Uncertainty Parameter U

The uncertainty parameter ''U'' is introduced by the Minor Planet Center (MPC) to quantify the uncertainty of a perturbed orbital solution for a minor planet. The parameter is a logarithmic scale from 0 to 9 that measures the anticipated longitudinal uncertainty in the minor planet's mean anomaly after 10 years. The larger the number, the larger the uncertainty. The uncertainty parameter is also known as condition code in JPL's Small-Body Database Browser. The ''U'' value should not be used as a predictor for the uncertainty in the future motion of near-Earth objects.

Orbital uncertainty

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.

Occasionally, the Minor Planet Center substitutes a letter-code (‘D’, ‘E’, ‘F’) for the uncertainty parameter.
:

Calculation

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

:$r=\left(\Delta\tau\cdot e + 10\cdot\frac\right) \cdot 3600 \cdot 3 \cdot \frac$

with
:

Then, the obtained in-orbit longitude runoff is converted to the "uncertainty parameter" , 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. The formula for cutting off the calculated value of is

:$U=\min \left\$

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 result is the same regardless of the choice of base for the logarithm, so long as the same logarithm is used throughout the formula; e.g. for "" = , , , or the calculated value of remains the same if the logarithm is the same in both places in the formula.

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.

References

{{reflist, 25em, refs=

{{cite web
, title=Orbits for Near Earth Asteroids (NEAs)
, department= Minor Planet Center
, publisher=International Astronomical Union
, url=https://www.minorplanetcenter.net/iau/MPCORB/NEA.txt
, access-date=25 June 2020
, place=
via
{{cite web
, title=M.P. Orbit Format
, department= Minor Planet Center
, publisher=International Astronomical Union
, url=https://www.minorplanetcenter.net/iau/info/MPOrbitFormat.html

{{cite web
, title=2003 UU{{sub, 291
, department= Minor Planet Center
, publisher=International Astronomical Union
, url=http://www.minorplanetcenter.net/db_search/show_object?object_id=2003+UU291

{{cite web
, title=Uncertainty parameter 'U'
, department= Minor Planet Center
, publisher=International Astronomical Union
, url=http://www.minorplanetcenter.org/iau/info/UValue.html
, access-date=2011-11-15 , df=dmy-all

{{cite web
, title=Export format for minor-planet orbits
, department= Minor Planet Center
, publisher=International Astronomical Union
, url=http://www.minorplanetcenter.net/iau/info/MPOrbitFormat.html
, access-date=2016-03-03 , df=dmy-all

{{cite report
, last=Drake , first=Bret G.
, date=2011
, title=Strategic implications of human exploration of near-Earth asteroids
, series=NASA Technical Reports
, publisher=NASA
, id=2011-0020788
, url=https://ntrs.nasa.gov/search.jsp?R=20110020788
, access-date=2016-03-03 , df=dmy-all

{{cite web
, title=Trajectory Browser User Guide
, series=Mission Design Center Trajectory Browser
, publisher=NASA
, department=Ames Research Center
, url=http://trajbrowser.arc.nasa.gov/user_guide.php
, access-date=2016-03-03 , df=dmy-all

{{cite web
, title=Definition / description for SBDB parameter / field: condition code
, department=JPL Solar System Dynamics
, url=http://ssd.jpl.nasa.gov/sbdb_help.cgi?name=condition_code
, access-date=2011-11-15 , df=dmy-all

{{cite web
, date=31 Aug 2005
, title=Near-Earth objects close-approach uncertainties
, publisher=NASA / JPL
, department=JPL Near-Earth Object Program Office
, url=http://neo.jpl.nasa.gov/ca/neo_ca_info.html
, url-status=dead , access-date=2011-11-15
, archive-url=https://web.archive.org/web/20040324140637/http://neo.jpl.nasa.gov/ca/neo_ca_info.html
, archive-date=24 March 2004 , df=dmy-all

{{cite report
, title=Editorial Notice
, series=The Minor Planet Circulars / Minor Planets and Comets
, date=1995-02-15
, id=MPC 24597–24780
, pages=24597
, url=http://www.minorplanetcenter.net/iau/ECS/MPCArchive/1995/MPC_19950215.pdf
, access-date=3 March 2016

{{cite journal
, last1=Desmars , first1=Josselin , last2=Bancelin , first2=David
, last3=Hestroffer , first3=Daniel , last4=Thuillot , first4=William
, date=Jun 2011
, title=Statistical analysis on the uncertainty of asteroid ephemerides
, url=http://hal.upmc.fr/hal-00647644
, editor1-last=Alecian , editor1-first=G. , editor2-last=Belkacem , editor2-first=K.
, editor3-last=Samadi , editor3-first=R. , editor4-last=Valls-Gabaud , editor4-first=D.
, journal=SF2A 2011: Annual Meeting of the French Society of Astronomy and Astrophysics
, pages=639–642
, location=Paris, France
, bibcode=2011sf2a.conf..639D , access-date=3 March 2016

Orbits
Measurement