Characterizing Super-Mercuries by their infrared orbital photometry
| hal.structure.identifier | SSE 2012 | |
| dc.contributor.author | MAURIN, A. S. | |
| hal.structure.identifier | SSE 2012 | |
| dc.contributor.author | SELSIS, Franck | |
| hal.structure.identifier | SSE 2012 | |
| dc.contributor.author | HERSANT, F. | |
| hal.structure.identifier | SSE 2012 | |
| dc.contributor.author | BELU, A. R. | |
| hal.structure.identifier | SSE 2012 | |
| dc.contributor.author | RAYMOND, Sean N. | |
| hal.structure.identifier | Laboratoire de Météorologie Dynamique (UMR 8539) [LMD] | |
| dc.contributor.author | LECONTE, J. | |
| hal.structure.identifier | Joseph Louis LAGRANGE [LAGRANGE] | |
| dc.contributor.author | DELBO, M. | |
| dc.date.issued | 2012-09 | |
| dc.date.conference | 2012 | |
| dc.description.abstractEn | The photometric signal we receive from a star hosting a planet is modulated by the variation of the planet signal with its orbital phase. Already observed for giant exoplanets, those thermal phase curves should be measured with future telescopes (JWST and EChO) for hot rocky Super-Earths in transiting and nontransiting configurations. The nontransiting ones are the most numerous. We show here that we can infer from the thermal phase curve of a synchronous rocky airless exoplanet its radius, Bond albedo and the inclination of the orbit. When the orbit is eccentric, the planetary rotational period can be determined from the infrared photometric monitoring. Furthermore, the tidal dissipation within the planet can be constrained, that can allow us to improve tidal models. | |
| dc.language.iso | en | |
| dc.source.title | European Planetary Science Congress 2012, held 23-28 September, 2012 in Madrid, Spain. | |
| dc.title.en | Characterizing Super-Mercuries by their infrared orbital photometry | |
| dc.type | Communication dans un congrès | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
| bordeaux.journal | EPSC | |
| bordeaux.page | 500 | |
| bordeaux.conference.title | - | |
| bordeaux.country | ES | |
| bordeaux.title.proceeding | European Planetary Science Congress 2012, held 23-28 September, 2012 in Madrid, Spain. | |
| bordeaux.conference.city | Madrid | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00811181 | |
| hal.version | 1 | |
| hal.invited | non | |
| hal.proceedings | oui | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00811181v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=European%20Planetary%20Science%20Congress%202012,%20held%2023-28%20September,%202012%20in%20Madrid,%20Spain.&rft.jtitle=EPSC&rft.date=2012-09&rft.spage=500&rft.epage=500&rft.au=MAURIN,%20A.%20S.&SELSIS,%20Franck&HERSANT,%20F.&BELU,%20A.%20R.&RAYMOND,%20Sean%20N.&rft.genre=unknown |
Fichier(s) constituant ce document
| Fichiers | Taille | Format | Vue |
|---|---|---|---|
|
Il n'y a pas de fichiers associés à ce document. |
|||