Palermo Technical Impact Hazard Scale
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).[1] A rating of +2 would indicate the hazard is 100 times greater than 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.
Contents
1 Scale
2 Positive rating
3 See also
4 References
5 External links
Scale
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≡log10pifBT{displaystyle Pequiv log _{10}{frac {p_{i}}{f_{B}T}}}
where
pi is the impact probability
T is the time interval over which pi is considered
fB is the background impact frequency
The background impact frequency is defined for this purpose as:
- fB=3100E−45 yr−1{displaystyle f_{B}={frac {3}{100}}E^{-{frac {4}{5}}}{text{ yr}}^{-1};}
where the energy threshold E is measured in megatons, yr is the unit of T divided by one year.
Positive rating
The near-Earth object (89959) 2002 NT7 was the first near-Earth object detected by NASA's latest NEO program to be given a positive rating on the scale of 0.06,[2] indicating a higher-than-background threat. The value was subsequently lowered after more measurements were taken. 2002 NT7 is no longer considered to pose any risk and was removed from the Sentry Risk Table on 1 August 2002.[3]
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.[4] By December 2015, the rating had been reduced all the way to −1.42.[5]
For a brief period in late December 2004, with an observation arc of 190 days, asteroid (99942) Apophis (then known only by its provisional designation 2004 MN4) held the record for the highest Palermo scale values, with a value of 1.10 for a possible collision in the year 2029.[6] The 1.10 value indicated that a collision with this object was considered to be almost 12.6 times as likely as a random background event: 1 in 37[7] instead of 1 in 472. With further observation through 2016 there is no significant risk from Apophis at any of the dates in question.
See also
- Asteroid deflection strategies
- Impact event
- Torino scale
References
^ "THE PALERMO TECHNICAL IMPACT HAZARD SCALE". NASA/JPL Near-Earth Object Program Office. 31 Aug 2005. Retrieved 2011-10-14..mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}
^ Dr. David Whitehouse (24 July 2002). "Space rock 'on collision course'". BBC News. Retrieved 2007-12-28.
^ "Sentry Risk Table - Removed Objects". NASA/JPL Near-Earth Object Program Office. Retrieved 2006-03-07.
^ "Asteroid 1950 DA". NASA/JPL Near-Earth Object Program Office. Retrieved 2011-10-14.
^ "Sentry: Earth Impact Monitoring: 29075". cneos.jpl.nasa.gov. Retrieved 2017-06-20.
^ Daniel Fischer (Dec 27, 2004). "2004 MN4 Earth Impact Risk Summary (computed on Dec 27, 2004)". The Cosmic Mirror. Archived from the original on 14 March 2005. Retrieved 2011-11-04.
^ "Predicting Apophis' Earth Encounters in 2029 and 2036". NASA/JPL Near-Earth Object Program Office. Retrieved 2007-12-28.
The primary reference for the Palermo Technical Scale is "Quantifying the risk posed by potential Earth impacts" by Chesley et al., Icarus 159, 423-432 (2002).
External links
- Description of the scale
- NASA list of potential impactors
