  When new objects are detected in the sky, an orbit determination needs to be
performed immediately to find out their origin, to determine the probability of
an Earth impact and possibly also to estimate the impact region on Earth. ESA's
Flyeye telescope is expected to revolutionize the effort of predicting
potential asteroid or deep space debris impact hazards due to the expected
increase of near-Earth object discoveries. As the observed orbit arc for such
an object is very short, classical Gaussian orbit determination cannot be used.
We adopt the systematic ranging technique to overcome the lack of information
and predict a region of the sky where the body can most likely be found. We
also provide a detection probability for follow-up observations and investigate
potential follow-up telescopes for the Flyeye telescope.
