extrasolar planets the next decade dante minniti, católica steve vogt, uc santa cruz chris tinney,...

26
Extrasolar Extrasolar Planets Planets The Next Decade The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar planets in the past decade The discovery of extrasolar planets in the past decade was one was one of the most remarkable achievements of the century, and of the most remarkable achievements of the century, and the the culmination of centuries of speculation. culmination of centuries of speculation. National Academy of Sciences, Decadal Review of Astrophysics National Academy of Sciences, Decadal Review of Astrophysics

Upload: leo-jasper-singleton

Post on 17-Jan-2016

218 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Extrasolar PlanetsExtrasolar PlanetsThe Next DecadeThe Next Decade

Dante Minniti, CatólicaSteve Vogt, UC Santa Cruz

Chris Tinney, UNSWPamela Arriagada, Católica

The discovery of extrasolar planets in the past decade was oneThe discovery of extrasolar planets in the past decade was oneof the most remarkable achievements of the century, and theof the most remarkable achievements of the century, and the

culmination of centuries of speculation.culmination of centuries of speculation.National Academy of Sciences, Decadal Review of AstrophysicsNational Academy of Sciences, Decadal Review of Astrophysics

Page 2: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

~45,000 parsecs

50 parsecs

10,000 parsecs

1000 parsecs

Page 3: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 4: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

16 Cygni B

Not sinusoidal

Page 5: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 6: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Planet Mass DistributionPlanet Mass Distribution

Fit ExcludesFit Excludes

11stst bin. bin.

Detection Detection Limit:Limit:

~ 0.2 M~ 0.2 MJUP JUP @ 1 @ 1 AUAU

Five Neptunes:Five Neptunes:Gl 436Gl 43655 Cnc d55 Cnc d AraAra• HD 190360HD 190360• Gliese 581Gliese 581

Butler et al.Butler et al.

McArthur et al.McArthur et al.

Santos et al. Santos et al.

Page 7: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Planet – Metallicity CorrelationPlanet – Metallicity Correlation

AbundanceAnalysis of1000 stars

onplanet search

.

22

PPplanetplanet ~ ~ ((NNFeFe

/ N/ NHH))

Previous Evidence: Previous Evidence: G.Gonzales, N.SantosG.Gonzales, N.Santos

Fischer & Valenti Fischer & Valenti 20052005

Metallicity Metallicity Models:Models:

Ida & LinIda & Lin

Kacper KornetKacper Kornet

et al. et al.

Page 8: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Doppler MeasurementsDoppler Measurements

Orbit:Orbit:

P = 2.876 dP = 2.876 d

K = 41.3 m/sK = 41.3 m/s

CircularCircular

M = 0.343 MM = 0.343 MJUPJUP

= 1.15 M= 1.15 MSATSAT

Page 9: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Photometry: Photometry:

Three TransitsThree Transits

3.0 millimag ->3.0 millimag ->

AAPLPL = 0.0028 A = 0.0028 Astarstar

RRPLPL = 0.053 R = 0.053 RStarStar

G. HenryG. Henry

Page 10: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Density & InteriorDensity & Interior R = 0.88 RR = 0.88 RSATSAT

M = 1.145 MM = 1.145 MSATSAT

SATSAT

R ~ MR ~ M-1/3 -1/3 (degeneracy)(degeneracy)

R ~ MR ~ M+1/3+1/3 (Coulomb, rock)(Coulomb, rock)

10% errors)10% errors)

= 1.69 = 1.69 SatSat

More RockMore Rock

Page 11: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Radius vs MassRadius vs MassMeasured for Transiting PlanetsMeasured for Transiting Planets

Mass (MMass (MJUPJUP))

Rad

ius

(RR

ad

ius

(RJU

PJU

P))

Page 12: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 13: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

The Next Decade:The Next Decade:3 m/s versus 1 m/s3 m/s versus 1 m/s

1 m/s1 m/s

3 m/s3 m/s

Jupiter analog is 10-sigma detectionJupiter analog is 10-sigma detectionUncertainty of eccentricity is +/-0.02Uncertainty of eccentricity is +/-0.02Saturn-mass at 5 AU is a 4-sigma detectionSaturn-mass at 5 AU is a 4-sigma detectionSuper-Earths detectable in 4-day orbitsSuper-Earths detectable in 4-day orbitsDetection sensitivity similar/better than SIMDetection sensitivity similar/better than SIM

Minimal (3-sigma) detection of Jupiter analogMinimal (3-sigma) detection of Jupiter analogEccentricity of Jupiter analog is uncertain (+/-0.2)Eccentricity of Jupiter analog is uncertain (+/-0.2)Non-detection of Saturn-mass at 5 AUNon-detection of Saturn-mass at 5 AU

Obstacles to 1 m/sObstacles to 1 m/sStellar oscillations PhotonsStellar oscillations PhotonsStellar granulation Systematic ErrorsStellar granulation Systematic ErrorsStellar rotationStellar rotation

Page 14: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

P-modes in Solar-type starsP-modes in Solar-type stars

Amp ~ 1.5 m/sAmp ~ 1.5 m/sPer = 5 minPer = 5 min

- Seismology- Seismology

-Noise:Noise:

Avg overAvg over P-modes !P-modes !

Alpha Cen A (G2 V)Alpha Cen A (G2 V)

Page 15: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

K dwarfs: 1 meter/secK dwarfs: 1 meter/sec

Acoustic p-modes:Acoustic p-modes:

Amp < 1 m/sAmp < 1 m/s

Alpha Cen B (K0V)Alpha Cen B (K0V)

Page 16: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

Doppler PrecisionDoppler Precision

Page 17: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

10 Earth-Masses10 Earth-MassesP = 50 dayP = 50 day

Single telescopeSingle telescope

AliasingAliasing

1 day Obs1 day Obs..

Page 18: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

5 Earth-Masses 5 Earth-Masses P = 50 dayP = 50 day

Single telescopeSingle telescope

Page 19: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

1 Earth-Mass1 Earth-MassP = 4.2 dP = 4.2 d

MMstarstar = 0.5 M = 0.5 MOO

Page 20: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

1 m/s: Long Data Strings1 m/s: Long Data Strings

APFAPF

AATAAT

USNO funded 2.4-m dedicated planet finderUSNO funded 2.4-m dedicated planet finder

48 continous nights Jan 10, 200748 continous nights Jan 10, 2007

KeckKeck 10 continous nights 10 continous nights

Page 21: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 22: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 23: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 24: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar
Page 25: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

1 m/s: Long View1 m/s: Long View

TPFTPF

SIMSIM 1.2-to-2 billion $ 150 stars 2020?1.2-to-2 billion $ 150 stars 2020?

5-to-?? billion $ ? Stars 2040?5-to-?? billion $ ? Stars 2040?

8-m8-m 0.1 billion $ 1,000 stars NOW?0.1 billion $ 1,000 stars NOW?

Page 26: Extrasolar Planets The Next Decade Dante Minniti, Católica Steve Vogt, UC Santa Cruz Chris Tinney, UNSW Pamela Arriagada, Católica The discovery of extrasolar

1 m/s: Long View1 m/s: Long View

8-m8-m 0.1 billion $ 1,000 stars NOW?0.1 billion $ 1,000 stars NOW?

Every Saturn mass planet out to 9 AUEvery Saturn mass planet out to 9 AU

Every Neptune mass planet out to 1 AUEvery Neptune mass planet out to 1 AU

Super-Earths out to 0.3 AUSuper-Earths out to 0.3 AU

Earth-mass planets out to 0.1 AUEarth-mass planets out to 0.1 AU

Solar System analogsSolar System analogs

Habitable planetsHabitable planets