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I guees we will have to wait until 2008<br /><br />b) The New Horizons mission to Pluto <br />On 19 Jan 2006 the New Horizons mission to Pluto and the Kuiper Belt was launched from Cape <br />Canaveral. Although it was not designed for precision tracking, it might be able to yield useful <br />information. <br />The first problem will be the on-board heat systematics. The large RTG is mounted on the side <br />of the craft, and produced ~4,500 W of heat at launch. A rough calculation shows that a <br />systematic of ~20 cm/s2 or larger will be produced. Since the post-launch modeling of heat <br />systematics is notoriously difficult, this makes this systematic an important problem to <br />overcome. <br /> <br /> Technically it is along the vector sum of the spacecraft velocity and the dark matter’s change in velocity.<br />A saving grace may be that soon after launch a 180 degree “Earth acquisition manoeuvre” <br />rotation was performed, to aim the main antenna at the Earth. The difference in the Doppler shift <br />immediately before and after the rotation can in principle yield a difference measurement of the <br />heat acceleration which would be pointed first in one direction and then in the opposite. But a <br />determination may be difficult because of the high solar radiation pressure (which will vary <br />somewhat in the two orientations) and the relatively small data set before the manoeuvre. <br />More gratifyingly, New Horizons will be in spin-stabilization mode for about the six months <br />before the Jupiter observing period (January-June, 2007, with encounter on 28 Feb. 2007). It <br />also will be spin-stabilized for much of the period after June 2007 until soon before the Pluto <br />encounter on 14 July 2015. This is designed to save fuel so it can be used to aim later at a <br />Kuiper Belt Object. With luck the Doppler and range data from these periods will supply a test, <br />at some level, of the Pioneer