satellite
Between … six Apollo spacecrafts sent to the moon. Gravity not strong enough to hold a significant atmosphere (no atmosphere) Surface temperatures vary widely. 134oC (day) to -170oC (night) Reflects light from the sun Less massive, 1/6th the gravity of Earth.
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The space race 1st man in space (Russian): 1961- Yuri Gagarin
1st American in space: Alan Shepard 1st American to orbit the earth: 1962-John Glenn 1st American space walk: 1965 – Ed White 1st Americans to land on moon: Neil Armstrong stepped down first, then Buzz Aldrin, and also Michael Collins
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The Lunar Surface Light patches - highlands * Dark patches
- solidified lava - “Maria” - “Mare” = “Sea” - basalt rocks Craters - depressions Rilles - long deep channels (lava) Ridges
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Rilles
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Regolith Lunar Rocks Dust & rock layer Due to meteorite impacts
Many similar to Earth Elements in different proportions Igneous Silicon and oxygen (surface) Basalts (lava flows) breccias
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Interior of the moon Data collected from seismographs Crust
Near Side (always facing Earth) thinner, more mare Far Side (always faces away) more mountainous Mantle – thick, solid Core – small, Fe (Iron)
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Formation of the moon Giant Impact Hypothesis
A large Mars-sized object collided with Earth 4 billion years ago Earth was molten, parts of Earth were ejected into space; the debris clumped together to form the moon. The moon started out molten and cooled over time. Many impact craters formed Craters that are more recent show rays (regolith).
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Moon’s formation
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Earth and moon revolve around each other
X= barycenter Rotation = 27.3 days Revolution = 27.3 days Earth and moon revolve around each other - Barycenter (the point of revolution) Apogee Point farthest in orbit Perigee Point closest in orbit
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Phases of the moon Due to the revolution of the moon
New moon – sunlight hits only far side of moon, not lighted Waxing – size of the lighted part of the moon is increasing Waxing crescent First quarter Waxing gibbous Full moon – sunlight hits the near side of the moon Waning – size of the lighted part of the moon is decreasing Waning gibbous Third quarter Waning crescent Time from new moon to new moon = 29.5 days Blue moon – the second full moon that happens in a month
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Eclipse – when one celestial body passes into the shadow of another
Lunar eclipse Solar eclipse The Earth is between the moon and the sun. Total lunar eclipse April 15, 2014 Partial lunar eclipse August 4, 2015 Moon looks red Moon is directly between the sun and earth. Sun’s light is blocked by moon. Total solar eclipse August 21, 2017 Partial solar eclipse October 23, 2014
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Solar eclipse Lunar eclipse
Only seen by those in umbra Seen by everyone on dark side of the Earth.
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Tides on Earth Tides form due to the moon’s (and the sun’s) gravitational pull on the Earth. The near side of the Earth is pulled more than the far side. Earth’s rotation sets up a regular rhythm of tidal bulges each day. Centrifugal force causes opposite sides of the earth to experience the same tidal rhythm.
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High and Low tides Semi-diurnal 2 highs and 2 lows/day
Diurnal 1 high and 1 low/day SUN Sun’s Gravitational Pull
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Spring and Neap tides Spring Tides Neap Tides
Occurs at full and new moons Every two weeks Combined effect Bigger tidal range Higher highs, lower lows. Neap Tides Occurs at 3rd and 1st quarter Opposing forces Less extreme tidal range
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