EARTH’S ORBITAL CHANGES

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    EARTHS ORBITALEARTHS ORBITALCHANGESCHANGES

    ANDAND

    ITS EFFECT ONITS EFFECT ONCLIMATECLIMATE

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    SOME BASIC CONCEPTSSOME BASIC CONCEPTS

    Earths climate engine is theEarths climate engine is theSUNSUN..

    Small variations in solar radiation can haveSmall variations in solar radiation can have

    large climatic effects.large climatic effects. Earths orbital movementsEarths orbital movements -- REVOLUTIONREVOLUTION,,

    ROTATIONROTATION andandWOBBLINGWOBBLING..

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    OLDER THEORIESOLDER THEORIES

    Joseph Alphonse AdhemarJoseph Alphonse Adhemar was the first to suggest thatwas the first to suggest that iceice

    agesages were controlled bywere controlled by astronomical forces. Adhemarastronomical forces. Adhemar

    reasoned that because the southern hemisphere had more hoursreasoned that because the southern hemisphere had more hours

    of darkness in winter, it must be cooling, and attributedof darkness in winter, it must be cooling, and attributed

    thethe AntarcticAntarctic ice sheetice sheet to this. Adhemar knew of the 22,000to this. Adhemar knew of the 22,000year cycle ofyear cycle of precession of the equinoxes, and theorised thatprecession of the equinoxes, and theorised that

    the ice ages occurred in this cycle.the ice ages occurred in this cycle.

    JamesJames CrollCroll, suggested in 1875 that long term changes in the, suggested in 1875 that long term changes in the

    amount of solar radiation reaching the earth were controlled byamount of solar radiation reaching the earth were controlled byrhythmic variations in the earths orbit around the sun and thatrhythmic variations in the earths orbit around the sun and that

    the solar radiation variations produced the periodic climatethe solar radiation variations produced the periodic climate

    changes which were being discovered by contemporarychanges which were being discovered by contemporary

    geologists.geologists.

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    Milankovitch VariationsMilankovitch Variations

    Milutin Milankovitch,Serbian mathematician.

    1924--He suggested variations in earths orbitvariations in earths orbit

    around the Sun affect the amount of solararound the Sun affect the amount of solar

    radiation received on Earths surface.radiation received on Earths surface.

    Orbital scale changes occur over tens toOrbital scale changes occur over tens to

    hundreds of thousands of years.hundreds of thousands of years.

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    Milankovitch CycleMilankovitch Cycle

    ECCENTRICITYECCENTRICITY-- EarthsElliptical Orbit.EarthsElliptical Orbit.

    OBLIQUITYOBLIQUITY-- Earths Tilt.Earths Tilt.

    PRECESSIONPRECESSION -- Earths Wobble.Earths Wobble.

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    EccentricityEccentricity Eccentricity is a measure of how elliptical an orbit is.Eccentricity is a measure of how elliptical an orbit is.

    A planets closest approach to the sun is called theA planets closest approach to the sun is called the perihelionperihelion

    and the furthest distance is theand the furthest distance is the aphelionaphelion..

    When e=0 , the orbit is circular. As e gets close to 1 , the orbitWhen e=0 , the orbit is circular. As e gets close to 1 , the orbit

    becomes more elongated.becomes more elongated.

    When e>0 , note that the sun is not in the centre of the ellipse.When e>0 , note that the sun is not in the centre of the ellipse.

    Eccentricity0 Eccentricity0.5

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    The larger the eccentricity ,the greater the difference in solarThe larger the eccentricity ,the greater the difference in solar

    radiation that reaches the earth at perihelion versus aphelion.radiation that reaches the earth at perihelion versus aphelion.

    At its current value of e=0.017 , this difference is 6.7%.At its current value of e=0.017 , this difference is 6.7%.

    When the orbit is at its most elliptical, the amount of solarWhen the orbit is at its most elliptical, the amount of solar

    radiation at perihelion will be about 23% more than at aphelion.radiation at perihelion will be about 23% more than at aphelion.

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    Eccentricity VariationsEccentricity Variations

    Current value:Current value: 0.0170.017

    Range:Range: 0.00050.0005 --0.06070.0607

    Period(s):Period(s): ~100,000 yrs~100,000 yrs

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    What makesWhat makes ECCENTRICITYECCENTRICITY vary?vary?

    TheThe gravitationalgravitational pull of the otherplanets.pull of the otherplanets.

    The pull of another planet is strongest when the planets

    are close together.

    The Earth's eccentricity varies primarily du

    eto interactions with the gravitational fields of

    Jupiter and Saturn.

    y y

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    ObliquityObliquity --Axial TiltAxial Tilt

    The changes in the axial tilt (22The changes in the axial tilt (22oo toto

    24.524.5oo) of the Earth.) of the Earth.

    The greater the tilt the greater theThe greater the tilt the greater thecontrast between summer and wintercontrast between summer and winter

    temperatures.temperatures.

    Cycle is about 41,000 years.Cycle is about 41,000 years.

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    OBLIQUITY VARIATIONSOBLIQUITY VARIATIONS

    Current value:Current value: 23.523.5oo

    Range:Range: 2222oo--24.524.5oo

    Period:Period: 41,000 yrs.41,000 yrs.

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    PrecessionPrecession The wobble of the Earth as it spins on its axisThe wobble of the Earth as it spins on its axis

    This wobble follows a 26,000 year cycle.This wobble follows a 26,000 year cycle.

    The earths axis now pointsThe earths axis now points

    at Polaris ,our north star.at Polaris ,our north star.

    In 13,000 years it willIn 13,000 years it will

    point towards the star Vegapoint towards the star Vega..

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    11,000 yrs ago*TODAY

    y

    N

    S

    y

    N

    S

    POLARIS VEGA

    *Actually, Vega would have been the North Star morelike 13,000 years ago.

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    PRECESSION VARIATIONSPRECESSION VARIATIONS

    Range:Range: 00--360360oo

    Current value:Current value: PerihelionPerihelion

    presently occurs aroundpresently occurs aroundJanuary 3, whileJanuary 3, whileaphelion is around Julyaphelion is around July4.4.

    North poleNorth pole is pointedis pointed

    almost directlyalmost directly awayaway fromfromthe Sun at perihelion.the Sun at perihelion.

    Periods:Periods: ~26,000 yrs~26,000 yrs

    y

    N

    S

    Today

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    What makes theWhat makes the OBLIQUITYOBLIQUITY andand PRECESSIONPRECESSION

    vary?vary?

    gEquator

    N

    S

    g

    The Moons torque on

    the Earth is about twice

    as strong as the Suns.

    ii) The pull of the Sun and the Moon on Earths) The pull of the Sun and the Moon on Earthsequatorial bulge.equatorial bulge.

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    ii) Also, the tilting of Earths orbital plane.ii) Also, the tilting of Earths orbital plane.

    N

    y

    S

    y

    S

    N

    Tilting of the orbital plane is like

    a dinner plate rolling on a tableIf the earth was perfectly spherical,

    its spin axis would always point in

    the same direction but it would make

    a different angle with its orbital plane

    as the plane moved around.

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    Optimal Conditions for Glaciation:

    1. Low obliquity (low seasonal contrast)

    2. High eccentricity and NH summers during aphelion

    (cold summers in the north).

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    Optimal Conditions forDeglaciation:

    1. High obliquity (high seasonal contrast)

    2. High eccentricity and NH summers during perihelion

    (hot summers in the north)

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    INSOLATIONINSOLATION

    Insolation is described as the intensity of SolarInsolation is described as the intensity of Solar

    radiation that is received on Earth.radiation that is received on Earth.

    The intensity of the solar radiation and itsThe intensity of the solar radiation and its

    correlation between eccentricity and obliquitycorrelation between eccentricity and obliquity

    help define seasons and play a major role inhelp define seasons and play a major role in

    glacial cycles.glacial cycles.

    Milankovitchs key insight:

    I

    ce and snow are not completely melted during very cold summers.

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    Orbital variations in received insolation:

    Each orbital influence has its own distinctive

    pattern of influence through time. They combine to

    vary sunlight on Earth.

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    INSOLATION AT 65INSOLATION AT 65NN

    High latitude summerHigh latitude summerinsolation (june, 65insolation (june, 65n) hasn) has

    been regarded as an index ofbeen regarded as an index oforbital forcing of glaciation.orbital forcing of glaciation.

    (This is the original(This is the originalMilankovitch hypothesis:Milankovitch hypothesis:cool summers are beneficialcool summers are beneficialto ice growth.)to ice growth.)

    For low summer insolation:For low summer insolation:

    aphelion in summer (esp.aphelion in summer (esp.With high eccentricity), lowWith high eccentricity), lowobliquity.obliquity.

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    http://www.ngdc.noaa.gov/paleo/slides/images/base/iceage13.gif

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    This diagram shows the combined effect of Eccentricity ,This diagram shows the combined effect of Eccentricity ,

    Obliquility and Precession on solar radiation.Obliquility and Precession on solar radiation.

    The blue strips marked on the graph shows the periods ofThe blue strips marked on the graph shows the periods of

    glaciation.glaciation.

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    HH1818OO andandGlobal Ice VolumeGlobal Ice Volume

    Asicesheetsgrow, thewaterremovedfromthe oceanAsicesheetsgrow, thewaterremovedfromthe ocean

    haslowerhaslowerHH1818O thanthewaterthatremains.O thanthewaterthatremains.

    ThustheThustheHH1818O value ofseawaterintheglobal oceanisO value ofseawaterintheglobal oceanis

    linearlycorrelatedwithice volume (largerlinearlycorrelatedwithice volume (largerHH1818OO largericesheets).largericesheets).

    Regions ofthe oceaninwhichevaporationexceedsRegions ofthe oceaninwhichevaporationexceeds

    precipitationareenrichedinprecipitationareenrichedinHH1818O, and vice versa.O, and vice versa.

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    This image (Below) is a graphical represtentation of

    the Milankovitch

    Climate Theory over a 15,000 yearperiod. It

    illustrates changesin insolation due the Milankovitch Cycles. Note the

    uniform insolation

    levels at -19000 yr, this would denote the end of a

    glacialperiod.Looking at this model we can see a visualrepresentation of our current interglacialperiod. At -

    11000 we were

    experiencing a maxima in solar radiation in thenorthern hemisphere.

    Difference in northern hemisphere insolation at summer solstice

    relative to today.

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    Orbital forcing of Earths climateOrbital forcing of Earths climate

    Changes in Earths orbital geometry

    (eccentricity, tilt, precession).

    Changes in the seasonal distribution of

    Insolation (heat) as a function of latitude.

    Glacial-interglacial climate change.