Uncertainty parameter

Orbital uncertainty is related to several parameters used in the orbit determination process including the number of observations (measurements), the time spanned by those observations (observation arc), the quality of the observations (e.g. radar vs. optical), and the geometry of the observations. Of these parameters, the time spanned by the observations generally has the greatest effect on the orbital uncertainty.[7]

As an extreme example, 2010 GZ60 has an uncertainty parameter of 9; it could be an Earth threatening asteroid, or may always remain beyond the asteroid belt.

Occasionally, the Minor Planet Center substitutes a letter-code (‘D’, ‘E’, ‘F’) for the uncertainty parameter. Objects such as 1995 SN55 with a condition code ‘E’ in the place of a numeric uncertainty parameter denotes orbits for which the listed eccentricity was assumed, rather than determined;[8] these are considered lost. Objects with a ‘D’ have only been observed for a single opposition, and have been assigned two (or more) different designations ("double"); objects with an ‘F’ fall in both categories ‘D’ and ‘E’.[8]

The U parameter is calculated in two steps.[2][9] First the in-orbit longitude runoff ${\displaystyle r}$ in seconds of arc per decade is calculated, (i.e. the discrepancy between the observed and calculated position extrapolated over ten years):

${\displaystyle r=\left(\Delta \tau \cdot e+10\cdot {\frac {\Delta P}{P}}\right)\cdot 3600\cdot 3\cdot {\frac {k_{o}}{P}}}$

with

${\displaystyle \Delta \tau }$	uncertainty in the perihelion time in days
${\displaystyle e}$	eccentricity of the determined orbit
${\displaystyle P}$	orbital period in years
${\displaystyle \Delta P}$	uncertainty in the orbital period in days
${\displaystyle k_{o}}$	${\displaystyle 0.01720209895\cdot {\frac {180^{\circ }}{\pi }}}$, Gaussian gravitational constant, converted to degrees

Then, the obtained in-orbit longitude runoff is converted to the "uncertainty parameter" U, which is an integer between 0 and 9. The calculated number can be less than 0 or more than 9, but in those cases either 0 or 9 is used instead. For instance: As of 10 September 2016, Ceres technically has an uncertainty of around −2.6, but is instead displayed as the minimal 0. The formula for cutting off the calculated value of U is

${\displaystyle U=\min \left(9,\max \left(0,\left\lfloor 9\cdot {\frac {\log r}{\log 648{,}000}}\right\rfloor +1\right)\right)}$

648 000 is the number of arc seconds in a half circle, so a value greater than 9 would mean that we would have basically no idea where the object will be in 10 years.

Function graph U(r)