sydney observatory teachers notes 2012
TRANSCRIPT
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WHAT WE OFFER FOR YOUR CLASS
Sydney Observatory oers educational tours
both day and night. Daytime tours can be booked
Monday to Friday during school terms or up to
80 students starting at 10.00 am or 12.00 noon.
Weekend tours can be arranged or country
schools. Night tour session times vary throughout
the year depending on daylight saving and start at
6.15 pm or 8.15 pm (except December and January
which start at 8.30 pm).
Each 90-minute day tour can be tailored to your
students needs and is guided by an astronomy
educator. See page 17 for booking details.
PROGRAM OVERVIEW
Astronomy tour (see page 7 for details)
Touroftheastronomyinstrumentsondisplay
in the Observatory
3-DSpaceTheatre Planetarium
Telescopeviewing
Weather tour (see page 9 for details)
VisittheObserving the weatherinteractive and
historic exhibition at the Observatory
DatacollectionusingObservatoryequipment
3-DSpaceTheatre
VisittonearbyBureauofMeteorology
instrument lawn
AlsoavailablearejointvisitswiththePowerhouse
Museum, IMAX, Sydney Learning Adventures,
Australian National Maritime Museum (see page 5
for details).
3-D Space Theatre (see page 11 for details)
Providinganamazing3-Dspaceexperience,the
3-D theatre technology was developed in
Australia by the Centre or Astrophysics and
Supercomputing at the Swinburne Institute o
TechnologyinMelbourneandshowsshortlmson the solar system, space exploration and
cosmology.
Planetarium
Thisisanastronomerledexperienceinacosyplanetarium.Thestareldcylinderusedincludes
an extraordinarily precise depiction o the Milky
Way based on the beautiul all-sky panoramas
created by astrophotographer Dr Axel Mellinger.
Telescopes (see page 13 for details)
TheObservatoryhastwofunctioningtelescope
domes.Theoldersouthdomenowhousesthe
oldest working telescope in Australia, a 290 mm or
11.5inchrefractingtelescope.Thenorthdome
houses a 400 mm computer controlled SchmidtCassegrain refecting telescope and a Coronado
Solar telescope or sae viewing o the Sun during
the day.
IN THESE NOTES YOU WILL FIND
Curriculumlinkspage2
Jointdiscountvisitspage5
Observatoryoorplanspage6
Astronomytourspage7
Weathertourspage9 3-DSpaceTheatrepage11
Backgroundinformationpage13
Astronomyresourcespage15
School visits
TEACHERS NOTES
SolarSystemMontage.PhotocourtesyGetty.
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SYDNEYOBSERVATORYTEACHERSNOTES2
Theastronomyandmeteorologyexhibitionscan
be easily integrated into content strands, units o
work or areas o teaching and learning in the
ollowing syllabus areas:
SCIENCE AND TECHNOLOGY(YEARS K6)
Built environments (Stage 2 and 3)
buildingsandthespaceswithinandsurrounding
these buildings, eg homes, schools, community
acilities and actories, parks and gardens.
naturalenvironmentsthathavebeenmodied
to suit particular needs, eg land cleared or
arming and altered waterways
servicesprovidedtocommunities,egelectricity,water, etc
Inormation and communications (Stage 2 and 3)
thenatureofcommunications
methodsofcommunicatingbetweenindividuals,
groups and communities, eg personal
conversation, telephones, satellite link-ups
changestoinformationandcommunication
technology over time.
Physical phenomena (Stage 2 and 3) relationshipsbetweentime,spaceand
movement
sourcesofenergy
lightandsomeofitscharacteristics
heatandsomeofitscharacteristics
Earth and its surroundings (Stage 1, 2 and 3)
thesolarsystem,planets,Earth,Moonandstars
aspectsofthephysicalenvironment,egthe
Earths crust, its oceans and atmosphere
naturalchangesthatoccur,suchassoilerosion,
volcanic eruption, climatic changes and
movement o water
thepassingoftimeandthenaturaleventsthat
make people aware o this passing, eg daily
cycles, lunar cycles and seasons
thevarietyandcharacteristicsofnaturally
occurring materials
themethodspeopleusetoobtainandprocess
materials
themethodspeopleusetomanagenatural
resources
limitationstoresourcesavailableonEarth
renewableresources.
Suggested units o work:
Stage1HotorCold,APlaceinTime
Stage2KeepinTouch,CyclesinourWorld
Stage3OutinSpace,WhatstheWeather
HUMAN SOCIETY AND ITSENVIRONMENT HSIE (K6)
Stage 2
Change and Continuity, Signifcant Events and
People
CCS2.1Describeseventsandactionsrelatedto
theBritishcolonisationofAustraliaand
assesseschangesandconsequences.
Change and Continuity Time and Change
CCS2.2Explainschangesinthecommunityand
amily lie and evaluates the eects o these on
dierent individuals, groups and
environments.
Environments, Patterns o Place and Location
ENS2.5Describesplacesinthelocalareaand
other parts o Australia and explains their
signicance.
Stage 3
Change and Continuity Cultures Signifcant
Events and People.
CCS3.1Explainsthesignicanceofparticular
people, groups, places, actions and events in
the past in developing Australian identities
and heritage.
Change and Continuity Cultures Cultural
Diversity. CUS3.4Examineshowcultureschangethrough
interactions with other cultures and the
environment.
MATHEMATICS (K0)
Early Stage 1 Measurement: Time
Describethedurationofeventsusingeveryday
language
Sequenceeventsintime
Namedaysoftheweekandseasons
CURRICULUM LINKS
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SYDNEYOBSERVATORYTEACHERSNOTES3
Stage 1 Measurement: Time
Useinformalunitstomeasureandcompare
the duration o events
Nameandorderthemonthsandseasonsof
the year
Identifythedayanddateonacalendar
Stage 2 Measurement: Time
Recognisethecoordinatedmovementsofthe
hands on a clock
Readandrecordtimeusingdigitalandanalog
notation
Convertbetweenunitsoftime
Readandinterpretsimpletimetables,
timelines and calendars
Stage 3 Measurement: Time
Convertbetweenam/pmnotationand24-hour
time ComparevarioustimezonesinAustralia,
including during daylight saving
Drawandinterpretatimelineusingascale
Usetimetablesinvolving24-hourtime
Stage 4 Measurement: Time
Performoperationsinvolvingtimeunits
Useinternationaltimezonestocomparetimes
Interpretavarietyoftablesandchartsrelated
to time
Stage 4 Data: Data
Draw,readandinterpretgraphs(line,sector,
travel, step, conversion, divided bar, dot plots
and stem-and-lea plots), tables and charts
Distinguishbetweentypesofvariablesusedin
graphs
Identifymisrepresentationofdataingraphs
Stage 2 Space and Geometry: Positions
DeterminethedirectionsN,S,EandW;NE,
NW, SE and SW, given one o the directions Describethelocationofanobjectonasimple
map using coordinates or directions
SCIENCE (710)
Outcome4.1Identieshistoricalexamples
ofhowscienticknowledgehaschanged
peoples understanding o the world
Outcome5.1Explainshowsocialfactors
infuence the development and acceptance o
scienticideas
Outcome4.2Usesexamplestoillustrate
how models, theories and laws contribute to an
understanding o phenomena
Outcome5.2Describestheprocessesthat
are applied to test and validate models,
theories and laws
Outcome4.4Identieschoicesmadeby
peoplewithregardtoscienticdevelopments
Outcome5.4Discussesscienticevidence
supporting dierent viewpoints
Outcome4.6Identiesanddescribes
energy changes and the action o orces in
common situations
Outcome5.6Appliesmodels,theoriesand
laws to situations involving energy, orce and
motion
Outcome4.9Describesthedynamic
structure o Earth and its relationship to other
parts o our solar system and the universe
Outcome5.9Relatesthedevelopmentof
the universe and the dynamic structure o
Earth to models, theories and laws and the
infuence o time
Outcome4.12Identies,usingexamples,
common simple devices and explains why they
are used
Outcome5.12Relatestheinteractions
involved in using some common technologies
totheirunderlyingscienticprinciples
Outcome4.13Clariesthepurposeofan
investigation and, with guidance, produces a
plan to investigate a problem
Outcome5.13Identiesaproblemand
independently produces an appropriate
investigation plan
Outcome4.15Usesgivencriteriatogather
rst-handdata
Outcome5.15Gathersrst-handdata
accurately
Outcome4.16Accessesinformationfrom
identiedsecondarysources
Outcome5.16Accessesinformationfroma
wide variety o secondary sources
Outcome4.22Undertakesavarietyof
individual and team tasks with guidance
Outcome5.22Plans,implementsand
evaluates the eectiveness o a variety o tasks
independently and as a team member
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SYDNEYOBSERVATORYTEACHERSNOTES4
GEOGRAPHY (710)
Focus Area 4G1 Investigating the World
readsynopticcharts
Focus Area 5A1 Investigating Australias Physical
Environments
readandinterpretsynopticcharts
Focus Area E1 Physical Geography
climate
globalcirculation:insolation,pressure,wind,
temperature, rainall
globalclimaticpatterns
factorsaffectingclimate:latitude,altitude,
maritime and continental infuences
climatechange
distinguishbetweenweatherandclimate
explaintheglobalcirculationoftheatmosphere
describeglobalclimaticpatterns
analyseclimatedatafromavarietyofsources
weather
typesofrainfall
factorsaffectingtemperatureandhumidity
extremeweatherevents:droughts,oods,
storms
examineissuesresultingfromclimatechange
collectandrecordweatherdata
describemeteorologicalprocesses
createamultimediapresentationassessingthe
impacts o an extreme weather event on a
community
PHYSICS
8.5 The Cosmic Engine
1. Our Sun is just one star in the galaxy and ours
isjustonegalaxyintheUniverse
2. TherstminutesoftheUniversereleased
energy which changed to matter orming stars
and galaxies3. Stars have a limited lie span and may
explode to orm supernovas
4. TheSunisatypicalstar,emitting
electromagnetic radiation and particles that
infuence the Earth.
9.2 Space
1. TheEarthhasagravitationaleldthatexertsa
orce on objects both on it and around it
3. TheSolarSystemisheldtogetherbygravity
4. Current and emerging understanding about
time and space has been dependent upon
earlier models o the transmission o light
9.7 Option Astrophysics
1. Our understanding o celestial objects
depends upon observations made rom Earth
or rom space near the Earth
2. Careul measurement o a celestial objects
position in the sky (astrometry) may be used
to determine its distance
3. Spectroscopy is a vital tool or astronomers
and provides a wealth o inormation
4. Photometricmeasurementscanbeusedfor
determining distance and comparing objects
5. Thestudyorbinaryandvariablestarsreveals
inormation about stars
6. Stars evolve and eventually die
SENIOR SCIENCE
9.9 Option Space Science1. While the atmosphere has limits there is no
such thing as empty space
2. Thestrengthofgravityvariesatdifferent
points in space
3. Space stations and probes provide
inormation about our solar system, galaxy and
deep space
AstronomerHALenehanusingthetransitcircleatSydney
Observatory19071908.
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SYDNEYOBSERVATORYTEACHERSNOTES5
Joint, discounted visits can be arranged with the
PowerhouseMuseum,IMAX,SydneyLearning
Adventures and Australian National Maritime
Museum.Visitingschoolgroupscantake
advantage o the Observatorys maximum groupofsizeofabout60byorganisinganexcursionof
120 students where one group o 60 visits Sydney
Observatory and the other group o 60 visits another
venue.Thetwogroupsthenswapvenues.
For all the learning programs and partnerships,
see www.sydneyobservatory.com.
POWERHOUSE MUSEUM
VisitthePowerhouseMuseumexhibitionsEcoLogic: creating a sustainable future, Space or
Pathways to space and then visit Sydney
Observatory.
Totalcost:$15perstudent(dayvisit:$9
Observatoryand$7Powerhouse).
Contact:PowerhouseMuseum,ph(02)92170222
or email [email protected]
www.powerhousemuseum.com
Sydney Observatory ph (02) 9921 3485
IMAX
VisitIMAXtoviewtheshowsHubble 3-D (rom
May 2010) orSpace station 3-D (terms 1 and 2 only)
andthenanObservatory3-DSpaceTheatreand
telescope viewing.
Totalcost:$18.50(dayvisit:$9Observatoryand
$9.50IMAX)/$20.50perstudent(nightvisit:$11
Observatoryand$9.50IMAX).
IMAXTheatreSydneyph(02)[email protected];www.imax.com.au
Sydney Observatory ph (02) 9921 3485
SYDNEY LEARNING ADVENTURES
VisitSydneyLearningAdventuresinTheRocksfor
theprimaryprogramHMSDiscoveryorthe
secondaryprogramRocksDreamingthenatourof
an astronomy or weather ully guided experience
attheObservatory.TheRocksDreamingtour
includesthePlanetarium,Cadi Eora Birrung
exhibition and (sae) telescope viewing o the Sun.
HMSDiscoverytotalcost:$19(dayvisit:$9
Observatoryand$10SydneyLearningAdventures)
RocksDreamingtotalcost:$23.40(dayvisit:$9
Observatoryand$14.40SydneyLearningAdventures)
Contact: Sydney Learning Adventures,
ph (02) 9240 8552 or email [email protected]
Sydney Observatory ph (02) 9921 3485
AUSTRALIAN NATIONAL MARITIMEMUSEUM
A ull day program on weather is available with a
combined Australian National Maritime Museum(ANMM) package,Ways of watching weather
Totalcost:$17(dayvisit:$9Observatoryand$8
ANMM)
Contact: ANMM, ph (02) 92983655 or email
Sydney Observatory ph (02) 9921 3485
Earnshaw520chronometer,madeabout17901801.
JOINT DISCOUNT VISITS WITH SYDNEY OBSERVATORY PARTNERS
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SYDNEYOBSERVATORYTEACHERSNOTES6
TOILETS(outside)
EMERGENCYEXIT
GROUND FLOOR
EMERGENCYEXIT
Planetarium(occasional sessions)
ENTRY/EXIT
EMERGENCYEXIT
Lectureroom
1
2
3
4
5 WHEELCHAIR/GROUPENTRY
FIRST FLOOR6
7 8
9
10
Balcony
Russellroom
SYDNEY OBSERVATORY FLOOR PLANS
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The90-minutetourisguidedbyanastronomy
educator and includes a tour through some o
Observatory displays, an awesome 3-D Space
Theatreexperience,alookatthenightskyinour
Planetariumandviewingthroughatelescope(weather permitting). During the day students can
safelyviewtheMoon,Venus,brightstarsthrough
a large telescope as well as the Sun using a
special (sae) solar telescope. At the end o the
visit each teacher will receive an up to date set o
Solar System notes or use at school.
ASTRONOMY INSTRUMENTS TOUR
Room 1 Watchers o a dierent sky
Find out what makes the southern sky specialand meet some o the astronomers and
explorers who have observed the night sky.
Some o the things you will see:
BrisbanestelescopeusedatGovernor
ThomasBrisbanesobservatorytoobserve
Enckes Comet in 1822
RepeatingcircleusedatParramatta
Observatory in the 1820s to measure angles
between stars
ApollofeedhornreceivedthehistorictelevisionimagesofNeilArmstrongsrst
ootsteps on the Moon in 1969 or a broadcast
watched by millions on Earth
Room 2 Knowing the time and fnding the way
Thisroomlooksattheinstrumentsusedby
Matthew Flinders to chart the Australian coastline
in the early 1800s.
Some o the things you will see:
Earnshaw520chronometeroneofthevechronometers used on Flinders voyage around
Australia and the only one still working at the
end o the journey
Earnshawastronomicalclockthishighly
accurateclockbuiltin1791wasusedby
Flinders to check the timekeeping o the
chronometers on his ship
SextantnavigatorslikeFlindersuseda
sextant to determine both the time and the
latitude
Room 3 Transit circle: the biggest clock in the
world
Thisroomisthehomeofthetransitcircle,a
telescope which was used to determine the exact
time, the positions o stars and the geographicalcoordinates o the Observatory.
Some o the things you will see:
Transitcircleaspecialtelescopethatonly
moves north and south and used the regular
daily spin o the Earth to determine the time
Chronographamachineusedtorecordthe
transit circle observations
Pendulumclockpurchasedin1860,thisisa
highly accurate astronomical regulator clock
Room 4 Planets and stars o the southern sky
Explore the solar system and discover the
constellations!DidyouknowthatPlutoisno
longer considered a planet? In 2006, astronomers
reclassiedtheice-coveredspherebydubbingit
a dwar planet.
Some o the things you will see:
SouthernCross3-Dmodelpeerthroughthe
eyepiece and see how the stars on the
Australian fag are really distributed in space.
Solarsystemmodels(orreries)watchayear
go by and discover why we have seasons, why
the Moon shows phases and how eclipses
occur..
Room 5 Cadi Eora Birrung: under the Sydney
stars
AboriginalpeoplewereAustraliasrst
astronomers and have watched the southern sky
formorethan50,000years.Thestarswereused
as a calendar, or navigation by land and sea and
toconveylawstofuturegenerations.Thisroom
looks at some o the Indigenous Dreaming stories
about the dierent constellations.
Room 6 Transit o Venus:
ThetransitofVenusisofspecialinterestto
Australians. Captain James Cook travelled to
TahititoobserveVenuspassinginfrontofthe
Sunin1769andonhisreturnvoyagemappedthe
east coast o Australia. Australia is in a prime
locationtoobservethenexttransitofVenusin
2012.
ASTRONOMY TOURS
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Some o the things you will see:
Thephotoheliographatelescopefor
photographing the Sun and one o only hal a
dozensuchinstrumentsintheworld
Thephotographicrevolverdesignedforuse
with the photoheliograph and the orerunner o
the movie camera.
THE TIME BALL TOWER
ThetimeballatopSydneyObservatorydropped
forthersttimeon5June1858,alerting
SydneysidersandshipsintheHarbourofthe
exacttime.Todaythetimekeepingtradition
continues, with Observatory sta dropping the
timeballdailyat1.00pm.Timemeasurement
and communication to shipping were vital
components o astronomical work dating back tothe20,000prizepromisedundertheLongitude
Actof1714tosolvetheproblemofdetermining
position at sea.
3-D SPACE THEATRE ANDTELESCOPE DOMES
Ater exploring the displays inside the
Observatory,experiencetheamazing3-DSpace
Theatreandtelescopeviewing(weather
permitting). In the day time students can view theMoon,Venus,brightstarsthroughalarge
telescope as well as saely view the Sun using a
special solar telescope.
PLANETARIUM
Thedigitallyproducedstareldsimulatesthe
night sky at any time, season or location on earth.
Over 3000 stars are projected to a limiting
magnitude o 5.5 with the brightest stars
individually lensed to produce intense pinpointimages. Star locations are accurate to within 1
minute o right ascension and 6 minutes o
declination.Betelgeuse,Rigel,Antares,Spica,
Arcturus,CapellaandPolluxappearinfullcolour.
Twelveaperaturesshowthepositionofthesun
throughouttheyear.ThePlanetariumissuitable
or students rom primary and high school and
includes both Indigenous stories and traditional
western mythology.
Sydney Observatory time ball.
Sunshineorsolarrecorder,madeabout18921905.
ViewofObservatoryHillandSydneyHarbourBridgefrom
Sydney Observatory.
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SYDNEYOBSERVATORYTEACHERSNOTES9
DevelopedwiththesupportoftheBureauof
Meteorology, this 90 minute program consists o
our key areas:
1. Observing the weatherexhibition and weatherwheel activities conducted by Observatory
sta. Exhibition sections include:
Whatwastheweatheronyourbirthday?
interactive
Tippingbucketraingaugeinteractive
Makeacloudinteractive
Historicanemometers,barometers,sun
gauge,andAustraliasrstweathermap
displays
2. Datacollectionusingourequipmentsupervised by Observatory sta.
Dont orget a pencil!
Temperature
Barometricpressure
Wetanddrytemperaturetocalculate
relative humidity
Windspeed
Theultra-violetindex
Rainfall
3. 3-DSpaceTheatrepresentationExtreme
places, which describes extreme weather
conditions throughout the Solar System,
includingthesurfacesofVenusandMarsalong
withtheicydepthsofthefrozenmoonof
Jupiter, Europa.
4. AvisittothenearbyBureauofMeteorology
instrumentlawn.Thissignicanthistoricsiteis
still one o the prime locations or the remote
collectionofweatherdatafortheBureau.
Instruments include:
Stevensonscreenfortemperatureand
humidity measurements
Pluviographsforrainfall
Raingaugeforrainfall
Tippingbucketraingaugeforrainfall
Each teacher will receive at the end o the visit a
copy o the bookStormy weathercourtesy o the
BureauofMeteorologyandSydneyObservatory.
OBSERVING THE WEATHEREXHIBITION
Room 7 Observing the weather: measuring and
orecastingWhen the Observatory opened in 1858, its
astronomers began recording Sydneys rainall
andtemperature.Thisroomdisplaysthemany
instruments that have measured the weather over
the many years since that time.
Some o the things you will see:
Laserceilometeramoderninstrumentused
to measure the height o clouds.
NewmanandBrosmercurybarometeran
instrument used at the Observatory in the late
1800s to measure atmospheric pressure.
Room 8 Observing the weather: surviving the
extremes
An exhibition looking at 150 years o Sydneys
weather. Find out about the heatwave o 1939, the
foods o 1984 and the hailstorm o 1999.
Some o the things you will see:
Cloudmakerlearnaboutdifferenttypesof
clouds through an interactive touch screen. I
you spot white puy rolls on a humid morning,expect these altocumulus clouds to bring rain
in the aternoon
Room 9 Russell Room
HCRussellwasanimportantpioneerof
photographyandasignicantastronomerwho
lived and worked at the Observatory between
1870and1905.
Some o the things you will see:
Historicastronomical,weatherandfamilyphotographs
Stunningviewsofthecity,HarbourBridge,the
time ball tower and fagsta rom the balcony.
Theagstaffiesavarietyofmeteorological,
astronomical and ceremonial fags that change
on a daily basis. A fag decoder is available or
50centsorasadownloadablePDFlefrom
the Observatorys website.
The time ball tower
A wind vane on the tower shows the direction
rom where the wind is coming and the fagsta
signals which way it is going.
WEATHER TOURS
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DATA COLLECTION
In the ground o the Observatory students will
use instruments to measure temperature,
barometric pressure, wet and dry temperature to
calculate relative humidity, wind speed, the
ultra-violet index and rainall
3-D SPACE THEATRE
Ater exploring the displays inside the Observatory,
experiencetheamazing3-DSpaceTheatre.
BUREAU OF METEOROLOGY LAWN
Only 50 metres rom the Observatory this lawn
housesmanyinstrumentsuseddailybytheBOM
to produce comprehensive weather reports or
Sydney. Instruments include:
Pluviographsnolongerusedbutthey
measured the amount o rainall over a certain
time.
Traditional 203 mm (or 8 inch) rain gauges
usedasbackups.Rainfallsintoafunneland
collects in a graduated measuring cylinder.
Tipping Bucket Rain Gauge (TBRG)asrain,or
precipitation alls into the unnel it drips into oneo two very careully calibrated buckets balanced
onapivot(likeaseesaw).Thetopbucketisheld
inplacebyamagnetuntilithaslledtothe
calibrated amount (usually approximately 0.2 mm
ofrain).Whenthebuckethaslledtothis
amount, the weight o the bucket is enough to
break ree o the magnet, causing the bucket to
tip. When the bucket tips, it triggers an electronic
switch. A computer counts the number o tips and
calculates the rainall in millimetres.
The instrument shelter orStevenson screen
the shelter contains several thermometers.
Typically,minimumtemperaturesoccurjust
beore dawn and maximum temperatures
typically beore 3.00 pm.
Westpac barometerthoughnotpartofthe
Bureaulawnthegeneralregiondoesprovidea
good view o the nearby Westpac building which
incorporatesabarometer.Theeighthorizontal
lights indicate the barometric pressure rom 990
hPato1025hPain5hPaincrements.
TheWestpacbuildingbarometer.
TheBureauofMeteorologylawn.
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SYDNEYOBSERVATORYTEACHERSNOTES11
The3-DTheatrehastheabilitytoshowawide
variety o astronomical and space related
materials relevant to the NSW primary and
secondarycurricula.Thisincludes3-Dmoviesand a selection o interactive experiences
delivered by our trained astronomy educators.
Presentationsinthe3-DTheatrecanbetailored
to meet student needs and the topics being
studied i prior notice is given.
Pleasefeelfreetoconsultwithourstafffor
selection recommendations.
MARS - NEW 3D MOVIE
Throughincrediblydetailed
terrain models and high-
resolution stereo
photographs rom key NASA
missions, we join the search
forsignsoflifeontheRed
Planet.Marsistheclosest
thing to going there yoursel.
Duration: 9 minutes
EXTREME PLACES
From the indescribable
heatofVenussurface,to
the raging dust-storms o
Mars and the violence o Io,
experience what it takes
to survive in the extremes
climates o our Solar
System.
Duration: 13 minutes
BIGGER-THAN-BIG
What is big? Is the Sun big?
WhataboutBetelgeusewhich
is 1000 times larger than the
Sun? Discover just how big
theUniversereallyis.
Duration: 7 minutes
DETECTIVE
Its a race to solve a case rom
outer space! Join young
reporterPennyandprivateinvestigator Sam Charleston
to research the acts behind a
video o an alien attack.
Duration: 13 minutes
THE LITTLE THINGS
Comets,asteroidsandKuiper
Beltobjects!Thisisthestory
oftheamazinglittlethingsin
the solar system and the
incredible space missions
that have visited them.
Duration: 10 minutes
OUR SUN: WHAT A STAR!
Haveyouwonderedwhere
theSuncamefrom?Howit
creates energy? And what its
ultimate ate is? Learn all
about our nearest, and most
important, star.
Duration: 19 minutes
ELYSIUM 7
Hoponboardthefuturistic
touristshipElysium7and
take a 3-D journey to Mars,
with surace eatures based
on data rom NASAs Mars
GlobalSurveyorspacecraft.
Duration: 9 minutes
AFTER STARS
A red supergiant star is
abouttoenditslifebut
when the star explodes will it
produce a black hole or a
pulsar? Join an alien
reporter, scientist and the
robotWLR-309tondout.
Duration: 11 minutes
3-D SPACE THEATRE AND INTERACTIVES
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SYDNEYOBSERVATORYTEACHERSNOTES12
EINSTEINS UNIVERSE
RealisingEinsteinsUniverse.Ajourneyintothe
universe Einstein envisaged almost 100 years
ago.Today,modernsupercomputersenable
scientists to visualise the most wondrous
astronomical objects, unlock their secrets and
allow everyone to comprehend the naturalbeautyofEinsteinsUniverse.
Duration: 9 minutes
During your visit our astronomy educators will
also use the 3-D interactives to demonstrate and
explain topics relevant to your needs including
the latest astronomical developments. For
primary level students, we can ocus on the solar
system, asteroids, space exploration,
constellationsorseasons,whilewithyears11/12
we can explore more advanced topics like theevolution o stars.
Earthbydayseenfromspace.Imagebasedonsatellitedata,createdbyRetoStcklifortheNASAGSFCEarthObservatory.
Examples o the types o topics covered by the
3-Dinteractives;
SolarSystem
Asteroids
ExplorationofMarsincludingPhoenix
EarthandMoon
SaturnandCassini
SunandSolarFlares
TransitofVenus
Scaleofthesolarsystem
Extra-solarPlanets
DwarfPlanets
Stars
LightandSpectra
SpaceProbes,Lofar,andHubble
Pulsars
Galaxies
MilkyWaymodel
Galaxyinteraction
Universe
LargescalestructuresoftheUniverse
-
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SYDNEYOBSERVATORYTEACHERSNOTES13
TELESCOPES
(fromtheGreek,tele ar and, skopein to look or
see;, teleskopos ar-seeing)
Therearemanydifferenttypesoftelescope.
SomeliketheHubbleandKeplerareinspace,
whileothersliketheParkesRadioTelescope
dont look at objects but rather listen to their
radio noise.
As ar as most people are concerned there are
twomaintypesofopticaltelescopes.Thosethat
use lenses to magniy are called reractors and
those that use mirrors to collect light are called
refectors.
Theinventoroftherefractorwasprobablythe
DutchopticianHansLippersheyalthoughothers
claimed to have made the same invention at the
time.
RefractorsliketheoneinSydneyObservatorys
south dome have at the ront o the tube a convex
glass lens that is thicker in the middle than at its
edge. As light rom distant objects passes through
the lens it bends or reracts more at the edge o
the lens than light passing through the centre. At
just the right distance rom the lens the light
comes to a ocus where the image is created.
Anotherlenscalledtheeyepiecemagniesthe
image.
Early reractors had problems as the images were
not always sharp or the right colour because
dierent colours bent dierently as they passed
throughthemainlens.Thedevelopmentofachromatic lenses made up o two pieces o glass
each with a dierent density solved the problem.
WhereasGalileostelescopeshadmagnications
o 8x up to 20x the Observatorys reractor works
at about 80x making objects look 80 times closer
or80timesbigger.However,allrefractorsdo
somethingunusualtotheview.Usethelightpath
above and try to work out what it is?
ReectingtelescopesliketheoneinSydney
Observatorys north dome work by bouncing light
offacombinationofcurvedandatmirrors.The
main mirror usually has a cross-section in the
shape o a parabola or sphere.
SirIsaacNewtoniscreditedwiththerstworking
refector in 1668. It was designed to overcome the
colour problems associated with early reractors.
As light enters the telescope tube it bounces o
the curved primary mirror. A smaller secondary
mirror angled at 45 degrees is placed in the light
path beore the ocus point and aims the light out
o the side o the tube. An eyepiece is then used
to magniy the image.
Forthesamesizeoftelescope,reectorsare
much cheaper to make and can be built too much
largerscales.Theytoosufferproblemsandbend
under there own weight when around 5m in
diameter. All modern large telescopes are a
modiedversionofNewtonsdesignandmany
use multiple small mirrors instead on one largeone.Themagnicationofthemirrortelescopein
theObservatorysnorthdomeisaround160x.The
HubbleSpaceTelescopeisavariationof
Newtons original design.
SIZE AND DISTANCES IN ASTRONOMY
ItisdifculttounderstandhowbigtheUniverse
is.Sizeisrelativesothatachipmayseemhuge
to an ant and an elephant at the Zoo may seem
hugetoachild.TheEarthsdiameteris12,700
km and it can take up to 20 hours to fy hal way
BACKGROUND INFORMATION
objective lens
eyepiece
flat secondary
mirror
concave primary mirror
eyepiece
-
7/31/2019 Sydney Observatory Teachers Notes 2012
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SYDNEYOBSERVATORYTEACHERSNOTES14
around in a commercial aeroplane rom Australia
to London, or example. Imagine fying to the Sun
which is a staggering 150 million km away! It is
also 114 times wider than the Earth but that is
airly average compared with other stars.
ThenextcloseststartotheSunisabout40,000
billion km away. Space becomes so large that
distances measured in km become meaningless
rowsofzeros.Asaresultotherlargerunitsof
distanceareused.Thelightyearistheonemost
commonly used in popular books and is simply
the distance that light travels in one year in the
vacuumofspace.Toworkitoutinkmmultiply
the speed o light in a vacuum, which is 300,000
km every second multiplied by the number o
secondsinayear.Thisworksouttoberoughly
9500billionkmor1x1015m.Thecentreofthe
Milky Way galaxy is about 33,000 light years away
and the nearest observable galaxy, the Large
Magellanic Cloud, is about 160,000 light years
away.
Astronomers use a slightly larger unit called the
parsec or the even larger units, Mega parsec
(Mpc)andGigaparsec(Gpc).Withadenition
based on the geometry o the Earths orbit around
theSun,theparsecisequalto3.26lightyears
and so a Mega parsec is 3.26 million light years
whileaGigaparsec3.26billionlightyears.
TheobservableUniversehasaradiusofabout4.2
Gpc!Spaceisreallyreallybig!
ELECTROMAGNETIC RADIATION ANDTHE DIFFERENT TYPES OF TELESCOPES
ThevisiblelightthatGalileoobservedthrough
his telescope 400 years ago represents only a
raction o the actual spectrum o light that we
today know radiates across the universe. Moderntelescopes on Earth and in space allow us to
detect electromagnetic radiation beyond the kind
that we can identiy with the human eye.
Electromagnetic radiation or light is a orm o
energy which travels through space as waves o
electricandmagneticelds.Electromagnetic
spectrum (see the illustration below) is the range
ofallpossiblewavelengthsorfrequenciesof
electromagnetic radiation.
Objects such as planets, asteroids, comets and
stars emit light o dierent wavelengths or
frequencies.Visibleoropticallight(red,orange,
yellow, green, blue and violet) that human eyes
can see only represents a small part o the whole
electromagnetic spectrum. It is only relatively
recently in human history that scientists have
been able to explore and study wavelengths
beyond the visible light spectrum, through the
useoftelescopes.Theillustrationbelowhighlights the types o telescopes used in
astronomy today, both in space and on the
ground. All o these allow views o the sky that
Galileo,backin1609,couldneverhaveimagined.
Utilisingdifferenttypesoflighttoexaminethe
cosmos provides us with a more complete
understandingoftheUniverse.
Isaac Newtons telescope.
-
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SYDNEYOBSERVATORYTEACHERSNOTES15
FollowusonFacebookorTwitter#sydneyobs
2012 Australian Sky
Guidethecelestial
equivalentofastreet
directory! Compact,
easy to use and
reliable, this popular
guide contains
everything you need to
know about the
southern night sky with
monthly star maps,
diagrams and details o
all the years exciting celestial events.
Wherever you are in Australia, easy calculations
allow you to determine
when the Sun, Moon and planets will rise
and set throughout the year. Available rom
large bookstores and online at
http://from.ph/8r
SolarSystemGuide,SydneyObservatorya
quickonlineoverviewofoursolarsystem
http://www.sydneyobservatory.com.au/
education/solar-system-guide/
SydneyObservatoryNewsandBlogndout
about the latest news and astronomy viewsrom the Sydney Observatory team
http://www.sydneyobservatory.com.au/
observations-blog/
MonthlySkyGuides,SydneyObservatory
learnaboutthestars,constellationsand
planets visible in the evening night sky rom
Sydney, with monthly star charts
http://www.sydneyobservatory.com.au/
category/astronomy/monthly-sky-guides/
SpaceWeatherthelatestinformationontheSuns weather.
www.spaceweather.com
TheAngloAustralianObservatory
Astronomical and astrophysical links and images
http://www.aao.gov.au/about/abouttheaao.html
AstronomyPictureoftheDay.Thegreatest
astronomical images rom around the world
with a simple explanation.
http://apod.nasa.gov/apod/
NASAforEducators.NASAsEducation
Materials Finder will help teachers locate
resources that can be used in the classroom.
http://www.nasa.gov/audience/foreducators/
index.html
TheNinePlanets.Informationaboutthe
planets and their moons.
http://nineplanets.org/
Exoplanets.Thecompletedatabaseforall
planets discovered beyond the Solar System
so ar.
http://exoplanets.org/
ScaleoftheUniverse.Nasa.Downloadable
pdfle.
http://www.cdscc.nasa.gov/Download/Scale_
Universe.pdf
ScaleoftheUniverseHarvard.
Downloadable activity.
http://www.cfa.harvard.edu/seuforum/mtu/
MTUrealms.pdf
Astronomy:ScienceWithoutLimits.AK12
resource book o ideas or teachers by the
AustralianScienceTeachersAssociation
http://www.asta.edu.au/national_science_
week_2010/2009_asta_national_science_wee_2
http://www.asta.edu.au/
WindowtotheUniverse.TheSquareKilometre
Array. Developed as part o the Questacon-
ScitechSKAEducationprojectforyears910
http://www.asta.edu.au/resources/windows_to_
the_universe
SpaceBasedAstronomyEducatorGuide,
NASA.Unitsofstudythatincludescience
demonstrations, lesson plans and student
sheets on Earths atmosphere, the
electromagnetic spectrum and telescopeshttp://www.nasa.gov/audience/foreducators/
topnav/materials/listbytype/Space.Based.
Astronomy.html
ExploreSpaceandBeyond,ABC.News,quizzes,
games and images on space and astronomy
http://www.abc.net.au/science/
topics/?topic=space
Science&Nature:Space,BBC.General
inormation and news on space and astronomy
http://www.bbc.co.uk/science/space/
ASTRONOMY RESOURCES
http://from.ph/8rhttp://www.sydneyobservatory.com.au/education/solar-system-guide/http://www.sydneyobservatory.com.au/education/solar-system-guide/http://www.sydneyobservatory.com.au/observations-blog/http://www.sydneyobservatory.com.au/observations-blog/http://www.sydneyobservatory.com.au/category/astronomy/monthly-sky-guides/http://www.sydneyobservatory.com.au/category/astronomy/monthly-sky-guides/http://www.spaceweather.com/http://www.aao.gov.au/about/abouttheaao.htmlhttp://apod.nasa.gov/apod/http://www.nasa.gov/audience/foreducators/index.htmlhttp://www.nasa.gov/audience/foreducators/index.htmlhttp://nineplanets.org/http://exoplanets.org/http://www.cdscc.nasa.gov/Download/Scale_Universe.pdfhttp://www.cdscc.nasa.gov/Download/Scale_Universe.pdfhttp://www.cfa.harvard.edu/seuforum/mtu/MTUrealms.pdfhttp://www.cfa.harvard.edu/seuforum/mtu/MTUrealms.pdfhttp://www.asta.edu.au/national_science_week_2010/2009_asta_national_science_wee_2http://www.asta.edu.au/national_science_week_2010/2009_asta_national_science_wee_2http://www.asta.edu.au/http://www.asta.edu.au/resources/windows_to_the_universehttp://www.asta.edu.au/resources/windows_to_the_universehttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.abc.net.au/science/topics/?topic=spacehttp://www.abc.net.au/science/topics/?topic=spacehttp://www.bbc.co.uk/science/space/http://www.bbc.co.uk/science/space/http://www.abc.net.au/science/topics/?topic=spacehttp://www.abc.net.au/science/topics/?topic=spacehttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.nasa.gov/audience/foreducators/topnav/materials/listbytype/Space.Based.Astronomy.htmlhttp://www.asta.edu.au/resources/windows_to_the_universehttp://www.asta.edu.au/resources/windows_to_the_universehttp://www.asta.edu.au/http://www.asta.edu.au/national_science_week_2010/2009_asta_national_science_wee_2http://www.asta.edu.au/national_science_week_2010/2009_asta_national_science_wee_2http://www.cfa.harvard.edu/seuforum/mtu/MTUrealms.pdfhttp://www.cfa.harvard.edu/seuforum/mtu/MTUrealms.pdfhttp://www.cdscc.nasa.gov/Download/Scale_Universe.pdfhttp://www.cdscc.nasa.gov/Download/Scale_Universe.pdfhttp://exoplanets.org/http://nineplanets.org/http://www.nasa.gov/audience/foreducators/index.htmlhttp://www.nasa.gov/audience/foreducators/index.htmlhttp://apod.nasa.gov/apod/http://www.aao.gov.au/about/abouttheaao.htmlhttp://www.spaceweather.com/http://www.sydneyobservatory.com.au/category/astronomy/monthly-sky-guides/http://www.sydneyobservatory.com.au/category/astronomy/monthly-sky-guides/http://www.sydneyobservatory.com.au/observations-blog/http://www.sydneyobservatory.com.au/observations-blog/http://www.sydneyobservatory.com.au/education/solar-system-guide/http://www.sydneyobservatory.com.au/education/solar-system-guide/http://from.ph/8r -
7/31/2019 Sydney Observatory Teachers Notes 2012
16/17
SYDNEYOBSERVATORYTEACHERSNOTES16
FREE APPLICATIONS
Celestiaarealtime3-Dspacesimulatorthat
runsonPC,LinuxorMacOS.
http://www.shatters.net/celestia/
GoogleSky.Viewtheskyandexplorethe
universe online.
http://www.google.com/sky/about.html
WEATHER RESOURCES
TheBureauofMeteorologyhasprovidedthe
ollowing list o websites that may be o use prior
and ater the visit.
LatestWarnings.
www.bom.gov.au/weather/nsw/
SevereThunderstormwarnings.
www.bom.gov.au/catalogue/warnings/GSTW/
graphicalproductsnsw.shtml
AboutWarnings.
www.bom.gov.au/catalogue/warnings/
LatestWeatherChart.
www.bom.gov.au/cgi-bin/nmoc/latest_MSLP.
pl?IDCODE=IDY00050
CurrentSatelliteLoop.
http://www.bom.gov.au/products/IDE00902.
loop.shtml
LatestSydneyObservations
http://www.bom.gov.au/products/IDN60900.
shtml
RecentObservatoryHillObservations.
http://www.bom.gov.au/climate/dwo/
IDCJDW2124.latest.shtml
Graphs.
www.bom.gov.au/watl/weather/observations/
nsw-latest-weather-graphs.shtml
RadarImages.
www.bom.gov.au/watl/rainfall/radar.shtml
AboutWebRadar.
http://www.bom.gov.au/weather/radar/about/
index.shtml
LatestRainfallMaps.
www.bom.gov.au/australia/ood
Forecasts
WeatherCharts.
www.bom.gov.au/products/IDG00073.shtml
NSWStateForecast:Providesanoverviewof
the coming weather:
www.bom.gov.au/cgi-bin/wrap_fwo.
pl?IDN10031.html
RainfallForecastMaps.
www.bom.gov.au/jsp/watl/rainfall/pme.jsp
WindForecastMaps.
www.bom.gov.au/jsp/watl/wind/index.jsp
Textforecasts.
www.bom.gov.au/weather/nsw/nsw-forecast-
map.shtml
Sydneyforecast.
http://www.bom.gov.au/products/IDN10064.
shtml
SydneyUVIndex.
http://www.bom.gov.au/products/UV/Sydney_NSW.shtml
Historical Data
ClimateofObservatoryHill.
http://www.bom.gov.au/climate/averages/
tables/cw_066062.shtml
HistoricalMonthlyData.
www.bom.gov.au/climate/data
Learn About Meteorology
ReadingtheWeatherMap.
www.bom.gov.au/info/weathmap/weathmap.htm
ForecastingtheWeather.
www.bom.gov.au/info/ftweather/
SevereWeatherinNSW.
www.bom.gov.au/weather/nsw/sevwx/facts/
index.shtml
WeatherWords.
www.bom.gov.au/info/wwords/
AustralianClimateInuences.
www.bom.gov.au/watl/about-weather-and-
climate/australian-climate-inuences.html
SummariesofSignicantThunderstormsinNSW.
http://www.bom.gov.au/weather/nsw/sevwx/
signicant.shtml
StormyWeather.
http://www.bom.gov.au/weather/nsw/sevwx/
facts/stormy-weather.shtml
Please note: the websites listed were available and suitableat the time o publication. We advise teachers to check sites
beore recommending them to students.
http://www.shatters.net/celestia/http://www.google.com/sky/about.htmlhttp://www.bom.gov.au/weather/nsw/http://www.bom.gov.au/catalogue/warnings/GSTW/graphicalproductsnsw.shtmlhttp://www.bom.gov.au/catalogue/warnings/GSTW/graphicalproductsnsw.shtmlhttp://www.bom.gov.au/catalogue/warnings/http://www.bom.gov.au/cgi-bin/nmoc/latest_MSLP.pl?IDCODE=IDY00050http://www.bom.gov.au/cgi-bin/nmoc/latest_MSLP.pl?IDCODE=IDY00050http://www.bom.gov.au/products/IDE00902.loop.shtmlhttp://www.bom.gov.au/products/IDE00902.loop.shtmlhttp://www.bom.gov.au/products/IDN60900.shtmlhttp://www.bom.gov.au/products/IDN60900.shtmlhttp://www.bom.gov.au/climate/dwo/IDCJDW2124.latest.shtmlhttp://www.bom.gov.au/climate/dwo/IDCJDW2124.latest.shtmlhttp://www.bom.gov.au/watl/weather/observations/nsw-latest-weather-graphs.shtmlhttp://www.bom.gov.au/watl/weather/observations/nsw-latest-weather-graphs.shtmlhttp://www.bom.gov.au/watl/rainfall/radar.shtmlhttp://www.bom.gov.au/weather/radar/about/index.shtmlhttp://www.bom.gov.au/weather/radar/about/index.shtmlhttp://www.bom.gov.au/australia/floodhttp://www.bom.gov.au/products/IDG00073.shtmlhttp://www.bom.gov.au/cgi-bin/wrap_fwo.pl?IDN10031.htmlhttp://www.bom.gov.au/cgi-bin/wrap_fwo.pl?IDN10031.htmlhttp://www.bom.gov.au/jsp/watl/rainfall/pme.jsphttp://www.bom.gov.au/jsp/watl/wind/index.jsphttp://www.bom.gov.au/weather/nsw/nsw-forecast-map.shtmlhttp://www.bom.gov.au/weather/nsw/nsw-forecast-map.shtmlhttp://www.bom.gov.au/products/IDN10064.shtmlhttp://www.bom.gov.au/products/IDN10064.shtmlhttp://www.bom.gov.au/products/UV/Sydney_NSW.shtmlhttp://www.bom.gov.au/products/UV/Sydney_NSW.shtmlhttp://www.bom.gov.au/climate/averages/tables/cw_066062.shtmlhttp://www.bom.gov.au/climate/averages/tables/cw_066062.shtmlhttp://www.bom.gov.au/climate/datahttp://www.bom.gov.au/info/weathmap/weathmap.htmhttp://www.bom.gov.au/info/ftweather/http://www.bom.gov.au/weather/nsw/sevwx/facts/index.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/index.shtmlhttp://www.bom.gov.au/info/wwords/http://www.bom.gov.au/watl/about-weather-and-climate/australian-climate-influences.htmlhttp://www.bom.gov.au/watl/about-weather-and-climate/australian-climate-influences.htmlhttp://www.bom.gov.au/weather/nsw/sevwx/significant.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/significant.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/stormy-weather.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/stormy-weather.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/stormy-weather.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/stormy-weather.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/significant.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/significant.shtmlhttp://www.bom.gov.au/watl/about-weather-and-climate/australian-climate-influences.htmlhttp://www.bom.gov.au/watl/about-weather-and-climate/australian-climate-influences.htmlhttp://www.bom.gov.au/info/wwords/http://www.bom.gov.au/weather/nsw/sevwx/facts/index.shtmlhttp://www.bom.gov.au/weather/nsw/sevwx/facts/index.shtmlhttp://www.bom.gov.au/info/ftweather/http://www.bom.gov.au/info/weathmap/weathmap.htmhttp://www.bom.gov.au/climate/datahttp://www.bom.gov.au/climate/averages/tables/cw_066062.shtmlhttp://www.bom.gov.au/climate/averages/tables/cw_066062.shtmlhttp://www.bom.gov.au/products/UV/Sydney_NSW.shtmlhttp://www.bom.gov.au/products/UV/Sydney_NSW.shtmlhttp://www.bom.gov.au/products/IDN10064.shtmlhttp://www.bom.gov.au/products/IDN10064.shtmlhttp://www.bom.gov.au/weather/nsw/nsw-forecast-map.shtmlhttp://www.bom.gov.au/weather/nsw/nsw-forecast-map.shtmlhttp://www.bom.gov.au/jsp/watl/wind/index.jsphttp://www.bom.gov.au/jsp/watl/rainfall/pme.jsphttp://www.bom.gov.au/cgi-bin/wrap_fwo.pl?IDN10031.htmlhttp://www.bom.gov.au/cgi-bin/wrap_fwo.pl?IDN10031.htmlhttp://www.bom.gov.au/products/IDG00073.shtmlhttp://www.bom.gov.au/australia/floodhttp://www.bom.gov.au/weather/radar/about/index.shtmlhttp://www.bom.gov.au/weather/radar/about/index.shtmlhttp://www.bom.gov.au/watl/rainfall/radar.shtmlhttp://www.bom.gov.au/watl/weather/observations/nsw-latest-weather-graphs.shtmlhttp://www.bom.gov.au/watl/weather/observations/nsw-latest-weather-graphs.shtmlhttp://www.bom.gov.au/climate/dwo/IDCJDW2124.latest.shtmlhttp://www.bom.gov.au/climate/dwo/IDCJDW2124.latest.shtmlhttp://www.bom.gov.au/products/IDN60900.shtmlhttp://www.bom.gov.au/products/IDN60900.shtmlhttp://www.bom.gov.au/products/IDE00902.loop.shtmlhttp://www.bom.gov.au/products/IDE00902.loop.shtmlhttp://www.bom.gov.au/products/IDE00902.loop.shtmlhttp://www.bom.gov.au/cgi-bin/nmoc/latest_MSLP.pl?IDCODE=IDY00050http://www.bom.gov.au/cgi-bin/nmoc/latest_MSLP.pl?IDCODE=IDY00050http://www.bom.gov.au/catalogue/warnings/http://www.bom.gov.au/catalogue/warnings/GSTW/graphicalproductsnsw.shtmlhttp://www.bom.gov.au/catalogue/warnings/GSTW/graphicalproductsnsw.shtmlhttp://www.bom.gov.au/weather/nsw/http://www.google.com/sky/about.htmlhttp://www.shatters.net/celestia/ -
7/31/2019 Sydney Observatory Teachers Notes 2012
17/17
TheAustralianAboriginalpeoplehavebeen
observing the southern sky or tens o thousands
o years and the early colonists also recognised
the importance o studying the, to them, unamiliar
southern stars. A young lieutenant by the name oWilliam Dawes was given the task o setting up an
observatory when he travelled to Australia with
theFirstFleetin1788.Hesetuphisinstruments
in a wooden building at what is now called Dawes
Pointthatwasonlyafewhundredmetrestothe
north o the present day Sydney Observatory and
located where the southern pylon o the Sydney
HarbourBridgeistoday.
In1821,GovernorThomasBrisbaneestablished
AustraliasrstmajorobservatorynearGovernmentHouseinParramatta.Personally
paying the salaries o two astronomers and
installinghisownequipment,GovernorBrisbane
with the help o his sta observed the southern
skyandbegandocumentingunknownstars.The
observations were published in the Catalogue o
7385starsfromobservationsmadeatthe
observatoryatParramattain1835.Withlittle
2011TrusteesoftheMuseumofAppliedArtsandSciences.Revised
August2012.Thedesignandimagesinthispublicationarecopyright.Apart rom air dealing or the purposes o research, study, criticism or
review, or as otherwise permitted under the Copyright Act, no part may be
reproduced by any process without written permission.
TextmaybeusedunderCreativeCommonsLicenceAttribution-Non Commercial-No Derivatives 3.0 Australia.
SydneyObservatory,partofthePowerhouseMuseum,isaNSWgovernmentcultural institution.
Imagesabove:insidethe3-Dspacetheatre;Sydney
Observatory,northdome;alunareclipse,photobyMelissa
Hulbert;SydneyObservatoryatnight.
BOOKING YOUR VISIT
Bookingsareessentialforalleducationgroups.
When you book, education sta are allocated to
assist your group on arrival. Discuss your needs
with our education sta on booking, to get the
most rom your visit.
Contact Details
Sydney Observatory
WatsonRoad,MillersPoint
Phone:(02)99213485Fax: (02) 9921 3489
Email: [email protected]
Web:www.sydneyobservatory.com
supportforitscontinuation,Parramatta
Observatorywasforcedtoclosein1847.However,
by 1855, the colonial government could not
ignore the need or a time ball to provide
accuratetimetoshipsintheHarbouraswellasor an observatory in Sydney.
Threeyearslaterconstructionofthenew
observatory with its time ball tower was
sufcientlyadvancedforobservationstobegin.
Work at the Observatory included determining
star positions, measuring precise longitudes and
latitudes, keeping time and making
meteorological (weather) observations.
More than 150 years later Sydney Observatory isa public observatory and is part o the
PowerhouseMuseum.Wespecialisein
astronomical, meteorological and archaeological
learning and enjoyment.
School programs operate throughout each term
day and night making it the busiest cultural
institution o its type in Australia.
Cancellation Policyschoolscancancelabookingupto
two weeks prior to the date o their tour. Cancellations made
less than two weeks prior to a visit are charged hal the ull
rate o the booked tour. You must cancel by ax.
A BRIEF HISTORY OF THE OBSERVATORY
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