Erth2404 l1 Intro

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    EngineeringGeoscience

    ERTH2404

    Dr.JasonMah

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    InstructorInformation

    JasonMah

    BASc inMechanicalEngineering

    PhDinEarthSciences

    Officehours

    Room2120Herzberg,5:30PM 7:00PM

    Emailforappointment

    Email:[email protected]

    2

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    CourseInformation Lectures:Mon&Wed,4:05 5:25

    TextRequired:GeologyforEngineersandEnvironmentalScientists,3rdEd.,A.E.Kehew Availableatthebookstore Textonreserveinlibrary

    Labs:5Sections ODD/EVEN(labseveryotherweek)

    Labmanualrequired:Coursepack AvailableatScienceStores,room118Steacie

    3

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    CourseEvaluationEvaluation

    Theoryexams Midtermexam

    Feb27

    Lectures

    beforethestudybreak

    35%

    Finalexam

    (Endofterm)

    Lectures

    afterthestudybreak

    35%

    Laboratorywork Labexam

    (March4 15)

    Labs1,2,3 15%

    LabQuizzes Labs1,2,3,4 10%

    Lab4Assignment (handedinfor

    grading)

    5%

    Total 100%

    Apassinggrademustbeachievedinthelabtocompletethecourse.

    4

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    ImportantDates

    Nolabsthisweek

    January14:StartofEVENlabgroup

    January31:Lastdaytowithdrawwithfullfee

    adjustment February27:MidtermExam(duringclass)

    March4 15:Labexam(duringlab)

    April8:Lastlecture

    5

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    StudentAccommodation

    Disability,pregnancy,religiousobligations

    Mayeffecttimingforexams,labs

    Alertmeduringfirsttwoweeksofclassif

    needaccommodation DeadlineisJan21,2013foracademic

    accommodationsforthelabexam

    EquityServiceswebsite:

    http://carleton.ca/equity/accommodation

    6

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    OtherInformation

    CuLearn

    Allcourseinformationpostedonline

    SignonthroughCarletonwebsitemainpage

    DiscussionGroupavailable

    Deferredexams

    Notificationrequiredwithin5workingdays

    Contactme(notClaireSamson)

    Plagiarism

    7

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    AsaCourtesy

    8

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    Whyshouldyoutakethiscourse?

    Studyofourplanet:

    atmosphere,hydrosphere,lithosphere;

    interactions Everythingisrelated

    Implicationsofearth

    scienceproblems

    to

    engineering

    9

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    ImpactofPlanetonOrganisms

    1989LomaPrieta

    Earthquake:

    Oakland,

    Cypress

    freeway

    10

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    ImpactofPlanetonOrganisms

    2011Thoku,Japan,earthquakeandtsunami

    11

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    ImpactofPlanetonOrganisms

    2012Strombolivolcano,Italy

    12

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    ImpactofPlanetonOrganisms

    2012,HurricaneIrene,NewYork13

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    ImpactofHumansonPlanet

    Climatechange

    Ozone

    depletion Airpollution

    Acidrain

    16

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    CourseTopics

    GeologicalTime

    MineralsandRocks

    Platetectonics,volcanoes,earthquakes

    Rockmechanicsandstructures Massmovement

    Hydrology

    Earthresources

    17

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    CourseObjectives

    Attheendofterm,youwillbe:

    Abletodescribeearthmaterialsandprocessesfrombothengineeringandgeologicalperspectives

    Awareoftheimpactofgeologicalprocesseson

    engineeringwork

    Familiar with thespecialized vocabulary ofearthsciences

    18

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    Lecture1:GeologicTime

    4.5Byearsofhistory

    recordedin

    rocks

    19

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    Readingassignment

    PleasereadKehews booktocomplementthematerialpresentedinthislecture:

    Chapter2,p.23

    27;

    p.60

    72;

    20

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    Lecturecontents

    TheoriginoftheSolarSystem

    Relativedating

    Absolutedating

    Geologicaltimescale

    21

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    Lectureobjectives Toreviewthetimescaleappliedtogeological

    processes Toreviewthedifferencebetweenrelativeand

    absolutegeologicaldating

    Toreviewtheprinciplebehindradiometricdating

    Toplacerockunitsandgeologicaleventsin

    chronologicalorderusingStenosRules ToreviewCanadasgeologicalhistory

    22

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    TheoriginoftheSolarSystem Modelmustaccountforthefollowing

    observations:

    AllplanetsrotateinsamedirectionaroundtheSun

    Theorbitsofallplanetslieinthesameplane,theinvariableplane(Earthsorbitalplaneistheeclipticplane)

    Thedistributionofplanetarybodies: Terrestrialplanets,asteroidbelt, giantplanets,comets

    Planetshavedifferent: Rotationperiods,spindirections,obliquity

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    TheoriginoftheSolarSystem ClassicalModel

    1. FormationofSolarNebula2. Planetesimals

    3. Planetaryaccretion

    4. Planetarydifferentiation

    TheSolarNebula(Kant,1755)

    Thesunandplanetsarebornfromarotatingdiskofcosmicgasanddust,thesolarnebula

    24

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    1.SolarNebular Thesolarnebularisinfluencedbygravity,gas

    pressure,androtation Masscollapsesatcentre formingtheSun

    Cloudspinsfasterandflattenstoformadisk,

    constrainingtheplanets: ExplainswhyallplanetsorbittheSuninthesame

    direction

    Explainswhyallplanetshavetheirorbitsinthesameplane

    25

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    2.Planetesimals

    Massflowbetweensunanddiskceases

    Accretionofplanetesimals(diameter 1km)

    Sourcesofenergy:

    Gravitationalenergy

    Impactenergy

    Controllingfactor:falloffinTwithdistancefromthesun

    26

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    3.Planetaryaccretion Planetsresultingfromaccretionfromasmallnumber

    oflargeplanetesimals inthefinalstage Disruptionofspinandobliquity

    Allplanetsformed:

    Atthesametime( 4.6Ga),inarelativelyshorttime

    27

    Nebula

    0 5 15 115Ma

    PlanetesimalsPlanetesimals

    Planetary

    accretion

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    4.EarthDifferentiation

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    Densermaterialmigratesgraduallytothecentre

    InitialEarthhot,mostlymolten;separatesintodenseFeNialloycoreandsilicatemantle bygravity

    Innercore:Solidiron

    Outercore:Liquidiron

    Mantle:Ironandmagnesium

    Crust:Siliconandoxygen

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    TheoriginoftheSolarSystem

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    Davidson et al., 2002

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    EarthsMoon Moonlessdensethan

    Earth,cannothaveformedatsametimebysameprocesses

    CollisionmodelforMoon;onlylessdensesilicatematerialejected

    intoorbittoformMoonat4.53Ga

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    Taylor, 1994

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    Meteorites TheytellustheageoftheSolarNebula!!

    Stonymeteoritesareprimitive

    Compositionsimilar

    to

    Earths

    mantle

    Chondrules aresolidifieddropletsofmatterfromtheearlySolarNebula

    Ironmeteoritesaredifferentiated CompositionsimilartoEarthscore

    31

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    Meteorites Stonymeteorite,Murchison,withabundant

    chondrules

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    Photo:D.

    Smith,

    CarletonU.

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    Meteorites Ironmeteorite,Annaheim,foundin1916,100

    kmeastofSaskatoonbyafarmermowinghay

    33

    Photo:http:

    //miac.uqac.ca

    /MIAC/

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    TheModernEarth

    34

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    TheEarthscoreiscooling Earth

    inheritedPrimordialHeat;also

    produces

    heatfrom

    radioactivedecayof K,U,Th

    35

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    EarthHistory: theAgeoftheEarth Theological,sedimentaccumulation,Earth

    coolingrates,radioactivedecay

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    106 = 1 million years

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    EarthHistory: theAgeoftheEarth JamesHutton(1726 1797)

    Founderofmoderngeology Majorcontribution:

    Earthscoreishot

    Basedonerosionrates,theEarthisseveralordersofmagnitudeolderthanpreviouslythought

    Keyfieldevidence:unconformityat

    Siccar Point

    37

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    EarthHistory: theAgeoftheEarth Siccar Point,

    Scotland Layerstiltedinto

    verticalposition

    byregional

    compression

    38

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    Relativedating Relativedating:taskofplacingrockunitsand

    geologicaleventsinchronologicalorder intheirpropersequence

    Weusefourlawstoguiderelativedatingingeology

    39

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    StenosRules

    NicholasSteno,16381686

    1.Principleoforiginalhorizontality2.Principleoflateralcontinuity

    3.Principleofsuperposition

    4.Principleofcrosscuttingrelationships

    StenosRules123applytosedimentaryrocks

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    Principle

    of

    Original

    horizontality Layersofsediments are

    alwaysdepositedin

    horizontalsheets Acceptableassumptionfor

    scale

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    Principle

    of

    Lateral

    continuity Sediments aredepositedincontinuous

    horizontalsheetsuptothepointwheretheyterminateagainstasolidsurface

    42

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    Rules1&2

    43

    Ref.:Kehew,A.E.1995.GeologyforEngineers&Environmental

    Scientists.2nd Edition.Fig.1.1.Shown with permission.

    conformable

    layers

    Oldersurfacepredating

    sedimentdeposition

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    Principle

    of

    Superposition Inundeformed

    sedimentaryrocks,eachlayerisolderthantheoneaboveit

    Iflayersarefoldedorinclinedatalargeangle,theyhavebeen

    disturbedafterdeposition

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    GrandCanyon,

    Arizona

    46

    Source:UnitedStatesGeologica

    lSurvey(USGS)

    Time

    increasing

    Older

    Younger

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    Law

    of

    included

    fragments Iffragmentsofonematerialarefoundin

    another,thentheincludedfragmentsmustbeolder

    47

    P i i l f

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    Principleof

    Crosscutting

    relationships

    Anyevent

    thatcutsorbreaksarock

    mustbe

    youngerthanthatrock

    Fault

    Dyke

    48

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    Unconformities InmostplacesonEarth,thereisnocomplete

    setofconformablelayers: Surfacesleftbyhaltsinsedimentationarecalled

    unconformities

    Angularunconformity:olderlayerdipatanangle

    differentfromyoungerlayer

    Disconformity: thenewlayersareparalleltotheolderlayersbutthereisatimegap inbetween

    Nonconformity:theerosionsurfaceisanigneousormetamorphicrock

    49

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    Unconformities

    Deposition

    of

    SequenceAinconformablelayers

    Deformation&

    metamorphismofsequenceA

    50

    A

    A

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    Unconformities Upliftand

    erosionofAErosionalsurface

    DepositionofsequenceB

    Nonconformity

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    A

    A

    B

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    Unconformities

    Deformation,upliftanderosionofA

    andB

    Erosionalsurface

    52

    A

    B

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    Unconformities

    Angularunconformity

    DepositionofsequenceC

    Inconformable

    layers

    53

    A

    B

    C

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    Unconformities

    IntrusionofigneousbodyDthroughA,B,

    andC

    Aistheoldest

    Distheyoungest

    54

    A B

    CD

    Example: Determine the order of

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    Example:Determinetheorderof

    relativeageofeachunit

    55

    unconformity

    unconformity

    E

    Example: Determine the order of

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    Example:Determinetheorderof

    relativeageofeachunit

    56

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    Answer

    57

    12

    34

    5

    6

    7

    8

    1 = oldest, 8 = youngest

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    James

    Hutton:

    re

    visited KeyobservationatSiccar Point,Scotland

    Horizontallayersoverlayverticallayers

    58

    Horizontal layerVertical layer

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    Next! Howdowedeterminehowoldrocksare?

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