exoplanetsweb.hep.uiuc.edu/home/jjt/exoplanets.pdf · the green regions are the “habitable...
TRANSCRIPT
JonThaler Exoplanets 2
Outline • Whatisanexoplanet?
• WhyaretheyinteresKng?
• Howcanwefindthem?
• Exolife??• Thefuture...
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What is an Exoplanet? Mostoftheobjectsthatweseearestars.Exoplanetsarethingsthatorbitstars.
Howdoweknowthatwearenotseeingbinarystars,whicharequitecommon?
•Theminimumstellarmassisabout0.075*MS(=75MJ).Otherwisethereisnofusionatthecore.
•Planetsdon’temitlight.
LowmassandnolightarebothusedtoidenKfyplanets.
Tcore
GravitaKonalpressureheatsthecore.Tcore~15milliondegreesforfusion.
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Why Are They Interesting? •Stars(includingbinaries)andplanetsarethoughttoformfromaprimordialblobofgas,butthedetailsarecontroversial.Iwon’tdiscussthistopic.
•Planetscomeintwotypes:° Gasgiants (e.g.,Jupiter)° Rocks (e.g.,Earth)We’dliketoknowifthereareotherEarth-likeplanetsthatcouldsupportlife:“Goldilocks”planets.Nottoohotandnottoocold
ThediskshapeisaresultoftherotaKon.
Thegreenregionsarethe“habitablezones”.
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How Can We Find Exoplanets?
Therearetwoprimarymethods:• Thestarwobblesastheplanetorbitsit.• Thestarbecomes(slightly)dimmeriftheplanetpassesinfrontofit(“transits”thestar).
Ideally,we’dliketoobserveaplanetbothways.
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The Wobble method WhenobjectsareorbiKngeachother,neitherisstaKonary.Thecenterofmassremainsfixed,andeachobjectmovesaroundit.TheraKoofspeedsequalstheraKoofmasses.Thismeansthatwecanmeasurethemassoftheplanetbymeasuringthespeedofthestar.TheSunismuchheavierthantheplanets:
MJ/MS=0.001andME/MS=0.000003(3×10-6)
ThismeansthattheSun’sspeedisquitesmall:
12.5m/sduetoJupiterand8.4cm/sduetotheEarth.
ThesespeedscanbemeasuredusingtheDopplereffect.
Radialvelocity
Star&planet
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The Doppler Effect You’veallheardthechangeofpitchasacarorambulancepassesby.ThesizeoftheeffectdependsontheraKoofthecar’sspeedtothespeedofsound.Inthisvideo,thepitchdropsfromabout475Hzto425Hz(BtoG),indicaKngthatthecarisgoingabout19m/s(43mph).
Lightisawave,justlikesound,sowecanusetheopKcalDopplereffecttomeasurespeeds.Thedifficultyisthatthespeedoflightishuge(300,000,000m/s)andthestarsarenotmovingveryfast(1m/s,orso).
Thefrequencyneedstobemeasuredtoanaccuracyof1/300,000,000!!(threepartsperbillion)
Carhorndoppler
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Some Doppler Data Fortunately,opKcaltechniquesarecapableofexquisiteaccuracy.Let’slookatsomedata.
Notethescarerofthedatapoints.Themeasurementaccuracyisabout±2m/s.Measurementaccuracylimitsourabilitytoobservesmalleffects.
Thisisa“Jupiter”(M~0.96MJ)orbiKnga“Sol”(M=0.88MS).Theorbitalperiodis9years(Jupiter’sis12),becausetheorbitisabitsmaller(4.2AUinsteadof5.2).Thisishowastronomers60light-yearsawaycoulddiscoverJupiter.
Radialvelocity
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More Doppler Data MostplanetobservaKonsinvolvemuchshorterorbitalperiods:
Notethattheplothasmarginalsignificance.Kepler10bwasnotdiscoveredbythewobblemethod.Thisdataservedonlytoconfirmthediscovery.
Thisisan“Earth”(M~4.6ME)orbiKnga“Sol”(M=0.90MS).Theperiodis0.84days(20hours),becausetheorbitisonly0.016AU).ItiscalledKepler10b(moreaboutitlater).It’stoohot(1800K)tobehabitable.
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Can We Discover a Goldilocks? Here’saplotofplanetsdiscoveredbythewobblemethod.Oursolarsystemislabeledinblue.OnlyJupitercouldbediscoveredwiththewobblemethod,unlessmeasurementaccuracyimproves.
Speed
Earth
Jupiter
TheSunmoves8.4cm/sduetoEarth’sorbit.
1m/sresoluKonmakesitundetectable.
Kepler10b
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Planetary Transits Whenaplanetpassesinfrontofastar,thestarappearsdimmer.ThefracKondependsontheraKooftheareas:
RadiusofSun: 7.0×105km Dimming:RadiusofJupiter: 7.1×104km 0.01(i.e.,1%)RadiusofEarth: 6.4×103km 0.0001(i.e.,0.01%)
VenusandMercurytransittheSun,butthedimmingisminiscule.Here’saninteresKngvideo:
1882transit!!
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Planetary Transits (2) Here’swhatoneexpectstoobserve:
Jupiter:10-3brightnessaccuracyrequired
Earth:10-5brightnessaccuracyrequired
10-3accuracyisachievabledirectly,but10-5canonlybeachievedbyaveragingmanymeasurements(requiresorbitswithshortperiods).
TransitSimulator
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NASA’s Kepler Mission “Asearchforhabitableplanets”hrp://www.nasa.gov/mission_pages/kepler/main/index.html
Itusesan85Megapixelcameratomonitormorethan100,000starsfortransiKngplanets.Launchedin2009,itisinsolar(notEarth)orbit.
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Keplerhasfound2321planetcandidatesand2165eclipsingbinarystars.
Here’sthediscovery(in2011)ofKepler10b,thefirstrockyplanet:
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Fig. 12.— The Kepler photometry and physical models are plotted as a function of both time
(upper two panels) and phase (lower two panels). The transits of KOI-72.02 are highlighted
by blue vertical lines in the topmost panel while a cutout (defined by the yellow box) is
expanded to show the transits of Kepler-10b highlighted by red vertical lines (second from
top). The bottom two panels shows the phase-folded light curves centered on phase zero
as defined by the central transit time. The modeled light curves are shown as colored lines
(blue corresponding to KOI-72.02 and red corresponding to Kepler-10b. Also shown is a
phase cutout of the lightcurve and model (green) centered on phase= 0.5 where occulations
would occur for a circular orbit. The relative intensity scale for phase= 0 can be read o↵
the y-axis on the left-hand-side of the plot while the relative intensity scale for phase= 0.5
can be read o↵ the y-axis on the right-hand-side of the plot.
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Fig. 12.— The Kepler photometry and physical models are plotted as a function of both time
(upper two panels) and phase (lower two panels). The transits of KOI-72.02 are highlighted
by blue vertical lines in the topmost panel while a cutout (defined by the yellow box) is
expanded to show the transits of Kepler-10b highlighted by red vertical lines (second from
top). The bottom two panels shows the phase-folded light curves centered on phase zero
as defined by the central transit time. The modeled light curves are shown as colored lines
(blue corresponding to KOI-72.02 and red corresponding to Kepler-10b. Also shown is a
phase cutout of the lightcurve and model (green) centered on phase= 0.5 where occulations
would occur for a circular orbit. The relative intensity scale for phase= 0 can be read o↵
the y-axis on the left-hand-side of the plot while the relative intensity scale for phase= 0.5
can be read o↵ the y-axis on the right-hand-side of the plot.
Some Kepler Data
Thisisprobablya“Neptune”.Orbitalperiodis45days.Radiusis2.2RE.ThisisKepler10b,arockyplanet.However,it’stoohot(1800K)forGoldilocks.Orbitalperiodis20hours!Orbitalradius~0.016AU.
LightcurvewhentheplanetisinfrontofthestarLightcurvewhentheplanetisbehindthestar
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Eclipsingbinarystarsdon’tlookthesameastransiKngplanets,becausebothobjectsemitlight.
Binary Stars Look Different
Eclipsingbinary
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The Search for Exolife
SupposewefindanEarth-likeplanetinthehabitablezone.Howcanwetellifithaslife?
Weneedtoknowmoreabouttheplanetthanitsmass.Wecannotyetimageexoplanets,butitisjustnowbecomingpossibletolearnsomethingabouttheirchemicalcomposiKon.
OnecandeterminethechemicalcomposiKonofagasbymeasuringtheabsorpKonoflightthatpassesthroughit.So,thispropertyofatransiKngexoplanet’satmospherecan,inprinciple,bemeasured.
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Absorption Spectra HerearetheabsorpKonspectraofvariousgases.Whenaplanetpassesinfrontofastar,someofthewavelengthsemiredbythestarareabsorbedbytheplanet’satmosphere.Forexample,carbonmonoxideabsorbsnear5microns.
1 5 10 15Wavelength(microns)
CO
CH4
N2O
CO2
HDO
O3
H2O
Directorate of Scientific Programmes M. FridlundM. Fridlund, August 2006
Bio markersBio markers
The goal is to find rocky planets with an atmosphere out of photo-chemical balance.
(cf. Lederberg, 1965 and Lovelock, 1965)
Working definition:
Life { O3 + H2O + CO2
Ideally, detect reduced molecules (CH4, N2O) as well
HerearetheabsorpKonspectraofthreeplanetary
atmospheres.Thisisrealdata!!
Whichplanethaslife?
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Exolife Waterand,especially,oxygen(inthiscaseozone)aresmokinggunindicatorsofourkindoflife.OxygenismuchtooreacKvetoremainintheatmospherewithoutplantlifetoreplenishit.
Thisisaverydifficultmeasurementtomakeinanexoplanet,especiallyasmall,Earthlikeone.
Directorate of Scientific Programmes M. FridlundM. Fridlund, August 2006
Bio markersBio markers
The goal is to find rocky planets with an atmosphere out of photo-chemical balance.
(cf. Lederberg, 1965 and Lovelock, 1965)
Working definition:
Life { O3 + H2O + CO2
Ideally, detect reduced molecules (CH4, N2O) as well
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A Proof of the Principle Thisyear,astronomersusedtheVeryLargeTelescope(VLT,asetoffour8mtelescopesinChile)todetectcarbonmonoxideintheatmosphereofa“SuperJupiter”thatorbitsTauBooKs(avisiblestar).Gasgiantshavelotsofatmosphere,sothisisan“easy”measurement.Unfortunately,thedataanalysisisquitecomplexanddoesn’tlenditselftoanicegraphic.Trustme!
Thestar:Mass: 1.3MSDistance:51l.y.Theplanet:Mass: 4.1MJOrbit: 0.05AU
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The Future ... TheEuropeanSpaceAgency(ESA)consideredasetofsatellites(theDarwinmission)tosearchforlifeonEarthlikeexoplanets,butabandoneditasunfeasibleatthisKme.NASAconsidered,andabandoned,asimilarproject(theTerrestrialPlanetFinder).
Perhapsin10-20years...ScienKficandtechnicalprogressareintertwined,butthat’sanothertalk.