Palermo Technical Impact Hazard Scale

Historic Palermo Ratings
(these objects have since dropped below −2)
Asteroid Palermo
rating
Background
risk
99942 Apophis 1.10 12.6x greater
(89959) 2002 NT7 0.18 1.51x greater
(29075) 1950 DA 0.17 1.48x greater
background risk 0 equal
(144898) 2004 VD17 −0.25 1.78x less
(410777) 2009 FD −0.44 2.75x less
2022 AE1 −0.66 4.57x less
2023 GQ2 −0.70 5.01x less
2013 TV135 −0.73 5.37x less
(367789) 2011 AG5 −1.00 10x less

The Palermo Technical Impact Hazard Scale is a logarithmic scale used by astronomers to rate the potential hazard of impact of a near-Earth object (NEO). It combines two types of dataprobability of impact and estimated kinetic yield—into a single "hazard" value. A rating of 0 means the hazard is equivalent to the background hazard (defined as the average risk posed by objects of the same size or larger over the years until the date of the potential impact).[1] A rating of +2 would indicate the hazard is 100 times as great as a random background event. Scale values less than −2 reflect events for which there are no likely consequences, while Palermo Scale values between −2 and 0 indicate situations that merit careful monitoring. A similar but less complex scale is the Torino Scale, which is used for simpler descriptions in the non-scientific media.

As of May 2024,[2] one asteroid has a cumulative Palermo Scale value above −2: 101955 Bennu (−1.41). Six have cumulative Palermo Scale values between −2 and −3: (29075) 1950 DA (−2.05), 2007 FT3 (−2.63), 1979 XB (−2.71), 2000 SG344 (−2.78), 2008 JL3 (−2.86), and 2010 RF12 (−2.98). Of those that have a cumulative Palermo Scale value between −3 and −4, one was discovered in 2024: 2024 BY15 (−3.30).

  1. ^ Cite error: The named reference palermo was invoked but never defined (see the help page).
  2. ^ "Sentry: Earth Impact Monitoring - Impact Risk Data". Jet Propulsion Laboratory. Retrieved 2 May 2024. Use Unconstrained Settings, sort by Palermo Scale (cum.)

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