5. moon motions-student

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    The Moon

    -Around the Earth and in the Sky

    Why do we see phases of the Moon?

    When do we see the phases of the Moon? What causes eclipses?

    Our goals for learning:

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    Why do we see phases of the Moon?

    Lunar phases are

    a consequence of

    the Moons 27.3-

    day orbit aroundEarth

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    Phases of Moon

    Half of Moon is lit

    by the Sun and

    half is dark We see a different

    amount of the

    bright and dark

    faces as Moonorbits

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    Phases of the Moon: The View from Earth

    new

    crescent

    first quarter

    gibbous

    full

    gibbous

    last quarter

    crescent

    waxingMoon visible in afternoon/evening.Gets fuller and rises later each day.

    waningMoon visible in late night/morning.Gets less and sets later each day.

    }

    }

    A 29.5-day cycle

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    Moon Rise/Set by Phase

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    Thought Question

    What phase of the Moon is this?

    A. First quarter

    B. Waxing crescentC. Waxing gibbous

    D. Third quarter

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    We see only one side of Moon

    Synchronous rotation:

    the Moon rotates exactly

    once with each orbit

    That is why only one side

    is visible from Earth

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    Eclipses

    Definition:

    When light from an astronomical

    body is blocked by another body

    passing between it and the observer.

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    Any object can eclipse another

    For example there are binary stars called eclipsing

    binaries, because they are detected when the orbiting

    star is eclipsed.

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    What causes eclipses?

    The Astronomical bodies cast shadows.

    When an object passes through anothers

    shadow, there is an eclipse.

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    Most Common Types of Eclipse

    Solar Eclipse(Sun is blocked by

    Moons shadow)

    -occurs at New Moon

    Lunar Eclipse

    (Moon is blocked by

    Earths shadow)

    -occurs at Full Moon

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    Types of Eclipse

    Partial - Sun or Moon is partly covered.

    Total - Sun or Moon is completely covered overand goes dark.

    Annular - center of Sun is covered over, leaving

    a ring of light.

    Penumbral Eclipse - Moon is solely in thepenumbral shadow, only

    mildly darkened.

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    Eclipses Every Month?

    The Moons orbit is tilted 5 to ecliptic plane. Most alignments

    occur above or below the ecliptic. As a result we do notget an

    eclipse every month.

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    Eclipses Every Month?View from Earth

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    When Do Eclipses Occur?We have about two eclipse seasonseach year, when

    the Sun, Earth and Moon are in alignment and theMoon is on the plane of the ecliptic.

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    When Do Eclipses Occur?

    We then get a solar eclipse at new moon and a lunar

    eclipse at full moon.

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    Solar Eclipses

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    Total Solar Eclipses

    The Sun is 400 timeslarger than the Moon.

    The Moon is 400 timescloser than the Sun.

    Consequently, they appear to be about the same angular size.

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    Solar Eclipses

    Eye Protection Vital!

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    Total Solar Eclipse, 1999

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    Eye Safety

    Sunlight can permanently burn out the

    receptors in your eyes.

    Retinas have no pain sensors, You won'tknow until it's too late!

    Eclipses are especially dangerous, sincepeople are deliberately looking at the Sun.

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    Eye Safety

    Welder's Glass- excellent if expensive.

    Telescopes with Sun filters -excellent, but need to

    make sure it dies not get scratched.

    Pin hole cameras -You do not look at the Sun (it's

    cheap and works, but is not a cool-looking)

    Mylar eclipse glasses - cheap but not recommended.(They scratch far too easily, high risk of line blindness)

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    Total Solar Eclipse, Zambia 2001

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    Start of

    Eclipse

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    Sunpartially

    eclipsed

    Second Contact: the

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    Second Contact: the

    Beginning of Totality

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    Totality !

    Z bi t T t lit

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    Zambia at Totality

    Cl f Ed d i T t lit

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    Close-up of Edge during Totality

    (Baileys Beads)

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    Diamond Ring : End of Totality

    Composite of Entire Eclipse

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    Composite of Entire Eclipse,

    Zambia 2001

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    Annular Eclipses

    Moon is further away, so its angular size is

    slightly smaller than the Sun's angular size.

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    Annular Eclipse Sequence

    Greenland, 2003

    Partial Eclipse at Sunset

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    Partial Eclipse at Sunset,

    WA, July 2000

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    Partial Eclipse at Sunset sequence,

    WA, July 2000

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    Total Lunar Eclipse

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    Lunar Eclipse

    M b i i t b li d ( ti l)

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    Moon beginning to be eclipsed (partial)

    Moon mostl eclipsed

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    Moon mostly eclipsed

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    Moon eclipsed by penumbra

    Beginning of Totality

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    Beginning of Totality

    End of Totality

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    End of Totality

    Moon still in penumbra

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    Moon still in penumbra

    Moon coming out of shadow

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    Moon coming out of shadow

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    Full Sequence of Total Lunar Eclipse

    P di ti E li

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    Predicting Eclipses Eclipses recur with the 18 yr, 11 1/3 day

    saros cycle, but type (e.g., partial, total)and location may vary.

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    What have we learned?

    Why do we see phases of the Moon? Half the Moon is lit by the Sun; half is in

    shadow, and its appearance to us is

    determined by the relative positions of Sun,

    Moon, and Earth during the Moon's orbit.

    What causes eclipses?

    Lunar eclipse: Earths shadow on the Moon

    Solar eclipse: Moons shadow on Earth Tilt of Moons orbit means eclipses occur

    during two periods each year