101955 Bennu

From Wikipedia, the free encyclopedia
  (Redirected from 1999 RQ36)
Jump to: navigation, search
101955 Bennu
NASA 1999 RQ36.gif
Radar image of 101955 Bennu (courtesy Arecibo Observatory and JPL)[1][2]
Discovery
Discovered by LINEAR
Discovery site Lincoln Lab's ETS
Discovery date 11 September 1999
Designations
MPC designation 101955 Bennu
Pronunciation /bɛˈn/
Named after
Bennu
1999 RQ36
Apollo · NEO · PHA
Orbital characteristics[3]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 13.36 yr (4880 days)
Aphelion 1.3559 AU (202.84 Gm)
Perihelion 0.89689 AU (134.173 Gm)
1.1264 AU (168.51 Gm)
Eccentricity 0.20375
1.20 yr (436.65 d)
63,000 mph
101.7039°
0° 49m 28.056s / day
Inclination 6.0349°
2.0609°
66.2231°
Earth MOID 0.0032228 AU (482,120 km)
Jupiter MOID 3.87795 AU (580.133 Gm)
Jupiter Tisserand parameter 5.525
Proper orbital elements[4]
0.21145
5.0415°
301.1345 deg / yr
1.19548 yr
(436.649 d)
Physical characteristics
Mean radius
246±10 m[1]
Equatorial radius
275±10 m[1]
Mass 6.0×1010 kg[5] to 7.76×1010 kg
Mean density
1.26 ± 0.070 g/cm3
Equatorial surface gravity
10 micro-g[6]
4.288 h (0.1787 d)
176 ± 2°[7]
0.046[4]
Surface temp. min mean max
Kelvin[8] 236 259 279
Fahrenheit -34.6 6.8 42.8
Celsius -37 -14 6
B[4]
20.9

101955 Bennu (provisional designation 1999 RQ36)[9] is a carbonaceous asteroid in the Apollo group, and classified as a potentially hazardous object, with a 1 in 2700 chance of impacting Earth in the 22nd century.[10] It was discovered by the LINEAR Project on September 11, 1999. It is the planned target of the OSIRIS-REx mission which is intended to return samples to Earth in 2023 for further study.[11][12] It is a potential Earth impactor and is listed on the Sentry Risk Table with the third highest rating on the Palermo Technical Impact Hazard Scale.[13]

101955 Bennu has a mean diameter of approximately 492 m (1,614 ft; 0.306 mi) and has been observed extensively with the Arecibo Observatory Planetary Radar and the Goldstone Deep Space Network.[1][2][14]

Possible Earth impact[edit]

On average, an asteroid with a diameter of 500 m (1,600 ft; 0.31 mi) can be expected to impact Earth about every 130,000 years or so.[15] A 2010 dynamical study by Andrea Milani and collaborators predicted a series of eight potential Earth impacts by Bennu between 2169 and 2199. The cumulative probability of impact is dependent on physical properties of Bennu that were poorly known at the time, but was not found to exceed 0.071% for all eight encounters.[16] The authors recognized that an accurate assessment of 101955 Bennu's probability of Earth impact would require a detailed shape model and additional observations (either from the ground or from spacecraft visiting the object) to determine the magnitude and direction of the Yarkovsky effect.

After the publication of the shape model and astrometry based on radar observations obtained in 1999, 2005, and 2011,[1] it was possible to estimate the Yarkovsky acceleration and to revise the impact assessment. The current (as of 2014) best estimate of the impact probability is a cumulative probability of 0.037% in the interval 2175 to 2196.[17] This corresponds to a score on the Palermo scale of −1.70.

Spacecraft missions[edit]

101955 Bennu has been considered as the target of spacecraft missions due to the low Δv required to reach it from Earth orbit.[18] The OSIRIS-REx mission of NASA's New Frontiers Program is planned to launch in September 8, 2016, reach 101955 Bennu in 2019, and return samples to Earth in 2023.[12]

Name[edit]

The name Bennu was selected from more than eight thousand student entries from dozens of countries around the world who entered a "Name That Asteroid!" contest run by the University of Arizona, The Planetary Society, and the LINEAR Project.[3][9] A third-grade student named Michael Puzio, from North Carolina proposed the name in reference to the Egyptian mythological bird Bennu. To Puzio, the OSIRIS-REx spacecraft with its extended TAGSAM arm resembles the Egyptian deity, which is typically depicted as a heron.[3]

Gallery[edit]

See also[edit]

References[edit]

  1. ^ a b c d e Nolan, M. C.; Magri, C.; Howell, E. S.; Benner, L. A. M.; Giorgini, J. D.; Hergenrother, C. W.; Hudson, R. S.; Lauretta, D. S.; Margot, J. L.; Ostro, S. J.; Scheeres, D. J. (2013). "Shape model and surface properties of the OSIRIS-REx target Asteroid (101955) Bennu from radar and lightcurve observations". Icarus. 226 (1): 629–640. Bibcode:2013Icar..226..629N. doi:10.1016/j.icarus.2013.05.028. ISSN 0019-1035. 
  2. ^ a b "Goldstone Delay-Doppler Images of 1999 RQ36". Asteroid Radar Research. Jet Propulsion Laboratory. 
  3. ^ a b c "JPL Small-Body Database Browser: 101955 Bennu (1999 RQ36)" (2013-01-20 last obs.). Jet Propulsion Laboratory. Retrieved 20 August 2016. 
  4. ^ a b c "(101955) Bennu". NEODyS. University of Pisa. Retrieved 1 December 2015. 
  5. ^ "101955 1999 RQ36: Earth Impact Risk Summary". NASA. Jet Propulsion Laboratory. August 5, 2010. Retrieved 24 November 2013. 
  6. ^ "One of NASA's cleanest spacecraft ever is ready to fly". Spaceflight Now. Spaceflight Now Inc. Retrieved 23 August 2016. 
  7. ^ Hergenrother, CW; Barucci, MA; Barnouin, O (16 Sep 2014). "The Design Reference Asteroid for the OSIRIS-REx Mission Target (101955) Bennu". Retrieved 20 August 2016. 
  8. ^ "Planetary Habitability Calculators". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. Retrieved 6 December 2015. 
  9. ^ a b Murphy, Diane (May 1, 2013). "Nine-Year-Old Names Asteroid Target of NASA Mission in Competition Run By The Planetary Society". The Planetary Society. Retrieved 20 August 2016. 
  10. ^ Lauretta, D. S.; Bartels, A. E.; et al. (April 2015). "The OSIRIS-REx target asteroid (101955) Bennu: Constraints on its physical, geological, and dynamical nature from astronomical observations". Meteoritics & Planetary Science. 50 (4): 834–849. doi:10.1111/maps.12353. 
  11. ^ Brown, Dwayne; Neal-Jones, Nancy (March 31, 2015). "RELEASE 15-056 – NASA's OSIRIS-REx Mission Passes Critical Milestone". NASA. Retrieved April 4, 2015. 
  12. ^ a b "NASA to Launch New Science Mission to Asteroid in 2016". NASA. 25 May 2011. Retrieved 21 May 2013. 
  13. ^ "Sentry Risk Table". NASA/JPL Near-Earth Object Program Office. Retrieved 2014-03-26. 
  14. ^ Hudson, R. S.; Ostro, S. J.; Benner, L. A. M. "Recent Delay-Doppler Radar Asteroid Modeling Results: 1999 RQ36 and Craters on Toutatis". Bulletin of the American Astronomical Society. American Astronomical Society. 32: 1001. Bibcode:2000DPS....32.0710H. 
  15. ^ Robert Marcus; H. Jay Melosh & Gareth Collins (2010). "Earth Impact Effects Program". Imperial College London / Purdue University. Retrieved 2013-02-07.  (solution using density of 2,600 kg/m^3, sped of 17km/s, and impact angle of 45 degrees)
  16. ^ Milani, Andrea; Chesley, Steven R.; Sansaturio, Maria Eugenia; Bernardi, Fabrizio; Valsecchi, Giovanni B.; Arratia, Oscar (2009). "Long term impact risk for (101955) 1999 RQ36". Icarus. 203 (2): 460–471. arXiv:0901.3631free to read. Bibcode:2009Icar..203..460M. doi:10.1016/j.icarus.2009.05.029. 
  17. ^ Chesley, Steven R.; Farnocchia, Davide; Nolan, Michael C.; Vokrouhlický, David; Chodas, Paul W.; Milani, Andrea; Spoto, Federica; Rozitis, Benjamin; Benner, Lance A.M.; Bottke, William F.; Busch, Michael W.; Emery, Joshua P.; Howell, Ellen S.; Lauretta, Dante S.; Margot, Jean-Luc; Taylor, Patrick A. (2014). "Orbit and bulk density of the OSIRIS-REx target Asteroid (101955) Bennu". Icarus. 235: 5–22. arXiv:1402.5573free to read. Bibcode:2014Icar..235....5C. doi:10.1016/j.icarus.2014.02.020. ISSN 0019-1035. 
  18. ^ Near-Earth Asteroid Delta-V for Space Rendezvous
  19. ^ Brown, Dwayne; Neal-Jones, Nancy (January 15, 2014). "NASA RELEASE 14-017 - NASA Invites Public to Send Names on an Asteroid Mission and Beyond". NASA. Retrieved January 16, 2014. 

External links[edit]