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AST 205. Lecture 9. October 13, 2003 Gravitational Microlensing Drake Equation context & the need for other planet detection methods Basic gravitational lensing theory Gravitational microlensing by planets Advantages & disadvantages of technique The PLANET project Early results of the microlensing search

AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

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Page 1: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

AST 205. Lecture 9. October 13, 2003Gravitational Microlensing

• Drake Equation context & the need forother planet detection methods

• Basic gravitational lensing theory• Gravitational microlensing by planets• Advantages & disadvantages of technique• The PLANET project• Early results of the microlensing search

Page 2: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

N = f(p)n(e)f(l)f(i)f(c)R*L• Radial velocity techniques have provided first

direct clues about f(p), ≥ 5 -10%• Wealth of data for the study of planetary systems

and their formation in general• BUT this information is incomplete and severely

biased• No direct information on n(e) yet• Radial velocity and astrometric methods are

poorly suited to detection of Earth-like planets inSolar System-like environments

Page 3: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitational Lensing History

• Deflection of light/radiation by gravity• Einstein (1915) = 2 x Newton prediction• Eddington confirms in 1919 eclipse obsv.• Chwolson (1924), Einstein (1936), Zwicky

(1937), Refsdal (1964) … developed theory• First observed in 1979 for a distant quasar• Became a common tool for astronomy in

the 1980s and 90s

Page 4: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitaional Deflection of Light

Eddington proves Einstein right in 1919 eclipse!

Page 5: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitational Deflection of Light Formula

a = 4GM(<b)/bc2

a = 4GM/DOLqIc2

For a circularly symmetric mass distribution

For a point mass (relevant for stars & planets)

Achromatic = wavelength independent!

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Gravitational Lensing Geometry

b

Page 7: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Geometrical Optics - Image Condition

DOSqI = DLSa + DOSqS

a = DOS(qI - qS)/DLS

Page 8: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Solution of Gravitational Lens Equations

Simultaneous solution of lens & optical equations

Page 9: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

The Einstein Ring and Lensed Images

Appearance in the sky

S = sourceO = observerI = imagesM = lens/mass

Page 10: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Einstein Ring Radius Formula

qE = [4GMDLS/DOSDOLc2]1/2

Page 11: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitational Lens Magnification Image Effect

Page 12: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitational Lens Magnification Formula

where u = qS/ qE

Page 13: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

A Gravitational Microlensing Event

During a micro-lensing event therelative positionsof the source andthe lens change due to the motionsof both throughcross the sky.

As a result both theimage positions andmagnifications change with time.

Planets can makesmall perturbationsin the microlensingevent produced bytheir primary star.

Page 14: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Gravitational Microlensing Light Curves

Page 15: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Duration of Gravitational Microlensing Events

Page 16: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Light Curves from Two Equal Point Masses

Page 17: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Light Curve Produced by a HypotheticalPlanetary System Gravitational Lens

Page 18: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

The Earth’s Perturbation of a Light CurveProduced by the Sun Acting as a Grav Lens

Page 19: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Advantages of Microlensing Technique

• Jupiter-like planets “always” detectable• Anomalies last hours to days (not years to

decades)• Earth-like planets “occasionally” detectable• Can measure mass ratio & projected

separations of planet and star• Based on chance alignments; ideal for

statistical characterization of Galacticplanetary system population

Page 20: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Regions of Sensitivity for Three PlanetDetection Techniques

Page 21: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Disadvantages of the Microlensing Technique

• Requires very precise chance alignment of asource and the foreground planetary system– Rare and unpredictable– Transient and non-repeating

• Planetary systems detected will typically bevery distant and impossible to study further

• Event durations are comparable to Earth’sdiurnal cycle (i.e., 24 hours)

Page 22: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

PLANET: Probing Lensing AnomaliesNETwork (http://mplanet.anu.edu.au/)

Page 23: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

PLANET Light Curve of a Well StudiedMicrolensing Event

Page 24: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

PLANET: Null Results for First Five Years

“Analysis of 43 microlensing events from fiveyears of PLANET team monitoring data hasrevealed no indication of the short-lived``wiggles'' that planets orbiting the lens wouldcreate on light curves of the background stars. Atthe level of the observational uncertainties, alllight curves were consistent with those due to anisolated stellar lens. The lack of any detectedplanetary signature in these 43 events impliesthat less than 1/3 of M-dwarfs have Jupiter-masscompanions orbiting at 1.5 to 4 AU. M-dwarfsare cool, low-mass stars that make up the bulk ofstars (and microlenses) in the Galaxy.”

Page 25: AST 205. Lecture 9. October 13, 2003 Gravitational ...gk/A205OLD/lecture9.pdf · A Gravitational Microlensing Event During a micro-lensing event the relative positions of the source

Summary of PLANET Null Result from FiveYears of Data (43 Events)

Assume

25%

33%

50%

67%

100%

of stars to

have planets.