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The Potentially Dangerous Asteroid (101955) Bennu
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We computed impact solutions of the potentially dangerous asteroid (101955) Bennu based on 569 optical observations from September 11.40624 UTC, 1999 to January 20.11189 UTC, 2013, and 29 radar observations from September 21, 1999, through September 29, 2011. Using the freely available OrbFit software package, we can follow its orbit forward in the future
searching for close approaches with the earth, which can lead to possible impacts up to 2200. With the A2 nongravitational parameter in the motion of the asteroid (101955) Bennu we computed possible impact solutions using different JPL planetary and lunar ephemerides and different number of additional massive perturbed asteroids. The possible impact path of risk for 2175 is presented. Additionally, we computed possible impact solutions using the normal places method of the selection of Bennu’s astrometric observations. Moreover, we computed time evolution of the mean orbital elements and the orbital nodes of Bennu 5 kyr in the backwards and 1 kyr in the future using the Yarkovsky effects. We computed the mean motion and secular orbital resonances of the Bennu. We also computed the influence of the JPL planetary and lunar ephemerides DE403, DE405, DE406, DE414, and DE423 on the close approaches of the asteroid (101955) Bennu with the earth.
Title: The Potentially Dangerous Asteroid (101955) Bennu
Description:
We computed impact solutions of the potentially dangerous asteroid (101955) Bennu based on 569 optical observations from September 11.
40624 UTC, 1999 to January 20.
11189 UTC, 2013, and 29 radar observations from September 21, 1999, through September 29, 2011.
Using the freely available OrbFit software package, we can follow its orbit forward in the future
searching for close approaches with the earth, which can lead to possible impacts up to 2200.
With the A2 nongravitational parameter in the motion of the asteroid (101955) Bennu we computed possible impact solutions using different JPL planetary and lunar ephemerides and different number of additional massive perturbed asteroids.
The possible impact path of risk for 2175 is presented.
Additionally, we computed possible impact solutions using the normal places method of the selection of Bennu’s astrometric observations.
Moreover, we computed time evolution of the mean orbital elements and the orbital nodes of Bennu 5 kyr in the backwards and 1 kyr in the future using the Yarkovsky effects.
We computed the mean motion and secular orbital resonances of the Bennu.
We also computed the influence of the JPL planetary and lunar ephemerides DE403, DE405, DE406, DE414, and DE423 on the close approaches of the asteroid (101955) Bennu with the earth.
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