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Lecture 2 - Distances, Sizes and Time

Apr 10, 2018

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  • 8/8/2019 Lecture 2 - Distances, Sizes and Time

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    1

    Lecture

    2

    :

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    2

    Time Item

    7:00 7:50pm Sizes &DistancesintheSolarSystem

    8:00 8:50pm Sizes &

    Distances

    beyond

    the

    Solar

    System

    9:00 9:30pm ReservedforCronyn projects

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    3

    Incaseyoudidntknow:theseprojectsareongoing: Clearskiesrequired!

    Cronyn status:

    htt : www.astro.uwo.ca cron nstatus.html

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    4

    Clickers:Last

    week

    not

    enough

    data

    to

    process.

    e s ryaga n o ay.

    WebCT quiz:justdoit.

    Diagnostictest:

    results

    next

    week.

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    5

    Earthhas

    the

    closest

    encounter

    with

    Jupiter

    until

    . ,bigintheCronyn telescope!

    MethaneinatmosphereofMarslastslessthana

    .

    .Andnow,byrequest,someselfpromotion.

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    6

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    7

    Whatsyourfavoritecolor? Textentryanswer!

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    8

    Today,wellsimplyhavealookattheBigPictureoftheUniverse:

    Whatis

    the

    Solar

    System,

    the

    Milky

    Way,

    the

    Local

    Group,galaxycluster??

    Howbigarethings,howfarapart?HowandwheredoesEarthfitin?

    Wewontreallyexplainhowweknowallthatwellsavethatfortheremainin lectures.

    Weresettingthestagefortherestofthiscourse.

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    9

    ,

    andvisualize sizes

    and

    distances

    in

    the

    Earth

    MoonSuns stemandbe ondb usin scalemodels.

    Youwill

    be

    able

    to

    ex ress

    astronomical

    distancesusinglighttraveltimes.

    Youwillknowhowdifferentstructuralelements

    ofthe

    Universe

    are

    related

    to

    one

    another.

    Youwillbeabletocompareeventsinthehistoryo e n verse oaoneyearca en ar.

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    Q:Do

    Ihave

    to

    know

    precise distances

    between

    , ,

    : o,you on t avetomemor zeprec senumbers.However,youshouldknowaballpark

    ,shouldnowhowthesenumbersrelatetoeach

    .

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    11

    Wellstart

    from

    Earth,

    and

    then

    gradually

    work

    collectionsofobjects.

    ,togetagoodsenseofrelativesizesand

    .

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    12

    Ascale

    model

    is

    arepresentation

    or

    copy

    of

    an

    sizeoftheobject.

    ,factor!!

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    13

    Sincemany

    numbers

    are

    so

    big

    we

    cant

    really

    ,models.

    bythesamefactor.

    . .40,000kmapartbecome:

    woo ec so 5an 10cm a are4mapar .

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    14

    Youdontneedto nows zestoseethatthe aresimilar!

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    15

    Diameter:12 2km.Youshouldapproximately12,000km.

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    16

    Wheninorbit,howfarawayistheSpaceShuttlefromEarth?

    A. Afewkilometers.C. Afewthousandkilometers.D. Closetoamillionkilometers.E. Closetoabillionkilometers.

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    17

    EarthasseenfromtheSpaceShuttle/ISS

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    18

    Wheninorbit,howfarawayistheSpaceShuttlefromEarth?

    A. Afewkilometers.C. Afewthousandkilometers.D. Closetoamillionkilometers.E. Closetoabillionkilometers.

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    19

    TheISSandtheshuttleasseenfrommoderatetelescope

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    20

    Equatorialdiameter

    :12,756

    km

    qua or a c rcum erence:40,075 m

    Around

    the

    world

    is

    about

    a

    400

    hour

    drive

    a t esst an17 aysnonstop .

    Convenientscalemodelfornow:

    sca e

    own

    ya

    actoro

    50

    m on

    >diameterabout24cm

    a ou es zeo a as e a .

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    21

    WithEarththesizeofabasketball,whereshouldweputtheInternationalSpaceStation?

    A. 1cmabovethesurfaceC. 1mabovethesurfaceD. 10mabovethesurfaceE. 100mabovethesurface

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    SpaceShuttle

    /ISS

    typically

    flies

    at

    about

    400

    km

    v e y50m on=0. cm

    The

    Hubble

    Space

    Telescope

    at

    about

    1.2

    cm

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    23

    Communicationsatellites

    are

    typically

    in

    earthinexactlyoneday.

    Physicsrequiresthemtobeatanaltitudeof

    ,

    Inourscalemodelthatwouldbe:71.6cm

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    24

    Howbig

    would

    the

    moon

    be?

    owcou we gureou

    Is

    the

    Moon

    bigger

    or

    smaller

    than

    the

    Sun? CloserorfurtherawaythantheSun?

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    25

    TheshadowoftheMoononEarthduringasolareclipse

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    26

    WithEarththesizeofabasketball,howbigshouldtheMoonbe?

    A. AboutthesizeofasmallballbearingC. AboutthesizeofabaseballD. AboutthesizeofagrapefruitE. AboutthesizeoftheEarthitself

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    Equatorialdiameter

    =3,476

    km

    o noursca emo e s ecomesa ou 7cm.

    8

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    Wheredoweputthemooninourscalemodel :A. Atadistanceoflessthan70cmC. Atadistanceofabout7mD. Atadistanceofamorethan10m

    Onecorrect

    answer

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    Thedistance

    to

    the

    moon

    is

    384,399

    km

    ca e =7 9cmor7.7m

    How

    do

    we

    know

    the

    distance

    ??> nce po o: unar aser ang ng

    Thisfigure

    has

    the

    correct

    scale

    !!

    30

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    30

    Pointlaser

    to

    mirror

    on

    the

    moon

    aser g sre ec e

    Detect

    laser

    pulse

    and

    measure

    time

    between

    r ng aseran etect ngt es gna

    Thisisthenthelighttraveltime

    Ifwe

    know

    the

    speed

    of

    light,

    we

    can

    calculate

    thedistance

    31

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    31

    c =299,792.458

    km

    /s

    Youshouldknow:about300,000km/s

    Thisistheabsolutefastestspeedpossibleinthe

    Universe!

    32

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    32

    LLRexperiments

    observe

    arrival

    of

    pulse

    about

    2.6

    secondsafterfirin thelaser.

    Withaspeedofabout300,000km/s,thiscorresponds

    toadistance

    of

    780,000

    km

    Butthisistwice thedistancetothemoon(lighthastogothemoon,andthengetback)

    o

    rue

    s ance

    s

    a

    o

    a ,

    or

    a ou

    390,000

    m Or:thedistancetothemoonisabout 1.3light

    33

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    33

    LLRextremely

    precise

    oon s r ngawaya a ou 3. cmperyear

    34

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    34

    Thephysical

    size

    of

    the

    Sun

    is

    about

    400

    times

    .

    35

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    35

    Howbigshouldthesunbeinourscalemodel?A. Diameterofabout30mC. Diameterabout500mD. Diameterabout1km

    Onecorrect

    answer

    36

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    36

    Diameterabout

    1,400,000

    km

    ca e =2 00cm=2 m

    SunsdiameterislargerthantheMoonsorbit!

    37

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    37

    Totalsolar

    eclipse:theapparentsizethemoonarethesame!

    38

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    3

    TheSunmustbeabout400timesfurtherawaythantheMoon

    True/False

    39

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    39

    Howfarawayisthisbigball?A. About100m C. About3km nearVictoriaPark,LondonOND. About20km

    One

    correct

    answer

    40

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    4

    Distanceto

    the

    sun

    is

    approximately

    150

    million

    .

    ThisisreferredtoasanAstronomicalUnit(AU)

    mostcommon yuse ast e as s ordistancescalesinthesolarsystem

    v e

    y50

    m on

    =3

    m

    nour

    sca e

    mo e

    41

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    Iflighttravelsabitmorethan1secondfromtheMoontoEarth,thenhowlongdoessunlightneedtotraveltoreachEarth?

    A. 1second.C. Abitmorethananhour.D. Manyhours.

    42

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    Usingthe

    right

    numbers,

    you

    can

    find

    that

    it

    Earth.

    SoiftheSunwouldstopshiningrightnow,we

    EarthSundistance:8lightminutes.

    43

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    Spaceis

    not

    as

    far

    away

    as

    you

    think

    when

    ,toOttawaorChicago!

    MoonisnotasclosetotheEarthasyouthink!

    ze

    o

    t e

    un

    s

    arger

    t an

    oon s

    or t

    aroun

    theEarth!

    44

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    Q:What

    is

    the

    Solar

    System?

    : e o ar ys em s eco ec ono o ec s a orbitstheSun includingplanets,comets,

    , Letsfocusonplanets.

    45

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    Distancesnot toscale!!

    46

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    Planet Distance(AU) Distanceinscalemodel Lighttravel timeMercury 0.4 AU 1.2 m 0 03.2min

    Venus 0.7 AU 2.1km 0h05.8min

    Earth 1.0

    AU 3.0

    km 0h

    08.3

    min

    Mars 1.5 AU 4.5km 0h12.45min

    Jupiter 5.2AU 15.6km 0h43min

    . .

    Uranus 20AU 60km 2h

    40

    min

    Neptune 30AU 90 km 4h

    Pluto 39AU 117km 5h20min

    47

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    Ourscale

    model

    that

    worked

    well

    for

    the

    Earth

    forlargerdistances..

    48

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    Insteadof

    scaling

    by

    afactor

    50

    million,

    lets

    try

    10

    .

    Sunisnowabout14cm grapefruitsized.

    1 =150m on mcorrespon stoa out15meters.

    stance

    to

    uto

    :

    a

    a

    ometer

    49

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    ApproximateSize or Distanceusinglight Scale model1(50million) Scalemodel2(10billion)distance(km) traveltime

    Earth 12 2 2 cm 1mm

    Moon 3,474 7cm 0.3mm

    un 1,392,000 2 m 14cm

    EarthMoon 384,000 1.3lightseconds

    7m 4cm

    SunEarth 150,000,000 8.3

    light

    minutes3km 15

    cm

    50

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    WiththeSunthesizeofagrapefruit,howfarawayistheneareststar Proxima Centauri?

    A. About3kmaway VictoriaPark,LondonON C. About1,000kmaway QuebecCityD. About4,000kmaway VancouverE. About15,000kmaway Sydney,Australia

    51

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    Insteadof

    scaling

    by

    afactor

    50

    million,

    lets

    try

    Sunisnowabout14cm grapefruitsized.

    =meters.

    DistancetoPluto:halfakilometer

    Distanceto

    Proxima Centauri

    :4,400

    km

    !

    T icaldistancebetweenstarsintheMilk Wa

    52

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    Stateof

    the

    art

    spacecraft

    :speed

    abit

    over

    , .

    Toreachtheneareststars,wouldstillneedabout

    ,

    53

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    Iflight

    takes

    more

    than

    4years

    to

    travel

    from

    ,Proxima Centauriasitwasmorethan4years

    . Wecannotnowwhatthepresentdaysituationis

    So:lookingfarther=lookingfurtherbackintime

    s ronomyasa memac ne

    54

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    55

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    Say..thatsalot

    stars

    youve

    got

    there.

    esun sas ar

    Itsjustoneofabout300billionstarsinourMilkyay

    a axy

    56

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    Sunis

    about

    28,000

    lightyears from

    the

    center

    of

    .

    DiameterofMW:about 100,000lightyears

    59

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    OurMilky

    Way

    is

    fairly

    close

    to

    other

    galaxies

    About30Galaxies,includingMagellanic Clouds,

    ,

    li h

    60

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    1 li h r

    LargeMagellanic Cloud

    SN1987A

    li h

    61

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    2 li h r

    li h

    62

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    2 li h r

    63

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    200millionlightyears

    64

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    OurMilky

    Way

    is

    one

    of

    at

    least

    100

    billion

    .

    Soroughly1022 starsintheobservableUniverse

    a out

    as

    muc

    as

    t ere

    are

    gra ns

    o

    san

    on

    a

    beachesonEarth.

    an

    t a t s

    on y

    or

    t at

    part

    o

    t e

    n verse

    we

    canactuallysee

    65

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    TheHubble

    Deep

    Field:

    Empty

    Space

    66

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    SolarSystem:

    Sun

    &

    What

    goes

    around

    spar o y ay a axy: a r y a collectionofbillionsofstars.

    ga axypart

    o

    oca

    roup:

    ew

    tens

    o

    galaxies,reasonableclosetogether

    oca

    roup

    part

    o

    oca

    uperc uster WhichispartoftheUniverse.

    67

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    Comparedto

    sizes

    of

    objects,

    distances

    between

    SotheUniverseismostlyempty!

    ut

    t e

    n verse

    sa so

    area y

    gp ace.

    68

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    Earthrotates

    around

    its

    axis

    (1

    day)

    r ear aroun esun 1year

    OrbitsuninMilkyWay

    Galaxies:expandinguniverse

    69

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    Rotationtakes

    24

    hour

    , km

    24hours.

    whichmeanswetravelatabout1 6 0km/h!

    Lowerspeeds

    at

    higher

    latitudes

    Rotationalvelocit =0at oles.

    70

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    Witharadius

    of

    150

    million

    km,

    the

    length

    of

    one

    km.

    ,

    billionkmperyear.

    ,

    71

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    Withrespect

    to

    local

    neighbourhood

    i.e.

    the

    Speedstypically70,000km/h

    ,

    onlyslightlyontimescalesof10,000years.

    : ,

    Evenwiththatspeed,solarsystemhasonlycomp e e 2030or s.

    72

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    Withinlocal

    Group

    :random

    velocities.

    . .wellover300,000km/h

    Universe

    :

    speedof

    light.

    73

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    HubblesLaw:

    the

    further

    away

    agalaxy

    is,

    the

    .

    Soareweinthecenterofitall??

    74

    Notehowforallraisins,allother

  • 8/8/2019 Lecture 2 - Distances, Sizes and Time

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    ,

    raisinsare

    moving

    away.

    The

    further

    awaytheyare,thefastertheyaremovingaway!

    75

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    Weare

    never

    sitting

    still!

    pee sareenormous; yp ca y e argersca escorrespondtofasterspeeds!

    76

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    Becauseof

    the

    expansion

    of

    the

    Universe,

    we

    can

    Lightfromobjectsthatarefartherawayhasnot

    theUniverse:

    TheUniverse

    has

    an

    observation

    limit

    :ahorizon

    77

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    Spaceitself

    is

    expanding

    o ngswerec oser n epas ere sauniquemomentintimewheretheentire

    . >BigBang,about14billionyearsago

    so ow ongago st at

    78

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    Idea:compress

    time

    so

    that

    the

    entire

    lifetime

    of

    .

    January1st :BigBang

    ecem er31 ,

    11:59:59pm:

    r g t

    now.

    >Soonedaycorrespondstoabout40millionyears.

    79

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    Onthiscosmiccalendar,whendidthedinosaursbecomeextinct?

    A. April1

    st

    ndC. November11thD. December30th

    Onecorrectanswer

    80

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    About65

    million

    years

    ago,

    so

    scaled

    down

    that

    st,

    midnight.

    81

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    82

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    Somewherein

    February

    :Milky

    Way

    forms

    ep em er3 : ar orms a ou 4.5 onyearsold)

    eptem er22 :

    ar y

    eon

    eart .

    Thatsquick!

    ecem er31s ,11:5 pm: o ern umansevo ve

    Entirehistoryofhumancivilization:thelastthirtyseconds.

    83

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    TheMW

    galaxy

    formed

    shortly

    after

    the

    Big

    ButittookawhilebeforetheSolarSystem

    LifeonEartharoseshortlyaftertheformationof

    Butit

    took

    along

    time

    before

    humans

    appeared

    on ep ane

    84

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    TheUniverse

    is

    abig,

    big

    place

    s ancesareo eng gan ccompare os zes:theUniverseseemsmostlyempty,oratleast

    Hierarchy:planets

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    Howbig

    is

    an

    Astronomical

    Unit,

    Light

    year,

    ,.

    Whataretypicalsizesanddistancesinthe

    AgeoftheUniverse:about14billionyears

    umans aven t eenaroun t at ong

    86

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    ReadChapter

    2(see

    lecture

    guide

    in

    course

    .