Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during ``Rosetta'' mission

Details Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during ``Rosetta'' mission Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during ``Rosetta'' mission

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003adspr..31.2501b&link_type=abstract

Advances in Space Research, Volume 31, Issue 12, p. 2501-2510.

Computer Science

1

Scientific paper

The work we present deals with the spectrometric measurements of VIRTIS instrument of the Comet P/Wirtanen planned for the Rosetta mission. This spectrometer can monitor (VIRTIS M channel: 0.250μm - 0.980μm Δκ=20cm-1 0.980 - 5.0 μm Δκ = 5cm-1 VIRTIS H channel: 2.0 μm - 5.0 μm Δκ=2cm-1) the nucleus and the coma in order to provide a general picture of coma's composition, the production of gas and dust, the relationship of coma production to surface composition and the structure and variation of mineralogy of the nucleus surface. During the mission the observation conditions of the spectroscopic investigation change due to different relative positions spacecraft/comet, and to the different illumination conditions of the surface at various distances of the comet to the Sun. The nucleus surface is continuously modified by the ice sublimation accompanied by gas and dust emission. Consequently the surface also its spectrophotometric properties changes and their monitoring can give a new insight. The important role of simulations is to predict the results of measurements in various experimental condition what, in the future, can help in interpretation of the measured data.
In this paper the first results of our simulation the radiance from the comet in the 0.25-5.0μm spectral range at two distances from the Sun (~1AU and ~3AU) are shown. The distance between the Rosetta orbiter and the nucleus surface as well as the sun zenith angles are taken into account according to the Rosetta mission phases. In fact the surface and coma properties vary along the comet orbit, and should be taken into account in our calculations. The optical parameters of the dust on the surface (e.g. reflectance) and in the coma (e.g. Qext) were calculated from optical constants of possible comet analogues. The thermodynamic parameters of the comet are taken from the models of comet evolution. Through this kind of modelling it is possible to identify the surface characteristics in spectra of the radiation from the surface of nucleus transmitted through the coma loaded with dust and gases.
Even if the ``Rosetta mission'' is postponed, with the consequence of a target change, we think that our idea and the method used for the simulations can be useful also for the new Rosetta target - the comet 67P/Churyumov Gerasimenko.

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