EFFICIENCY OF NEW METHODS FOR ESTIMATING ORBITS OF UNKNOWN NEAREARTH SPACE OBJECTS USING SHORT OPTICAL TRACKS OBTAINED OVER A FEW WEEKS INTERVAL
The work on a representative array of data demonstrates the capabilities of a new, essentially non‑linear algorithm for estimating the orbital parameters of near‑Earth space objects on several short optical tracks separated by long time pauses. The analysis of the work of the algorithm was carried out for five space objects moving in different orbits, including circular, high‑elliptical and low‑orbit with deceleration in the atmosphere and without it. When obtaining estimates of the parameters of the orbits, a priori information was not used. In all the experiments performed, including for very short tracks separated by a long pause in the observations, the minimum possible values of the quality criterion were achieved. The algorithm does not require large computing power – the calculation of the orbit on two tracks on a portable personal computer takes a split second.