A dataset provided by the European Space Agency

Name OT2_elellouc_2
Title Pluto.s seasonal evolution and surface thermal properties
URL

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DOI 10.5270/esa-q84b3t4
Author lellouch, e.
Description In 2015, Pluto and its system of satellites will be explored by the New Horizons space mission. Pluto is the most prominent representative of large Kuiper-belt objects with volatile ices (N2, CH4, CO) on their surfaces. Due to its elliptic orbit and strong polar inclination, the large seasonal and spatial variability of the insolation is expected to drive global scale transport of the volatile ices, whose thermal balance determines the atmospheric state. Recent observations of Pluto of various kinds have revealed that it is undergoing seasonal evolution, with changes in its atmosphere, surface spectrum, and thermal emission. In particular, Spitzer observations over 2004-2007 indicated a surprising dimming of the dwarf planet at thermal wavelengths, most probably associated with extension of the coldest, N2-ice dominated, regions. We propose to measure the thermal lightcurve of the Pluto-Charon system (i.e. the rotational variation of its thermal emission) with PACS and SPIRE in order to (i) assess the changes in the ice distribution (ii) determine the emissivities (spectral and bolometric) of Pluto.s different terrains (iii) determine their thermal inertia on seasonal timescales. These parameters are needed to constrain volatile transport and general circulation models, and to put the upcoming New Horizons measurements in a broader, time-evolving, perspective.
Publication The long-wavelength thermal emission of the Pluto-Charon system from Herschel observations. Evidence for emissivity effects . Lellouch E. et al. . Astronomy & Astrophysics, Volume 588, id.A2, 15 pp. . 588 . 10.1051\/0004-6361\/201527675 . 2016A&A...588A...2L ,
The subsurface of Pluto from submillimetre observations . Greaves J. S. et al. . Monthly Notices of the Royal Astronomical Society: Letters, Volume 449, Issue 1, p.L82-L85 . 449 . 10.1093\/mnrasl\/slv016 . 2015MNRAS.449L..82G ,
Instrument PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small, SPIRE_SpirePhoto_large
Temporal Coverage 2012-02-29T20:08:23Z/2012-04-12T01:13:39Z
Version SPG v14.2.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2012-10-12T00:22:04Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-10-12T00:22:04Z, OT2_elellouc_2, SPG v14.2.0. https://doi.org/10.5270/esa-q84b3t4