Computer modelling of a penetrator thermal sensor

The Philae lander is part of the Rosetta mission to investigate comet 67P/Churyumov-Gerasimenko. It will use a harpoon like device to anchor itself onto the surface. The anchor will perhaps reach depths of 1–2 m. In the anchor is a temperature sensor that will measure the boundary temperature as part of the MUPUS experiment. As the anchor attains thermal equilibrium with the comet ice it may be possible to extract the thermal properties of the surrounding ice, such as the thermal diffusivity, by using the temperature sensor data. The anchor is not an optimal shape for a thermal probe and application of analytical solutions to the heat equation is inappropriate. We prepare a numerical model to fit temperature sensor data and extract the thermal diffusivity. Penetrator probes mechanically compact the material immediately surrounding them as they enter the target. If the thermal properties, composition and dimensions of the penetrator are known, then the thermal properties of this pristine material may be recovered although this will be a challenging measurement. We report on investigations, using a numerical thermal model, to simulate a variety of scenarios that the anchor may encounter and how they will affect the measurement.

[1]  A. Coradini,et al.  Numerical simulations of the radiance from the comet 46P/Wirtanen in the various configurations of the measurements during “Rosetta” mission , 2003 .

[2]  Grant Heiken,et al.  Book-Review - Lunar Sourcebook - a User's Guide to the Moon , 1991 .

[3]  Günter Kargl,et al.  Determination of physical properties of planetary sub-surface layers by artificial impacts and penetrometry , 2001 .

[4]  T. Hyde,et al.  Charging in a dusty plasma , 1997 .

[5]  E. Marquardt,et al.  Cryogenic Material Properties Database , 2002 .

[6]  M. Nolan,et al.  Radar observations of Comet 2P/Encke during the 2003 apparition , 2004 .

[7]  Tetsuo Yamamoto,et al.  Thermal conductivity of granular materials relevant to the thermal evolution of cometary nuclei , 1997 .

[8]  F. Agblevor,et al.  A Thermistor Based Method for Measurement of Thermal Conductivity and Thermal Diffusivity of Moist Food Materials at High Temperatures , 1997 .

[9]  T. Keller,et al.  Theoretical aspects and interpretation of thermal measurements concerning the subsurface investigation of a cometary nucleus , 2002 .

[10]  J. Biele,et al.  The Rosetta Lander (“Philae”) Investigations , 2007 .

[11]  M. L. Urquhart,et al.  Estimation of Soil Thermal Conductivity from a Mars Microprobe-type Penetrator , 2000 .

[12]  H. Kochan,et al.  Laboratory Studies on Cometary Crust Formation: The Importance of Sintering , 1991 .

[13]  M. Banaszkiewicz,et al.  Mupus – A Thermal and Mechanical Properties Probe for the Rosetta Lander Philae , 2007 .

[14]  T. Spohn,et al.  A heat flow and physical properties package for the surface of Mercury , 2001 .

[15]  H. Melosh,et al.  Deep Impact: Excavating Comet Tempel 1 , 2005, Science.

[16]  S. Szutowicz,et al.  Comet 46P/Wirtanen: Evolution of the subsurface layer , 1998 .

[17]  J. Klinger Some consequences of a phase transition of water ice on the heat balance of comet nuclei , 1981 .

[18]  Thomas M Truskett,et al.  Is random close packing of spheres well defined? , 2000, Physical review letters.

[19]  K. Glassmeier,et al.  The Rosetta Mission: Flying Towards the Origin of the Solar System , 2007 .

[20]  K. Seiferlin The guarded torus: numerical model of a novel transient method for thermal conductivity measurements , 2006 .

[21]  S. Patankar Numerical Heat Transfer and Fluid Flow , 2018, Lecture Notes in Mechanical Engineering.

[22]  Andrew J. Ball,et al.  Penetrometry in the solar system , 1999 .

[23]  T. Ahrens,et al.  An instrument for in situ comet nucleus surface density profile measurement by gamma ray attenuation , 2001 .

[24]  Tilman Spohn,et al.  Line heat-source measurements of the thermal conductivity of porous H2O ice, CO2 ice and mineral powders under space conditions , 1996 .

[25]  E. C. Bullard,et al.  The flow of heat through the floor of the Atlantic Ocean , 1954, Proceedings of the Royal Society of London. Series A. Mathematical and Physical Sciences.

[26]  M. Kaasalainen,et al.  A Portrait of the Nucleus of Comet 67P/Churyumov-Gerasimenko , 2007 .