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Impact Risk for Object (29075) 1950 DA and Object (101955) 1999 RQ36, Update (NASA NEO, edited)

Giuseppe

Emeritus
Impact Risk for Object (29075) 1950 DA and Object (101955) 1999 RQ36, Update (NASA NEO, edited)

[Source: NASA, Near Earth Object Program, Sentry Risk Table, <cite cite="http://neo.jpl.nasa.gov/risk/">Current Impact Risks</cite>. 7/27/10.]

Impact Risk for Object (29075) 1950 DA and Object (101955) 1999 RQ36, Update


  • 2010-Jul-26
    • In some cases, investigations into potential impacts are conducted for more than 100 years into the future. Currently, there are two well-observed objects for which long-term analyses have been carried out.
      1. Asteroid (29075) 1950 DA, has a significant possibility of impact on March 16, 2880. A careful computation of the impact probability, which is less than 0.33%, is challenging because the orientation of its spin pole is poorly known. Giorgini et al. (Science, Vol. 296. no. 5565, pp. 132 - 136, 2002) analyzed this object's motion, which is discussed here (LINK)
      2. The second object, (101955) 1999 RQ36, currently has non-zero impact probabilities on numerous occasions during the years after 2165. This is analyzed in a paper published by Milani et al. (Icarus, Vol. 203, pp. 460-471, 2009), which is available as here: (LINK).
    • Note the Torino Scale is formally undefined for potential impacts more than one century into the future and so not applicable in such cases.
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Re: Impact Risk for Object (29075) 1950 DA and Object (101955) 1999 RQ36, Update (NASA NEO, edited)

Potentially hazardous asteroid might collide with the Earth in 2182

[Source: EurekAlert, View Original Article. 7/27/10.]

The potentially hazardous asteroid, (101955) 1999 RQ36, has a one-in-a-thousand chance of impacting the Earth, and more than half of this probability indicates that this could happen in the year 2182, based on a global study in which Spanish researchers have been involved. Knowing this fact may help design in advance mechanisms aimed at deviating the asteroid's path.
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