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  <title><![CDATA[MS Defense by Michela Mancini]]></title>
  <body><![CDATA[<p>Michela Mancini<br />
(Advisor: Dr. John A. Christian] will defend a master&rsquo;s thesis entitled,<br />
An analysis on the application of algebraic geometry in initial orbit<br />
determination problems<br />
On<br />
Wednesday, November 16 at 10:30 a.m.<br />
Weber 200</p>

<p><br />
Abstract<br />
Initial Orbit Determination (IOD) is a classical problem in astrodynamics. The space around Earth&nbsp;<br />
is crowded by a great many objects whose orbits are unknown, and the number of space debris is&nbsp;<br />
constantly increasing because of break-up events and collisions. Reconstructing the orbit of a body&nbsp;<br />
from observations allows us to create catalogs that are used to avoid collisions and program&nbsp;<br />
missions for debris removal. Also, comparing the observations of celestial bodies with predictions&nbsp;<br />
of their positions made on the basis of our knowledge of the universe has been in the past, and is&nbsp;<br />
still today, one of the most effective means to make improvements in our cosmological model.<br />
In this work, a purely geometric solution to the angles-only IOD problem is analyzed and its&nbsp;<br />
performance under various scenarios of observations is tested. The problem formulation is based on&nbsp;<br />
a re- parameterization of the orbit as a disk quadric, and relating the observations to the&nbsp;<br />
unknowns leads to a polynomial system that can be solved using tools from numerical algebraic&nbsp;<br />
geometry. This method is time-free and does not require any type of initialization. This makes it&nbsp;<br />
unaffected by the problems related to the use of time that usually must be accounted for to improve&nbsp;<br />
the accuracy of the solution.<br />
A similar approach may be used to analyze the performance of the solver when streaks are used,&nbsp;<br />
together with lines of sight, as inputs to the problem. Streaks on digital images form, together&nbsp;<br />
with the camera location, planes that are tangent to the orbit. This produces two different types&nbsp;<br />
of constraint that can be imposed, and also in this case a polynomial system is obtained. The&nbsp;<br />
accuracy and the robustness of the solver are decreased by the presence of streaks, but they remain&nbsp;<br />
a valid input when diversity in the observed directions guarantees the departure from the singular&nbsp;<br />
configuration of almost coplanar observations.<br />
Committee<br />
&bull; &nbsp;Dr. John A. Christian &ndash; School of Aerospace Engineering (advisor)<br />
&bull; &nbsp;Dr. Brian C. Gunter&ndash; School of Aerospace Engineering<br />
&bull; &nbsp;Dr. Anton Leykin &ndash; School of Mathematics<br />
&nbsp;</p>
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