Main Page | See live article | Alphabetical index 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. 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 as likely as 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 more likely than a random background event. A similar but less complex scale is the Torino scale, which is used for simpler descriptions in the non-scientific media. The Palermo Scale value, P, is defined as the base 10 logarithm of the ratio of the impact probability pi to the background impact probability over the time T to the event: The annual background impact frequency is defined for this purpose as: where the energy threshold E is measured in megatons. The near-Earth object 2002 NT7 was the first near-Earth object detected by NASA's latest NEO programme to be given a positive rating on the scale of 0.06, indicating a higher than background threat. The value was subsequently lowered to -0.25 after more measurements were taken. However, asteroid 1950 DA holds the record for Palermo scale values, with a value of 0.17 for a possible collision in the year 2880. See also: Torino scale, Near-Earth object External Links NASA NEO Programme http://neo.jpl.nasa.gov/index.html Description of the scale http://neo.jpl.nasa.gov/risk/doc/palermo.html 2002 NT7 is the first object discovered with a positive measurement on the Palermo scale This article is from Wikipedia. All text is available under the terms of the GNU Free Documentation License.