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Adaptive Optics for Astronomy
Kathy Cooksey
AO Basics
• Photons – Travel in straight lines
• Wavefront– Line perpendicular to all photons’ paths
• Atmospheric turbulence– Due to temperature differences– Acts like many lenses– Distorts wavefront
• AO System– Corrects wavefront– Makes it linear
Photons Travel in Straight Lines
Wavefronts
Atmospheric Turbulence
Atmospheric Turbulence
Lick Observatory, 1 m telescope
Long exposureimage
Short exposureimage
“Perfect” image: diffraction limit of
telescope
Distant stars should resemble “points” if it were not for turbulence in Earth’s atmosphere
Speckle Images
• Turbulence changes rapidly with time
• Sequence of short snapshots of star
• Much slower than real time
Applied Optics Group (Imperial College), Herschel 4.2-m Telescope
AO Straighten Wavefront
BEFORE AFTER
Incoming, distorted
wavefront (“aberrated”)
DEFORMABLE MIRROR
Corrected wavefront
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AO in ActionLick Observatory adaptive optics system
Star without adaptive optics Star with adaptive optics
AO Specifics: Correcting for Atmosphere and Improving
ImagesEven the largest ground-based astronomical telescopes have no better resolution than an
8” backyard telescope!
Basic AO Process(a) Measure details of blurring from “guide star” near object you want to observe
(b) Calculate shape to apply to deformable mirror to correct blurring
(c) Light from both guide star and astronomical object is reflected from deformable mirror
Schematic of AO System
Gemini: AO in “Action”
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How to Measure Distortion
Shack-Hartmann Wavefront Sensor
…you will see this again
Ground-based AO Complements Space Telescopes
Advantages of AO on 8-10 m ground-based telescopes
• Four times better spatial resolution in infrared
• Better faint-object sensitivity at wavelengths > 2 microns
• Outstanding infrared spectroscopy– Higher spectral & spatial
resolution
Advantages of 2.4 m Hubble Space Telescope
• Full wavelength coverage, from UV to visible to near-infrared light
• Can “see” virtually whole sky
• More precise brightness measurements
• Very sensitive spectroscopy for faint objects in infrared – Lower spectral & spatial
resolution
Beautiful AO Images
Satellites for the Small • Adaptive Optics has opened up study of
smaller bodies of solar system
Double Asteroid 90 Antiope Eugenia and its moon
Merine et al. CFHTMerine et al. Keck
Neptune at 1.65 micronsWithout adaptive optics With Keck adaptive optics
June 27, 1999
2.3
arc
sec
May 24, 1999
Neptune Movie
• AO allows us to monitor weather on outer planets
Institute for Astronomy (University of Hawaii) CFHT
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Titan Occults Two Stars• Occultation is when planet or moon passes
in front of star
Original
Titan “subtracted”
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Sharmer et al. Swedish Solar Vacuum Telescope
Lightbridges on Sun
• Lightbridges discovered with AO
• Those shown are ~5000 km in length– Golden Gate ~2 km
• Believed to be “normal” solar granulation that penetrates strongly magnetic sunspot umbras
AO Reveals Faint Companions to Bright Stars
Mike Brown (CalTech)
Galactic Center
UCLA Galactic Center Group
Evidence for Black Hole at Center of Milky Way
• Black hole is revealed by presence of fast moving stars at small radii
• Stellar orbits in central parsec, 1995-2006
NGC 6934 from Gemini North• Adaptive Optics allows us to discern
separate stars in crowded cores of globular clusters
Gemini Obs., NSF, & U. Hawaii IfA
Summary of Astronomical AO
• Remove effect of atmospheric turbulence – “Twinkle” of stars
• Must “sense” blurring of star – Either real or laser “star”
• Computers calculate how to correct light – Send this signal to deformable mirror
• Resulting performance can equal or exceed Hubble Space Telescope in some areas
• Astronomers use AO to study asteroids, moons, planets, stars, and galaxies
More AO Tidbits
Titan’s Surface at Keck Without AO Typical at 1.65 μm
With AOAt 1.581 μm (surface window)
Surface Reflectivity
Model inputs:Haze optical depthOptical properties of haze particles (varies with depth)Model outputs: Image of atmosphere
Atmospheric properties:
Haze optical depth, variation with altitude
AO image
Surface albedo map
Model image of atmosphere
AO Image Sequence of 216 Kleopatra
• Movie of the asteroid Kleopatra, observed during seven-hour period with CFHT AO System
Merine et al. CFHT
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Extra-Solar Planetary System Science with AO
• Dust disks as signatures of planetary systems• Close-up views of forming planetary systems• Detection and characterization of planets
eXtreme Adaptive Optics Planet Imager
• XAOPI project (in progress)
• System at Keck observatory
• First images of extra-solar planets