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Transit Confirmation and Improved Stellar and Planet Parameters for the Super-Earth HD 97658 b and its Host Star

Author(s): Van Grootel, V; Gillon, M; Valencia, D; Madhusudhan, N; Dragomir, D; et al

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dc.contributor.authorVan Grootel, V-
dc.contributor.authorGillon, M-
dc.contributor.authorValencia, D-
dc.contributor.authorMadhusudhan, N-
dc.contributor.authorDragomir, D-
dc.contributor.authorHowe, AR-
dc.contributor.authorBurrows, Adam S-
dc.contributor.authorDemory, B-O-
dc.contributor.authorDeming, D-
dc.contributor.authorEhrenreich, D-
dc.contributor.authorLovis, C-
dc.contributor.authorMayor, M-
dc.contributor.authorPepe, F-
dc.contributor.authorQueloz, D-
dc.contributor.authorScuflaire, R-
dc.contributor.authorSeager, S-
dc.contributor.authorSegransan, D-
dc.contributor.authorUdry, S-
dc.date.accessioned2019-04-10T19:30:52Z-
dc.date.available2019-04-10T19:30:52Z-
dc.date.issued2014-05-01en_US
dc.identifier.citationVan Grootel, V, Gillon, M, Valencia, D, Madhusudhan, N, Dragomir, D, Howe, AR, Burrows, AS, Demory, B-O, Deming, D, Ehrenreich, D, Lovis, C, Mayor, M, Pepe, F, Queloz, D, Scuflaire, R, Seager, S, Segransan, D, Udry, S. (2014). Transit Confirmation and Improved Stellar and Planet Parameters for the Super-Earth HD 97658 b and its Host Star. apj, 786 (2 - 2. doi:10.1088/0004-637X/786/1/2en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr13q5s-
dc.description.abstractSuper-Earths transiting nearby bright stars are key objects that simultaneously allow for accurate measurements of both their mass and radius, providing essential constraints on their internal composition. We present here the confirmation, based on Spitzer transit observations, that the super-Earth HD 97658 b transits its host star. HD 97658is a low-mass (M∗=0.77±0.05M ) K1 dwarf, as determined from the Hipparcos parallax and stellar evolution modeling. To constrain the planet parameters, we carry out Bayesian global analyses of Keck–High Resolution Echelle Spectrometer (Keck-HIRES) radial velocities and Microvariability and Oscillations of STars (MOST) and Spitze rphotometry. HD 97658 b is a massive (MP=7.55+0.83−0.79M⊕) and large (RP=2.247+0.098−0.095R⊕at 4.5μm) super-Earth. We investigate the possible internal compositions for HD 97658 b. Our results indicate a large rocky component, of at least 60% by mass, and very little H–He components, at most 2% by mass. We also discuss how future asteroseismic observations can improve the knowledge of the HD 97658 system, in particular by constraining its age. Orbiting a bright host star, HD 97658 b will be a key target for upcoming space missions such as the Transiting Exoplanet Survey Satellite (TESS), the Characterizing Exoplanet Satellite (CHEOPS), the Planetary Transits and Oscillations of stars (PLATO), and the James Webb Space Telescope to characterize thoroughly its structure and atmosphere.en_US
dc.language.isoen_USen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.rightsFinal published version. This is an open access article.en_US
dc.titleTransit Confirmation and Improved Stellar and Planet Parameters for the Super-Earth HD 97658 b and its Host Staren_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1088/0004-637X/786/1/2-
dc.date.eissued2014-04-08en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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