G
T
Last name: GUILLOT
First name: T.
Physica Scripta Volume T, 130, p. 4023, http://dx.doi.org./10.1088/0031-8949//t130/014023
Annual Review of Earth and Planetary Sciences, 33, pp. 493-530, http://dx.doi.org./10.1146/annurev.earth.32.101802.120325
Physica Scripta Volume T, 130, p. 4023, http://dx.doi.org./10.1088/0031-8949//t130/014023
Astronomy and Astrophysics, 500, pp. 561-562 (2009)
International audience
Astrophysics and Space Science, 298, pp. 135-140, http://dx.doi.org./10.1007/s10509-005-3923-3
Planetary and Space Science, 57, pp. 816-821 (2009)
International audience
Astronomy and Astrophysics, 504, pp. 605-615 (2009)
Astrophysical Journal, 686, pp. 1292-1301, http://dx.doi.org./10.1086/591903
We present a time-dependent radiative model of the atmosphere of HD 209458b and investigate its thermal structure and chemical composition. In a first step, the stellar heating profile and radiative timescales were calculated under planetaveraged insolation conditions. We find that 99.99% of the incoming stellar flux has been absorbed before...
After publication of Miguel et al. (2016), we found an error in the calculation of Jupiter internal structure when using REOS3b-H and REOS3sc-H equations of state (EOSs). The lowest pressure in those tables (see appendix in Miguel et al. 2016) was P = 31.623 bars, while our calculations of Jupiter's internal structure started at P = 1 bar. This...
Aims. In this work we generalize the notion of convective inhibition to apply it to cases where there is an infinite reservoir of condensible species (i.e., an ocean). We propose a new model for the internal structure and thermal evolution of super-Earths with hydrogen envelopes. Methods. We derive the criterion for convective inhibition in a...
Astronomy and Astrophysics, 516, p. id.A20 (2010)
The formation of planetesimals is expected to occur via particle-gas instabilities that concentrate dust into self-gravitating clumps. Triggering these instabilities requires the prior pile-up of dust in the protoplanetary disk. This has been successfully modelled exclusively at the disk's snowline, whereas rocky planetesimals in the inner disk...
International audience
International audience
International audience
Astronomy and Astrophysics, 501, pp. L23-L26 (2009)
Space exploration and ground-based observations have provided outstanding evidence of the diversity and the complexity of the outer solar system. This work presents our current understanding of the nature and distribution of water and water-rich materials from the water snow line to the Kuiper Belt. This synthesis is timely, since a thorough...
International audience
International audience
International audience
International audience