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A Ground-based Albedo Upper Limit for HD 189733b from Polarimetry

Wiktorowicz, Sloane J. and Nofi, Larissa A. and Jontof-Hutter, Daniel and Kopparla, Pushkar and Laughlin, Gregory P. and Hermis, Ninos and Yung, Yuk L. and Swain, Mark R. (2015) A Ground-based Albedo Upper Limit for HD 189733b from Polarimetry. Astrophysical Journal, 813 (1). Art. No. 48. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20151218-114523995

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Abstract

We present 50 nights of polarimetric observations of HD 189733 in the B band using the POLISH2 aperture-integrated polarimeter at the Lick Observatory Shane 3-m telescope. This instrument, commissioned in 2011, is designed to search for Rayleigh scattering from short-period exoplanets due to the polarized nature of scattered light. Since these planets are spatially unresolvable from their host stars, the relative contribution of the planet-to-total system polarization is expected to vary with an amplitude of the order of 10 parts per million (ppm) over the course of the orbit. Non-zero and also variable at the 10 ppm level, the inherent polarization of the Lick 3-m telescope limits the accuracy of our measurements and currently inhibits conclusive detection of scattered light from this exoplanet. However, the amplitude of observed variability conservatively sets a 99.7% confidence upper limit to the planet-induced polarization of the system of 60 ppm in the B band, which is consistent with a previous upper limit from the POLISH instrument at the Palomar Observatory 5-m telescope. A physically motivated Rayleigh scattering model, which includes the depolarizing effects of multiple scattering, is used to conservatively set a 99.7% confidence upper limit to the geometric albedo of HD 189733b of A_g < 0.40. This value is consistent with the value A_g = 0.226 ±0.091 derived from occultation observations with Hubble Space Telescope STIS, but it is inconsistent with the large A_g = 0.61 ± .012 albedo reported by Berdyugina et al.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/813/1/48DOIArticle
http://iopscience.iop.org/article/10.1088/0004-637X/813/1/48/metaPublisherArticle
ORCID:
AuthorORCID
Wiktorowicz, Sloane J.0000-0003-4483-5037
Jontof-Hutter, Daniel0000-0002-6227-7510
Kopparla, Pushkar0000-0002-8951-3907
Laughlin, Gregory P.0000-0002-3253-2621
Yung, Yuk L.0000-0002-4263-2562
Swain, Mark R.0000-0002-0919-4468
Additional Information:© 2015. The American Astronomical Society. Received 2015 July 13; accepted 2015 September 29; published 2015 October 27. We would like to acknowledge the tireless efforts of the Lick Observatory staff. This work was performed (in part) under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute. S.J.W. and L.A.N. acknowledge support from the NASA Origins of Solar Systems program through grant NNX13AF63G. P.K. and Y.L.Y. acknowledge support from an NAI Virtual Planetary Laboratory grant from the University of Washington to the Jet Propulsion Laboratory and California Institute of Technology. Research at Lick Observatory is partially supported by a generous gift from Google. Facility: Shane (POLISH2) - .
Funders:
Funding AgencyGrant Number
NASA/CaltechUNSPECIFIED
NASA Sagan FellowshipUNSPECIFIED
NASANNX13AF63G
NAI Virtual Planetary LaboratoryUNSPECIFIED
GoogleUNSPECIFIED
Subject Keywords:dust, extinction; planetary systems; planets and satellites: atmospheres; planets and satellites: individual (HD 189733b) ; polarization; techniques: polarimetric
Issue or Number:1
Record Number:CaltechAUTHORS:20151218-114523995
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20151218-114523995
Official Citation:Sloane J. Wiktorowicz et al 2015 ApJ 813 48
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:63075
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:18 Dec 2015 19:51
Last Modified:09 Mar 2020 13:19

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