The Impact Risk page lists a number of
lost minor planets that are, for all practical purposes, permanent residents of the risk page; their removal may depend upon a
serendipitous rediscovery. is the asteroid with greatest probability (10%) of impacting Earth, but is only ~7 meters in diameter. The only
numbered objects with
observation arcs of several years are
(29075) 1950 DA and
101955 Bennu. The diameter of most near-Earth asteroids that have not been studied by
radar or
infrared can generally only be estimated within about a factor of 2 based on the asteroid's
absolute magnitude (H). Their mass, consequently, is uncertain by about a factor of 10. For near-Earth asteroids without a well-determined diameter, Sentry assumes a generic
albedo of 0.15. In August 2013, the Sentry Risk Table started using planetary
ephemeris (
DE431) for all NEO orbit determinations. DE431 (
JPL small-body perturber ephemeris: SB431-BIG16) better models the gravitational
perturbations of the planets and includes the 16 most massive
main-belt asteroids. In April 2021, Sentry transitioned to
DE441 which removed the very low impact probability of short-arc
2014 MV67 which had been less than 1:1-billion. The switch to DE441 also briefly added in the harmless Jupiter trojan
2014 ES57 with a very low impact probability of about 1:1-billion. JPL launched major changes to the website in February 2017 and re-directed the classic page on 10 April 2017. In 2021 JPL launched Sentry-II which handles the
Yarkovsky effect that can significantly change a small asteroid's path over decades and centuries. Sentry-II defaults to an impact pseudo-observation (IOBS) analysis technique that runs an extended orbit-determination filter that tries to converge to an impacting solution compatible with the observational data. == Numbers ==