| 1.10 | 12.6x greater | ||
| 0.18 | 1.51x greater | ||
| 0.17 | 1.48x greater | ||
| background risk | 0 | equal | |
| −0.25 | 1.78x less | ||
| −0.44 | 2.75x less | ||
| −0.66 | 4.57x less | ||
| −0.70 | 5.01x less | ||
| −0.73 | 5.37x less | ||
| −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 data - probability 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). 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,[1] 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), (−2.63), 1979 XB (−2.71), (−2.78), (−2.86), and (−2.98). Of those that have a cumulative Palermo Scale value between −3 and −4, one was discovered in 2024: 2024 BY15 (−3.30).
The scale compares the likelihood of the detected potential impact with the average risk posed by objects of the same size or larger over the years until the date of the potential impact. This average risk from random impacts is known as the background risk. The Palermo Scale value, P, is defined by the equation:
P\equivlog10
| pi | |
| fBT |
The background impact frequency is defined for this purpose as:
fB=0.03
| ||||
| E |
yr-1
For instance, this formula implies that the expected value of the time from now until the next impact greater than 1 megatonne is 33 years, and that when it occurs, there is a 50% chance that it will be above 2.4 megatonnes. This formula is only valid over a certain range of E.
However, another paper[2] published in 2002 – the same year as the paper on which the Palermo scale is based – found a power law with different constants:
fB=0.00737E-0.9
This formula gives considerably lower rates for a given E. For instance, it gives the rate for bolides of 10 megatonnes or more (like the Tunguska explosion) as 1 per thousand years, rather than 1 per 210 years as in the Palermo formula. However, the authors give a rather large uncertainty (once in 400 to 1800 years for 10 megatonnes), due in part to uncertainties in determining the energies of the atmospheric impacts that they used in their determination.
In 2002 the near-Earth object reached a positive rating on the scale of 0.18, indicating a higher-than-background threat. The value was subsequently lowered after more measurements were taken. is no longer considered to pose any risk and was removed from the Sentry Risk Table on 1 August 2002.
In September 2002, the highest Palermo rating was that of asteroid (29075) 1950 DA, with a value of 0.17 for a possible collision in the year 2880. By March 2022, the rating had been reduced to −2.0.[3]
For a brief period in late December 2004, with an observation arc of 190 days, asteroid (then known only by its provisional designation) held the record for the highest Palermo scale value, with a value of 1.10 for a possible collision in the year 2029. The 1.10 value indicated that a collision with this object was considered to be almost 12.6[4] times as likely as a random background event: 1 in 37 instead of 1 in 472. With further observation through 2021 there is no risk from Apophis for the next 100+ years.