Phase functions and light curves of wide-separation extrasolar giant planets

David Sudarsky, Adam Burrows, Ivan - Hubeny, Aigen Li

Research output: Contribution to journalArticle

50 Citations (Scopus)

Abstract

We calculate self-consistent extrasolar giant planet (EGP) phase functions and light curves for orbital distances ranging from 0.2 to 15 AU. We explore the dependence on wavelength, cloud condensation, and Keplerian orbital elements. We find that the light curves of EGPs depend strongly on wavelength, the presence of clouds, and cloud particle sizes. Furthermore, the optical and infrared colors of most EGPs are phase-dependent, tending to be reddest at crescent phases in V - R and R - I. Assuming circular orbits, we find that at optical wavelengths most EGPs are 3-4 times brighter near full phase than near greatest elongation for highly inclined (i.e., close to edge-on) orbits. Furthermore, we show that the planet/star flux ratios depend strongly on the Keplerian elements of the orbit, particularly inclination and eccentricity. Given a sufficiently eccentric orbit, an EGP's atmosphere may make periodic transitions from cloudy to cloud-free, an effect that may be reflected in the shape and magnitude of the planet's light curve. Such elliptical orbits also introduce an offset between the time of the planet's light-curve maximum and the time of full planetary phase, and for some sets of orbital parameters, this light-curve maximum can be a steeply increasing function of eccentricity. We investigate the detectability of EGPs by proposed space-based direct-imaging instruments.

Original languageEnglish (US)
Pages (from-to)520-533
Number of pages14
JournalAstrophysical Journal
Volume627
Issue number1 I
DOIs
StatePublished - Jul 1 2005

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light curve
planets
planet
curves
wavelength
eccentricity
wavelengths
orbits
elliptical orbits
orbitals
eccentric orbits
orbital elements
circular orbits
elongation
inclination
condensation
particle size
color
atmospheres
stars

Keywords

  • Binaries: general
  • Planetary systems
  • Planets and satellites: general
  • Radiative transfer

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Phase functions and light curves of wide-separation extrasolar giant planets. / Sudarsky, David; Burrows, Adam; Hubeny, Ivan -; Li, Aigen.

In: Astrophysical Journal, Vol. 627, No. 1 I, 01.07.2005, p. 520-533.

Research output: Contribution to journalArticle

Sudarsky, David ; Burrows, Adam ; Hubeny, Ivan - ; Li, Aigen. / Phase functions and light curves of wide-separation extrasolar giant planets. In: Astrophysical Journal. 2005 ; Vol. 627, No. 1 I. pp. 520-533.
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