|Discovery site||Lincoln Lab's ETS|
|Discovery date||11 September 1999|
|Apollo · NEO · PHA · risk listed|
|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)|
|1.1955 yr (436.65 d)|
Average orbital speed
|28.0 km/s (63,000 mph)|
|0° 49m 28.056s / day|
|Earth MOID||0.0032228 au (482,120 km)|
|Venus MOID||0.194 au (29,000,000 km)|
|Mars MOID||0.168 au (25,100,000 km)|
|Jupiter MOID||3.877 au (580.0 Gm)|
|Proper orbital elements|
Proper mean motion
|301.1345 deg / yr|
Proper orbital period
|Dimensions||565 m × 535 m × 508 m|
Equatorial surface gravity
North pole right ascension
North pole declination
101955 Bennu (provisional designation 1999 RQ36) is a carbonaceous asteroid in the Apollo group discovered by the LINEAR Project on 11 September 1999. It is a potentially hazardous object that is listed on the Sentry Risk Table with the second-highest cumulative rating on the Palermo Technical Impact Hazard Scale. It has a cumulative 1-in-2,700 chance of impacting Earth between 2175 and 2199. It is named after the Bennu, the ancient Egyptian mythological bird associated with the Sun, creation, and rebirth.
Bennu was the target of the OSIRIS-REx mission which is intended to return its samples to Earth in 2023 for further study. On 3 December 2018, the OSIRIS-REx spacecraft arrived at Bennu after a two-year journey. It orbited the asteroid and mapped out Bennu's surface in detail, seeking potential sample collection sites. Analysis of the orbits allowed calculation of Bennu's mass and its distribution.
On 18 June 2019, NASA announced that the OSIRIS-REx spacecraft had closed in and captured an image from a distance of 600 metres (2,000 ft) from Bennu's surface.
In October 2020, OSIRIS-REx successfully touched down on the surface of Bennu, collected a sample using an extendable arm, secured the sample and prepared for a return trip to Earth. On 10 May 2021, OSIRIS-REx successfully completed its departure from the Bennu asteroid while still carrying the sample of the asteroid rubble.
Discovery and observation
Bennu was discovered on 11 September 1999 during a Near-Earth asteroid survey by the Lincoln Near-Earth Asteroid Research (LINEAR). The asteroid was given the provisional designation 1999 RQ36 and classified as a near-Earth asteroid. Bennu was observed extensively by the Arecibo Observatory and the Goldstone Deep Space Network using radar imaging as Bennu closely approached Earth on 23 September 1999.
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 in 2012. Third-grade student 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 resembled the Egyptian deity, which is typically depicted as a heron.
Its features will be named after birds and bird-like creatures in mythology.
Bennu has a roughly spheroidal shape, resembling a spinning top. Bennu's axis of rotation is tilted 178 degrees to its orbit; the direction of rotation about its axis is retrograde with respect to its orbit. While the initial ground based radar observations indicated that Bennu had a fairly smooth shape with one prominent 10–20 m boulder on its surface, high resolution data obtained by OSIRIS-REx revealed that the surface is much rougher with more than 200 boulders larger than 10 m on the surface, the largest of which is 58 m across. The boulders contain veins of high albedo carbonate minerals believed to have formed prior to the formation of the asteroid due to hot water channels on the much larger parent body. The veins range from 3 to 15 centimeters wide, and can be over one meter in length, much bigger than carbonate veins seen in meteorites.
There is a well-defined ridge along the equator of Bennu. The presence of this ridge suggests that fine-grained regolith particles have accumulated in this area, possibly because of its low gravity and fast rotation. Observations by the OSIRIS-REx spacecraft has shown that Bennu is rotating faster over time. This change in Bennu's rotation is caused by the Yarkovsky–O'Keefe–Radzievskii–Paddack effect, or the YORP effect. Due to the uneven emission of thermal radiation from its surface as Bennu rotates in sunlight, the rotation period of Bennu decreases by about one second every 100 years.
Observations of this minor planet by the Spitzer Space Telescope in 2007 gave an effective diameter of 484±10 m, which is in line with other studies. It has a low visible geometric albedo of 0.046±0.005. The thermal inertia was measured and found to vary by approximately 19% during each rotational period. It was based on this observation scientists (incorrectly) estimated a moderate regolith grain size, ranging from several millimeters up to a centimeter, evenly distributed. No emission from a potential dust coma has been detected around Bennu, which puts a limit of 106 g of dust within a radius of 4750 km.
Astrometric observations between 1999 and 2013 have demonstrated that 101955 Bennu is influenced by the Yarkovsky effect, causing the semimajor axis of its orbit to drift on average by 284±1.5 meters/year. Analysis of the gravitational and thermal effects has given a bulk density of ρ = 1190±13 kg/m3, which is only slightly denser than water. Therefore, the predicted macroporosity is 40±10%, suggesting the interior has a rubble pile structure or even hollow. The estimated mass is (7.329±0.009)×1010 kg.
Photometry and spectroscopy
Photometric observations of Bennu in 2005 yielded a synodic rotation period of 4.2905±0.0065 h. It has a B-type classification, which is a sub-category of carbonaceous asteroids. Polarimetric observations show that Bennu belongs to the rare F subclass of carbonaceous asteroids, which is usually associated with cometary features. Measurements over a range of phase angles showed a phase function slope of 0.040 magnitudes per degree, which is similar to other near-Earth asteroids with low albedo.
Before OSIRIS-REx, spectroscopy indicated a correspondence with the CI and/or CM carbonaceous chondrite meteorites, including carbonaceous-chondrite mineral magnetite. Magnetite, a spectrally prominent water product but destroyed by heat, is an important proxy of astronomers including OSIRIS-REx staff.
Preliminary spectroscopic surveys of the asteroid's surface by OSIRIS-REx confirmed magnetite and the meteorite-asteroid linkage, dominated by phyllosilicates. Phyllosilicates, among others, hold water. Bennu's water spectra were detectable on approach, reviewed by outside scientists, then confirmed from orbit.
OSIRIS-REx observations have resulted in a (self-styled) conservative estimate of about 7 x 108 kg water in one form alone, neglecting additional forms. This is a water content of ~1 wt.%, and potentially much more. In turn this suggests transient pockets of water beneath Bennu's regolith. The surficial water may be lost from the collected samples. However, if the sample return capsule maintains low temperatures, the largest (centimeter-scale) fragments may contain measurable quantities of adsorbed water, and some fraction of Bennu's ammonium compounds.
Bennu is an active asteroid, sporadically emitting plumes of particles and rocks as large as 10 cm (3.9 in), (not dust, defined as tens of micrometers). Scientists hypothesize the releases may be caused by thermal fracturing, volatile release through dehydration of phyllosilicates, pockets of subsurface water, and/or meteoroid impacts.
Before the arrival of OSIRIS-REx, Bennu had displayed polarization consistent with Comet Hale-Bopp and 3200 Phaethon, a rock comet. Bennu, Phaethon, and inactive Manx comets are examples of active asteroids. B-type asteroids displaying a blue color in particular, may be dormant comets. If the IAU declares Bennu to be a dual-status object, its comet designation would be P/1999 RQ36 (LINEAR).
All geological features on Bennu are named after various species of birds and bird-like figures in mythology. The first features to be named were the final four candidate OSIRIS-REx sample sites, which were given unofficial names by the team in August 2019. On 6 March 2020 the IAU announced the first official names for 12 Bennu surface features, including regiones (broad geographic regions), craters, dorsa (ridges), fossae (grooves or trenches) and saxa (rocks and boulders).
Candidate sample sites
|Nightingale||56°N 43°E||Abundant fine-grained material with a large variation in color. Primary sample collection site.|
|Kingfisher||11°N 56°E||A relatively new crater with the highest water signature of all four sites.|
|Osprey||11°N 80°E||Located on a low albedo patch with a large variety of rocks. Backup sample collection site.|
|Sandpiper||47°S 322°E||Located between two young craters, located in rough terrain. Minerals vary in brightness with hints of hydrated minerals.|
On 12 December 2019, after a year of mapping Bennu's surface, a target site was announced. Named Nightingale, the area is near Bennu's north pole and lies inside a small crater within a larger crater. Osprey was selected as the backup sample site.
IAU named features
|Aellopus Saxum||Aello, one of the half-bird half-woman Harpy sisters from Greek mythology||25.44°N 335.67°E|
|Aetos Saxum||Aetos, childhood playmate of the god Zeus who was turned into an eagle from Greek mythology||3.46°N 150.36°E|
|Amihan Saxum||Amihan, bird deity from Philippine mythology||17.96°S 256.51°E|
|Benben Saxum||Benben, Ancient Egyptian primordial mound that arose from the primordial waters Nu||45.86°S 127.59°E|
|Boobrie Saxum||Boobrie, shapeshifting entity from Scottish mythology that often takes the form of a giant water bird||48.08°N 214.28°E|
|Camulatz Saxum||Camulatz, one of four birds in the K'iche' creation myth in Maya mythology||10.26°S 259.65°E|
|Celaeno Saxum||Celaeno, one of the half-bird half-woman Harpy sisters from Greek mythology||18.42°N 335.23°E|
|Ciinkwia Saxum||Ciinkwia, thunder beings from Algonquian mythology that look like giant eagles||4.97°S 249.47°E|
|Dodo Saxum||Dodo, a dodo bird character from Alice's Adventures in Wonderland||32.68°S 64.42°E|
|Gamayun Saxum||Gamajun, prophetic bird from Slavic mythology||9.86°N 105.45°E|
|Gargoyle Saxum||Gargoyle, dragon-like monster with wings||4.59°N 92.48°E|
|Gullinkambi Saxum||Gullinkambi, rooster from Norse mythology that lives in Valhalla||18.53°N 17.96°E|
|Huginn Saxum||Huginn, one of two ravens that accompany the god Odin in Norse mythology||29.77°S 43.25°E|
|Kongamato Saxum||Kongamato, giant flying creature from Kaonde mythology||5.03°N 66.31°E|
|Muninn Saxum||Muninn, one of two ravens that accompany the god Odin in Norse mythology||29.34°S 48.68°E|
|Ocypete Saxum||Ocypete, one of the half-bird half-woman Harpy sisters from Greek mythology||25.09°N 328.25°E|
|Odette Saxum||Odette, princess that turns into the White Swan in Swan Lake||44.86°S 291.08°E|
|Odile Saxum||Odile, the Black Swan from Swan Lake||42.74°S 294.08°E|
|Pouakai Saxum||Poukai, monstrous bird from Maori mythology||40.45°S 166.75°E|
|Roc Saxum||Roc, giant bird of prey from Arabic mythology||23.46°S 25.36°E|
|Simurgh Saxum||Simurgh, benevolent bird that possesses all knowledge from Iranian mythology||25.32°S 4.05°E|
|Strix Saxum||Strix, bird of ill omen from Roman mythology||13.4°N 88.26°E|
|Thorondor Saxum||Thorondor, the King of the Eagles in Tolkien's Middle-earth||47.94°S 45.1°E|
|Tlanuwa Regio||Tlanuwa, giant birds from Cherokee mythology||37.86°S 261.7°E|
Origin and evolution
The carbonaceous material that composes Bennu originally came from the breakup of a much larger parent body—a planetoid or a proto-planet. But like nearly all other matter in the Solar System, the origins of its minerals and atoms are to be found in dying stars such as red giants and supernovae. According to the accretion theory, this material came together 4.5 billion years ago during the formation of the Solar System.
Bennu's basic mineralogy and chemical nature would have been established during the first 10 million years of the Solar System's formation, where the carbonaceous material underwent some geologic heating and chemical transformation inside a much larger planetoid or a proto-planet capable of producing the requisite pressure, heat and hydration (if need be)—into more complex minerals. Bennu probably began in the inner asteroid belt as a fragment from a larger body with a diameter of 100 km. Simulations suggest a 70% chance it came from the Polana family and a 30% chance it derived from the Eulalia family. Impactors on boulders of Bennu indicate that Bennu has been in near earth orbit (separated from the main asteroid belt) for 1–2.5 million years.
Subsequently, the orbit drifted as a result of the Yarkovsky effect and mean motion resonances with the giant planets, such as Jupiter and Saturn. Various interactions with the planets in combination with the Yarkovsky effect modified the asteroid, possibly changing its spin, shape, and surface features.
Cellino et al. have suggested a possible cometary origin for Bennu, based on similarities of its spectroscopic properties with known comets. The estimated fraction of comets in the population of near Earth objects is 8%±5%. This includes rock comet 3200 Phaethon, originally discovered as, and still numbered as an asteroid.
Bennu currently orbits the Sun with a period of 1.1955 years. Earth gets as close as about 480,000 km (0.0032 au) from its orbit around 23 to 25 September. On 22 September 1999 Bennu passed 0.0147 au from Earth, and six years later on 20 September 2005 it passed 0.033 au from Earth. The next close approaches of less than 0.09 au will be 30 September 2054 and then 23 September 2060, which will perturb the orbit slightly. Between the close approach of 1999 and that of 2060, Earth completes 61 orbits and Bennu 51. An even closer approach will occur on 23 September 2135 between 0.0008 and 0.0036 au (see below). In the 75 years between the 2060 and 2135 approaches, Bennu completes 64 orbits, meaning its period will have changed to about 1.17 years.
|2054-09-30||0.0392991 AU (5.87906 million km)||±46 km|
|2060-09-23||0.005008 AU (749.2 thousand km)||±42 km|
|2080-09-22||0.0155615 AU (2.32797 million km)||±21 thousand km|
|2135-09-25||0.0019912 AU (297.88 thousand km)||±210 thousand km|
|2196-09-24||0.03 AU (4.5 million km) (Horizons)
2.2 AU (330 million km) (NEODyS)
|±370 million km|
Possible Earth impact
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. 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 found to not exceed 0.071% for all eight encounters. 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.
The publication of the shape model and of astrometry based on radar observations obtained in 1999, 2005, and 2011 made possible an improved estimate of the Yarkovsky acceleration and a revised assessment of the impact probability. The current (as of 2014)[update] best estimate of the impact probability is a cumulative probability of 0.037% in the interval 2175 to 2196. This corresponds to a cumulative score on the Palermo scale of −1.71. If an impact were to occur, the expected kinetic energy associated with the collision would be 1,200 megatons in TNT equivalent (for comparison, TNT equivalent of Little Boy was approx 0.015 megaton).
2060 close approach
Bennu will pass 0.005 au (750,000 km; 460,000 mi) from Earth on 23 September 2060, while the Moon's average orbital distance (Lunar Distance, LD) is 384,402 km (238,856 mi) today and will be 384,404 km in 50 years time. It will be too dim to be seen with common binoculars. The close approach of 2060 causes divergence in the close approach of 2135. On 25 September 2135, the nominal approach distance is 0.002 au (300,000 km; 190,000 mi) from Earth, but Bennu could pass as close as 0.0007 au (100,000 km; 65,000 mi). There is no chance of an Earth impact in 2135. The 2135 approach will create many lines of variations and Bennu may pass through a gravitational keyhole during the 2135 passage which could create an impact scenario at a future encounter. The keyholes are all less than 55 km wide.
On 25 September 2175, there is a 1 in 24,000 chance of an Earth impact, but the nominal trajectory has the asteroid more than 1 AU from Earth on that date. The most threatening virtual impactor is on 24 September 2196 when there is a 1 in 11,000 chance of an Earth impact, but the asteroid is still expected to be several million kilometers from Earth. There is a cumulative 1 in 2,700 chance of an Earth impact between 2175 and 2199.
Lauretta et al. reported in 2015 their results of a computer simulation, concluding that it is more likely that 101955 Bennu will be destroyed by some other cause:
The orbit of Bennu is intrinsically dynamically unstable, as are those of all NEOs. In order to glean probabilistic insights into the future evolution and likely fate of Bennu beyond a few hundred years, we tracked 1,000 virtual "Bennus" for an interval of 300 Myr with the gravitational perturbations of the planets Mercury–Neptune included. Our results ... indicate that Bennu has a 48% chance of falling into the Sun. There is a 10% probability that Bennu will be ejected out of the inner Solar System, most likely after a close encounter with Jupiter. The highest impact probability for a planet is with Venus (26%), followed by the Earth (10%) and Mercury (3%). The odds of Bennu striking Mars are only 0.8% and there is a 0.2% chance that Bennu will eventually collide with Jupiter.
|Asteroid||Date||Nominal approach distance (LD)||Min. distance (LD)||Max. distance (LD)||Absolute magnitude (H)||Size (meters)|
|(152680) 1998 KJ9||1914-12-31||0.606||0.604||0.608||19.4||279–900|
|(458732) 2011 MD5||1918-09-17||0.911||0.909||0.913||17.9||556–1795|
|(163132) 2002 CU11||1925-08-30||0.903||0.901||0.905||18.5||443–477|
|(153814) 2001 WN5||2028-06-26||0.647||0.647||0.647||18.2||921–943|
|99942 Apophis||2029-04-13||0.0981 (GEO is 0.109)||0.0963||0.1000||19.7||310–340|
|(153201) 2000 WO107||2140-12-01||0.634||0.631||0.637||19.3||427–593|
As an active asteroid with a small minimum orbit intersection distance from Earth, Bennu may be the parent body of a weak meteor shower. Bennu particles would radiate around 25 September from the southern constellation of Sculptor. The meteors are expected to be near the naked eye limit and only produce a Zenith hourly rate of less than 1.
The OSIRIS-REx mission of NASA's New Frontiers program was launched towards 101955 Bennu on 8 September 2016. On 3 December 2018, the spacecraft arrived at the asteroid Bennu after a two-year journey. One week later, at the American Geophysical Union Fall Meeting, investigators announced that OSIRIS-REx had discovered spectroscopic evidence for hydrated minerals on the surface of the asteroid, implying that liquid water was present in Bennu's parent body before it split off.
On 20 October 2020, OSIRIS-REx descended to the asteroid and "pogo-sticked off" it while successfully collecting a sample. OSIRIS-REx is expected to return samples to Earth in 2023 via a capsule-drop by parachute, ultimately, from the spacecraft to the Earth's surface in Utah on 24 September. On 7 April 2021, OSIRIS-REx completed its final flyover of the asteroid and began slowly drifting away from it. On 10 May 2021, the departure was completed with OSIRIS-REx while still managing to contain the asteroid sample.
The asteroid Bennu was selected from over half a million known asteroids by the OSIRIS-REx selection committee. The primary constraint for selection was close proximity to Earth, since proximity implies low impulse (Δv) required to reach an object from Earth orbit. The criteria stipulated an asteroid in an orbit with low eccentricity, low inclination, and an orbital radius of 0.8–1.6 au. Furthermore, the candidate asteroid for a sample-return mission must have loose regolith on its surface, which implies a diameter greater than 200 meters. Asteroids smaller than this typically spin too fast to retain dust or small particles. Finally, a desire to find an asteroid with pristine carbon material from the early Solar System, possibly including volatile molecules and organic compounds, reduced the list further.
With the above criteria applied, five asteroids remained as candidates for the OSIRIS-REx mission, and Bennu was chosen, in part for its potentially hazardous orbit.
Animation of OSIRIS-REx collecting a sample from the surface of Bennu.
- List of minor planets and comets visited by spacecraft
- (341843) 2008 EV5, provisional target of the cancelled Asteroid Redirect Mission
- 162173 Ryugu, an asteroid being studied JAXA concurrent with the NASA mission to 101955 Bennu
- 73P/Schwassmann–Wachmann, a disintegrating-comet
- "JPL Small-Body Database Browser: 101955 Bennu (1999 RQ36)" (2018-05-15 last observation. Solution includes non-gravitational parameters). Jet Propulsion Laboratory. Archived from the original on 19 March 2018. Retrieved 28 March 2021.
- "Bennu". Dictionary.com Unabridged. Random House.
- "(101955) Bennu = 1999 RQ36 Orbit". Minor Planet Center. Retrieved 21 March 2018.
- "(101955) Bennu". NEODyS. University of Pisa. Retrieved 1 December 2015.
- Barnouin, O. S. (19 March 2019). "Shape of (101955) Bennu indicative of a rubble pile with internal stiffness". Nature Geoscience. 12 (4): 247–252. Bibcode:2019NatGe..12..247B. doi:10.1038/s41561-019-0330-x. PMC 6505705. PMID 31080497.
- "Planetary Habitability Calculators". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. Retrieved 6 December 2015.
- Lauretta, D. S. (19 March 2019). "The unexpected surface of asteroid (101955) Bennu". Nature. 568 (7750): 55–60. Bibcode:2019Natur.568...55L. doi:10.1038/s41586-019-1033-6. PMC 6557581. PMID 30890786.
- Hergenrother, Carl W; Maria Antonietta Barucci; Barnouin, Olivier; Bierhaus, Beau; Binzel, Richard P; Bottke, William F; Chesley, Steve; Clark, Ben C; Clark, Beth E; Cloutis, Ed; Christian Drouet d'Aubigny; Delbo, Marco; Emery, Josh; Gaskell, Bob; Howell, Ellen; Keller, Lindsay; Kelley, Michael; Marshall, John; Michel, Patrick; Nolan, Michael; Rizk, Bashar; Scheeres, Dan; Takir, Driss; Vokrouhlický, David D; Beshore, Ed; Lauretta, Dante S (2018). "Unusual polarimetric properties of (101955) Bennu: similarities with F-class asteroids and cometary bodies". Monthly Notices of the Royal Astronomical Society: Letters. 481 (1): L49–L53. arXiv:1808.07812. Bibcode:2018MNRAS.481L..49C. doi:10.1093/mnrasl/sly156. S2CID 119226483.
- Murphy, Diane (1 May 2013). "Nine-Year-Old Names Asteroid Target of NASA Mission in Competition Run By The Planetary Society". The Planetary Society. Retrieved 20 August 2016.
- "Sentry Risk Table". NASA/JPL Near-Earth Object Program Office. Archived from the original on 11 September 2016. Retrieved 20 March 2018. (Use Unconstrained Settings)
- "101955 1999 RQ36: Earth Impact Risk Summary". NASA. Jet Propulsion Laboratory. 25 March 2016. Retrieved 20 March 2018.
- 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. Bibcode:2015M&PS...50..834L. CiteSeerX 10.1.1.723.9955. doi:10.1111/maps.12353.
- "Goldstone Delay-Doppler Images of 1999 RQ36". Asteroid Radar Research. Jet Propulsion Laboratory. Archived from the original on 30 August 2000.
- Hudson, R. S.; Ostro, S. J.; Benner, L. A. M. (2000). "Recent Delay-Doppler Radar Asteroid Modeling Results: 1999 RQ36 and Craters on Toutatis". Bulletin of the American Astronomical Society. 32: 1001. Bibcode:2000DPS....32.0710H.
- Corum, Jonathan (8 September 2016). "NASA Launches the Osiris-Rex Spacecraft to Asteroid Bennu". The New York Times. Retrieved 9 September 2016.
- Chang, Kenneth (8 September 2016). "The Osiris-Rex Spacecraft Begins Chasing an Asteroid". The New York Times. Retrieved 9 September 2016.
- Brown, Dwayne; Neal-Jones, Nancy (31 March 2015). "RELEASE 15-056 – NASA's OSIRIS-REx Mission Passes Critical Milestone". NASA. Retrieved 4 April 2015.
- Chang, Kenneth (3 December 2018). "NASA's Osiris-Rex Arrives at Asteroid Bennu After a Two-Year Journey". The New York Times. Retrieved 12 February 2021.
- Plait, Phil (4 December 2018). "Welcome to Bennu!". SYFY WIRE. Retrieved 5 December 2018.
- "NASA captures closest-ever photo of massive asteroid Bennu flying near Earth". Sky News. 18 June 2019.
- Chang, Kenneth (20 October 2020). "Seeking Solar System's Secrets, NASA's OSIRIS-REX Mission Touches Bennu Asteroid". The New York Times. Retrieved 12 February 2021.
- Hautaluoma, Grey; Johnson, Alana; Jones, Nancy Neal; Morton, Erin (29 October 2020). "Release 20-109 - NASA's OSIRIS-REx Successfully Stows Sample of Asteroid Bennu". NASA. Retrieved 30 October 2020.
- Chang, Kenneth (29 October 2020). "NASA's Asteroid Mission Packs Away Its Cargo. Next Stop: Earth". The New York Times. Retrieved 12 February 2021.
- Chang, Kenneth (10 May 2021). "Bye-Bye, Bennu: NASA Heads Back to Earth With Asteroid Stash in Tow - The OSIRIS-REX mission will spend two years cruising home with space rock samples that could unlock secrets of the early solar system". The New York Times. Retrieved 11 May 2021.
- Marcia Dunn, Associated Press (10 May 2021). "NASA spacecraft begins 2-year trip home with asteroid rubble". WJHL. Retrieved 10 May 2021.
- 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.
- Hille, Karl (8 August 2019). "Asteroid's Features To Be Named After Mythical Birds". NASA. Retrieved 10 August 2019.
- Voosen P (2020). "NASA mission set to sample carbon-rich asteroid". Science. 370 (6513): 158. doi:10.1126/science.370.6513.158. PMID 33033199.
- Kaplan HH, Lauretta DS, Simon AA, Eno HL (2020). "Bright carbonate veins on asteroid (101955) Bennu: Implications for aqueous alteration history". Science. 370 (6517): eabc3557. doi:10.1126/science.abc3557. PMID 33033155.
- Morton, Erin (19 March 2019). "NASA Mission Reveals Asteroid Has Big Surprises". AsteroidMission.org. Retrieved 19 March 2019.
- Emery, J.; et al. (July 2014), Muinonen, K. (ed.), "Thermal infrared observations and thermophysical characterization of the OSIRIS-REx target asteroid (101955) Bennu", Conference Proceedings Asteroids, Comets, Meteors 2014: 148, Bibcode:2014acm..conf..148E.
- Scheeres, D.J. (8 October 2020). "Heterogeneous mass distribution of the rubble-pile asteroid (101955) Bennu". Science Advances. 6 (41): eabc3350. doi:10.1126/sciadv.abc3350. PMC 7544499. PMID 33033036.
- Hergenrother, Carl W.; et al. (September 2013), "Lightcurve, Color and Phase Function Photometry of the OSIRIS-REx Target Asteroid (101955) Bennu", Icarus, 226 (1): 663–670, Bibcode:2013Icar..226..663H, doi:10.1016/j.icarus.2013.05.044.
- King, A; Solomon, J; Schofield, P; Russell, S (December 2015). "Characterising the CI and CI-like carbonaceous chondrites using thermogravimetric analysis and infrared spectroscopy". Earth, Planets and Space. 67: 1989. Bibcode:2015EP&S...67..198K. doi:10.1186/s40623-015-0370-4.
- Takir, D; Emery, J; Hibbits, C (2017). 3-μm Spectroscopy Of Water-Rich Meteorites And Asteroids: New Results And Implications. Hayabusa Symposium 2017.
- Bates, H; Hanna, K; King, A; Bowles, N (2018). Thermal Infrared Spectra of Heated CM and C2 Chondrites and Implications for Asteroid Sample Return Missions. Hayabusa Symposium 2018.
- Hamilton, V; Simon, A; Kaplan, H; Christensen, P; Reuter, D; DellaGiustina, D; Haberle, C; Hanna, R; Brucato, J; Praet, A; Glotch, T; Rogers, A; Connolly, H; McCoy, T; Emery, J; Howell, E; Barucci, M; Clark, B; Lauretta, D (March 2020). "OVIRS Results". VNIR and TIR spectral characteristics of (101955) Bennu from OSIRIS-REx Detailed Survey and Reconnaissance Observations. 51st LPSC.
- Mason, B (1962). Meteorites. New York and London: John Wiley and Sons Inc. p. 60.
an important constituent in many of the carbonaceous chondrites
- Takir, D; Emery, J; McSween, H; Hibbits, C; Clark, R; Pearson, N; Wang, A (2013). "Nature and degree of aqueous alteration in CM and CI carbonaceous chondrites". Meteoritics & Planetary Science. 48 (9): 1618. Bibcode:2013M&PS...48.1618T. doi:10.1111/maps.12171.
- Bates, H; King, A; Donaldson-Hanna, K; Bowles, N; Russell, S (19 November 2019). "Linking mineralogy and spectroscopy of highly aqueously altered CM and CI carbonaceous chondrites in preparation for primitive asteroid sample return". Meteoritics & Planetary Science. 55 (1): 77–101. doi:10.1111/maps.13411.
observations of primitive, water‐rich asteroids
- King, A; Schofield, P; Russell, S (2017). "Type 1 aqueous alteration in CM carbonaceous chondrites: Implications for the evolution of water-rich asteroids". Meteoritics & Planetary Science. 52 (6): 1197. Bibcode:2017M&PS...52.1197K. doi:10.1111/maps.12872.
small amounts of opaque phases (e.g., magnetite, Fe-sulfides) known to ...have a large effect on the overall spectral shape
- Kerridge, J; Mackay, A; Boynton, W (27 July 1979). "Magnetite in CI Carbonaceous Meteorites: Origin by Aqueous Activity on a Planetesimal Surface". Science. 205 (4404): 395–7. Bibcode:1979Sci...205..395K. doi:10.1126/science.205.4404.395. PMID 17790849. S2CID 9916605.
- Brearley, A (2006). "The Action of Water". Meteorites and the Early Solar System II. Tucson: University of Arizona Press. p. 587. ISBN 9780816525621.
- Rubin, A; Li, Y (December 2019). "Formation and destruction of magnetite in CO3 chondrites and other chondrite groups". Geochemistry. 79 (4): article 125528. Bibcode:2019ChEG...79l5528R. doi:10.1016/j.chemer.2019.07.009.
- Yang, B; Jewitt, D (2010). "Identification of Magnetite in B-type asteroids". Astronomical Journal. 140 (3): 692. arXiv:1006.5110. Bibcode:2010AJ....140..692Y. doi:10.1088/0004-6256/140/3/692. S2CID 724871.
evidence of water ice" "an important product of parent-body aqueous alteration
- Kita, J; Defouilloy, C; Goodrich, C; Zolensky, M (2017). "O isotope ratios of magnetite in CI-like clasts from a polymict ureilite".
ratios of magnetite are of special interest because...Cite journal requires
- Cloutis, E; Hiroi, T; Gaffey, M; Alexander, C; Mann, P (2011). "Spectral Reflectance Properties of carbonaceous chondrites: 1. CI chondrites". Icarus. 212 (1): 180. Bibcode:2011Icar..212..180C. doi:10.1016/j.icarus.2010.12.009.
- Clark, B; Binzel, R; Howell, E; Cloutis, E; Ockert-Bell, M; Christensen, P; Barucci, M; DeMeo, F; Lauretta, D; Connolly, H; Soderberg, A; Hergenrother, C; Lim, L; Emery, J; Mueller, M (2011). "Asteroid (101955) 1999 RQ36: Spectroscopy from 0.4 to 2.4 μm and meteorite analogs". Icarus. 216 (2): 462. Bibcode:2011Icar..216..462C. doi:10.1016/j.icarus.2011.08.021.
- Stolte, D (9 January 2014). "7 Questions for Dante Lauretta, Leader of UA's Biggest Space Mission". Retrieved 31 December 2020.
We think Bennu is a water-rich asteroid
- "OSIRIS-REx Arrives at Bennu -- 2018 AGU Press Conference". 10 December 2018. Retrieved 31 December 2020.
- Lauretta, D (25 September 2019). "OSIRIS-REx Explores Asteroid Bennu". Retrieved 31 December 2020.
- All About Bennu: A Rubble Pile with a Lot of Surprises. Kimberly M. S. Cartier, EOS Planetary Sciences. 21 March 2019. "In terms of spectra and minerology, Bennu's rocks 'look a lot like the rarest, most fragile meteorites in our collection,' Lauretta said, referring to the CM carbonaceous chondrites"
- Hamilton, V. E.; Simon, A. A. (2019). "Evidence for widespread hydrated minerals on asteroid (101955) Bennu". Nature Astronomy. 3 (4): 332–340. Bibcode:2019NatAs...3..332H. doi:10.1038/s41550-019-0722-2. hdl:1721.1/124501. PMC 6662227. PMID 31360777.
- Lauretta, D (4 April 2019). "The unexpected surface of asteroid (101955) Bennu". Nature. 568 (7750): 55–60. Bibcode:2019Natur.568...55L. doi:10.1038/s41586-019-1033-6. PMC 6557581. PMID 30890786. "This finding is in agreement with pre-encounter measurements and consistent with CI and CM chondrites."
- "NASA's Newly Arrived OSIRIS-REx Spacecraft Already Discovers Water on Asteroid". NASA. 11 December 2018.
- "Water found on asteroid, confirming Bennu as excellent mission target". Science Daily. 10 December 2018. Retrieved 10 December 2018.
- Lauretta, D. "Welcome to Bennu Press Conference - First Mission Science Results". Retrieved 24 July 2019. "Report Card" at 25:15
- Feierberg, M; Lebofsky, L; Tholen, D (1985). "The nature of C-class asteroids from 3u spectrophotometry". Icarus. 63 (2): 191. Bibcode:1985Icar...63..183F. doi:10.1016/0019-1035(85)90002-8.
- Sears, D (2004). The Origin of Chondrules and Chondrites. Cambridge University Press. ISBN 978-1107402850.
- Russell, Sara S.; Ballentine, Chris J.; Grady, Monica M. (17 April 2017). "The origin, history and role of water in the evolution of the inner Solar System". Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences. 375 (2094): 20170108. Bibcode:2017RSPTA.37570108R. doi:10.1098/rsta.2017.0108. PMC 5394259. PMID 28416731.
Water in chondrites is contained within clay minerals, with H2O accounting for up to 10% weight percent...water is also stored in chondrites in direct liquid form as inclusions
- Kaplan, H; Hamilton, V; Howell, E; Anderson, S; Barrucci, M; Brucato, J; Burbine, T; Clark, B; Cloutis, E; Connolly, H; Dotto, E; Emery, J; Fornasier, S; Lantz, C; Lim, L; Merlin, F; Praet, A; Reuter, D; Sandford, S; Simon, A; Takir, D; Lauretta, D (2020). "Visible-near infrared spectral indices for mapping mineralogy and chemistry with OSIRIS-REx". Meteoritics & Planetary Science. 55 (4): 744–65. Bibcode:2020M&PS...55..744K. doi:10.1111/maps.13461.
- Potin, S; Beck, P; Usui, F; Bonal, L; Vernazza, P; Schmidtt, B (September 2020). "Style and intensity of hydration among C-complex asteroids: A comparison to desiccated carbonaceous chondrites". Icarus. 348: article 113826. arXiv:2004.09872. Bibcode:2020Icar..34813826P. doi:10.1016/j.icarus.2020.113826. S2CID 216036128.
- Praet, A; Barucci, M; Kaplan, H; Merlin, F; Clark, B; Simon, A; Hamilton, V; Emery, J; Howell, E; Lim, L (March 2020). Estimated hydration of Bennu's surface from OVIRS observations by the OSIRIS-REx mission. 51st LPSC.
- Simon, A A; Kaplan, H H; Hamilton, V E; Lauretta, D S; Campins, H; Emery, J P; Barucci, M A; DellaGiustina, D N; Reuter D C; Sandford S A; Golish D R; Lim L F; Ryan A; Rozitis B; Bennett C A (8 October 2020). "Widespread carbon-bearing materials on near-Earth asteroid (101955) Bennu" (PDF). Science. 370 (6517): eabc3522. doi:10.1126/science.abc3522. PMID 33033153.
water-rich, similar to the CM class of chondrites
- Nuth, III, J; Abreu, N; Ferguson, F; Glavin, D; Hergenrother, C; Hill, H; Johnson, N; Pajola, M; Walsh, K (December 2020). "Volatile-rich Asteroids in the Inner Solar System". Planetary Science Journal. 1 (3): 82. doi:10.3847/PSJ/abc26a.
- Connolly, H; Jawin, E; Ballouz, R; Walsh, K; McCoy, T; Dellagiustina, D (2019). OSIRIS-REx sample science and the geology of active asteroid Bennu. 82nd Meteoritical Society Meeting. p. 2157.
- Lim, L (2019). OSIRIS-REx update. 21st NASA Small Bodies Assessment Group. "Bennu is an Active Asteroid!"
- Barrucci, M; Michel, P (September 2019). Asteroid-Comet continuum: no doubt but many questions. 2019 EPSC-DPS conference. pp. 202–1.
- Hergenrother, C; Adam, C; Antreasian, P; Al Asad, M; Balram-Knutson, S (September 2019). (101955) Bennu is an active asteroid. 2019 EPSC-DPS conference. pp. 852–1.
- "Feb 11, 2019". Retrieved 15 November 2019.
- Hergenrother, C; Maleszweski, C; Nolan, C; Li, J; Drouet D'aubigny, C (19 March 2019). "The Operational Environment and Rotational Acceleration of Asteroid (101955) Bennu from OSIRIS-REx Observations". Nature Communications. 10 (1): 1291. Bibcode:2019NatCo..10.1291H. doi:10.1038/s41467-019-09213-x. PMC 6425024. PMID 30890725.
- No One Knows Why Rocks Are Exploding From Asteroid Bennu. Daniel Oberhaus, Wired. 5 December 2019.
- Lauretta, D. S.; Hergenrother, C. W.; Chesley, S. R.; Leonard, J. M.; Pelgrift, J. Y.; et al. (6 December 2019). "Episodes of particle ejection from the surface of the active asteroid (101955) Bennu" (PDF). Science. 366 (6470): eaay3544. Bibcode:2019Sci...366.3544L. doi:10.1126/science.aay3544. PMID 31806784. S2CID 208764910..
- "Definitions of terms in meteor astronomy" (PDF). Retrieved 31 July 2020.
- Grun, E; Krüger, H; Srama, R (2019). "The Dawn of Dust Astronomy". Space Science Reviews. 215 (7): 46. arXiv:1912.00707. Bibcode:2019SSRv..215...46G. doi:10.1007/s11214-019-0610-1. S2CID 208527737. 3. Multifaceted Scientific Dust Observations
- Boe, B; Jedicke, R; Wiegert, P; Meech, K; Morbidelli, A (September 2019). Distinguishing Between Solar System Formation Models with Manxes (or not). 2019 EPSC-DPS conference. pp. 626–2.
- Gounelle, M (2012). The Asteroid-Comet Continuum: Evidence from Extraterrestrial Samples. 2012 European Planetary Science Congress. p. 220.
- Rickman, H (2018). Origin and Evolution of Comets: Ten Years after the Nice Model, One Year after Rosetta. Singapore: World Scientific. pp. 162–68. Sec. 4.3 Dormancy and Rejuvenation
- Nuth, J; Johnson, N; Abreu, N (March 2019). Are B-type Asteroids Dormant Comets? (PDF). 50th LPSC. p. 2132.
- Schroder, S; Poch, I; Ferrari, M; De Angelis, S; Sultana, R (September 2019). Experimental evidence for the nature of Ceres blue material (PDF). 2019 EPSC-DPS conference. Epsc-DPS Joint Meeting 2019. 2019. pp. EPSC–DPS2019–78. Bibcode:2019EPSC...13...78S.
- Marsset, M; DeMeo, F; Polishook, D; Binzel, R (September 2019). Near-infrared spectral variability on the newly active asteroid (6478) Gault. 2019 EPSC-DPS conference. Epsc-DPS Joint Meeting 2019. 2019. pp. EPSC-DPS2019-280. Bibcode:2019EPSC...13..280M.
- Fukai, R; Arakawa, S (2021). "Assessment of Cr isotopic heterogeneities of volatile-rich asteroids based on multiple planet formation models". The Astrophysical Journal. 908: 64. arXiv:2012.05467. doi:10.3847/1538-4357/abd2b9.
- Bauer, G (2019). Active Asteroids (PDF). 21st NASA Small Bodies Assessment Group.
- Chang, Kenneth; Stirone, Shannon (19 March 2019). "The Asteroid Was Shooting Rocks Into Space. 'Were We Safe in Orbit?' - NASA's Osiris-Rex and Japan's Hayabusa2 spacecraft reached the space rocks they are surveying last year, and scientists from both teams announced early findings on Tuesday (03/19/2019)". The New York Times. Retrieved 21 March 2019.
- "Asteroid's Features to be Named After Mythical Birds". 8 August 2019.
- Davis, Jason (15 August 2019). "OSIRIS-REx Team Picks 4 Candidate Sample Sites on Asteroid Bennu". The Planetary Society. Retrieved 24 May 2021.
- "First Official Names Given to Features on Asteroid Bennu". AsteroidMission.org. NASA. 6 March 2020. Retrieved 6 May 2020.
- "CANDIDATE SAMPLE SITES". AsteroidMission.org. NASA. Retrieved 2 January 2019.
- "X Marks the Spot: Sample Site Nightingale Targeted for Touchdown" (Press release). AsteroidMission.org. NASA. 12 December 2019. Retrieved 28 December 2019.
- "Bennu". Gazetteer of Planetary Nomenclature. International Astronomical Union. Archived from the original on 7 May 2020. Retrieved 6 May 2020.
- Bensby, T.; Feltzing, S. (2006). "The origin and chemical evolution of carbon in the Galactic thin and thick discs" (PDF). Monthly Notices of the Royal Astronomical Society. 367 (3): 1181–1193. arXiv:astro-ph/0601130. Bibcode:2006MNRAS.367.1181B. doi:10.1111/j.1365-2966.2006.10037.x. S2CID 7771039.
- Bottke, William F.; et al. (February 2015), "In search of the source of asteroid (101955) Bennu: Applications of the stochastic YORP model", Icarus, 247: 191–217, Bibcode:2015Icar..247..191B, doi:10.1016/j.icarus.2014.09.046.
- Ballouz R, Walsh KJ, Barnouin OS, Lauretta DS (2020). "Bennu's near-Earth lifetime of 1.75 million years inferred from craters on its boulders" (PDF). Nature. 5 (587): 205–209. doi:10.1038/s41586-020-2846-z. PMID 33106686.
- Lauretta, D. S.; 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, Bibcode:2015M&PS...50..834L, CiteSeerX 10.1.1.723.9955, doi:10.1111/maps.12353.
- Hergenrother, C (12 December 2013). "The Strange Life of Asteroid Phaethon – Source of the Geminid Meteors". Dslauretta: Life on the Asteroid Frontier. Archived from the original on 24 March 2019. Retrieved 25 July 2019.
- Maltagliati, L (24 September 2018). "Cometary Bennu?". Nature Astronomy. 2 (10): 761. Bibcode:2018NatAs...2..761M. doi:10.1038/s41550-018-0599-5. S2CID 189930305.
- "Horizons Batch for Bennu 2196-09-24 07:55 Virtual Impactor Time". JPL Horizons. Retrieved 10 April 2021. RNG_3sigma = uncertainty range in km. (JPL#97/Soln.date: 2018-May-19 generates RNG_3sigma = 366952778 for 2196-Sep-24 07:55.)
- "(101955) Bennu Ephemerides for 24 September 2196". NEODyS (Near Earth Objects – Dynamic Site). Archived from the original on 28 March 2021. Retrieved 28 March 2021.
- Robert Marcus; H. Jay Melosh & Gareth Collins (2010). "Earth Impact Effects Program". Imperial College London / Purdue University. Retrieved 7 February 2013. (solution using density of 2,600 kg/m^3, sped of 17km/s, and impact angle of 45 degrees)
- 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:0901.3631. Bibcode:2009Icar..203..460M. doi:10.1016/j.icarus.2009.05.029. S2CID 54594575.
- 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:1402.5573. Bibcode:2014Icar..235....5C. doi:10.1016/j.icarus.2014.02.020. ISSN 0019-1035. S2CID 30979660.
- "(101955) Bennu Ephemerides for September 2060". NEODyS (Near Earth Objects – Dynamic Site). Retrieved 15 May 2019.
- Paul Chodas (24 March 2018). "Recent Bennu Press Stories Need Correction". Center for NEO Studies (CNEOS).
- "(101955) Bennu Ephemerides for 25 September 2175". NEODyS (Near Earth Objects – Dynamic Site). Retrieved 26 October 2020.
- Ye, Quanzhi (2019). "Prediction of Meteor Activities from (101955) Bennu" (PDF). American Astronomical Society. 3 (3): 56. Bibcode:2019RNAAS...3...56Y. doi:10.3847/2515-5172/ab12e7.
- Wall, Mike (10 December 2018). "Asteroid Bennu Had Water! NASA Probe Makes Tantalizing Find". Space.com. Retrieved 6 January 2019.
- "Touching the Asteroid" (video, 54:03 min.), Nova on PBS, 21 October 2020. Retrieved 20-10-22.
- "NASA to Launch New Science Mission to Asteroid in 2016". NASA. 25 May 2011. Retrieved 21 May 2013.
- "NASA's OSIRIS-REx Completes Final Tour of Asteroid Bennu". NASA. 7 April 2021. Retrieved 10 May 2021.
- Near-Earth Asteroid Delta-V for Space Rendezvous
- "Why Bennu?". OSIRIS-REx Mission. Arizona Board of Regents. Retrieved 10 September 2016.
|Wikimedia Commons has media related to 101955 Bennu.|
- Video (2:53) – Asteroid Bennu Mission Overview (NASA; 11 May 2021).
- Video (01:12) – Asteroid Bennu ejecting material into space (CNN; 5 December 2019)
- Video (01:32) – OSIRIS REx's approach to asteroid Bennu (NASA; 7 January 2019)
- Earth Impact Risk Summary: 101955 1999 RQ36 (Years: 2175–2199) – Jet Propulsion Laboratory near-Earth object site
- NEODyS-2 Ephemerides for 2135 (step size: 10 days)
- Delbo, Marco; Michel, Patrick (2011). "Temperature History and Dynamical Evolution of (101955) 1999 Rq 36: A Potential Target for Sample Return from a Primitive Asteroid". The Astrophysical Journal. 728 (2): L42. Bibcode:2011ApJ...728L..42D. doi:10.1088/2041-8205/728/2/L42.
- Hergenrother, Carl W.; et al. (2012). "Physical Properties of OSIRIS-REx Target Asteroid (101955) 1999 RQ36 derived from Herschel, ESO-VISIR and Spitzer observations". Astronomy & Astrophysics. 548: A36. arXiv:1210.5370. Bibcode:2012A&A...548A..36M. doi:10.1051/0004-6361/201220066. S2CID 55689658.
- Hergenrother, Carl W.; et al. (2014). "The Design Reference Asteroid for the OSIRIS-REx Mission Target (101955) Bennu". arXiv:1409.4704 [astro-ph.EP].
- 101955 Bennu at NeoDyS-2, Near Earth Objects—Dynamic Site
- 101955 Bennu at the JPL Small-Body Database