Relevant bibliographies by topics / Bennu

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Bennu'

Author: Grafiati
Published: 10 March 2023

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Journal articles on the topic "Bennu"

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Stewart, Arthur J. "Asteroid Bennu." Hoosier Science Teacher 44, no. 1 (November 5, 2021): 14. http://dx.doi.org/10.14434/thst.v44i102.

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This poem, Asteroid Bennu, highlights the essence of a common scientific pathway: as surprise finding, followed by a careful analysis that culminates in an either-or type of outcome, usually testable as a hypothesis.
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Maltagliati, Luca. "Cometary Bennu?" Nature Astronomy 2, no. 10 (September 24, 2018): 761. http://dx.doi.org/10.1038/s41550-018-0599-5.

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Włodarczyk, I. "The Potentially Dangerous Asteroid (101955) Bennu." Physics Research International 2014 (December 15, 2014): 1–13. http://dx.doi.org/10.1155/2014/561680.

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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.
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Fornasier, S., P. H. Hasselmann, J. D. P. Deshapriya, M. A. Barucci, B. E. Clark, A. Praet, V. E. Hamilton, et al. "Phase reddening on asteroid Bennu from visible and near-infrared spectroscopy." Astronomy & Astrophysics 644 (December 2020): A142. http://dx.doi.org/10.1051/0004-6361/202039552.

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Context. The NASA mission OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer) has been observing near-Earth asteroid (101955) Bennu in close proximity since December 2018. In October 2020, the spacecraft collected a sample of surface material from Bennu to return to Earth. Aims. In this work, we investigate spectral phase reddening – that is, the variation of spectral slope with phase angle – on Bennu using spectra acquired by the OSIRIS-REx Visible and InfraRed Spectrometer (OVIRS) covering a phase angle range of 8–130°. We investigate this process at the global scale and for some localized regions of interest (ROIs), including boulders, craters, and the designated sample collection sites of the OSIRIS-REx mission. Methods. Spectra were wavelength- and flux-calibrated, then corrected for the out-of-band contribution and thermal emission, resampled, and finally converted into radiance factor per standard OVIRS processing. Spectral slopes were computed in multiple wavelength ranges from spectra normalized at 0.55 μm. Results. Bennu has a globally negative spectra slope, which is typical of B-type asteroids. The spectral slope gently increases in a linear way up to a phase angle of 90°, where it approaches zero. The spectral phase reddening is monotonic and wavelength-dependent with highest values in the visible range. Its coefficient is 0.00044 μm−1 deg−1 in the 0.55–2.5 μm range. For observations of Bennu acquired at high phase angle (130°), phase reddening increases exponentially, and the spectral slope becomes positive. Similar behavior was reported in the literature for the carbonaceous chondrite Mukundpura in spectra acquired at extreme geometries. Some ROIs, including the sample collection site, Nightingale, have a steeper phase reddening coefficient than the global average, potentially indicating a surface covered by fine material with high micro-roughness. Conclusions. The gentle spectral phase reddening effect on Bennu is similar to that observed in ground-based measurements of other B-type asteroids, but much lower than that observed for other low-albedo bodies such as Ceres or comet 67P/Churyumov-Gerasimenko. Monotonic reddening may be associated with the presence of fine particles at micron scales and/or of particles with fractal structure that introduce micro- and sub-micro roughness across the surface of Bennu.
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Hanna, Kerri Donaldson. "Playing TAG with Bennu." Astronomy & Geophysics 62, no. 1 (February 1, 2021): 1.14–1.18. http://dx.doi.org/10.1093/astrogeo/atab038.

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Simon, A. A., H. H. Kaplan, E. Cloutis, V. E. Hamilton, C. Lantz, D. C. Reuter, D. Trang, S. Fornasier, B. E. Clark, and D. S. Lauretta. "Weak spectral features on (101995) Bennu from the OSIRIS-REx Visible and InfraRed Spectrometer." Astronomy & Astrophysics 644 (December 2020): A148. http://dx.doi.org/10.1051/0004-6361/202039688.

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Context. The NASA Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer (OSIRIS-REx) mission has obtained thousands of spectra of asteroid (101955) Bennu with the OSIRIS-REx Visible and InfraRed Spectrometer. Aims. We present a spectral search for minor absorption bands and determine compositional variations on the surface of Bennu. Methods. Reflectance spectra with low and high spatial resolutions were analyzed for evidence of weak absorption bands. Spectra were also divided by a global average spectrum to isolate unique spectral features, and variations in the strongest band depths were mapped on a surface shape model. The global visible to near-IR spectrum of Bennu shows evidence of several weak absorption bands with depths of a few percent. Results. Several observed bands are consistent with phyllosilicates, and their distribution correlates with the stronger 2.74-μm hydration band. A 0.55-μm band is consistent with iron oxides and is deepest in the spectrally reddest areas on Bennu. The presence of hydrated phyllosilicates and iron oxides indicates substantial aqueous alteration in Bennu’s past. Conclusions. Bennu’s spectra are not identical to a limited set of carbonaceous chondrite spectra, possibly due to compositional properties and spatial scale differences; however, returned samples should contain a mixture of common chondrite materials.
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Edmundson, K. L., K. J. Becker, T. L. Becker, C. A. Bennett, D. N. DellaGiustina, D. R. Golish, N. A. Porter, et al. "PHOTOGRAMMETRIC PROCESSING OF OSIRIS-REX IMAGES OF ASTEROID (101955) BENNU." ISPRS Annals of Photogrammetry, Remote Sensing and Spatial Information Sciences V-3-2020 (August 3, 2020): 587–94. http://dx.doi.org/10.5194/isprs-annals-v-3-2020-587-2020.

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Abstract. The principal objective of the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) mission is to retrieve a sample of the asteroid (101955) Bennu and return it to Earth. OSIRIS-REx arrived at Bennu in December 2018. Images of the asteroid by the OSIRIS-REx Camera Suite (OCAMS) were photogrammetrically controlled to produce a global basemap and site-specific image mosaics essential to the selection of a primary and backup sample site, which were announced in December 2019. In the control process, OCAMS images were registered to shape models created from OSIRIS-REx Laser Altimeter (OLA) data and from the process of stereophotoclinometry. This paper summarizes the photogrammetric control to date of images collected at Bennu. We briefly review the mission and the OCAMS imaging sensors. We then describe the photogrammetric control process for the global mapping campaign and targeted reconnaissance surveys of candidate sample sites. Finally, we discuss ongoing and future work.
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Merlin, F., J. D. P. Deshapriya, S. Fornasier, M. A. Barucci, A. Praet, P. H. Hasselmann, B. E. Clark, et al. "In search of Bennu analogs: Hapke modeling of meteorite mixtures." Astronomy & Astrophysics 648 (April 2021): A88. http://dx.doi.org/10.1051/0004-6361/202140343.

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Context. The OSIRIS-REx Visible and InfraRed Spectrometer onboard the Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer spacecraft obtained many spectra from the surface of the near-Earth asteroid (101955) Bennu, enabling the characterization of this primitive small body. Bennu is spectrally similar to the hydrated carbonaceous chondrites (CCs), but questions remain as to which CCs, or combinations thereof, offer the best analogy to its surface. Aims. We aim to understand in more detail the composition and particle size of Bennu’s surface by refining the relationship between this asteroid and various CC meteorites. Methods. We used published absorbance and reflectance data to identify new optical constants for various CC meteorites measured in the laboratory at different temperatures. We then used the Hapke model to randomly generate 1000 synthetic spectra in order to find the combinations of these potential meteoritic analogs that best reproduce the spectral features of the asteroid. Results. Our investigations suggest that the surface of Bennu, though visibly dominated by boulders and coarse rubble, is covered by small particles (tens to a few hundreds of μm) and that possibly dust or powder covers the larger rocks. We further find that the surface is best modeled using a mixture of heated CM, C2-ungrouped, and, to some extent, CI materials. Conclusions. Bennu is best approximated spectrally by a combination of CC materials and may not fall into an existing CC group.
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Crane, Leah. "Up close with asteroid Bennu." New Scientist 240, no. 3207 (December 2018): 12. http://dx.doi.org/10.1016/s0262-4079(18)32238-3.

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Henshall, Tom. "The surface of asteroid Bennu." Nature Reviews Materials 4, no. 4 (March 22, 2019): 228. http://dx.doi.org/10.1038/s41578-019-0102-7.

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Dissertations / Theses on the topic "Bennu"

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Uribe, Suarez Diego Alejandro. "Combinaison d’éléments cohésifs et remaillage pour gérer la propagation arbitraire du chemin de fissure : des matériaux fragiles à l’analyse de fatigue thermique des petits corps du système solaire." Thesis, Université Côte d'Azur, 2021. http://www.theses.fr/2021COAZ4047.

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La présente thèse de doctorat a pour objectif d’améliorer la modélisation du phénomène de rupture dans les matériaux fragiles. Elle porte une attention particulière aux mécanismes de rupture des objets célestes. L’un des problèmes posant le plus de défis aux scientifiques spécialisés dans l’étude de la mécanique de la rupture est la propagation d’une fissure dans un maillage éléments finis, et ce pour des chemins arbitraires. Dans cette étude, ce problème est abordé en utilisant une technique de remaillage avancée utilisant des éléments finis cohésifs permettant la propagation de fissures suivant des directions arbitraires et indépendantes du maillage. La direction de la fissure est calculée suivant le critère du taux de restitution d’énergie maximal, implémentée à l’aide d’un modèle éléments finis et de la méthode Gθ. Les effets de différents paramètres numériques et physiques relatifs à la fissure ou à l’énergie libérée lors de la rupture sont investigués.Bien que différentes preuves de fissures et/ou fragments à la surface de corps célestes de notre système solaire induits par des variations cycliques de la température ont été détaillées, la compréhension de ces mécanismes de propagation dans des objets célestes reste très parcellaire. La fracturation thermique de roches en surface associée à l’impact de micro-météorites peutéventuellement conduire à la rupture complète de fragments de matière et à la production de régolithes. Cette dernière est définie comme la couche de matériau non consolidée qui recouvre la surface des planètes. Afin de comprendre ces mécanismes, l’étude s’attarde sur un exemple précis, celui de l’astéroïde (101955) Bennu. Pour ce faire, elle utilise un modèle thermoélastique couplé avec un modèle linéaire élastique de mécanique de la rupture permettant de considérer les variations cycliques de température liées aux alternances jour/nuit. En utilisant cette méthodologie, il a été observé que les fissures se propagent préférentiellement dans les directions : Nord vers Sud, Nord-Est vers Sud-Ouest et Nord-Ouest vers Sud-Est. Finalement, une analyse de fatigue est effectuée afin d’estimer la vitesse de croissance de la fissure.Les méthodes détaillées précédemment ont été implémentées dans Cimlib, une librairie C++ dévelopée au CEMEF. Au sein de cette librairie, une méthode permettant la propagation d’une ou plusieurs fissures, suivant des directions arbitraires, en 2D et au sein d’un environnement de calcul en parallèle est à présent disponible. Concernant l’extension de cette méthode à des problèmes 3D, une première approche a été mise au point. Elle permet de propager un front de fissure suivant une direction arbitaire. La structure développée permet d’ouvrir de nouvelles possibilités pour de nombreuses applications, telles que l’étude de la rupture de matériaux composites à l’échelle mesoscopique
The present PhD thesis aims at providing a better modeling of fracture phenomenon in brittle materials, with special attention focused on fracture processes taking place in astronomical bodies. One of the most challenging issues in computational fracture mechanics is the propagation of a crack through a finite element mesh for arbitrary crack paths. In this work, this problem is approached by means of an advanced remeshing technique that propagates a crack using cohesive elements through arbitrary directions (mesh-independent). The crack direction is computed using the maximal energy release rate criterion which is implemented using finite elements and the Gθ method. The effects of different numerical and physical parameters regarding the crack path and fracture energy have been investigated. Even though it has been shown that temperature cycles on airless bodies of our Solar System can cause damaging of surface materials (Thermal cracking), propagation mechanisms in the case of space objects are still poorly understood. Thermal cracking of surface rocks, in addition to the impact of micrometeorties, can eventually lead to rocks’ breakup and produce fresh regolith, the latter being the layer of unconsolidated material that covers planetary surfaces. For this reason, the present work combines a thermoelasticity model together with linear elastic fracture mechanics theory to predict fracture propagation in the presence of thermal gradients generated by diurnal temperature cycling and under conditions similar to those existing on asteroid (101955) Bennu. Using the implemented methodologies, it is found that in asteroid Bennu, cracks preferentially propagate in the North to South (N-S), in the North-East to South-West (NE-SW) and in the North-West to South-East (NW-SE) directions. Finally, thermal fatigue analysis was performed in order to estimate the crack growth rate.Aforementioned methodologies have been implemented in Cimlib, a C++ in-house finite element library developed at CEMEF. Inside Cimlib, a methodology allowing two-dimensional crack propagation through arbitrary directions with the option of handling multiple cracks in the domain and inside a parallel environment was developed. Regarding three-dimensional scenario, a first approach where a crack front was propagated through an arbitrary direction was achieved. Concerning numerical modeling of crack propagation, the developed framework opens new possibilities for various applications such as composites cracking at the meso-scale
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Solf, Mark-Alexander [Verfasser], Walter Benno [Akademischer Betreuer] [Gutachter] Eichinger, and Rüdiger [Gutachter] Lange. "Psychoherzchirurgie - Krankheitsverarbeitung kardiochirurgischer Patienten / Mark Alexander Solf. Betreuer: Walter Benno Eichinger. Gutachter: Walter Benno Eichinger ; Rüdiger Lange." München : Universitätsbibliothek der TU München, 2016. http://d-nb.info/1105646599/34.

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Pignol, Alexandra. "Gottfried Benn : poésie et philosophie." Université Marc Bloch (Strasbourg) (1971-2008), 2002. http://www.theses.fr/2002STR20036.

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Gottfried Benn est connu pour son oeuvre poétique. Il est pourtant aussi nouvelliste et essayiste : c'est dans ses essais qu'il élabore une poétique du faire, une poi͏̈étique. Les questions qu'il pose sont d'ordre philosophique. Pourquoi ? Parce que Benn considère que l'art permet de dépasser la fin de la métaphysique. Benn affirme que l'art, la création sont une manière de surmonter le nihilisme. Puisque le nihilisme a détruit tous les contenus, il reste la forme. "Les formes". . . , c'est là l'important, voilà le fin mot de sa morale. Ce qu'elles sont reste à décider mais sûrement quelque chose de très élémentaire : rythme, tension, "processus,. . . " (Double vie, p. 160). Gottfried Benn veut créer une poétique de la forme. Une poétique doit pour lui tenir compte de cette réalité élémentaire et essentielle à la fois ; la création est un processus, l'oeuvre d'art est un faire. C'est une poi͏̈étique, faite de tensions, de rythmes, qui expriment le moi lyrique. .
Gottfried Benn is a well known writer because of his poetry. But he is also a short-story-writer as well as an essayist. In his essays, he elaborates a poetic of making, a poi͏̈esis. The questions he asks are philosophical. Why ? Because Benn considers that art is the way of going beyond the end of metaphysics. Benn states positively that art, creation are a way of surmounting nihilism. .
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Rosch, Laura [Verfasser], Benno [Akademischer Betreuer] Weigmann, and Benno [Gutachter] Weigmann. "Molekulare Analyse des Januskinase-Inhibitors Tofacitinib in chronisch entzündlichen Darmerkrankungen / Laura Rosch ; Gutachter: Benno Weigmann ; Betreuer: Benno Weigmann." Erlangen : Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), 2021. http://d-nb.info/1238898858/34.

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Gaspar, Paulo Jorge Fialho. "Benny Goodman: o clarinete e a improvisação." Doctoral thesis, Universidade de Évora, 2010. http://hdl.handle.net/10174/17584.

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Benny Goodman é uma referência essencial no contexto da ambivalência musical. Enquanto desenvolvia uma carreira brilhante no contexto do jazz, Goodman teve sempre uma estreita relação com a música e os compositores eruditos, da qual resultaram algumas das obras do repertório para clarinete mais importantes da História. Esta dissertação pretende mostrar esta ambivalência de Goodman através de três aspectos essenciais: (1) interpretação do repertório que lhe foi dedicado, (2) o seu estilo enquanto improvisador e (3) a sua contribuição para o ensino. Pretende-se fazer uma reflexão sobre o pensamento do intérprete sobre as práticas a incorporar na performance do repertório tradicional e daquele com influências do jazz, bem como sobre as ferramentas para o desenvolvimento da capacidade de improvisação em diversos estilos musicais. Em jeito de conclusão será apontada uma proposta metodológica para o ensino do clarinete, que poderá também ser útil no ensino de outros instrumentos; ABSTRACT:Benny Goodman is an essential reference within the concept of musical ambivalence. While developing a brilliant jazz career, Goodman always had a close relationship with classical musicians and composers, which resulted in some of the most important works of the repertoire for clarinet. This thesis intends to show Goodman's ambivalence through three essential aspects: (1) the interpretation of the repertoire that was dedicated to him, (2) his improvisational style, and (3) his contribution to education. A reflection is made on the performer’s concepts regarding the performance practice of the classical and jazz repertoire, as well as the tools to allow the development of improvisational abilities in different music genres. In the final part it is presented a methodology for clarinet teaching, which may also be useful when teaching other instruments.
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Willke, Benno [Verfasser]. "Stabilisierte Festkörperlaser hoher Leistung für Gravitationswellenmessungen / Benno Willke." Hannover : Technische Informationsbibliothek und Universitätsbibliothek Hannover (TIB), 2011. http://d-nb.info/1017334862/34.

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Zerlin, Benno [Verfasser]. "CLARA : Cross-Layer Assisted Resource Allocation / Benno Zerlin." Aachen : Shaker, 2007. http://d-nb.info/1170535321/34.

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Kjar, Renée Giay Benny. "The invisible aristocrat Benny Giay in Papuan history /." [Sydney, Australia] : Australiann National University, Discipline of Asian Studies, 2002. http://www.papuaweb.org/dlib/s123/kjar/%5Fba.pdf.

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Thesis (B.A.)--Discipline of Asian Studies, Australian National University, 2002.
Title from thesis home page (viewed Dec. 6, 2004). Title from start screen (viewed Aug. 19, 2004). "December 2002."
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Burger, Hilda Martine. "De zandloper van Genesis de visie van Benno Jacob op Genesis 22 in het licht van zijn tijd en van de Traditie /." [Zoetermeer : Amsterdam : Boekencentrum] ; Universiteit van Amsterdam [Host], 2002. http://dare.uva.nl/document/62150.

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Chi, Wu-Chen Anne. "Not just the "king of swing" : Benny Goodman's classical style." Thesis, Connect to this title online; UW restricted, 2000. http://hdl.handle.net/1773/11376.

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Books on the topic "Bennu"

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Rāmacandran, Si En. Neraḷugaḷa bennu hatti: Ātmakathana. Beṅgaḷūru: Aṅkita Pustaka, 2013.

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Benny, Benny baseball nut. New York: Scholastic, 1987.

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Benn. Frankfurt am main: Fischer, 1986.

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Hillebrand, Bruno. Benn. Frankfurt am Main: Fischer, 1986.

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Rest, Franz, Astrid Spatzier, and Stefan Wehmeier, eds. Benno Signitzer. Wiesbaden: Springer Fachmedien Wiesbaden, 2013. http://dx.doi.org/10.1007/978-3-658-03505-1.

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Benny & Shrimp. London: Short, 2008.

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Preminger, Miḳi. Boḳer benenu. Tel-Aviv: ʻEḳed, 1988.

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Gbana-Bendu. Alexandria, VA: Alexander Street Press, 2002.

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Lawrence, Elizabeth. Benny Bear. Walton-on-Thames: Nelson, 1986.

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Crowther, Bruce. Benny Goodman. London: Apollo, 1988.

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Book chapters on the topic "Bennu"

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Levasseur-Regourd, Anny-Chantal. "Bennu Asteroid." In Encyclopedia of Astrobiology, 1–2. Berlin, Heidelberg: Springer Berlin Heidelberg, 2022. http://dx.doi.org/10.1007/978-3-642-27833-4_5564-1.

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Wild, Gerhard. "Benni, Stefano." In Kindlers Literatur Lexikon (KLL), 1. Stuttgart: J.B. Metzler, 2020. http://dx.doi.org/10.1007/978-3-476-05728-0_2709-1.

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Strauß, Frithjof. "Andersen, Benny." In Kindlers Literatur Lexikon (KLL), 1. Stuttgart: J.B. Metzler, 2020. http://dx.doi.org/10.1007/978-3-476-05728-0_4480-1.

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Gooch, Jan W. "Benne Oil." In Encyclopedic Dictionary of Polymers, 73. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4419-6247-8_1201.

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Ridley, Hugh. "Benns Leben." In Gottfried Benn, 13–31. Wiesbaden: VS Verlag für Sozialwissenschaften, 1990. http://dx.doi.org/10.1007/978-3-322-91526-9_2.

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Zabrucky, Karen M., Rebecca B. Bays, David L. Seim, Kevin Rustam, David C. Devonis, Debbie Joffe Ellis, David C. Devonis, et al. "Erdmann, Benno." In Encyclopedia of the History of Psychological Theories, 396–98. New York, NY: Springer US, 2012. http://dx.doi.org/10.1007/978-1-4419-0463-8_90.

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Schroeder, David. "Benny Golson." In From the Minds of Jazz Musicians, 44–53. New York, NY : Routledge, 2018.: Routledge, 2017. http://dx.doi.org/10.4324/9781315282572-9.

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Seldes, Gilbert. "Mr. Benny." In The Public Arts, 153–57. New York: Routledge, 2021. http://dx.doi.org/10.4324/9780429339325-17.

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Rest, Franz, Astrid Spatzier, and Stefan Wehmeier. "Benno Signitzer: Wirken und Werk eines Pioniers." In Benno Signitzer, 7–14. Wiesbaden: Springer Fachmedien Wiesbaden, 2013. http://dx.doi.org/10.1007/978-3-658-03505-1_1.

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Spatzier, Astrid, and Benno Signitzer. "Reconsidering Contemporary Public Relations: Theoretical Engagement of Practitioners in a Communication Society." In Benno Signitzer, 199–215. Wiesbaden: Springer Fachmedien Wiesbaden, 2013. http://dx.doi.org/10.1007/978-3-658-03505-1_10.

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Conference papers on the topic "Bennu"

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Elkins, Kel, Dan Gallagher, Adriana Manrique Gutierrez, Jonathan North, and Ernie Wright. "@Tour of Asteroid Bennu." In SIGGRAPH '21: Special Interest Group on Computer Graphics and Interactive Techniques Conference. New York, NY, USA: ACM, 2021. http://dx.doi.org/10.1145/3446562.3456718.

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Elkins, Kel, Daniel Gallagher, Greg Shirah, and Ernie Wright. "A web around asteroid bennu." In SIGGRAPH '22: Special Interest Group on Computer Graphics and Interactive Techniques Conference. New York, NY, USA: ACM, 2022. http://dx.doi.org/10.1145/3512752.3526118.

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Scheeres, Daniel J., Daniel Wibben, Peter G. Antreasian, Kenneth M. Getzandanner, Shota Takahashi, Jay W. McMahon, and Dante Lauretta. "The Dynamics about Asteroid (101955) Bennu." In AIAA SCITECH 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-2468.

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Englert, Matthias. "Modeling Asteroid (101955) Bennu as a Real-time Terrain." In SIGGRAPH '21: Special Interest Group on Computer Graphics and Interactive Techniques Conference. New York, NY, USA: ACM, 2021. http://dx.doi.org/10.1145/3450623.3464628.

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Antreasian, Peter G., Coralie D. Adam, Kevin Berry, Jeroen Geeraert, Kenneth M. Getzandanner, Dolan Highsmith, Jason M. Leonard, et al. "OSIRIS-REx Proximity Operations and Navigation Performance at Bennu." In AIAA SCITECH 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-2470.

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Jawin, Erica R., Kevin J. Walsh, Timothy J. McCoy, Harold C. Connolly, Ronald L. Ballouz, Olivier S. Barnouin, Chloe B. Beddingfield, et al. "GLOBAL GEOLOGY OF BENNU FROM NASA'S OSIRIS-REX SPACE MISSION." In GSA Annual Meeting in Phoenix, Arizona, USA - 2019. Geological Society of America, 2019. http://dx.doi.org/10.1130/abs/2019am-332108.

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Groath, Dalton J., John P. Basart, and Bong Wie. "Computational Estimation of the Yarkovsky Effect on Asteroid 101955 Bennu." In AIAA/AAS Astrodynamics Specialist Conference. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2014. http://dx.doi.org/10.2514/6.2014-4145.

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Hamilton, Victoria, A. Simon, H. Kaplan, P. Christensen, D. Reuter, D. DellaGiustina, C. Haberle, L. Breitenfeld, B. Clark, and D. Lauretta. "THE COMPOSITION OF ASTEROID BENNU FROM THE OSIRIS-REX MISSION." In GSA Connects 2021 in Portland, Oregon. Geological Society of America, 2021. http://dx.doi.org/10.1130/abs/2021am-368652.

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Haberle, Christopher, Christopher Edwards, Christian Tai Udovicic, Joshua L. Bandfield, and Ben Clark. "SURFACE ROUGHNESS OF BENNU DERIVED FROM OSIRIS-REX THERMAL EMISSION SPECTROMETER OBSERVATIONS." In GSA Connects 2021 in Portland, Oregon. Geological Society of America, 2021. http://dx.doi.org/10.1130/abs/2021am-367787.

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Leonard, Jason M., Jeroen Geeraert, John Pelgrift, Peter G. Antreasian, Coralie D. Adam, Daniel Wibben, Kenneth M. Getzandanner, Benjamin W. Ashman, and Dante Lauretta. "Navigation Prediction Performance During the OSIRIS-REx Proximity Operations at (101955) Bennu." In AIAA SCITECH 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-2389.

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Reports on the topic "Bennu"

1

Horváth, Kathryn. Versuch einer ästhetischen Wertsetzung: zur Kunsttheorie von Benn und Nietzsche. Portland State University Library, January 2000. http://dx.doi.org/10.15760/etd.923.

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