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Transcript
STR
S RO
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TABLEOFCONTENTS
Introduction...............................................................................................................................................................................................................3 EducationalGoalsforAstronomy1.................................................................................................................................................................4 MasterMaterialsListforAllLabs.....................................................................................................................................................................5 LabSafety...................................................................................................................................................................................................................6 Lesson#1:PlanetariumandStarShow.........................................................................................................................................................7 Lesson#2:SolarSystemTreasureHunt......................................................................................................................................................10 Lesson#3:MagneticTornadoes.....................................................................................................................................................................28 Lesson#4:SkyinaJar.........................................................................................................................................................................................31 Lesson#5:PlanetaryMagneticFields..........................................................................................................................................................34 Lesson#6:Seasons...............................................................................................................................................................................................36 Lesson#7:IndoorRainClouds........................................................................................................................................................................40 Lesson#8:Volcanoes..........................................................................................................................................................................................42 Lesson#9:StarGazing........................................................................................................................................................................................46 Lesson#10:SongoftheSun.............................................................................................................................................................................49 Lesson#11:SimpleMicroscope&Telescope............................................................................................................................................53 Lesson#12:StarCharting.................................................................................................................................................................................56 Astronomy1Evaluation.....................................................................................................................................................................................58 Astronomy1Quiz..................................................................................................................................................................................................59 Astronomy1LabPractical................................................................................................................................................................................60 AnswerstoExercisesandActivities..............................................................................................................................................................61 VocabularyfortheUnit.......................................................................................................................................................................................66 ©2014SuperchargedScience
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Introduction
GreetingsandwelcometothestudyofAstronomy.Thisunitwascreatedbyamechanicalengineer,university
instructor,airplanepilot,astronomer,robot‐builderandrealrocketscientist…me!Ihavethehappyopportunityto
teachyoueverythingIknowaboutastronomyoverthenextsetoflessons.Ipromisetogiveyoumybeststuffso
youcantakeitandrunwithit…orfly!
Astrophysicscombinestheknowledgeoflight(electromagneticradiation),chemicalreactions,atoms,energy,and
physicalmotionallintoone.Togetthemostoutoftheselabs,therearereallyonlyacoupleofthingstokeepin
mind.Sinceweareallheretohavefunandlearnsomethingnew,thisshouldn’tbetoohard.
Oneofthebestthingsyoucandoasthestudentistocultivateyourcuriosityaboutthings.Whydidthatmove?How
didthatspin?What’sreallygoingonhere?
ThisunitonAstronomyischock‐fullofdemonstrationsandexperimentsfortwobigreasons.First,they’refun.But
moreimportantly,thereasonwedoexperimentsinscienceistohoneyourobservationalskills.Science
experimentsreallyspeakforthemselvesmuchbetterthanIcaneverputintowordsorshowyouonavideo.And
I’mgoingtohityouwithalotofthesesciencedemonstrationsandexperimentstohelpyoudevelopyourobserving
techniques.
Scientistsnotonlylearntoobservewhat’sgoingonintheexperiment,buttheyalsolearnhowtoobservewhat
theirexperimentistellingthem,whichisfoundbylookingatyourdata.It’snotenoughtoinventsomenewkindof
experimentifyoudon’tknowhowitwillperformwhentheconditionschangeabit,likeonMars.We’regoingto
learnhowtopredictwhatwethinkwillhappen,designexperimentsthatwilltestthisidea,andlookoverthe
resultswegottofigureoutwheretogofromthere.Scienceisaprocess,it’sawayofthinking,andwe’regoingto
getplentyofpracticeatit.
Goodluckwiththisastronomyunit!
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FortheParent/Teacher:
EducationalGoalsforAstronomy1
Astrophysicsisthebranchofastronomythatdealswiththephysicsoftheuniverse.Astronomersstudycelestial
objects(thingslikestars,planets,moons,asteroids,comets,galaxies,andsoforth)thatexistoutsideEarth’s
atmosphere.It’stheonefieldofstudythatcombinesthemostscience,engineeringandtechnologyareasinonefell
swoop.Astronomyisalsooneoftheoldestsciencesontheplanet.We’regoingtobestudyingdifferentareaswithin
astronomythatcoverthemoon,planets,stars,andotherobjects.
Herearethescientificconcepts:
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Objectsintheskymoveinregularandpredictablepatterns.Thepatternsofstarsstaythesame,although
theyappeartomoveacrosstheskynightly,anddifferentstarscanbeseenindifferentseasons.
ThetiltoftheEarthanditslocationinorbitarethereasonsfortheseasons.
TheEarthisoneofseveralplanetsthatorbittheSun,andtheMoonorbitstheEarth.
ThesolarsystemconsistsofplanetsandotherbodiesthatorbittheSuninpredictablepaths.
Oursolarsystemincludesrockyterrestrialplanets(Mercury,Venus,Earth,andMars),gasgiants(Jupiter
andSaturn),icegiants(UranusandNeptune),andassortedchunksoficeanddustthatmakeupvarious
cometsandasteroids.
Twoplanets(CeresandPluto)havebeenreclassifiedafterastronomersfoundoutmoreinformationabout
theirneighbors.
TelescopesmagnifytheappearanceoftheMoonandtheplanets.
TelescopesmagnifytheappearanceoftheSunusingspeciallensesandmakeitpossibletolocateSunspots
andsolarflares.
Starsarethesourceoflightforallbrightobjectsinouterspace.TheMoonandplanetsshinebyreflected
Sunlight,notbytheirownlight.
Thenumberofstarsthatcanbeseenthroughtelescopesisdramaticallygreaterthancanbeseenbythe
unaidedeye.
Bytheendofthelabsinthisunit,studentswillbeableto:
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Designandbuildatelescopeusingopticalequipmentlikelenses.
Knowhowtodemonstratehowthepositionofobjectsintheskychangesovertime.
Knowthecelestialobjectsinthesolarsystemandhowtheyrelateandinteractwitheachother.
Formulateandjustifypredictionsbasedoncause‐and‐effectrelationships.
Conductmultipletrialstotestapredictionanddrawconclusionsabouttherelationshipsbetween
predictionsandresults.
Constructandinterpretgraphsfrommeasurements.
Followasetofwritteninstructionsforascientificinvestigation.
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MasterMaterialsListforAllLabs
Thisisabrieflistofthematerialsthatyouwillneedtodoalloftheactivities,experimentsandprojectsinthisunit.
Thesetofmaterialslistedbelowisjustforonelabgroup.Ifyouhaveaclassof10labgroups,you’llneedtoget10
setsofthematerialslistedbelow.Mostmaterialsarereusable.
Aluminumpan
Bakingsoda(1/4cup)
Balloon
Barmagnet
Circular(disk)magnet
Compass
Dirt(3cups)
Dollarbill
Ducttape(optional)
Fingernailpolish(red,yellow,
green,blue)
Flashlights(3or4)
Flexibletubing(18")‐optional
©2014SuperchargedScience
Flour(9cups)
Glassjar
Hand‐heldmagnifyinglenses(2)
Horseshoemagnet
Liquidcrystalthermometers(2)
Liquiddishsoap
Marker
Maskingtape
Milk(coupledrops)
Musicalinstruments(anyyou
alreadyhave)
Pencil
Penny
Plasticbottles(2litersoda
bottles)
Protractor
Rocks
Ruler
Salt(4cups)
Steelwasherwitha3/8inch
hole
Stopwatch
String
Tape(clear,notfrosted)
Vegetableoil(1/2cup)
Waterbottle(empty)
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LabSafety
Goggles:Theseshouldbewornwhenworkingwithchemicals,heat,fire,orprojectiles.Theseprotectyoureyes
fromchemicalsplatter,explosions,andtinyfast‐movingobjectsaimedattheeyes.Ifyouwearglasses,youcanfind
gogglesthatfitoverthem.Don’tsubstituteeyeglassesforgoggles,becauseofthelackofsideprotection.Eyeglasses
don’tprovidethisimportantprotection.
CleanupMesses:Yourlabareashouldbeneat,organized,andspotlessbeforeyoustart,duringyourexperiment,
andwhenyouleave.Scientistswastemoretimehuntingforlostpapers,piecesofanexperiment,andtryingto
repositionsensitiveequipment…allofwhichcouldhaveeasilybeenavoidedhadtheybeentaughtorganizational
skillsfromthestart.
DisposeofPoisons:Ifapoisonoussubstancewasused,created,orproducedduringyourexperiment,youmust
followtheproperhandlingproceduresfordisposal.You’llfinddetailsforthisintheexperimentsasneeded.
SpecialNotesonBatteries:Donotusealkalinebatterieswithyourexperiments.Findthesuper‐cheapkindof
batteries(usuallylabeled“HeavyDuty”or“SuperHeavyDuty”)becausethesetypesofbatterieshaveacarbon‐zinc
core,whichdoesnotcontaintheacidthatalkalinebatterieshave.Thismeanswhenyouwireupcircuitsincorrectly
(whichyoushouldexpecttodobecauseyouarelearning),thecircuitswillnotoverheatorleak.Ifyouusealkaline
batteries(likeEnergizerandDuracell)andyourstudentsshortacircuit,theirwiresandcomponentswillget
super‐hotandleakacid,whichisverydangerous.
NoEatingorDrinkingintheLab:Allfoodsanddrinksarebannedfromyourclassroomduringscience
experimentation.Whenyoueatordrink,youruntheveryrealriskofingestingpartofyourexperiment.For
electricityandmagnetismlabs,alwayswashyourhandsafterthelabisovertorinseofftheleadfromtheelectrical
components.
NoHorsePlay:Whenyougoofaround,accidentshappen,whichmeanschemicalsspill,circuitsshort,andallkinds
ofhazardscanoccurthatyouweren’texpecting.Neverthrowanythingtoanotherpersonandbecarefulwhereyou
putyourhands–itcouldbeinthemiddleofasensitiveexperiment,especiallywithmagnetismandelectricity.You
don’twanttoruntheriskofgettingshockedorelectrifiedwhenit’snotpartofyourexperiment.
Fire:Ifyouthinkthere’safireintheroom(evenifyou’renotsure),letyourteacherknowrightaway.Iftheyare
notaround(theyalwaysshouldbe),smotherthefirewithafireblanketoruseafireextinguisherandsend
someonetofindanadult.Stop,drop,androll!
Questions:Ifyou’renotsureaboutsomething,stopandask,nomatterwhatit’sabout.Ifyoudon’tknowhowto
properlyhandleachemical,dopartofanexperiment,ask!Ifyou’renotcomfortabledoingpartoftheexperiment,
thendon’tdoit.
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Lesson#1:PlanetariumandStarShow
OverviewGreetingsandwelcometothestudyofastronomy!Thisfirstlessonissimplytogetyouexcitedand
interestedinastronomysoyoucandecidewhatitisthatyouwanttolearnaboutastronomylateron.
WhattoLearnWe’regoingtocoveralotinthispresentation,including:TheSun,anaveragestar,isthecentral
andlargestbodyinthesolarsystemandiscomposedprimarilyofhydrogenandhelium.
ThesolarsystemincludestheEarth,Moon,Sun,eightotherplanetsandtheirsatellites,andsmallerobjectssuchas
asteroidsandcomets.Thestructureandcompositionoftheuniversecanbelearnedfromthestudyofstarsand
galaxies.Galaxiesareclustersofbillionsofstars,andmayhavedifferentshapes.TheSunisoneofmanystarsin
ourownMilkyWaygalaxy.Starsmaydifferinsize,temperature,andcolor.
Materials


Popcorn(toeatifyou’dliketo)
Pencil
Experiment
Beforewatchingthevideo,printoutyourworksheetsoyoucanjotthingsdownasyoulisten.Thengrabyour
pencil(andahandfulofpopcorn)andfillitinasyougoalong,orsimplyenjoytheshowandfillitoutattheend.
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PlanetariumStarShowTable
Planet
InterestingFactYouDidn’tKnow‘TilNow
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Reading
Astrophysicsisthebranchofastronomythatdealswiththephysicsoftheuniverse.Astronomersstudycelestial
objects(thingslikestars,planets,moons,asteroids,comets,galaxies,andsoforth)thatexistoutsideEarth’s
atmosphere.It’stheonefieldofstudythatcombinesthemostscience,engineeringandtechnologyareasinonefell
swoop.Astronomyisalsooneoftheoldestsciencesontheplanet.
Earlyastronomerstrackedthemovementofthestarssoaccuratelythatinmostcases,we’veonlymademinor
adjustmentstotheirdata.AlthoughGalileowasn’tthefirstpersontolookthroughatelescope,hewasthefirstto
pointitatthestars.Originally,astronomywasusedforcelestialnavigationandwasinvolvedwiththemakingof
calendars,butnowadaysit’smostlyclassifiedinthefieldcalledastrophysics.
QuestionstoAnswer:
1. WhathappenedtoPluto?Whyisn’titaplanetanymore?
2. HowdoestheSunmakeenergy?
3. Whichplanetisyourfavoriteandwhy?
4. HowmanymoonsaroundJupiterandSaturncanyouseewithbinoculars?
5. What’sthedifferencebetweenagalaxyandablackhole?
6. HowmanyEarthscanfitinsidetheSun?
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Lesson#2:SolarSystemTreasureHunt
Overview:Funday!Yougettodonotone,buttwotreasurehuntstoday.Thefirstisonpaperandasksquestions
aboutthepresentationfromlasttime.Thesecondactivityhas10clueswithrealtreasure.Themoreyouknow
aboutastronomy,thefasteryou’llmovethroughthese.
WhattoLearn:Todayyou’lldiscoverhowmuchyoualreadyknowaboutthespecificdetailsaboutalleight
planets,theSunanditscomposition,selectednaturalsatellites,andsmallerobjectssuchasasteroids,dwarf
planets,andcomets.
Materials


Apencil
Printoutthecluecards(haveanadulthelperhidethemforyou)
Experiment
1. Therearetworoundsforthistreasurehunt:indoorsandoutdoors(iftheweather’scooperating).Ina
moment,youaregoingtosearchyourindoorareaforanswerstotheseclues.
2. HavesomeoneelsecutouttheFirstTreasureHuntClueCardsandhidetheminplainviewforyoutofind.
3. Whiletheyarehidingthecluesforyou,printouttheFirstTreasureHuntClueWorksheet.You’llusethis
whenyousearchfortheclues.
4. Whenready,gofindyourcluecardsandfilloutyourworksheet!
5. Whileyou’reworkingonfindingtheclues,yourassistantwillgetbusyhidingthecluesfromtheSecond
TreasureHunt.
6. Onceyou’vecompletedthefirsttreasurehuntandcompletedyourworksheet,letyourassistantknowand
theywillhandyouthefirstcardfromtheSecondTreasureHuntandsendyouonyourway.
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FirstTreasureHuntClueCards:Havesomeoneelsecuttheseoutandpasteinplainviewallovertheroomtofind
easily.Youwillbeanswering50questions.Somecardscontaininformationformorethanonequestion,soyou’ll
findthereare37cluecardsforthefirstpartoftheactivity.
AllimagesprovidedcourtesyofNASA.
Shapeofoursolarsystemisapproximately
circular.
TheSunrotatesonceevery31daysatthepoles
andonceevery27daysattheequator.
PlutoisnowpartoftheKuiperBelt.
Oursolarsystemhaseightplanets,theirmoons,
asteroidsandcomets.
ThecoretemperatureoftheSunis15million
degreesCelsius.
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AplanetisanobjectthatorbitstheSun,is
massiveenoughforitsowngravitytomakeit
round,andhascleareditsorbitofsmaller
objects.
Mercuryisthesecondhottestplanetat800oF
(427oC).ThesidefacingawayfromtheSunis
‐280oF(‐173oC)
Venusisthehottestplanetat863oF(462oC).
AlthoughUranusismademostlyofhydrogenand
helium,it’sthecoldmethanegasthatgivesthe
blue‐greencolor.
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TheSunismadeupof25%heliumand75%
hydrogen.
Venustakeslongertospinonceonitsownaxis
thanitdoestoorbittheSun.Notonlythat,it
rotatesintheoppositedirectionfromtherestof
theplanets.
Cometsaremadeofdustandice,makingthem
justlikedirtysnowballs.Wethinkthattheiceon
Mercurywasleftbyimpactsfromcomets.
TheEarth’satmosphereismadeupof21%
oxygenand78%nitrogen,withtraceamountsof
othermolecules.
Venuswasnamedafterthegoddessofloveand
beautybecauseitisthebrightestobjectinthe
sky,otherthantheSunandMoon.
TheMooncausesbothoceanandlandtideson
theEarth.
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ThetwomoonsofMarsarenamedafter
Fear/Panic(Phobos)andFleeing(Deimos).
Jupiterismadeofhydrogenandheliumwitha
metallichydrogencore.It’saslargeasitcanbe
withoutshrinking.Ifyouaddedmoremass
(hydrogengas)toit,Jupiterwouldcondenseand
getsmaller.Ifyouincreaseditsmassby80X,it
wouldcompressandbecomeastar.
Ironoxide(rust)givesMarsitsredcolor.The
whiteatthepolesaredryice(frozencarbon
dioxide)andwaterice.
1400EarthscanfitinsideofJupiter.IfJupiter
werethesizeofasoccerball,theEarthwouldbe
amarble.Alltheotherplanetscanfittogether
insideJupiter.
Saturn’sringsaremademostlyoutofice
travellingat75,000mph.
ThereareshepherdmoonsinsideSaturn’srings.
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Mercury,Venus,EarthandMarsarerocky
terrestrialplanets.JupiterandSaturnaregas
giants.UranusandNeptuneareicegiants.Pluto,
Ceres,Haumea,Makemake,andErisaredwarf
planets.
Titanhasanatmospheremademostlyof
nitrogen.
WethinkSaturn’smoon,Iapetus,usedtohavea
ringaroundit.
Saturn’smoonMimasiswhereStarWarsgotthe
ideafortheDeathStar.
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Uranusistheonlyplanetthatrollsaroundthe
Sun,tippedoveronitsside.
PhobosisslowlymovinginwardtowardMars,
andwhenthetidalforcesinsidethismoon
becomestronger,theywilleithershatterthe
moonintoameteorshowerorcausethebitsto
formaringaroundMars.
TheaveragedailywindspeedonNeptuneis
1200mph.Neptuneradiates2.6timesasmuch
energyoutasitreceivesfromtheSun.
Neptune’sbluecolorisfromthemethanegas,but
it’salsomadeupofhydrogenandhelium.Since
it’sthefurthestplanetfromtheSun(30au,or4.5
billionkm,or2billionmiles),it’salsothecoldest.
Notethatthefivedwarfplanetsarecolder
objectsthanNeptune,sincetheyarefurtherstill.
PlutoandCharonorbiteachother,andarealso
orbitedbyHydraandNix.
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70%oftheEarthiscoveredbywater.2%ofthis
islockedinice.
TheSunis1au(astronomicalunit)fromthe
Earth.1auis93millionmiles.Ittakeslightabout
8minutestotravelthisdistance.
Venusisthehottestplanetbecauseittrapsthe
heatinsideonceitentersthethickatmosphere.
ThevolcanoesonVenusaresoactivethatthe
planetisconstantlyresurfacingitself.
Bluestarsmeasureabove10,000K(17,540oFor
9,727oC)atthesurface.Redstarsareabout
2500K(4,040oFor2,227oC).OurSun,awhite
star,is6,000K(10,340oFor5,727oC).
Note:K(Kelvin)istheabsolutetemperature
scaleforCelsius.
ThePistolstarreleasesasmuchenergyinone
secondasourSundoesinoneyear.
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12peoplehavewalkedontheMoon.
Approximately7billionpeoplewalkontheEarth
today.
Jupiter’sgiantstorm,theGreatRedSpot,is
actuallygettingsmaller.Thecurrentsizeisabout
twoEarthdiameters.
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FirstTreasureHunt:Answerthequestionsbelowasyousearcharoundyouforcluestotheanswer.Goodluck!
1. TheshapeofourSolarSystemis_________________________.
2. Howmanyplanetsdowehaveinoursolarsystem?____________________________
3. Plutoisnowpartofthe___________________________Belt.
4. TheSunrotatesonceevery_____________________atitsequatorand___________________atthepoles.
5. ThecoretemperatureoftheSunis________________________________.
6. Aplanethasthreecriteria:itorbitsthe_____________________________________,has_________________________________
itsorbitofsmallerobjects,andislargeenoughsoitsown_______________________________makesitround.
7. Therearethreetypesofplanets:____________________________,___________________________________,and
________________________.
8. _______________________istheclosest,butnotthehottestplanet.ThesidefacingtheSungetsto
_______________________oF,andthesidefacingawayfromtheSungetsto____________________________oF.
9. Thesolarsystemincludes________________________planets,their____________________,the__________________atthe
center,andsmallerobjectssuchas________________________and____________________________.
10. TheSunismadeoutof75%___________________and25%_____________________.
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11. Venusiscalledthegoddessof_______________________,becauseitlookssobrighttousfromEarth,butitreally
hasasurfacetemperatureof_______________________oF.
12. Cometsarereallydirty____________________________________________.
13. ____________________isthebrightestthinginthesky,otherthantheSunandMoon.
14. Cold_____________________iswhatgivesUranusitsblue‐greencolor.It’sclassifiedas_________________giant.
15. Onedayislongerthanayearon______________________________.Notonlythat,itrotates_____________________.
16. Earth’satmosphereismadeupof21%_______________and78%_________________.
17. TheMoonpullsonthesurfaceontheEarthandcausestidesonboththe____________and_______________.
18. Mars’smoonsarenamedafter________________________and___________________________.
19. ________________________givesMarsitsredcolor.
20. IftheEarthwasthesizeofamarble,Jupiterwouldbethesizeofa______________________________.
21. Jupitercanfit____________________________Earthsinside.
22. Ifyouaddedmoremassto_______________________________itwouldgetsmallerbecauseit’sabigballof
__________________________.
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23. Jupiterismadeoutof__________________________and__________________________withametallic__________________
core.
24. ThevolcanoesonJupiter’smoon____________spewiceash_____________________mileshigh.
25. Saturnissurroundedbyringsmademostlyof__________________movingat__________________mph.
26. InsideSaturn’sringsare__________________.
27. Titanhasan________________________________mademostlyof__________________________,sothickthatifyou
strappedwingsontoyourarmsandflapped,you’dfly!
28. Scientiststhinkthat________________________usedtohavearingaroundit,anditcrasheddownontothe
surface.
29. Jupiterissolargethatallofthe________________inthesolarsystemcouldfitinsideofit.
30. _______________________looksjustliketheDeathStar.
31. Theplanet_____________________rollsaroundtheSunwhiletippedonitsside.
32. Phobosisslowlymovinginwardtoward________________andwilleithershatterorforma_________________
around__________________________.
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33. OurbestguessisthattheiceonMercurywascausedby_____________________________________
34. AveragedailywindspeedonNeptuneis_____________mph.
35. Neptuneisagiantballof____________________,whichisalsoknownas_________________.
36. __________________andPlutoareapairofobjectsbecausetheybothrotatearoundapointoutsideofeach.
Thesetwoarealsoorbitedby______________and_______________.
37. SeventypercentoftheEarth'ssurfaceiscoveredby_________________________.
38. TheSunis__________________________________milesfromtheEarth,alsoknownas_______________________________.
39. Thehottestplanetis_________________________________________________becausetheheatthatcomesintotheplanet
gets________________________________________________________________________________________________.
40. Therearehowmanystarsareinoursolarsystem?___________________________________________
41. Whichcolorstarsarethehottest?____________________________________Coolest?_______________________________
42. The_____________________________staristhebiggestonewe’vefoundanditreleasesasmuchenergyinone
_________________________asourSundoesinoneyear.
43. Theplanetsandmoonsthatpeoplehavewalkedonare___________________________________________________
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44. Jupiter's_____________________________isgetting_________________________.It’saboutthesizeoftwo
__________________rightnow.
45. __________________________and________________________aregasgiants,and_______________________and
_________________________areicegiants.
46. ____________________________isthecoldestplanetinoursolarsystem.
47. Thefivedwarfplanetsinoursolarsystemare:
______________________________________________________________________________________________________________
48. Ittakeslight_______________________________totravelfromtheSuntoEarth.
49. _____________________________hassomuchvolcanicactivitythatitconstantlyresurfacesitself.
50. WhatkindoficeisonMars?_____________________________and_______________________________________.
STOP!!!You’redonewiththefirstactivity!
Greatjobansweringthequestions!Stapleyourpaperstogether(orputyournameatthetopofeachpageatthe
veryleast)andturnitinsoyoucanstartonthesecondactivity.
Forthesecondtreasurehunt,selectoneofthefollowingthreepages.Eachpagehasasetofcluesdependingon
whereyoudoyourhunt.Youonlyneedtocompleteoneofthethreehunts.Remember,forthisnextpart,you
MUSTfindthecluesinorder,meaningthatyouhavetofindtheobjecttheclueisdescribingoritdoesn’tcount.
Havefun!
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CluesforthePlaygroundHunt:Cuttheseoutandtapethemaroundtheplayground.Youcanaddapictureof
eachobjectalongwiththeclueifyouwish.Makesureyou’vewarnedthekidsnottotaketheclues,butjustLOOK
atthem.Inadditiontoaplayground,you’llneedtotossasoccerballandfootballonyourfieldfarapartfromeach
other.Asyouplaceeachclueinitsproperspot,ripoffthetabontheleftwiththeinstructionsthatwerejustfor
you.Makesureyou’vegotthetreasurewithyouwhenthekidscometearingbacktoyouwiththefinalclue.Have
fun!
The Sun (CLUE #1): Show
this clue to get started.
Mercury (CLUE #2): Tape
this clue under one of the
swings.
Venus (CLUE #3): Tape
this clue to a football.
Earth (CLUE #4): Tape this
clue in a tree (or plant).
Mars (CLUE #5): Tape this
clue near the drinking
fountain.
Jupiter (CLUE #6): Tape
this clue at the top of a
slide.
Saturn (CLUE #7): Tape
this clue on the monkey
bars.
Uranus (CLUE #8): Tape
this clue on the exterior of a
nearby door.
Neptune (CLUE #9): Tape
this clue on the exterior of a
window.
Pluto (CLUE #10): Tape
this clue on a soccer ball.
©2014SuperchargedScience
This object is hot, but not on fire.
Explore the swings but don’t perspire!
This planet is closest, but not the hottest.
Check the football, and don’t be modest!
This planet is so hot it can melt a cannonball,
Crush spaceships, rain acid, and is in a tree tall.
Most of this planet is covered with water.
Find some water that never gets hotter.
This planet is basically a rusty burp.
Discover the slide and take a ride.
A planet so large it can hold the rest,
Explore the bars with infinite zest!
This planet had rings, but not made of gold.
Explore near a door like an astronaut bold!
Smacked so hard it now rolls on its side,
Find the window that is ever so wide.
Check the soccer ball for hurricane,
gigantic blue farts, and diamond rain.
Instead of one there were two, then four…
Visit your teacher for the one that is no more.
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CluesfortheClassroomHunt:Cuttheseoutandhidetheminenvelopesaroundyourclassroom.Youcanadda
pictureofeachobjectalongwiththeclueifyouwish.Thisisgreatforrainyschooldays.Remindthekidsthatthey
havetofindtherightclueandgoinorder!Youcannumberthemifyouwantto,orhavetheirlabpartnershold
themaccountable.Alsoremindthemnottotaketheclues,butlookatthemandmoveon.Whenyouplacetheclue
initsproperspot,ripoffthetabontheleftwiththeinstructionsthatwerejustforyou.Placethetreasureunder
yourdeskforthefinalclue.Havefun!
The Sun (CLUE #1): Show
this clue to get started.
This object is hot, but not on fire.
Explore the coats but don’t perspire!
Mercury (CLUE #2): Tape
this clue with the coats.
This planet is closest, but not the hottest.
Check the floor, and don’t be modest!
Venus (CLUE #3): Tape
this clue in a corner on the
floor.
Earth (CLUE #4): Tape this
clue on something very tall.
This planet is so hot it can melt a cannonball,
Crush spaceships, rain acid, and is on an object tall.
Most of this planet is covered with water.
Find some water but don’t make it hotter.
Mars (CLUE #5): Tape this
clue to your sink or a water
bottle left out on the
counter.
Jupiter (CLUE #6): Tape
this clue next to where they
store lunches. You can also
stick it right on a lunchbox.
Saturn (CLUE #7): Hide
this clue with a stack of
books.
Uranus (CLUE #8): Tape
this clue on the classroom
door.
Neptune (CLUE #9): Tape
this clue on a window.
This planet is basically a rusty burp.
Where would you take a bite and slurp?
A planet so large it can hold the rest,
Explore our library with infinite zest!
This planet had rings, but not made of gold.
Explore the door like an astronaut bold!
Smacked so hard it now rolls on its side,
Find the window that is ever so wide.
Check the ceiling for hurricane,
gigantic blue farts, and diamond rain.
Pluto (CLUE #10): Tape
this clue on the ceiling.
©2014SuperchargedScience
Instead of one there were two, then four…
Look under a desk for the one that is no more.
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CluesfortheHouseholdHunt:Cuttheseoutandhidetheminenvelopesaroundyourhouse.Youcanadda
pictureofeachobjectalongwiththeclueifyouwish.Thisisgreatforhomeworkassignments,homeschool
students,andhomestudyprograms.Remindthekidsthattheyhavetofindtherightclueandgoinorder!When
youplacetheclueinitsproperspot,ripofthetabontheleftwiththeinstructionsthatwerejustforyou.Placethe
treasureinthemailboxforthefinalclue.Havefun!
The Sun (CLUE #1): Show
this clue to get started.
This object is hot, but not on fire.
Explore the dryer but don’t perspire!
Mercury (CLUE #2): Hide
this in the dryer.
This planet is closest, but not the hottest.
Check the sock drawer, and don’t be modest!
This planet is so hot it can melt a cannonball,
Crush spaceships, rain acid, and is in a tree tall.
Venus (CLUE #3): Hide
this in the sock drawer.
Earth (CLUE #4): Hide this
clue in a tree (or plant).
Most of this planet is covered with water.
Visit the bathtub without making it hotter.
Mars (CLUE #5): Hide this
clue in the bathtub.
This planet is basically a rusty burp.
Discover the refrigerator and take a slurp.
Jupiter (CLUE #6): Hide
this clue next to the milk.
A planet so large it can hold the rest,
Explore our library with infinite zest!
Saturn (CLUE #7): Hide
this clue with a stack of
books.
Uranus (CLUE #8): Hide
this clue on the front door.
This planet had rings, but not made of gold.
Explore near the front door like an astronaut bold!
Smacked so hard it now rolls on its side,
Find the window that is ever so wide.
Neptune (CLUE #9): Hide
this clue by sticking it on a
window.
Pluto (CLUE #10): Hide
this clue in the sink.
©2014SuperchargedScience
Check the sink for hurricane,
gigantic blue farts, and diamond rain.
Instead of one there were two, then four…
Visit the mailbox for the one that is no more.
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Reading
Oursolarsystemincludesrockyterrestrialplanets(Mercury,Venus,Earth,andMars),gasgiants(Jupiterand
Saturn),icegiants(UranusandNeptune),andassortedchunksoficeanddustthatmakeupvariouscometsand
asteroids.
Twoplanets(CeresandPluto)havebeenreclassifiedafterastronomersfoundoutmoreinformationabouttheir
neighbors.CeresisnowanasteroidintheAsteroidBeltbetweenMarsandJupiter.BeyondNeptune,theKuiper
Beltholdsthechunksoficeanddust,likecometsandasteroidsaswellaslargerobjectslikedwarfplanetsErisand
Pluto.
BeyondtheKuiperbeltisanareacalledtheOortCloud,whichholdsanestimated1trillioncomets.TheOortCloud
issofarawaythatit’sonlylooselyheldinorbitbyourSun,andconstantlybeingpulledgravitationallybypassing
starsandtheMilkyWayitself.TheVoyagerSpacecraftarebeyondtheheliosphere(theregioninfluenced
gravitationallybyourSun)buthavenotreachedtheOortCloud.
TheSunholds99%ofthemassofoursolarsystem.TheSun’sequatortakesabout25daystorotatearoundonce,
butthepolestake34days.YoumayhaveheardthattheSunisahugeballofburninggas.ButtheSunisnotonfire,
likeacandle.Youcan’tblowitoutorreigniteit.So,wheredoestheenergycomefrom?
Thenuclearreactionsdeepinthecoretransform600milliontonspersecondofhydrogenintohelium.Thisgives
offhugeamountsofenergywhichgraduallyworksitswayfromthe15million‐degreeCelsiustemperaturecoreto
the15,000‐degreeCelsiussurface.
Starsliketolivetogetherinfamilies.Galaxiesaregroupsofstarsthatarepulledandheldtogetherbygravity.Some
galaxiesaresparsewhileothersarepackedsodenselyyoucan’tseethroughthem.Galaxiesalsoliketohangout
withothergalaxies(calledgalaxyclusters),butnotallgalaxiesbelongtoclusters,andnotallstarsbelongtoa
galaxy.
Activegalaxieshaveveryunusualbehavior.Thereareseveraldifferenttypesofactivegalaxies,includingradio
galaxies(edge‐onviewofgalaxiesemittingjets),quasars(3/4viewofthegalaxyemittingjets),blazars(alignedso
we’relookingstraightdownintotheblackholejet),andothers.Ourowngalaxy,theMilkyWay,hasasuper‐
massiveblackholeatitscenter,whichiscurrentlyquietanddormant.
Dyingstarsblowoffshellsofheatedgasthatglowinbeautifulpatterns.WilliamHershel(1795)coinedtheterm
“planetarynebula”becausetheoneshelookedatthrough18thcenturytelescopeslookedlikeplanets.They
actuallyhavenothingtodowithplanets–theyareshellsofdustfeatheringaway.
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Lesson#3:MagneticTornadoes
Overview:ThislabisaphysicalmodelofwhathappensonMercurywhentwomagneticfieldscollideandform
magnetictornadoes.
WhattoLearn:You’llgettoinvestigatewhataninvisiblemagnetictornadolookslikewhenitsweepsacross
Mercury.
Materials





Twoclearplasticbottles(2litersodabottlesworkbest)
Steelwasherwitha3/8inchhole
Rulerandstopwatch
Glitterorconfetti(optional)
Ducttape(optional)
Experiment
1. Determinethedifferentwaterconditions,suchas:changingthetemperature,changingthevolume(height
ofwater),addinganothermoleculesuchasoil,isopropylalcohol,vinegar,anddishsoap,addingsolid
piecessuchasglitter,salt,sugar,orsmallgrains.Thedifferentmixtureswillgivedifferentvortexrotation
speedsanddifferentdraintimes.ThisisequivalenttochangingtheatmosphereonEarthandseeinghowit
affectsweather(notmagnetic)tornadoes.Writetheconditionsyouwishtotestinthedatatablebeforeyou
start.
2. Filloneofthesodabottleswithwaterusingthedatatable.Setthebottleuprightonthetable.
3. Setthewasherontopofthebottleopening.Makesurethere’snocaponthebottle.
4. Inverttheemptybottleoverthewater‐filledbottleandlineuptheopeningssotheycanbeeasilytaped
together.Youwanttotapethembeforetheygetwetwiththewasherbetweenthem.
5. Placethetwobottlesonatableandwatchthewaterdripfromthetoptothelowerbottleasairbubbles
movefrombottomtotop.
6. Invertsothewaterisinthetopbottleandcircleitacoupleoftimestostartawhirlpoolinthebottle.You
shouldseeavortexforminsideasthetopdrainsintothelowerbottle.Theholeinthevortexletstheair
fromthelowerbottlefloweasilyintotheupperbottle,sotheupperdrainseasily.
7. Whenyou’vefinished,emptyyourbottleandaddadifferentsolutionandrepeattheexperiment.Fillout
thedatatable.
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MagneticTornadoesDataTable
Note:Waterheightismeasuredwhenallthewaterisinthelowercontainer.
WaterCondition
HeightoftheWater
HowLongDidItTaketo
DraintoLowerBottle?
(measureinseconds)
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Reading
Mercurylookspeacefulatfirstglance.However,whenyoumeasurethesurfacewithscientificinstruments,you’ll
seehowtheSunblastsawayanyhopeMercuryhasofathinatmospherewithitsradiationandsolarwind.Notonly
that,Mercuryisravagedbyinvisiblemagnetictornadoesthatstartfromtheplanet’sinteriormagneticfield.If
you’veeverexperiencedatornado,youknowhowterrifyingtheycanbe.Nowimaginetheyarethediameterof
yourentireplanet.
ThesetornadoesaredifferentfromtheEarth’s,whichformwhentwoweathersystemssmackintoeachother,
creatinginstabilityintheatmosphere.ThemagnetictornadoesonMercuryformwhentwomagneticfieldscollide.
Thesemonstrouscyclonesformwithoutwarninganddisappearwithinminutes.
Magneticfields,liketheEarth’s,areinvisibleshieldsthatconstantlyprotectusfromtheSun.OurEarthis
constantlybeingbombardedwithhighenergyparticlesthataredeflectedoffthemagnetosphereofourplanet.
Mercury’smagneticfieldisweakandit’sconstantlybeingblastedbysolarwind,whichalsocarriesamagnetic
field.Whenthesetwofieldscollide,themagneticfieldsspiralandtwisttoformamagnetictornado.(Solarwindisa
streamofhighenergyparticlesfromtheSun’souteratmosphere.)
QuestionstoAnswer
1. Defineanatmosphere.
2. Whatisamagneticfield?
3. Wheredomagneticfieldscomefrominplanets?
4. Whichplanetsdonothaveamagneticfield?
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Lesson#4:SkyinaJar
Overview:Haveyoueverwonderedwhytheskyisblue?Orwhythesunsetisred?Orwhatcoloroursunsetwould
beifwehadabluegiantinsteadofawhitestar?Thislabwillanswerthosequestionsbyshowinghowlightis
scatteredbytheatmosphere.
WhattoLearn:Particlesintheatmospheredeterminethecoloroftheplanetandthecolorsweseeonitssurface.
Thecolorofthestaralsoaffectsthecolorofthesunsetandoftheplanet.
Materials







Glassjar
Flashlight
Fingernailpolish(red,yellow,green,blue)
Cleartape
Water
Darkroom
Fewdropsofmilk
Experiment
1.
2.
3.
4.
5.
6.
7.
8.
9.
10.
Makeyourroomasdarkaspossibleforthisexperimenttowork.
Makesureyourlabelisremovedfromtheglassjaroryouwon’tbeabletoseewhat’sgoingon.
Filltheclearglassjarwithwater.
Addateaspoonortwoofmilk(orcornstarch)andswirl.
Shinetheflashlightdownfromthetopandlookfromtheside–thewatershouldhaveabluishhue.The
smallmilkdropletsscatterthelightthesamewayouratmosphere’sdustparticlesscattersunlight.
Tryshiningthelightupfromthebase–wheredoyouneedtolookinordertoseeafaintred/pinktint?If
not,it’sbecauseyouarelookingforhuesthatmatchourrealatmosphere,andthejarjustisn’tthatbig,nor
isyourflashlightstrongenough!Instead,lookforaveryslightcolorshift.Ifyoudothisexperimentafter
beinginthedarkforabout10minutes(lettingyoureyesadjusttothelackoflight),itiseasiertoseethe
subtlecolorchanges.Justbecarefulthatyoudon’tletthebrilliantflashlightruinyournewlyacquirednight
vision,oryou’llhavetostartthe10minutesalloveragain.
Ifyouarestillhavingtroubleseeingthecolorchanges,shineyourlightthroughthejarandontoanindex
cardontheotherside.Youshouldseeslightcolorchangesonthewhitecard.
Covertheflashlightlenswithcleartape.
Paintonthetape(notthelens)thefingernailpolishyouneedtocompletethetable.
Repeatsteps7‐9andrecordyourdata.
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SkyinaJarDataTable
FlashlightColor
Location
Color(s)
White
Sideofjar
White
BottomofJar
Red
Sideofjar
Red
BottomofJar
Yellow
Sideofjar
Yellow
BottomofJar
Green
Sideofjar
Green
BottomofJar
Blue
Sideofjar
Blue
BottomofJar
Reading
Whyisthesunsetred?Thecolorsyouseeintheskydependonhowlightbouncesaround.Thered/orangecolors
ofsunsetandsunrisehappenbecauseofthelowangletheSunmakeswiththeatmosphere,skippingthelightoff
dustanddirt(nottomentionsolidaerosols,soot,andsmog).Sunsetsareusuallymorespectacularthansunrises,
asmore“stuff”floatsaroundattheendoftheday(therearelessparticlespresentinthemornings).Sometimes
justaftersunset,agreenflashcanbeseenejectingfromthesettingSun.
TheEarthappearsbluetotheastronautsinspacebecausetheshorter,faster
wavelengthsarereflectedofftheupperatmosphere.Thesunsetsappearredbecause
theslower,longerwavelengthsbounceofftheclouds.
Sunsetsonotherplanetsaredifferentbecausetheyarefarther(orcloser)totheSun,
andalsobecausetheyhaveadifferentatmospherethanplanetEarth.Theimageshown
hereisasunsetonMars.UranusandNeptuneappearbluebecausethemethaneinthe
upperatmospherereflectstheSun’slightandthemethaneabsorbstheredlight,
allowingbluetobouncebackout.
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QuestionstoAnswer
1. Whatcolorsdoesthesunsetgothrough?
2. Doesthecolorofthelightsourcematter?
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Lesson#5:PlanetaryMagneticFields
Overview:You’regoingtouseacompasstofigureoutthemagneticlinesofforcefromamagnetbymappingthe
twodifferentpolesandhowthelinesofforceconnectthetwo.Amagneticfieldmustcomefromanorthpoleofa
magnetandgotoasouthpoleofamagnet(oratomsthathaveturnedtothemagneticfield.)
WhattoLearn:Compassesareinfluencedbymagneticlinesofforce.Theselinesarenotnecessarilystraight.
Whentheybend,thecompassneedlemoves.TheEarthhasahugemagneticfield.TheEarthhasaweakmagnetic
force.ThemagneticfieldcomesfromthemovingelectronsinthecurrentsoftheEarth’smoltencore.TheEarthhas
anorthandasouthmagneticpolewhichisdifferentfromthegeographicNorthandSouthPole.
Materials






Barmagnet
Horseshoemagnet
Circular(disk)magnet
Compass
String
Ruler
Experiment
1.
2.
3.
4.
Tieastringaroundyourmagnet.
Bringitclosetothecompass.
Whichendisthenorthendofyourmagnet?Labelitwithapencilrightonthemagnet.
Flipthemagnetaroundbytwistingthestringsothatthecompassflipstotheoppositepole.Labelthe
oppositesiteofthemagnetwiththeappropriateletter(NorS).
5. Bringasecondmagnetclosetothefirstone.Whathappenswhenyoubringtwooppositepolestogether?
Whatifthepolesarethesame?
Nowuntieorcutthestringforthenextpartofyourlab.
6. Layapieceofpaperonyourdesk.
7. Placethemagnetinthemiddleofthepaperandtracetheoutline.
8. Draw12dots(justlikeonaclock)allthewayaroundthemagnet.Thesearethelocationswhereyouwill
placeyourcompass,somakesurethattheyarecloseenoughtothemagnetsothemagnetinfluencesthe
compass.
9. Placeyourcompassononeofthedotsandlookatthedirectionthearrowispointing.Removethecompass
anddrawthatexactarrowdirectionrightoveryourdot.Dothisforall12dots.
10. Drawanotherringofdotsaninchortwooutfromthefirstringandrepeatstep9.
11. Repeatsteps6‐10withacircularmagnetonanewsheetofpaper.
12. Repeatsteps6‐10forthehorseshoemagnetonanothersheetofpaper.
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Reading
Rightunderyourfeet,there’samagnet.Goaheadtakealook.Liftupyourfeetandseewhat’sunderthere.Doyou
seeit?It’shuge!Infact,it’sthelargestmagnetontheEarth.Asamatteroffact,itistheEarth!That’sright;the
Earthisonehuge,gigantic,monolithicmagnet!We’regoingtouseamagnettosubstitutefortheEarthandplotout
themagneticfieldlines.
ThemagneticpolewhichwasattractedtotheEarth’sNorthPolewaslabeledastheBorealor“north‐seekingpole”
inthe1200s,whichwaslatershortenedto“northpole.”Toaddtotheconfusion,geologistscallthispoletheNorth
MagneticPole.
QuestionstoAnswer
1. Howarethelinesofforcedifferentforthetwomagnets?
2. Howfarout(ininchesmeasuredfromthemagnet)doesthemagnetaffectthecompass?
3. Whatmakesthecompassmovearound?
4. Doyouthinkthecompass’snorth‐southindicatorisflipped,ortheEarth’sNorthPolewheretheSouth
Poleis?Howdoyouknow?
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Lesson#6:Seasons
Overview:OnecommonmisconceptionisthattheseasonsarecausedbyhowclosetheEarthistotheSun.Today
yougettodoanexperimentthatshowshowseasonsareaffectedbyaxistilt,notbydistancefromtheSun.Andyou
alsofindoutwhichplanetdoesn’thavesunlightfor42years.
WhattoLearnTheseasonsarecausedbytheEarth’saxistiltof23.4ofromtheeclipticplane.
Materials







Brightlightsource(notfluorescent)
Balloon
Protractor
Maskingtape
2liquidcrystalthermometers
Ruler,yardstickormeterstick
Marker
Experiment
1. Foralightsource,trylampswith100Wbulbs(withoutlampshades).Makesurethere’sroomtowalkall
thewayaroundit.You’llwanttocirclethelampatadistanceofabout2feetaway.
2. Markonthefloorwithtapeandlabelthefourpositions:winter,spring,summer,andfall.Theyshouldbeat
the12,3,6,and9o’clockpositions.Winterisdirectlyacrossfromsummer.TheEarthrotates
counterclockwisearoundtheSunwhenviewedfromabove.
3. Blowupyourballoonsoit’sroughlyround‐shaped(don’tblowitupalltheway).Markandlabelthenorth
andsouthpoleswithyourmarker.Drawanequatoraroundthemiddlecircumference.
4. TheEarthdoesn’tpointitsnorthpolestraightupasitgoesaroundtheSun.It’stiltedover23.4o.here’show
youfindthispointonyourballoon:
a. PuttheSouthPolemarkonthetable,withnorthpointingstraightup.Findthemidwaypoint
betweentheequatorandtheNorthPoleandmakeatinymark.Thisisthe45olatitudepoint.You’ll
needthistofindthe23omark.
b. Findthemidwaypointbetweenthe45omarkandtheNorthPoleandmakeanothermark,larger
thistimeandlabelitwith23o.Whenthismarkispointingup,theEarthistiltedovertheright
amount.
c. You’llneedtodothisthreemoretimessoyoucandrawalineconnectingthedots.Youwantto
drawthelatitudelineat23osoyoucanrotatetheballoonasyoumovearoundtothedifferent
seasons.Thelinewillalwaysbepointedup.
5. Placethethermometersontheballoonattheselocations:
a. FindthehalfwaypointbetweentheSouthPoleandtheequator.Putonethermometeronthismark.
b. Puttheotherthermometeronthenorthernhemisphere’s45omarkfromabove.
6. Makesureyourlampisfacingtheballoonasyoustandonsummer.Lettheballoonbeheatedbythelamp
foracoupleofminutesandthenrecordthetemperatureinthedatatable.
7. Rotatethelamptopointtofall.Moveyourballoontofall,rotatingtheballoonsothatthethermometersare
facingthelamp.Waitafewmoreminutesandtakeanotherreading.
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8. Rotatethelamptopointtowinter.Moveyourballoontowinter,rotatingtheballoonsothatthe
thermometersarefacingthelamp.Waitafewmoreminutesandtakeanotherreading.
9. Rotatethelamptopointtospring.Moveyourballoontospring,rotatingtheballoonsothatthe
thermometersarefacingthelamp.Waitafewmoreminutesandtakeanotherreading.You’vecompleteda
datasetforplanetswithanaxistiltofabout23o,whichincludestheEarth,Mars,SaturnandNeptune.
10. Repeatsteps1‐9forMercury.NotethatMercurydoesnothaveanaxistilt,sotheNorthPolereallypoints
straightup.Jupiter(3.1oaxistilt)andVenus(2.7o)areverysimilar.TheMoon’saxistiltis6.7o,soyoucan
approximatethesefourobjectswitha0oaxistilt.
11. Repeatsteps1‐9forUranus.Sincetheaxistiltis97.8o,youcanapproximatethisbypointingthenorthpole
straightattheSunduringsummer(90oaxistilt).TheorbitforUranusis84years,whichmeans21years
passesbetweeneachseason.Thenorthpolewillexperiencecontinuedsunlightfor42yearsfromspring
throughfall,thendarknessfor42years.
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SeasonsDataTable
Don’tforgettocircleorlabelyourunits!
NotethatUranus’saxistiltisapproximatedby90oandVenus,Jupiter,andMercury’saxistiltareapproximatedby0o
AxisTilt
Season
23o
Summer
23o
Fall
23o
Winter
23o
Spring
0o
Summer
0o
Fall
0o
Winter
0o
Spring
90o
Summer
90o
Fall
90o
Winter
90o
Spring
NorthernHemisphere
Temperature(oC/oF)
SouthernHemisphere
Temperature(oC/oF)
Reading
TheNorthandSouthPolesonlyexperiencetwoseasons:winterandsummer.DuringaSouthPolewinter,theSun
willnotriseforseveralmonths,andalsotheSundoesnotsetforseveralmonthsinthesummer.Wegointomore
detailabouthowthisworksinalaterlessonentitled:StarTrailsandPlanetPatterns.
Attheequator,there’sawetseasonandadryseasonduetothetropicalrainbelt.Sincetheequatorisalways
orientedatthesamepositiontotheSun,itreceivesthesameamountofsunlightandalwaysfeelslikesummer.
ThechangingoftheseasonsiscausedbytheangleoftheSun.Forexample,inJuneduringsummersolstice,theSun
ishighintheskyforlongerperiodsoftime,whichmakeswarmertemperaturesfortheNorthernHemisphere.
DuringtheDecemberwintersolstice,theSunspendslesstimeintheskyandispositionedmuchlower.Thismakes
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thewinterscolder.(Don’tforgetthatseasonsarealsoaffectedbyoceansandwinds,thoughthisisoutofthescope
ofthisparticularactivity.)
QuestionstoAnswer
1. WhatisthemainreasonwehaveseasonsonEarth?
2. WhyaretherenosunsetsonUranusfordecades?
3. ArethereseasonsonVenus?
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Lesson#7:IndoorRainClouds
Overview:Todayyougettovaporizeliquidoceansofmoleculesandmakeitrainwhentherisingclouddeckshit
thecoldnessofspace.Soundlikefun?
WhattoLearn:Themovementofatmospheresondifferentplanetsisaffectedbythetemperatureoftheplanet
andthemoleculesintheatmosphere.
Materials




Glassoficewater
Glassofhotwater
Towel
Ruler
Experiment
1. Pleasebecarefulwiththislab!Thehotwatercanburnyou!
2. Taketwoclearglassesthatfitsnuglytogetherwhenstacked.(Cylindricalglasseswithstraightsideswork
well.)
3. Filloneglasshalf‐fullwithicewaterandtheotherhalf‐fullwithveryhotwater(definitelyanadultjob–
andtakecarenottoshattertheglasswiththehotwater!).Besuretoleaveenoughairspacefortheclouds
toforminthehotglass.
4. Placethecoldglassdirectlyontopofthehotglassandwaitseveralminutes.Ifthesealholdsbetweenthe
glasses,araincloudwillformjustbelowthebottomofthecoldglass,anditactuallyrainsinsidetheglass!
(Youcanuseadamptowelaroundtherimtohelpmakeabetterseal,ifneeded.)
5. Completethedatatable.Measurethewaterheightcarefullywithyourruler.Ifyouhave2”ofwaterinthe
hotwaterglass,thenwrite2”.Pleasebecarefulwhenmeasuringhotwater!
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IndoorRainCloudsDataTable
HotWaterHeight
IceWaterHeight
Howwelldiditrain?
Reading
Thisexperimentdemonstratesstatechangesofmatter.Whenhotvaporrises(likefromthehotcoreofagaseous
planet)andhitsacoldfront(likethecoldnessofouterspaceintheupperatmosphere),thevaporcondensesinto
liquiddropsandrains,orcanevenfreezesolidintoicechunks.NeptuneandUranusbothhavemethaneiceintheir
upperatmospheres.BothJupiterandSaturnhaveupperclouddecksofwatervaporandcloudsofammonia.The
watervaporcloudsarerightatthefreezingtemperatureofwater.
QuestionstoAnswer
1. Whichcombinationmadeitrainthebest?Whydidthiswork?
2. Drawyourexperimentaldiagram,labelingthedifferentcomponents:
3. Addinlabelsforthedifferentphasesofmatter.Canyouidentifyallthreestatesofmatterinyour
experiment?
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Lesson#8:Volcanoes
Overview:Marshassomeofthebiggestcanyonsandthehighestvolcanoesinthesolarsystem.VallesMarineris
measures2,800feetwideand4milesdeep.That’s40timesthesizeoftheGrandCanyon.AndOlympusMonsis15
½mileshigh,nearlythreetimesthesizeofMountEverest.Sohowdoesthishappen?That’swhatthislabwillhelp
youfigureout.
WhattoLearn:ThereactionyouaremakingtodayissimilartotheactionMarssawwithitsshieldvolcanoes.The
gasproducediscarbondioxide.Thebubblesthatgettrappedinsidemakepockets,andthedishsoaphelpsthem
stayasbubbleslongenoughforyoutocatchtheminaction.
Experiment
1. Dothislaboutdoors,becauseofthemessitmakesthatseemstofloweverywhere.Findanice‐weatherday
anddothisoutside.Thereareacoupleofchoiceswiththisexperiment.Yougettopickwhatthevolcanois
madeoutof(therearetwodifferentdoughrecipes),andalsowhichkindofchemicalreactionyou’dliketo
demonstrate(therearetwodifferentoneshere,too).Ifyou’reinahurry,useaslabofclayforthedough
andusethefirstsetofchemicals.
2. Ifyou’dliketofilloutthedatatablefortheirexperiment(thisisquestionable,asit’sgoingtobeamessy
lab),thenyou’llneedmeasuringcups.
3. Thefirstthingyouwilldoismixupvolcanodough.Therearetwodifferentrecipesprovidedwiththislab:
StandardVolcanoDoughisjustlikeplaydough,andEarthyVolcanoDoughlooksmoreliketherealthing.
Yourteacherwillletyouknowwhichoneyouaretomake.Thenproceedtothechemicalreactionthatyour
teacherhasselectedforyou.
MakingtheVolcano
StandardVolcanoDough
a. Mixtogether6cupsflour,2cupssalt,½cupvegetableoil,and2cupswarmwater.
b. Theresultingmixtureshouldbefirmbutsmooth.
c. Standawaterorsodabottleinaroastingpanandmoldthedougharounditintoavolcanoshape.
EarthyVolcanoDough
a. Mix2½cupsflour,2½cupsdirt,1cupsand,and1½cupssalt.
b. Addwaterbythecupuntilthemixturestickstogether.
c. Buildthevolcanoaroundanemptywaterbottleonadisposableturkey‐styleroastingpan.
d. Itwilldryintwodaysifyouhavethetime,butwhywait?Youcaneruptwhenwetifthemixtureis
stiffenough!(Andifit'snot,addmoreflouruntilitis.)
ChemicalReactions:
SodaVolcanoes
a. Fillthebottlemostofthewaywithwarmwaterandabitofredfoodcoloring.
b. Addasplashofliquidsoapand¼cupbakingsoda.Stirgently.
c. Whenready,addvinegarinasteadystreamandwatchthatlavaflow.
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AirPressureSulfurVolcanoes
a. Wrapthevolcanodougharoundan18”pieceofclear,flexibletubing.
b. Shapethedoughintoavolcanoandplaceinadisposableroastingpan.
c. Pushandpullthetubefromthebottomuntiltheotherendofthetubeisjustbelowthevolcanotip.
Ifyouclogtheendsofthetubingwithclay,justtrimawaytheclogwithscissors.
d. Usingyourfingers,shapetheinsidetopofthevolcanotoresembleasmallpapercup.
e. Yoursolutionneedsachambertomixandgrowinbeforeoverflowingdownthemountain.The
tubegoesatthebottomoftheclay‐cupspace.
f. BesurethevolcanoisSEALEDtothecookiesheetatthebottom.Youwon’twantthesolution
runningoutofthebottomofthevolcanoinsteadofpoppingoutthetop!
MakeyourchemicalreactantsforAirPressureSulfurVolcanoes:
g. Solution1:Fillonebuckethalfwaywithwarmwaterandadd1to2cupsbakingsoda.Add1cupof
liquiddishsoapandstirverygentlysoyoudon’tmaketoomanybubbles.
h. Solution2:Fillasecondbuckethalfwaywithwaterandadd1cupofaluminumsulfate(alsocalled
alum.)Addredfoodcoloringandstir.
i. Puttingitalltogether:CountONE(andpourinSolution1)…TWO(inhaleaironly!)……andTHREE
(pourinSolution2asyouputyourlipstothetubefromthebottomofthevolcanoandpuffashard
asyoucan!)Lavashouldnotonlyflowbutburpandspitallovertheplace!
SodaVolcanoesDataTable
HowMuchBakingSoda?
HowMuchVinegar?
HowLongDidItReact?
(measureinseconds)
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AirPressureSulfurVolcanoesDataTable
Note:Don’tblowthroughthetubewhentakingyourdata.
HowMuchSolution1?
HowMuchSolution2?
HowLongDidItReact?
(measureinseconds)
Reading
Haveyouevernoticedhowlotsofvolcanicrockshavebubblesinside?Thegasthatbubbledupthroughtherocks
astheycooledgivesthemaporousappearance.
Whatdoyouthinkwouldhappenifthelavadoesn’tmakeitallthewayoutofthevolcano?Itcoolsandcoatsthe
inside,andthengetsreheatedwiththenextexplosion.Thiscanhappenoverandoveragain,makingthelava
undergosomeprettyradialchanges,molecularlyspeaking.
ThereactionthekidsaremakingtodayissimilartotheactionMarssawwithitsshieldvolcanoes.Thegas
producediscarbondioxide.Thebubblesthatgettrappedinsidemakepockets,andthedishsoaphelpsthemstay
asbubbleslongenoughforyoutocatchtheminaction.
Marsisalitterboxforvolcanoes.Someofthesevolcanoesaredead,butothersaresimplydormant.Nearlyall
volcanoesonMarsareshieldvolcanoes,createdbycurrentsandhotspotsbeneaththesurface(justliketheonesin
Hawaii).TherearesomanyvolcanoesonMarsthatscientistshavedrawnlinestocorralthemintovolcanic
provinces.Withouttectonicplates,thecurrentsunderthevolcanoescanfloweasilyandfreely.
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QuestionstoAnswer
1. HowisthisactivitysimilartothevolcanoesonMars?
2. Whatgasisproducedwiththisreaction?
3. Whichplanetshavevolcanoes?
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Lesson#9:StarGazing
Overview:We’regoingtolearnhowtogostargazingusingplanetariumsoftware,andhowtocustomizetoyour
locationintheworldsoyouknowwhatyou’relookingatwhenyoulookupintotheskytonight!
WhattoLearn:Telescopesandbinocularsareprettyuselessunlessyouknowwheretopointthem.Iamgoingto
showyousomestandardconstellationsandhowtofindtheminthenightsky,soyou’llneverbelostagaininthe
oceanofstarsoverhead.
Materials:


Planetariumsoftware(Stellariumisfreeatthislink:http://www.stellarium.org/)
ORuseastarwheel(http://www.skyandtelescope.com/letsgo/familyfun/Make_a_Star_Wheel.html)
LabTime:
You’reabouttolocateseveraldifferentcelestialobjectsbyfirstfindingtheminyourplanetariumsoftware(orafter
assemblingyourstarwheel.
1. Ifyouhaven’talready,customizeyourplanetariumsoftwaretoyourlocationbyenteringinyourlocation
andelevation.
2. Nowadjustthetimesothatit’ssettothetimeyou’dliketostargazetonight.Whattimewillyoustargaze
tonight?Writeithere…Time:_________________________
3. ForfolksintheNorthernHemisphere,findtheBigDipper(orthePlough).ForSouthernHemispherefolks,
findtheSouthernCross(ortheCrux,butitreallylookslikeabigkite).Theseareoneofthemost
recognizablepatterns,andeasyforbeginnerstofind.
4. ForNortherners,usetheBigDippertolocatePolaris,theNorthStar.Thetwostarsattheedgeofthedipper
pointstraighttotheNorthStar.
5. ForSoutherners,usetheSouthernCrosstofindthesouthpoleofthesky(sometimescalledthe“southpole
pit”sincethere’snostarthereattheexactpolepointofthesouthernsky).Thelongerbarinthecross
pointsalmostexactlytowardtheSouthPole.
6. UsingtheSearchoption,findtheplanetsthatwillbevisibletonightbytypingintheirnameintothesearch
window.Whichoneswillbevisibleforyoutonight?
PlanetName: Whereisitinthesky?(Whereshouldyoulook?)
____________________________________________________________________________________________________________
____________________________________________________________________________________________________________
____________________________________________________________________________________________________________
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7. InStellarium,clickthe“Search”icon,thenthe“Lists”tab,andselect“Constellations”.Selecttwodifferent
constellationsyou’dliketofindtonightthatarevisibletoyou,andrecordinformationaboutthemhere:
ConstellationName: PointerStars/LocationIndicators(Howwillyoufindit?):
____________________________________________________________________________________________________________
____________________________________________________________________________________________________________
8. Whenyou’reready,flipovertotheobservingdatatable,grabaflashlight,pencil,andthengooutsidetolog
yourobservations,justlikearealscientist!
ObservingTip:Trytoobservewhenthemoonislessthanfirstquarterphaseormorethanthreequarters
(meaningthatthemoonislessthan50%illuminated).Youdon’tneedanyfancyviewingequipment,onlyyourlog
sheet,andifyoucandoit,bringyourplanetariumsoftwareprogramwithyououtsidetohelpyoulocatethe
objects.Startsmall,andfindacoupleofthingsonthefirstnight.Ifyoudon’tfigureitoutthefirsttime,tryagainthe
nextnight.IlearnedthenorthernskybylearningonenewconstellationeverytimeIwentstargazing,andpretty
soonIhadalotofthemthatIcouldidentifyeasily.
Note:Thisisn’tsomethingthat’sgoingtoworkbyosmosis.Youwillhavetogooutside,figureoutwheretolook,
andfindtheobject.Figureoutwhatyou’relookingfor,andaboutwhereyoucanexpecttofindit,andpracticeand
testyourselfoverandoveruntilyoucansuccessfullyfinditeverytime.Ifyou’regettingfrustrated,it’stimetostop
andhaveasipofhotcocoabeforeyoutryagain.Thisissupposedtobeafuntreasurehunt,somakeitenjoyable!
HowtoFindtheNorthStar(Polaris)
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AstronomyStarGazingObservationalLog
ObservingDate:_________________________Lat/Long:___________________________SiteElev:________________________
ObservingLocation/Site:____________________________________________________________MoonPhase:_________________
Weatherconditions:_________________________________________DimmestStarVisibleOverhead:___________________
Notes:_________________________________________________________________________________________________________________
Time:
(UTCorLocalTime)
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SketchofObject
Observed:
ObjectNameor
Classification:
Notes:
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Lesson#10:SongoftheSun
Overview:HelioseismologyisthestudyofwaveoscillationsintheSun.Bystudyingthewaves,scientistscan
tellwhat’sgoingoninsidetheSun.It’sbelikestudyingearthquakestolearnwhat’sgoingoninsidethe
earth.TheSunisfilledwithsound,andstudyingthesesoundwavesiscurrentlytheonlywayscientists
cantellwhat’sgoingoninside,sincethelightweseefromtheSunisjustfromtheuppersurface.
WhattoLearn:Moleculesarevibratingbackandforthatfairlyhighratesofspeed,creatingwaves.Energymoves
fromplacetoplacebywaves.Soundenergymovesbylongitudinalwaves(thewavesthatarelikeaslinky).The
moleculesvibratebackandforth,crashingintothemoleculesnexttothem,causingthemtovibrate,andsoonand
soforth.Allsoundscomefromvibrations.
Materials

Musicalinstruments:triangles,glassbottlesthatcanbeblownacross,metalforks,tuningforks,recorders,
jawharps,harmonicas,etc.Whateveryouhavewillworkfine.
Experiment
1. Yourteacherwillpulloutabinofmusicalinstrumentsofvarioustypes.
2. Assignonestudenttobethenoisemaker.Therestwilllistenwiththeireyesclosedandrecordtheir
observations.
3. Everyoneshutstheireyesexceptforthenoisemaker.
4. Thenoisemakerselectsaninstrumentandplaysitonce.Everyoneelselistens.
5. Thenoisemakerselectsanotherinstrumentandplaysitonce.Everyonelistens.
6. Thenoisemakerselectsathirdinstrumentandplaysitonce.Everyonelistens.
7. Thenoisemakerselectsoneofthethreeinstrumentsandplaysitasitmoves.Forexample,ifyou’replaying
thetriangle,youcanhititandspinit.Orhititasyouarewalkingpasttheclosed‐eyelisteners.Sound
changeswhentheobjectismoving,somakethesoundtheyhearappeartobedifferentsomehow.
8. Thenoisemakerputstheinstrumentsbackandeveryoneopenstheireyesandrecordstheirdatainthe
table.
9. Switchrolesandfindanewnoisemakerforthenexttrial.Repeatsteps2‐8.
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SongoftheSunDataTable
Makesureyoureyesareclosedwhentheinstrumentsareplayed!Fortheinstrumentcolumnstwothroughfour,write
downa1,2,or3fortheinstrumentyouthinkanswersthequestionbest.
NOTE:Youdon’thavetoknowwhattheinstrumentwas,justwhereitwasplayedinsequence.
Thenoisemakerwillletyouknowaftereveryonehasplacedtheirguessesontheirdatatableforthetrial.
Whichmadethe
highestnote?
Trial#
Whichmadethe
lowestnote?
Whichonemoved?
1
2
3
4
5
6
7
8
Reading
TheSunislikethebiggestmusicalinstrumentyou’veeverseen.Apianohas88keys,whichmeansyoucanplay88
differentmusicalnotes.TheSunhas10million.
Toplayaguitar,youpluckoneofthesixstrings.Toplaythepiano,youhitakeyandsoundcomesout.Toplaythe
flute,youblowacrossahole.Drumsrequiresmackingthingstogether.SohowdoyouplaytheSun?
Moleculesarevibratingbackandforthatfairlyhighratesofspeed,creatingwaves.Energymovesfromplaceto
placebywaves.Soundenergymovesbylongitudinalwaves(thewavesthatarelikeaslinky).Themolecules
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vibratebackandforth,crashingintothemoleculesnexttothem,causingthemtovibrate,andsoonandsoforth.
Allsoundscomefromvibrations.
Wavesarethewayenergymovesfromplacetoplace.Soundmovesfromamouthtoanearbywaves.Lightmoves
fromalightbulbtoabookpagetoyoureyesbywaves.Wavesareeverywhere.Asyousittherereadingthis,you
aresurroundedbyradiowaves,televisionwaves,cellphonewaves,lightwaves,soundwavesandmore.(Ifyou
happentobereadingthisinaboatorabathtub,you’resurroundedbywaterwavesaswell.)Therearewaves
everywhere!
Doyourememberwhereallwavescomefrom?Vibratingparticles.Wavescomefromvibratingparticlesandare
madeupofvibratingparticles.
Here’sruleonewhenitcomestowaves…thewavesmove,theparticlesdon’t.Thewavemovesfromplaceto
place.Thewavecarriestheenergyfromplacetoplace.Theparticleshowever,stayput.Hereareacoupleof
examplestokeepinmind.
Ifyou’veeverseenacrowdofpeopledothe“wave”inthestandsofasportingeventyoumayhavenoticedthatthe
peopleonly“vibrated”upanddown.Theydidnotmovealongthewave.Thewave,however,movedthroughthe
stands.
Anotherexamplewouldbeaduckfloatingonawavylake.Theduckismovingupanddown(vibrating)justlikethe
waterparticlesbutheisnotmovingwiththewaves.Thewavesmove,buttheparticlesdon’t.WhenItalktoyou,
thevibratingairmoleculesthatmadethesoundinmymouthdonottravelacrosstheroomintoyourears.(Which
isespeciallyhandyifI’vejusteatenanonionsandwich!)Theenergyfrommymouthismoved,bywaves,acrossthe
room.
Convectionstartsthewavesmoving.You’veseenconvectionwhenahotpotofwaterbubblesup.Youcaneven
hearitwhenitstartstoboilifyoulistencarefully.JustbelowthesurfaceoftheSun,theenergythatstarteddeepin
thecorehasbubbleduptothesurfacetomakegiganticbubblesemergethatarebiggerthanthestateofAlaska.It’s
alsoanoisyprocess,andthesoundwavesstaytrappedbeneaththesurface,makingwavesappearonthesurfaceof
theSun.ThismakestheSun’ssurfacelooklikeit’smovingupanddown.
ScientistsusespecialcamerastowatchthesurfaceoftheSunwiggleandmove,andtheylookforpatternssothey
candeterminewhat’sgoingondowninsidetheSun.SincethesoundisinsidetheSununderthepartwecansee,
weusesoundtodiscoverwhat’sinsidetheSun.
HaveyoueverheardtheSun?ThevideoisanactualrecordingofthesongoftheSun.
Ifyou’veeverbeeninsideanunfurnishedroom,you’veheardechoesindoors.Soundbouncesallaroundtheroom,
justlikeitdoesinsidethesurfaceoftheSun.
Cansoundwavestravelthroughspace?No.Soundrequiresamediumtotravelthrough,sinceittravelsbyvibrating
molecules,andtherearen’tenoughmoleculesinspacetodothiswith(thereareacouplerandomonesfloating
aroundhereandthere,butwaytoofaraparttobeusefulforsoundwaves).
Ifyouhaveaslinky,takeitoutandstretchitouttoitsfulllengthonthetableortheground,askingsomeoneto
helpyouholdoneend.Nowmovetheslinkyquicklytotheleftandbackagain,andwatchthewavetraveldownthe
lengthandreturn.Nowmoveyourendquicklyupandthenbackdownthetable,makingalongitudinalwave.
Whenthiswavefinishes,takeyourendandshoveitquicklytowardyourhelper,thenpullbackagaintomakea
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compressionwave.Pointouttothestudenthowwhenthewavereturns,it’sanecho.That’swhathappensinside
theSunwhenthesoundwaveshitthesurfaceoftheSun.Theydon’tgothroughthesurface,butgettrapped
beneathitastheyechoofftheinsidesurfaceoftheSun.
QuestionstoAnswer
1. Whatdidyounoticethatisdifferentaboutthesoundsyouheard?
2. Howcanyoutellthattwosoundsaredifferentthatcamefromthesameinstrument?(Movement
causessoundwavestosounddifferent.)
3. Whatdidyounoticeaboutyourguesses?Whatkindofinstrumentswereyoumorecorrectabout?
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Lesson#11:SimpleMicroscope&Telescope
Overview:Didyouknowyoucancreateacompoundmicroscopeandarefractortelescopeusingthesame
materials?It'sallinhowyouusethemtobendthelight.Thesetwoexperimentscoverthefundamentalbasicsof
howtwodouble‐convexlensescanbeusedtomakeobjectsappearlargerwhenrightupcloseorfartheraway.
WhattoLearn:Thingslikelensesandmirrorscanbendandbouncelighttomakeinterestingthings,like
compoundmicroscopesandreflectortelescopes.Telescopesmagnifytheappearanceofsomedistantobjectsinthe
sky,includingthemoonandtheplanets.Thenumberofstarsthatcanbeseenthroughtelescopesisdramatically
greaterthancanbeseenbytheunaidedeye.
Materials





Awindow
Dollarbill
Penny
Twohand‐heldmagnifyinglenses
Ruler
Experiment
1. Placeapennyonthetable.
2. Holdonemagnifierabovethepennyandlookthroughit.
3. Bringthesecondmagnifyinglensabovethefirstsonowyou’relookingthroughboth.Movethesecondlens
closerand/orfurtherfromthepennyuntilthepennycomesintosharpfocus.You’vejustmadea
compoundmicroscope.
4. Who’sinsidethebuildingonanolderpenny?
5. Tryfindingthespider/owlonthedollarbill.(Hint:It’sinacornernexttothe“1”.)
6. Keepingthedistancebetweenthemagnifiersaboutthesame,slowlyliftupthemagnifiersuntilyou’renow
lookingthroughbothtoawindow.
7. Adjustthedistanceuntilyourimagecomesintosharp(andupside‐down)focus.You’vejustmadea
refractortelescope,justlikeGalileoused400yearsago.
8. Findeightdifferentitemstolookatthroughyourmagnifiers.Makefourofthemup‐closesoyouusethe
magnifiersasamicroscope,andfourofthemfar‐awayobjectssoyouusethemagnifierslikeatelescope.
Completethedatatable.
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SimpleMicroscope&TelescopeDataTable
Forthelasttwocolumns,measurewithyourrulercarefully.Don’tforgettolabelyourunits!
MagnificationUsed:______________________________________________(multiplythemagnificationofbothlensestogether)
Object
LookedAt
HowFarApartare
theLenses?
DidyouusetheMagnifiers
asaMicroscopeor
Telescope?
HowFarisyour
Eyefromthe
Eyepiece?
Reading
WhatIlikebestaboutthisactivityishoweasilywecanbreakdownthebasicideasofsomethingthatseemsmuch
morecomplexandintimidating,likeatelescopeormicroscope,inawaythatkidsreallyunderstand.
Whenabeamoflighthitsadifferentsubstance(likeawindowpaneoralens),thespeedatwhichthelighttravels
changes.(Soundwavesdothis,too!)Insomecases,thischangeturnsintoachangeinthedirectionofthebeam.
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Forexample,ifyoustickapencilisaglassofwaterandlookthroughthesideoftheglass,
you'llnoticethatthepencilappearsshifted.Thespeedoflightisslowerinthewater
(140,000milespersecond)thanintheair(186,000milespersecond).Thisiscalled
opticaldensity,andtheresultisbentlightbeamsandbrokenpencils.
You'llnoticethatthepencildoesn'talwaysappearbroken.Dependingonwhereyour
eyeballsare,youcanseeanintactorbrokenpencil.Whenlightentersanewsubstance
(likegoingfromairtowater)perpendiculartothesurface(lookingstraighton),
refractionsdonotoccur.
However,ifyoulookattheglassatanangle,thendependingonyoursightangle,you'llseeadifferentamountof
shiftinthepencil.Wheredoyouneedtolooktoseethegreatestshiftinthetwohalvesofthepencil?
Whydoesthepencilappearbent?Isitalwaysbent?Doesthetemperatureofthewateraffecthowbentthepencil
looks?Whatifyouputtwopencilsinthere?
Dependingonifthelightisgoingfromalightertoanopticallydensermaterial(orviceversa),itwillbenddifferent
amounts.Glassisopticallydenserthanwater,whichisdenserthanair.
Notonlycanyouchangetheshapeofobjectsbybendinglight(brokenpencilorwhole?),butyoucanalsochange
thesize.Magnifyinglenses,telescopes,andmicroscopesusethisideatomakeobjectsappeardifferentsizes.
QuestionstoAnswer
1. Canlightchangespeeds?
2. CanyouseeALLlightwithyoureyes?
3. Givethreeexamplesofalightsource.
4. What'sthedifferencebetweenamicroscopeandatelescope?
5. Whyisthetelescopeimageupside‐down?
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Lesson#12:StarCharting
Overview:IfyouwanttogetfromNewYorktoLosAngelesbycar,you’dpulloutamap.Ifyouwanttofindthe
nearestgasstation,you’dpulloutasmallermap.Whatifyouwantedtofindournearestneighboroutsideoursolar
system?Astarchartisamapofthenightsky,dividedintosmallerparts(grids)soyoudon’tgettoooverwhelmed.
Astronomersusethesestarchartstolocatestars,planets,moons,comets,asteroids,clusters,groups,binarystars,
blackholes,pulsars,galaxies,planetarynebulae,supernovae,quasars,andmorewildthingsintheintergalactic
zoo.
WhattoLearn:Howtofindtwoconstellationsintheskytonight,andhowtogetthoseconstellationsdownon
paperwithsomedegreeofaccuracy.
Materials





Dark,cloud‐freenight
Twofriends
String
Rocks
Pencil
Experiment
1. Tapeyourstringtothepencil.
2. Looselywrapthestringaroundyourfingerseveraltimessothatthetipofthepencilisaboutaninchabove
theground.
3. Findaconstellation.Pointtoastarintheconstellation.
4. Haveasecondpersonplacearockunderthepenciltip.
5. Whenthey’veplacedtherockinposition,pointtoanotherstar.
6. Haveasecondpersonplacearockunderthepenciltipagain.
7. Repeatthisprocessuntilallthestarshaverocksundertheirpositions.
8. Youshouldseeasmallversionoftheconstellationonyourpaper.
Reading
Peoplehavebeenchartingstarssincelongbeforepaperwasinvented.Infact,we’vefoundstarchartsonrocks,
insidebuildings,andevenonivorytusks.Celestialcartographyisthescienceofmappingthestars,galaxies,and
astronomicalobjectsonacelestialsphere.
Celestialnavigation(astronavigation)madeitpossibleforsailorstocrossoceansbysightingtheSun,Moon,
planets,oroneofthe57pre‐selectednavigationalstarsalongwiththevisiblehorizon.
Watchthevideothatshowshowthestarsappeartomovedifferently,dependingonwhichpartoftheEarthyou’re
viewingfrom.What’sthedifferencebetweenlivingontheequatororinAntarctica(explainedinvideo)?
ThefirstthingtostarchartistheBigDipper,orothereasy‐to‐findconstellation(alternates:Cassiopeiafor
northernhemisphereortheSouthernCrossforthesouthernhemisphere).TheBigDipperisalwaysvisibleinthe
northernhemisphereallyearlong,sothismakesforagoodtarget.
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Useglow–in‐the‐darkstarsinsteadofrocks,andchargethemwithaquickflashfromacamera(oraflashlight).
Keepyourhandasstillasyoucanwhilethesecondpersonlinestherockintoposition.Youcanalsounrollalarge
sheetof(butcherorcraft)paperandusemarkerstocreateamorepermanentstarchart.
QuestionstoAnswer:
1. Ifyouhaveconstellationsonyourclassceiling,chartthemonaseparatepagemarkingthepositionsofthe
rockswithX’s.
2. Tonight,findtwoconstellationsthatyouwillchart.Bringthemwithyoutomorrowusingthetechnique
outlinedaboveinExperiment.
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Astronomy1Evaluation
StudentWorksheet
Overview:Today,you’regoingtotaketwodifferenttests:thequizandthelabpractical.You’regoingtotakethe
writtenquizfirst,andthelabpracticalattheendofthislab.Thelabpracticalisn’tapapertest–it’swhereyouget
toshowyourteacherthatyouknowhowtodosomething.
LabTest&Homework
1. Yourteacherwillaskyoutosharehowmuchyouunderstandaboutastronomy.Sincescienceissomuch
morethanjustreadingabookorcirclingtherightanswer,thisisanimportantpartofthetesttofindout
whatyoureallyunderstand.
2. Whileyouarewaitingtoshowhowmuchofthisstuffyoualreadyknow,yougettochoosewhich
homeworkassignmentyouwanttocomplete.Theassignmentisduetomorrow,andhalfthecreditisfor
creativityandtheotherhalfisforcontent,soreallyletyourimaginationflyasyouworkthroughit.Choose
one:
a. Writeashortstoryorskitaboutgravityfromtheperspectiveoftheplanetorobject(likeasunor
moon).You’llreadthisaloudtoyourclass.
b. Makeaposterthatteachesoneofthemainconceptsofastronomyyouenjoyedmost.Whenyou’re
finished,you’lluseittoteachtoaclassofyoungerstudentsanddemonstratetheprinciplesthat
you’velearned.
c. Writeandperformapoemorsongaboutastronomy,telescopes,gravity,moonsoratmospheres.This
willbeperformedforyourclass.
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Astronomy1Quiz
StudentQuizSheet
Name__________________________________________________________
1. Whyisn’tPlutoaplanetanymore?
2. HowmanyEarthscanfitinsidetheSun?
3. Whatarecometsmadeoutof?
4. WhatistheEarth’satmospheremadeupof?
5. HowmanyEarthsfitinsideJupiter?
6. HowfaristheEarthfromthesun?
7. Whatisanatmosphere?
8. Whatisamagneticfield?
9. Aresunsetsthesamecoloronallplanets?
10. Whatmakesacompassneedlemovearound?
11. WhydowehaveseasonsonEarth?Doallplanetshaveseasons?
12. Namethreeplanetsthathavevolcanoes(activeorextinct)?
13. Canyoudetectallkindsoflightwithyoureyes?
14. Whyisthetelescopeimageupside‐down?
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Astronomy1LabPractical
StudentWorksheet
Thisisyourchancetoshowhowmuchyouhavepickeduponimportantkeyconcepts,andifthereareany
holes.Youalsowillbeworkingonahomeworkassignmentasyoudothistestindividuallywithateacher.
Materials:



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Twohandheldmagnifiers
Sheetofpaper
BallwithatoothpickstickingoutofthetopandbottomtorepresenttheEarth’snorthandsouthpoles(or
useaglobeifyouhaveone)
Strongflashlight
LabPractical:

Designandbuildanexperimentthatshowshowarefractortelescopeworks.

DemonstratewhytheEarthhasseasons.
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AnswerstoExercisesandActivities
Lesson#1:PlanetariumandStarShow
1.WhathappenedtoPluto?(Plutowasreclassifiedasadwarfplanet.BeyondNeptune,theKuiperBeltholdsthe
chunksoficeanddust,likecometsandasteroidsaswellaslargerobjectslikedwarfplanetsErisandPluto.)
2.HowdoestheSunmakeenergy?(Thenuclearreactionsdeepinthecoretransform600milliontonspersecond
ofhydrogenintoheliumbysmackingprotonstogether,callednuclearfusion.)
3.Whichplanetisyourfavoriteandwhy?(Refertostudentresponses.)
4.HowmanymoonsaroundJupiterandSaturncanyouseewithbinoculars?(Foureach.)
5.What’sthedifferencebetweenagalaxyandablackhole?(Galaxiesaregroupsofstarsthatarepulledandheld
togetherbygravity.Blackholesaretheleftoverremnantsofasupernovaexplosionthatrequireanescapevelocity
greaterthanthespeedoflight.)
6.HowmanyEarthscanfitinsidetheSun?(1.3million)
Lesson#2:SolarSystemTreasureHunt
1.TheshapeofourSolarSystemiscircular.
2.Howmanyplanetsdowehaveinoursolarsystem?8
3.PlutoisnowpartoftheKuiperBelt.
4.TheSunrotatesonceevery27daysatitsequatorand31daysatthepoles.
5.ThecoretemperatureoftheSunis15milliondegreesCelsius.
6.Aplanethasthreecriteria:ItorbitstheSun,hascleareditsorbitofsmallerobjects,andislargeenoughsoits
owngravitymakesitround.
7.Therearethreetypesofplanets:rockyterrestrial,gasgiantsandicegiants.
8.Mercuryistheclosest,butnotthehottestplanet.ThesidefacingtheSungetsto800oF,andthesidefacingaway
fromtheSungetsto‐280oF.
9.Thesolarsystemincludeseightplanets,theirmoons,theSunatthecenter,andsmallerobjectssuchascomets
andasteroids.
10.TheSunismadeoutof75%hydrogenand25%helium.
11.VenusiscalledthegoddessoflovebecauseitlookssobrighttousfromEarth,butitreallyhasasurface
temperatureof863oF.
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12.Cometsarereallydirtysnowballs.
13.Venusisthebrightestthinginthesky,otherthantheSunandMoon.
14.ColdmethaneiswhatgivesUranusitsblue‐greencolor.It’sclassifiedasanicegiant.
15.OnedayislongerthanayearonVenus.Notonlythat,itrotatesintheoppositedirection.
16.Earth’satmosphereismadeupof21%oxygenand78%nitrogen
17.TheMoonpullsonthesurfaceontheEarthandcausestidesonboththelandandocean.
18.Mars’smoonsarenamedafterFear/PanicandFleeing/Flight.
19.Ironoxide(rust)givesMarsitsredcolor.
20.IftheEarthwasthesizeofamarble,Jupiterwouldbethesizeofasoccerball.
21.Jupitercanfit1,321Earthsinside.
22.IfyouaddedmoremasstoJupiteritwouldgetsmallerbecauseit’sabigballofgas.
23.Jupiterismadeoutofhydrogenandheliumwithametallichydrogencore.
24.ThevolcanoesonJupiter’smoonIospewitsiceash300mileshigh.
25.Saturnissurroundedbyringsmademostlyoficemovingat75,000mph.
26.InsideSaturn’sringsareshepherdmoons.
27.Titanhasanatmospheremademostlyofnitrogensothickthatifyoustrappedwingsontoyourarmsand
flapped,you’dfly!
28.ScientiststhinkthatIapetususedtohavearingaroundit,anditcrasheddownontothesurface.
29.Jupiterissolargethatalloftheplanetsinthesolarsystemcouldfitinsideofit.
30.MimaslooksjustliketheDeathStar.
31.TheplanetUranusrollsaroundtheSunwhiletippedonitsside.
32.PhobosisslowlymovinginwardtowardMarsandwilleithershatterorformaringaroundMars.
33.OurbestguessisthattheiceonMercurywascausedbycomets.
34.AveragedailywindspeedonNeptuneis1,200mph.
35.Neptuneisagiantballofgas,whichisalsoknownasanicegiant.
36.CharonandPlutoareapairofobjectsbecausetheybothrotatearoundapointoutsideofeach.Thesetwoare
alsoorbitedbyHydraandNix.
37.SeventypercentoftheEarth'ssurfaceiscoveredbywater.
38.TheSunis93millionmilesfromtheEarth,alsoknownas1AU.
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39.ThehottestplanetisVenusbecausetheheatthatcomesintotheplanetgetstrappedinside.
40.Therearehowmanystarsareinoursolarsystem?One.TheSun.
41.Whichcolorstarsarethehottest?Blue.Coolest?Red.
42.ThePistolstaristhebiggestonewe’vefoundanditreleasesasmuchenergyinonesecondasourSundoesin
oneyear.
43.TheplanetsandmoonsthatpeoplehavewalkedonareEarthandtheMoon.
44.Jupiter'sGreatRedSpotisgettingsmaller.It’saboutthesizeoftwoEarthsrightnow.
45.JupiterandSaturnaregasgiants,andUranusandNeptuneareicegiants.
46.Neptuneisthecoldestplanetinoursolarsystem.
47.Thefivedwarfplanetsinoursolarsystemare:Eris,Makemake,Haumea,Pluto,andCeres.
48.Ittakeslight8minutestotravelfromtheSuntoEarth.
49.Venushassomuchvolcanicactivitythatitconstantlyresurfacesitself.
50.WhatkindoficeisonMars?Dryiceandwaterice.
Lesson#3:MagneticTornadoes
1.Defineanatmosphere.(Anenvelopesurroundinganobjectlikeaplanetoramoonthatisheldinplacebythe
object’sgravitationalfield.)
2.Whatisamagneticfield?(Aforcefieldaroundamagnet.)
3.Wheredomagneticfieldscomefrominplanets?(Wethinktheyoriginatefromthemoltenmetalliccoreofa
planet.Whenthecorecoolsoff,themagneticfielddisappears.)
4.Whichplanetsdonothaveamagneticfield?(Venusdoesnotbecauseofitssuper‐slowrotation,andMarsdoes
nothaveaplanet‐widemagneticfield,thoughitdoeshavemagnetichotspots.)
Lesson#4:SkyinaJar
1.Whatcolorsdoesthesunsetgothrough?(ThesunsetgoesthroughthecolorsoftherainbowastheSunsets
lowerinthesky,startingwithyellow,thenorange,andthenredasitsets.)
2.Doesthecolorofthelightsourcematter?(Yes.Whitelightgivesthebestresults.)
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Lesson#5:PlanetaryMagneticFields
1.Howarethelinesofforcedifferentforthetwomagnets?(Sincethisisgoingtodependonthekindofmagnets
youuse,refertothedatacollected.)
2.Howfarout(ininchesmeasuredfromthemagnet)doesthemagnetaffectthecompass?(Sincethisisgoingto
dependonthekindofmagnetsyouuse,refertothedatacollected.)
3.Whatmakesthecompassmovearound?(Themagneticlinesofforcethatareinvisibletoyoureye.)
4.Doyouthinkthecompass’snorth‐southindicatorisflipped,ortheEarth’sNorthPolewheretheSouthPoleis?
Howdoyouknow?(It’sanarbitrarydenotation,buttheEarth’sNorthPoleisdeemedtobenorth.)
Lesson#6:Seasons
1.WhatisthemainreasonwehaveseasonsonEarth?(Becausetheaxisistilted23.4o,exposingonehemisphereto
moresunlighteachdayandwarmingtheplanet.)
2.WhyaretherenosunsetsonUranusfordecades?(TheorbitforUranusis84years,whichmeans21yearspass
betweeneachseason.Thenorthpolewillexperiencecontinuedsunlightfor42yearsfromspringthroughfall,then
darknessfor42years.)
3.ArethereseasonsonVenus?(No.It’sthesametemperature(460oC)everywhereyougoontheplanetfortwo
reasons:firsttheaxistiltmakesalmostdifferencebetweensummerandwinter.Second,thethickatmosphere
trapstheheat,whichflowsaroundtheplanet.)
Lesson#7:IndoorRainClouds
1.Whichcombinationmadeitrainthebest?Whydidthiswork?(Thegreaterthetemperaturedifference,the
betterthisexperimentwillwork.Themorewateryouhave,thelessthetemperaturewillfluctuateforeachglass,
thusmakingitabletorainforlongerperiodsoftime.)
2.Drawyourexperimentaldiagramhere,labelingthedifferentcomponents:
3.Addinlabelsforthedifferentphasesofmatter.Canyouidentifyallthreestatesofmatterinyourexperiment?
(Ice=solid;water=liquid,gasbetweentwoglassesiswatervapor,nitrogen,andoxygen.)
Lesson#8:Volcanoes
1.HowisthisactivitysimilartothevolcanoesonMars?(Thebubblesthatgettrappedinsidemakepockets,andthe
dishsoaphelpsthemstayasbubbleslongenoughforyoutocatchtheminaction).
2.Whatgasisproducedwiththisreaction?(Carbondioxide)
3.Whichplanetshavevolcanoes,activeorextinct?(Mercury,Mars,Venus,Earth,Io(moonofJupiter),Triton
(moonofNeptune),Enceladus(moonofSaturn),andourveryownMoon.)
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Lesson#10:SongoftheSun
1.Whatdidyounoticethatisdifferentaboutthesoundsyouheard?
2.Howcanyoutellthattwosoundsaredifferentthatcamefromthesameinstrument?(Movementcausessound
wavestosounddifferent.)
3.Whatdidyounoticeaboutyourguesses?Whatkindofinstrumentswereyoumorecorrectabout?
Lesson#11:SimpleMicroscope&Telescope
1.Canlightchangespeeds?(Yes,whenittravelsthroughdifferentmediums.)
2.CanyouseeALLlightwithyoureyes?(No,onlyvisiblelight,likearainbow.)
3.Givethreeexamplesofalightsource.(Answerwillvary,butherearemine:Sun,acandle,andaglowstick.)
4.What'sthedifferencebetweenamicroscopeandatelescope?(Amicroscopemagnifiesanimagebeforethefocal
point;atelescopemagnifiesanimageafterthefocalpoint.Bothareusedtomakeimagesappearcloserandlarger.
Amicroscopeisusedwhenobjectsarenear;atelescopeisusedforfarawayobjects.)
5.Whyisthetelescopeimageupside‐down?(Becauseyou’vefocusedtheimagebeyondthefocalpoint.)
Lesson#12:StarCharting
1.Ifyouhaveconstellationsonyourclassceiling,chartthemonaseparatepagemarkingthepositionsoftherocks
withX’s.
2.Tonight,findtwoconstellationsthatyouwillchart.Bringthemwithyoutomorrowusingthetechniqueoutlined
aboveinLabTime.
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VocabularyfortheUnit
Asteroid.ObjectinorbitaroundtheSun,intermediateinsizebetweenmeteoroidsandplanets.
Asteroidbelt.Theregionofthesolarsysteminwhichmostasteroidshavetheirorbits,betweenMarsandJupiter.
BlackholesaretheleftoversofaBIGsupernova.Whenastarexplodes,itcollapsesdownintoawhitedwarfora
neutronstar.However,ifthestarislargeenough,thereisnothingtokeepitfromcollapsing,soitcontinuesto
collapseforever.Itbecomessosmallanddensethatthegravitationalpullissogreatthatlightitselfcan’tescape.
Centerofmass.Meanpositionofthemassesthatcompriseasystemorlargerbody:fortwobodies,thecenterof
massisapointonthelinejoiningthem.Forabinarystarsystem,themotionofeachstarcanbecomputedabout
thecenterofmass.
Comet.Smallbodyinthesolarsystem,inorbitaroundtheSun.Someofitsfrozenmaterialvaporizesduringthe
closerpartsofitsapproachtotheSuntoproducethecharacteristictail,behindtherighthead.
Conjunction.Closestapparentapproachoftwocelestialobjects.Planetaryconjunctionswereonceconsidered
importantomensforeventsonEarth.
Constellation.Agroupofstarsthatseemedtosuggesttheshapeofsomegod,person,animalorobject.Nowa
termusedtodesignatearegionofthesky.Thereare88constellations.
Darkmatter:Matterinthecosmosthatisundetectablebecauseitdoesn’tglow.Darkmatter,someofitintheform
ofas‐yet‐undiscoveredexoticparticles,isthoughttocomprisemostoftheuniverse.
Eclipse.Blockingoflightfromonebodybyanotherthatpassesinfrontofit.Eclipsecanbetotalorpartial.
Eclipsepath.NarrowpathontheEarth’ssurfacetracedbytheMoon’sshadowduringaneclipse.
Eclipsingbinarystar.Binarystarwhosemutualorbitisviewedalmostedge‐onsothatlightobservedisregularly
decreasedeachtimeonestareclipsestheother.
Ecliptic.PaththattheSunappearstofollow,againstthestarsonthecelestialsphere,duringthecourseofayear.
Eclipticplane.PlanedefinedbytheEarth’sorbitaroundtheSun.
Electromagneticwave:Astructureconsistingofelectricandmagneticfieldsinwhicheachkindoffieldgenerates
theothertokeepthestructurepropagatingthroughemptyspaceatthespeedoflight.Electromagneticwaves
includeradioandTVsignals,infraredradiation,visiblelight,ultravioletlight,X‐rays,andgammarays.
Ellipse.Typeofclosedcurvewhoseshapeisspecifiedintermsofitsdistancefromoneortwopoints.Acircleisa
specialformofellipse.Inappearance,anellipseisoval‐shaped.
Escapespeed:Thespeedneededtoescapetoinfinitelygreatdistancefromagravitatingobject.ForEarth,escape
speedfromthesurfaceisabout7milespersecond;forablackhole,escapespeedexceedsthespeedoflight.
Equinox.TwodayseachyearwhentheSunisaboveandbelowthehorizonforequallengthsoftime.
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Eventhorizon:Asphericalsurfacesurroundingablackholeandmarkingthe“pointofnoreturn”fromwhich
nothingcanescape.
Field:Awayofdescribinginteractingobjectsthatavoidsactionatadistance.Inthefieldview,oneobjectcreatesa
fieldthatpervadesspace;asecondobjectrespondstothefieldinitsimmediatevicinity.Examplesincludethe
electricfield,themagneticfield,andthegravitationalfield.
Galaxiesaregroupsofstarsthatarepulledandheldtogetherbygravity.
Globularclustersaremassivegroupsofstarsheldtogetherbygravity,usinghousingbetweentensofthousands
tomillionsofstars(thinkNewYorkCity).
Gravitationallensingisonewaywecan“see”ablackhole.Whenlightleavesastar,itcontinuesinastraightline
untilyankedonbythegravityofablackhole,whichbendsthelightandchangesitscourseandshowsupasstreaks
ormultiple,distortedimagesonyourphotograph.
Gravitationaltimedilation:Theslowingoftimeinregionsofintensegravity(largespacetimecurvature).
Gravitationalwaves:Literally,“ripples”inthefabricofspacetime.Theypropagateatthespeedoflightandresult
intransientdistortionsinspaceandtime.
Gravity:AccordingtoNewton,anattractiveforcethatactsbetweenallmatterintheuniverse.Accordingto
Einstein,ageometricalpropertyofspacetime(spacetimecurvature)thatresultsinthestraightestpathsnotbeing
Euclideanstraightlines.
Latitude.Coordinateusedtomeasure(indegrees)theangulardistanceofapointorcelestialobjectsaboveor
belowanequator.
Lightyear.Distancethatlighttravelsin1year.
Longitude.Coordinateusedtospecifythepositionofapointordirectionaround(orparallelto)anequator.
TheKuiperBeltisanicyregionthatextendsfromjustbeyondNeptune(from3.7billionmilesto7.4billionmiles
fromthesun).Thisiswheremostcometsandasteroidsfromoursolarsystemhangout.
NeutronstarswithHUGEmagneticfieldsareknownasmagnetars.
Magneticfield.Regionsurroundingamagnetorelectriccurrent,inwhichmagneticforcecanbedetectedinsucha
region,high‐speedelectricallychargedparticleswillgenerallymovealongcurvedpathsandradiateenergy.
Magneticpole.OneofthetworegionsonEarthtowhichacompassneedlewillpoint.Polesalsoexistonmagnets,
andthemagneticfieldsofsomeelectriccurrentscanhaveanequivalentbehavior.
Magnetoshpere.Regionsurroundingstarorplanet(includingEarth)inwhichamagneticfieldexists.
Meridian.Greatcircle,onthecelestialsphereortheEarth,thatpassesthroughbothnorthandsouthpolesandan
observer’szenithorlocation.
Meteor.Glowingtrailintheupperatmosphere,producedbymeteoroidburningupasitmovesathighspeed.
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Meteorshower.NumerousmeteorsseeninshorttimespanastheEarthmovesthroughacloudofmeteoroids,
probablyremnantsofacometandstillfollowingthecomet’sorbit.
Meteorite.RemnantofmeteoroidthathasbeenpartiallyerodedinpassagethroughtheEarth’satmospherebefore
hittingthesurface.Termnowalsoappliedtosimilarbodiesthatcollidewiththesurfacesoftheotherplanetsand
theirsatellites,producingcraters.
Meteoroid.Largerock(butmuchsmallerthanminorplanets)movinginanorbitinthesolarsystem.Meteoroids
thatenterintheEarth’satmospherearetermedmeteorsormeteorites,dependingontheirbehavior.
Neutronstarsareformedfromstarsthatgosupernova,butaren’tbigandfatenoughtoturnintoablackhole.
TheOortCloudliesjustbeyondtheKuiperbelt,housinganestimated1trillioncomets.
Orbit.Pathtracedoutbyoneobjectaroundanother.
Thevisiblesurfaceofthesuniscalledthephotosphere,andismademostlyofplasma(remembertheplasma
grapeexperiment?)thatbubblesuphotandcoldregionsofgas.
Dyingstarsblowoffshellsofheatedgasthatglowinbeautifulpatternscalledplanetarynebula.
Pulsarsareatypeofneutronstarthatspinsveryfast,spewsjetsofhigh‐energyx‐rayparticlesoutthepoles,and
haslargemagneticfields.
Oursolarsystemincludesrockyterrestrialplanets(Mercury,Venus,Earth,andMars),gasgiants(Jupiterand
Saturn),icegiants(UranusandNeptune),andassortedchunksoficeanddustthatmakeupvariouscomets(dusty
snowballs)andasteroids(chunksofrock).
Spacetime:Thefour‐dimensionalcontinuuminwhichtheeventsoftheuniversetakeplace.Accordingto
relativity,spacetimebreaksdownintospaceandtimeindifferentwaysfordifferentobservers.
Spacetimecurvature:Thegeometricalpropertyofspacetimethatcausesitsgeometrytodifferfromordinary
Euclideangeometry.Thecurvatureiscausedbythepresenceofmassiveobjects,andotherobjectsnaturallyfollow
thestraightestpossiblepathsincurvedspacetime.Thisistheessenceofgeneralrelativity’sdescriptionofgravity.
Spacetimeinterval:Afour‐dimensional“distance”inspacetime.Unlikeintervalsoftimeordistance,whichare
differentforobserversinrelativemotion,thespacetimeintervalbetweentwoeventshasthesamevalueforall
observers.
Specialtheoryofrelativity:Einstein’sstatementthatthelawsofphysicsarethesameforallobserversinuniform
motion.
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