The browser you are using is not supported by this website. All versions of Internet Explorer are no longer supported, either by us or Microsoft (read more here: https://www.microsoft.com/en-us/microsoft-365/windows/end-of-ie-support).

Please use a modern browser to fully experience our website, such as the newest versions of Edge, Chrome, Firefox or Safari etc.

Lego Figure holding a lego telescope. Photo

Jens Hoeijmakers

ASSOCIATE SENIOR LECTURER

Lego Figure holding a lego telescope. Photo

Physically-motivated basis functions for temperature maps of exoplanets

Author

  • Brett M. Morris
  • Kevin Heng
  • Kathryn Jones
  • Caroline Piaulet
  • Brice Olivier Demory
  • Daniel Kitzmann
  • H. Jens Hoeijmakers

Summary, in English

Thermal phase curves of exoplanet atmospheres have revealed temperature maps as a function of planetary longitude, often by sinusoidal decomposition of the phase curve. We construct a framework for describing two-dimensional temperature maps of exoplanets with mathematical basis functions derived for a fluid layer on a rotating, heated sphere with drag/friction, which are generalisations of spherical harmonics. These basis functions naturally produce physically-motivated temperature maps for exoplanets with few free parameters. We investigate best practices for applying this framework to temperature maps of hot Jupiters by splitting the problem into two parts: (1) we constrain the temperature map as a function of latitude by tuning the basis functions to reproduce general circulation model outputs, since disk-integrated phase curve observations do not constrain this dimension; and (2) we infer the temperature maps of real hot Jupiters using original reductions of several Spitzer phase curves, which directly constrain the temperature variations with longitude. The resulting phase curves can be described with only three free parameters per bandpass an efficiency improvement over the usual five or so used to describe sinusoidal decompositions of phase curves. Upon obtaining the hemispherically averaged day side and night side temperatures, the standard approach would be to use zero-dimensional box models to infer the Bond albedo and redistribution efficiency. We elucidate the limitation of these box models by demonstrating that negative Bond albedos may be obtained due to a choice of boundary condition on the night side temperature. We propose generalized definitions for the Bond albedo and heat redistribution efficiency for use with two-dimensional (2D) temperature maps. Open-source software called kelp is provided to efficiently compute the 2D temperature maps, phase curves, albedos and redistribution efficiencies.

Department/s

  • Lund Observatory - Undergoing reorganization
  • Astrophysics

Publishing year

2022-04

Language

English

Publication/Series

Astronomy and Astrophysics

Volume

660

Document type

Journal article

Publisher

EDP Sciences

Topic

  • Astronomy, Astrophysics and Cosmology

Keywords

  • Methods: analytical
  • Methods: observational
  • Planets and satellites: atmospheres
  • Planets and satellites: gaseous planets
  • Radio continuum: planetary systems
  • Techniques: photometric

Status

Published

ISBN/ISSN/Other

  • ISSN: 0004-6361