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Fainter and closer: finding planets by symmetry breaking
Erez N. Ribak and Szymon Gladysz »View Author Affiliations
1Physics Department, Technion – Israel Institute of Technology, Haifa 32000, Israel
2Applied Optics Group, School of Physics, National University of Ireland, Galway
*Corresponding author: eribak@physics.technion.ac.il
Optics Express, Vol. 16, Issue 20, pp. 15553-15562 (2008)
http://dx.doi.org/10.1364/OE.16.015553
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Abstract
Imaging of planets is very difficult, due to the glare from their nearby, much brighter suns. Static and slowly-evolving aberrations are the limiting factors, even after application of adaptive optics. The residual speckle pattern is highly symmetrical due to diffraction from the telescope’s aperture. We suggest to break this symmetry and thus to locate planets hidden beneath it. An eccentric pupil mask is rotated to modulate the residual light pattern not removed by other means. This modulation is then exploited to reveal the planet’s constant signal. In well-corrected ground-based observations we can reach planets six stellar magnitudes fainter than their sun, and only 2-3 times the diffraction limit from it. At ten times the diffraction limit, we detect planets 16 magnitudes fainter. The stellar background drops by five magnitudes.
© 2008 Optical Society of America
OCIS Codes
(010.1080) Atmospheric and oceanic optics : Active or adaptive optics
(030.6610) Coherence and statistical optics : Stellar speckle interferometry
(050.1220) Diffraction and gratings : Apertures
(350.1260) Other areas of optics : Astronomical optics
(110.4155) Imaging systems : Multiframe image processing
(070.6120) Fourier optics and signal processing : Spatial light modulators
ToC Category:
Imaging Systems
History
Original Manuscript: August 8, 2008
Revised Manuscript: September 10, 2008
Manuscript Accepted: September 13, 2008
Published: September 17, 2008
Citation
Erez N. Ribak and Szymon Gladysz, "Fainter and closer: finding planets by symmetry breaking," Opt. Express 16, 15553-15562 (2008)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-16-20-15553
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- J.-L. Beuzit, M. Feldt, K. Dohlen, D. Mouillet, P. Puget, J. Antici, A. Baruffolo, P. Baudoz, A. Berton, A. Boccaletti, M. Carbillet, J. Charton, R. Claudi, M. Downing, P. Feautrier, E. Fedrigo, T. Fusco, R. Gratton, N. Hubin, M. Kasper, M. Langlois, C. Moutou, L. Mugnier, J. Pragt, P. Rabou, M. Saisse, H. M. Schmid, E. Stadler, M. Turrato, S. Udry, R. Waters, and F. Wildi, "SPHERE: a 'Planet Finder' Instrument for the VLT," The Messenger 125, 29-34 (2006).
- C. Marois, D. Lafrenière, R. Doyon, B. Macintosh, and D. Nadeau, "Angular differential imaging: a powerful high-contrast imaging technique," Astrophys. J. 641, 556-559 (2006). [CrossRef]
- R. Racine, G. A. H. Walker, D. Nadeau, R. Doyon, and C. Marois, "Speckle noise and the detection of faint companions," Publ. Astron. Soc. Pac. 111, 587-594 (1999). [CrossRef]
- P. Dierickx, D. Enard, R. Geyl, J. Paseri, M. Cayrel, and P. Béraud, "The VLT primary mirrors: mirror production and measured performance," Proc. SPIE 2871, 385-392 (1997). [CrossRef]
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- R. Racine, G. A. H. Walker, D. Nadeau, R. Doyon, and C. Marois, "Speckle noise and the detection of faint companions," Publ. Astron. Soc. Pac. 111, 587-594 (1999). [CrossRef]
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- J.-L. Beuzit, M. Feldt, K. Dohlen, D. Mouillet, P. Puget, J. Antici, A. Baruffolo, P. Baudoz, A. Berton, A. Boccaletti, M. Carbillet, J. Charton, R. Claudi, M. Downing, P. Feautrier, E. Fedrigo, T. Fusco, R. Gratton, N. Hubin, M. Kasper, M. Langlois, C. Moutou, L. Mugnier, J. Pragt, P. Rabou, M. Saisse, H. M. Schmid, E. Stadler, M. Turrato, S. Udry, R. Waters, and F. Wildi, "SPHERE: a 'Planet Finder' Instrument for the VLT," The Messenger 125, 29-34 (2006).
- J.-L. Beuzit, M. Feldt, K. Dohlen, D. Mouillet, P. Puget, J. Antici, A. Baruffolo, P. Baudoz, A. Berton, A. Boccaletti, M. Carbillet, J. Charton, R. Claudi, M. Downing, P. Feautrier, E. Fedrigo, T. Fusco, R. Gratton, N. Hubin, M. Kasper, M. Langlois, C. Moutou, L. Mugnier, J. Pragt, P. Rabou, M. Saisse, H. M. Schmid, E. Stadler, M. Turrato, S. Udry, R. Waters, and F. Wildi, "SPHERE: a 'Planet Finder' Instrument for the VLT," The Messenger 125, 29-34 (2006).
- D. Gisler, H. M. Schmid, C. Thalmann, H. P. Povel, J. O. Stenflo, F. Joos, M. Feldt, R. Lenzen, J. Tinbergen, R. Gratton, R. Stuik, D. M. Stam, W. Brandner, S. Hippler, M. Turatto, R. Neuhauser, C. Dominik, A. Hatzes, T. Henning, J. Lima, A. Quirrenbach, L. B. F. M. Waters, G. Wuchterl, and H. Zinnecker, "CHEOPS/ZIMPOL: a VLT instrument study for the polarimetric search of scattered light from extrasolar planets," Proc. SPIE 5492, 463-474 (2004). [CrossRef]
- F. Malbet, J. W. Yu, and M. Shao, "High dynamic range imaging using a deformable mirror for space coronography," Pub. Astron. Soc. Pac. 107, 386-398 (1995). [CrossRef]
- R. B. Makidon, A. Sivaramakrishnan, and R. van der Marel, "Observing extrasolar giant planet environments with JWST," Proc. SPIE 7010, 7010-7024 (2008).
- S. Hinkley, B. R. Oppenheimer, R. Soummer, A. Sivaramakrishnan, L. C. Roberts, Jr., J. Kuhn, R. B. Makidon, M. D. Perrin, J. P. Lloyd, K. Kratter, and D. Brenner, "Temporal evolution of coronagraphic dynamic range and constraints on companions to Vega," Astrophys. J. 654, 633-640 (2007). [CrossRef]
- S. Hinkley, B. R. Oppenheimer, R. Soummer, A. Sivaramakrishnan, L. C. Roberts, Jr., J. Kuhn, R. B. Makidon, M. D. Perrin, J. P. Lloyd, K. Kratter, and D. Brenner, "Temporal evolution of coronagraphic dynamic range and constraints on companions to Vega," Astrophys. J. 654, 633-640 (2007). [CrossRef]
- W. B. Sparks and H. C. Ford, "Imaging spectroscopy for extrasolar planet detection," Astrophys. J. 578, 543-564 (2002). [CrossRef]
- N. J. Kasdin, R. J. Vanderbei, D. N. Spergel, and M. G. Littman, "Extrasolar planet finding via optimal apodized-pupil and shaped-pupil coronagraphs," Astrophys. J. 582, 1147-1161 (2003). [CrossRef]
- J.-L. Beuzit, M. Feldt, K. Dohlen, D. Mouillet, P. Puget, J. Antici, A. Baruffolo, P. Baudoz, A. Berton, A. Boccaletti, M. Carbillet, J. Charton, R. Claudi, M. Downing, P. Feautrier, E. Fedrigo, T. Fusco, R. Gratton, N. Hubin, M. Kasper, M. Langlois, C. Moutou, L. Mugnier, J. Pragt, P. Rabou, M. Saisse, H. M. Schmid, E. Stadler, M. Turrato, S. Udry, R. Waters, and F. Wildi, "SPHERE: a 'Planet Finder' Instrument for the VLT," The Messenger 125, 29-34 (2006).
- D. Gisler, H. M. Schmid, C. Thalmann, H. P. Povel, J. O. Stenflo, F. Joos, M. Feldt, R. Lenzen, J. Tinbergen, R. Gratton, R. Stuik, D. M. Stam, W. Brandner, S. Hippler, M. Turatto, R. Neuhauser, C. Dominik, A. Hatzes, T. Henning, J. Lima, A. Quirrenbach, L. B. F. M. Waters, G. Wuchterl, and H. Zinnecker, "CHEOPS/ZIMPOL: a VLT instrument study for the polarimetric search of scattered light from extrasolar planets," Proc. SPIE 5492, 463-474 (2004). [CrossRef]
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- N. Thatte, R. Abuter, M. Tecza, E. L. Nielsen, F. J. Clarke, and L. M. Close, "Very high contrast integral field spectroscopy of AB Doradus C: 9-mag contrast at 0.2 arcsec without a coronagraph using spectral deconvolution," Monthly Notices of the Royal Astronomical Society 378, 1229-1236 (2007). [CrossRef]
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Astrophys. J.
- S. Hinkley, B. R. Oppenheimer, R. Soummer, A. Sivaramakrishnan, L. C. Roberts, Jr., J. Kuhn, R. B. Makidon, M. D. Perrin, J. P. Lloyd, K. Kratter, and D. Brenner, "Temporal evolution of coronagraphic dynamic range and constraints on companions to Vega," Astrophys. J. 654, 633-640 (2007). [CrossRef]
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J. Opt. Soc. Am. A
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Nature
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The Messenger
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2008, Makidon, Proc. SPIE
- R. B. Makidon, A. Sivaramakrishnan, and R. van der Marel, "Observing extrasolar giant planet environments with JWST," Proc. SPIE 7010, 7010-7024 (2008).
- S. Gladysz and J. C. Christou, "Detection of faint companions through stochastic speckle discrimination," Astrophys. J. 684, 1486-1495 (2008). [CrossRef]
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