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Day 2 notes Ch. 1 second half Motion of the Moon and eclipses
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Motion of the Moon and Phases of the Moon The development of the current model of the solar system began with careful measurement of the movement of the Sun and the Moon. To understand this, let’s review the motion and the phases of the Moon, as we currently understand them. When we watch the Moon, it’s shape changes from one night to the next:
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From the astronomy picture of the day web site ( link )link
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Earth and Moon, separately From Apollo 17 spacecraftFrom Earth
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Earth and Moon, in one picture from the Galileo space probe as it traveled by the Earth on its way to Jupiter.
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Lunar Phases
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Lunar Eclipse (there are many good web resources) (link)(link)
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Lunar Eclipse
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Solar Eclipse
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Solar Eclipse over China
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Solar Eclipse over Zambia sequence of photos superimposed to show the movement of the Sun
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Solar Eclipse over Antarctica
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Solar Eclipse – composite picture
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Solar Eclipse – composite picture (cropped)
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Solar Eclipse Types
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Penumbra and Umbra
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Shadow of Moon seen from Mir space station
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Animation of Moon eclipsing the Sun, as seen from inside the umbra.
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Animation of the view from the dark side of the Moon, looking down on the Earth during a solar eclipse.
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Eclipse Geometry is favorable close to the equinoxes.
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Eclipse Tracks (also see NASA Eclipse page, Mr. Eclipse and Eclipser)NASA Eclipse pageMr. Eclipse Eclipser
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Web page at NASA devoted to this eclipse (link)link
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Example of a map of the eclipse path, showing the center line and boundaries of the region under the umbra (total) For the total eclipse of 29 March 2006
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Transits occur when a planet crosses between the Earth and the Sun, so we see a dark spot cross the Sun. This can only happen with Venus link or Mercury link.link Occultations occur when the Moon blocks out (occults) a planet. linklink
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To do: Get the textbook. Finish Ch. 1. Start Ch. 2 ! Look at the syllabus and the dates. Mark your calendars for exam dates. First exam is exactly 2 weeks away! Enjoy the weekend.
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