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A radiative-convective equilibrium model for young giant exoplanets: Application to β Pictoris b

  • Jean-Loup Baudino (a1), Bruno Bézard (a1), Anthony Boccaletti (a1), Mickael Bonnefoy (a2) and Anne-Marie Lagrange (a3)...

Abstract

We present a radiative-convective equilibrium model for young giant exoplanets. Model predictions are compared with the existing photometric measurements of the planet β Pictoris b in the J, H, Ks, L', NB 4.05, M' bands. This model will be used to interpret future photometric and spectroscopic observations of exoplanets with SPHERE, mounted at the VLT with a first light expected mid-2014.

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Bonnefoy, M., Boccaletti, A., Lagrange, A.-M., Allard, F., Mordasini, C., Beust, H., Chauvin, G., Girard, J. H. V., Homeier, D., Apai, D., Lacour, S., & Rouan, D. 2013, A&A, 555, 107
Lodders, K. 2010, Solar system abundances of the elements, Lecture Notes of the Kodai School, 379–417
Mordasini, C., Alibert, Y., Georgy, C., Dittkrist, K.-M., Klahr, H., & Henning, T. 2012, A&A, 547, A112
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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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