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Plausible parent bodies for enstatite chondrites and mesosiderites: Implications for Lutetia's fly-by
DOI: 10.1016/j.icarus.2009.03.016 Bibcode: 2009Icar..202..477V

Fulchignoni, M.; Vernazza, P.; Strazzulla, G. +4 more

We present new irradiation experiments performed on the enstatite chondrite Eagle (EL6) and the mesosiderite Vaca Muerta. These experiments were performed with the aims of (a) quantifying the spectral effect of the solar wind on their parent asteroid surfaces and (b) identifying their parent bodies within the asteroid belt. For Vaca Muerta we obse…

2009 Icarus
Rosetta 76
Fully 3-dimensional calculations of dust mantle formation for a model of Comet 67P/Churyumov-Gerasimenko
DOI: 10.1016/j.icarus.2009.01.028 Bibcode: 2009Icar..201..740R

Rosenberg, Eric D.; Prialnik, Dina

A fully 3-dimensional implicit numerical model for comet nucleus evolution is presented, emphasizing dust mantle formation. A spherical configuration is considered with an initial composition of amorphous H 2O ice and dust, taking into account a discrete dust-grain size distribution. The model is applied to Comet 67P/Churyumov-Gerasimen…

2009 Icarus
Rosetta 27
No satellites detected around 21 Lutetia
DOI: 10.1016/j.icarus.2009.06.025 Bibcode: 2009Icar..203..681B

Kulkarni, Shrinivas R.; Busch, Michael W.; Conrad, Al

The Asteroid 21 Lutetia is the target of a flyby by the Rosetta spacecraft in mid-2010. We observed Lutetia with the Keck adaptive-optics system, and searched for satellites. We find none, to a flux limit of 1/350 (Δ-mag = 6.4), corresponding to a size limit of roughly 6 km, at a separation of 0.15″ (3 primary radii or 0.006 Hill radii).

2009 Icarus
Rosetta 4