Relevant bibliographies by topics / Asteroid Dynamics

Contents

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

Academic literature on the topic 'Asteroid Dynamics'

Author: Grafiati
Published: 7 June 2025
Last updated: 2 August 2025

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Journal articles on the topic "Asteroid Dynamics"

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Lobanova, K. S., and A. V. Melnikov. "On perturbations in the rotational motion of an asteroid during its close approach to the Earth." Publications of the Pulkovo Observatory 229 (August 2023): 1–13. http://dx.doi.org/10.31725/0367-7966-2023-229-5.

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By means of numerical simulation of the rotational dynamics of the asteroid (99942)Apophis, the perturbations occurring in the rotational motion of asteroids during their close approaches to the Earth are studied. It has been established that such events can lead to significant changes in the asteroid's own rotation velocity and the orientation of its rotation axis in space. The dependences of the change in the period of rotation of the asteroid on the parameters of the orbit and its rotational state before approaching the Earth are studied. It is shown that disturbances in the rotational moti
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Ferraz-Mello, S. "Slow and Fast Diffusion in Asteroid-Belt Resonances: A Review." International Astronomical Union Colloquium 172 (1999): 25–37. http://dx.doi.org/10.1017/s0252921100072389.

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AbstractThis paper reviews recent advances in several topics of resonant asteroidal dynamics as the role of resonances in the transportation of asteroids and asteroidal debris to the inner and outer solar system; the explanation of the contrast of a depleted 2/1 resonance (Hecuba gap) and a high-populated 3/2 resonance (Hilda group); the overall stochasticity created in the asteroid belt by the short-period perturbations of Jupiter’s orbit, with emphasis in the formation of significant three-period resonances, the chaotic behaviour of the outer asteroid belt, and the depletion of the Hecuba ga
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Martyusheva, A. A., and A. V. Melnikov. "On the magnitude of the Yarkovsky effect in the dynamics of potentially hazardous asteroids." Publications of the Pulkovo Observatory 228 (May 2023): 1–10. http://dx.doi.org/10.31725/0367-7966-2023-228-11.

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Estimates of the influence of the solar radiation pressure and the Yarkovsky effect on the long-term orbital dynamics are obtained for a number of asteroids experiencing successive approaches to planets. Based on the estimates of the change in the value of the asteroid’s proper rotation period obtained in (Melnikov, 2022) due to its approaches to the planets, the influence of such events on the further orbital dynamics of an asteroid through the Yarkovsky effect is considered. It is shown that close encounters with the planets of small asteroids (tens of meters in diameter) with fast rotation
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Jiang, Yu, Yanshuo Ni, Hexi Baoyin, Junfeng Li, and Yongjie Liu. "Asteroids and Their Mathematical Methods." Mathematics 10, no. 16 (2022): 2897. http://dx.doi.org/10.3390/math10162897.

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In this paper, the basic classification of asteroids and the history and current situation of asteroid exploration are introduced. Furthermore, some recent research progress on the orbital dynamics of asteroids, including models of the gravitational potential field, the dynamics near asteroids, hopping motion on the surface, and bifurcations under varying external parameters, is reviewed. In the meanwhile, the future research development such as the configuration and evolution of binary or triple asteroid systems and near-Earth asteroid defense is briefly discussed.
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Lobanova, K. S., and A. V. Melnikov. "The influence of the rotation speed and shape of an asteroid on the magnitude of disturbances in its rotational dynamics during close approach to the Earth." Publications of the Pulkovo Observatory 233 (June 2024): 39–50. http://dx.doi.org/10.31725/0367-7966-2024-233-39-50.

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By means of numerical experiments, the influence of the value of the asteroid’s own rotational velocity, orientation of the axis of rotation, and figure parameters on the magnitude of perturbations in its rotational dynamics arising during close approach to the Earth is studied. Two cases are considered: 1) asteroid (99942) Apophis with a relatively slow rotation (period ≈ 30 h) and 2) asteroid 2012 TC4, which has a fast rotation (period ≈ 12 min). It was found that in the case of asteroids with slow rotation, perturbations can be large: in the case of Apophis, when approaching the Earth in 20
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Dermott, S. F., and P. D. Nicholson. "Iras Dust Bands and the Origin of the Zodiacal Cloud." Highlights of Astronomy 8 (1989): 259–66. http://dx.doi.org/10.1017/s1539299600007863.

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AbstractPrevious discussions of the origin of the zodiacal cloud have attempted to distinguish between an asteroidal and a cometary source on the basis of collisional dynamics, that is, by calculating the rates of production and destruction of particles from the two possible sources. The uncertainties in these calculations are too large to permit a useful conclusion. The recognition that the solar system dust bands discovered by IRAS are probably produced by the gradual comminution of the asteroids in the major Hirayama asteroid families may allow us to estimate, with comparative confidence, t
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Érdi, B. "On the dynamics of Trojan asteroids." Symposium - International Astronomical Union 172 (1996): 171–76. http://dx.doi.org/10.1017/s0074180900127305.

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The author's theory of Trojan asteroids (Érdi, 1988) is developed further. The motion of the Trojans is considered in the framework of the three-dimensional elliptic restricted three-body problem of the Sun-Jupiter-asteroid system including also the secular changes of Jupiter's orbital eccentricity and the apsidal motion of Jupiter's elliptic orbit. An asymptotic solution is derived, by applying the multiple-timescale method, for the cylindrical coordinates of the asteriods and for the perturbations of the orbital elements. This solution is used for the analysis of the long-time dynamical beha
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Yan, Weifeng, Ruoyu Feng, and Hexi Baoyin. "Stability of a Flexible Asteroid Lander with Landing Control." Aerospace 9, no. 11 (2022): 719. http://dx.doi.org/10.3390/aerospace9110719.

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Stable landing on asteroids is of considerable scientific and economic value but accompanied by huge difficulties. This paper proposes a novel flexible lander suitable for asteroids with microgravity and rugged surface. The gravity model with the artificial neural network and the surface model with the spherical harmonic method are introduced to establish the target asteroid’s dynamical environment. The flexible dynamics with the discrete shell model, the collision with the spring-damping model and viscous sliding friction, and the rigid coupling with the constraint violation stabilization met
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Ershkov, Sergey, and Dmytro Leshchenko. "Inelastic Collision Influencing the Rotational Dynamics of a Non-Rigid Asteroid (of Rubble Pile Type)." Mathematics 11, no. 6 (2023): 1491. http://dx.doi.org/10.3390/math11061491.

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We have considered here a novel particular model for dynamics of a non-rigid asteroid rotation, assuming the added mass model instead of the concept of Viscoelastic Oblate Rotators to describe the physically reasonable response of a ‘rubble pile’ volumetric material of asteroid with respect to the action of a projectile impacting its surface. In such a model, the response is approximated as an inelastic collision in which the projectile pushes the ‘rubble pile’ parts of the asteroid together to form a mostly solidified plug in the crater during the sudden impact on the asteroid’s surface. Afte
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Milic-Zitnik, I. "The relationship between the `limiting' Yarkovsky drift speed and asteroid families' Yarkovsky V-shape." Serbian Astronomical Journal, no. 200 (2020): 25–41. http://dx.doi.org/10.2298/saj2000025m.

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The Yarkovsky effect is an important force to consider in order to understand the long-term dynamics of asteroids. This non-gravitational force affects the orbital elements of objects revolving around a source of heat, especially their semi-major axes. Following the recently defined `limiting' value of the Yarkovsky drift speed at 7x10-5 au/Myr in Milic Zitnik (2019) (below this value of speed asteroids typically jump quickly across the mean motion resonances), we decided to investigate the relation between the asteroid family Yarkovsky V-shape and the `limiting' Yarkovsky drift speed of aster
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Dissertations / Theses on the topic "Asteroid Dynamics"

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Dykhuis, Melissa Joy. "Asteroid Family Dynamics in the Inner Main Belt." Diss., The University of Arizona, 2015. http://hdl.handle.net/10150/565904.

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The inner main asteroid belt is an important source of near-Earth objects and terrestrial planet impactors; however, the dynamics and history of this region are challenging to understand, due to its high population density and the presence of multiple orbital resonances. This dissertation explores the properties of two of the most populous inner main belt family groups - the Flora family and the Nysa-Polana complex - investigating their memberships, ages, spin properties, collision dynamics, and range in orbital and reflectance parameters. Though diffuse, the family associated with asteroid (8
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Anthony, Niklas. "Prometheus Asteroid Redirection Mission : Mission Design, Spacecraft Design, Orbital Dynamics Code Development." Thesis, Luleå tekniska universitet, Institutionen för system- och rymdteknik, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-174.

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This report will design a mission and spacecraft to redirect the first Near-Earth Object (NEO) to a stable orbit in the Earth-Moon system. The mission profile includes a soon-as-possible launch, spiral-out escape from the Earth-Moon system, rendezvous, ion beam redirection method, and decommissioning phases, each with accompanying orbital dynamics code written in Matlab. The spacecraft design will include power and mass budgets for each of the subsystems including power, thermal, communications, GNC, fuel, and thrusters. The orbital dynamics code is detailed in the final section of the report.
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Minton, David A. "Dynamical History of the Asteroid Belt and Implications for Terrestrial Planet Bombardment." Diss., The University of Arizona, 2009. http://hdl.handle.net/10150/194083.

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The main asteroid belt spans ~2-4 AU in heliocentric distance and is sparsely populated by rocky debris. The dynamical structure of the main belt records clues to past events in solar system history. Evidence from the structure of the Kuiper belt, an icy debris belt beyond Neptune, suggests that the giant planets were born in a more compact configuration and later experienced planetesimal-driven planet migration. Giant planet migration caused both mean motion and secular resonances to sweep across the main asteroid belt, raising the eccentricity of asteroids into planet-crossing orbits and d
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Maddock, Christie Alisa. "On the dynamics, navigation and control of a spacecraft formation of solar concentrators in the proximity of an asteroid." Thesis, University of Glasgow, 2010. http://theses.gla.ac.uk/1572/.

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This purpose of this dissertation is to ascertain whether solar sublimation is a viable method for the deflection of a Near Earth Asteroid. From a research view point, the methods and analysis are applicable to proximal motion around a celestial body, in particular one with a non-Keplerian or irregular orbit as in the case here with the orbit being constantly altered by the deflection action and subject to perturbations, such as solar radiation pressure. Two concepts, and the corresponding dynamics and control, are presented based on previous trade-off and optimisation studies. The first uses
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Skoglöv, Erik. "The Dynamical Spin Vector Evolution of the Asteroids." Doctoral thesis, Uppsala University, The Uppsala Astronomical Observatory, 2002. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-2877.

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<p>The dynamical evolution of the spin axis direction due to gravitational and thermal factors is examined. It is found that the spin axis variations generally are regular and relatively small for the bodies in the asteroid main belt. There are also reasons to believe that this is the case for minor objects beyond the main belt. However, it is found that these regular variations are larger when the orbital inclination of the objects is increased. This effect may explain certain features in the spin vector distribution of the main belt asteroids, not possible to explain by collisional factors.
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Bottke, William Frederick Jr. "The collisional and dynamical evolution of asteroids." Diss., The University of Arizona, 1995. http://hdl.handle.net/10150/187125.

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Understanding asteroid collisional and dynamical evolution necessitates the use of statistical methods, since an asteroid's physical and orbital characteristics are modified throughout its lifetime by collisions and planetary perturbations. Thus, my thesis investigates evolutionary trends for asteroids by calculating and applying parameters such as collision probabilities, impact velocities, and collisional and dynamical lifetimes. I found that previous calculations of collision probabilities between pairs of asteroids on independent Keplerian orbits often yielded inconsistent results. By corr
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Cotto-Figueroa, Desireé. "Radiation Recoil Effects on the Dynamical Evolution of Asteroids." Ohio University / OhioLINK, 2013. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1380464245.

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Lecomte, Charles-Edouard. "Instabilités dans un milieu granulaire : tôle ondulée sur un lit de sable, et ségrégation au sein des astéroïdes lâches." Thesis, Lyon, 2018. http://www.theses.fr/2018LYSEN024/document.

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Cette thèse, composée de deux parties, porte sur l’étude d’instabilités au sein d’un milieugranulaire.La première partie de cette thèse est consacrée à l’instabilité de tôle ondulée, c’est-àdirel’apparition d’un motif de rides sur une piste soumise au passage répété de véhicules.Nos travaux expérimentaux ainsi que des simulations numériques de dynamique moléculairenous ont permis de progresser dans la compréhension de ce phénomène. Pour uneroue rigide tirée à vitesse constante, nous avons étudié quantitativement l’impact de lacohésion du milieu granulaire sur les caractéristiques de l’instabil
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Kehoe, Thomas James Joseph. "Long-term dynamics of small bodies in the solar system using mapping techniques." Thesis, Queen Mary, University of London, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.481693.

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Fein, Brian. "A Dynamic Simulation of Trajectory and Attitude Stabilization for a Solar Sail Mission to Study the Asteroid Vesta." Honors in the Major Thesis, University of Central Florida, 2004. http://digital.library.ucf.edu/cdm/ref/collection/ETH/id/706.

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This item is only available in print in the UCF Libraries. If this is your Honors Thesis, you can help us make it available online for use by researchers around the world by following the instructions on the distribution consent form at http://library.ucf.edu/Systems/DigitalInitiatives/DigitalCollections/InternetDistributionConsentAgreementForm.pdf You may also contact the project coordinator, Kerri Bottorff, at kerri.bottorff@ucf.edu for more information.<br>Bachelors<br>Engineering and Computer Science<br>Aerospace Engineering
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Books on the topic "Asteroid Dynamics"

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C, Ambrosius B. A., Ip W. -H, Melosh H. J, et al., eds. Asteroid and spacecraft dynamics: Proceedings of the topical meeting of the COSPAR Interdisciplinary Scientific Commission B and P (Meetings B4 and P1) of the COSPAR Twenty-eighth Plenary Meeting held in The Hague, The Netherlands, 25 June-6 July 1990. Published for the Committee on Space Research by Pergamon Press, 1991.

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Yabushita, Shin, and Jacques Henrard, eds. Dynamics of Comets and Asteroids and Their Role in Earth History. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-017-1321-4.

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Huggett, Richard J. Catastrophism: Asteroids, comets, and other dynamic events in Earth history. Verso, 1997.

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Alexander von Humboldt Colloquium on Celestial Mechanics (5th 2000 Badhofgastein, Austria). New developments in the dynamics of planetary systems: Proceedings of the Fifth Alexander von Humboldt Colloquium on Celestial Mechanics held in Badhofgastein (Austria), 19-25 March 2000. Kluwer Academic, 2001.

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Alexander von Humboldt Colloquium on Celestial Mechanics (4th 1996 Ramsau am Dachstein, Austria). The dynamical behaviour of our planetary system: Proceedings of the Fourth Alexander von Humboldt Colloquium on Celestial Mechanics. Sprinter, 1997.

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Alexander von Humboldt Colloquium on Celestial Mechanics (4th 1996 Ramsau am Dachstein, Austria). The dynamical behaviour of our planetary system: Proceedings of the Fourth Alexander von Humboldt Colloquium on Celestial Mechanics. Kluwer Academic, 1997.

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International Astronomical Symposium (1992 Pléneuf-Val-André, France). Interactions between physics and dynamics of solar system bodies: Proceedings of the International Astronomical Symposium held in Pléneuf-Val-André (France) from June 21 to June 28, 1992. Kluwer Academic Publishers, 1993.

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1936-, Yabushita Shin, and Henrard J, eds. Dynamics of comets and asteroids and their role in earth history: Proceedings of a workshop held at the Dynic Astropark 'Ten-Kyu-Kan', August 14-18, 1997. Kluwer Academic, 1998.

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Asteroid & Spacecraft Dynamics: Proceedings of the Topical Meetings of the Cospar Interdisciplinary Scientific Commission B & P (Meetings B4 & P1) of. Elsevier Science Pub Co, 1991.

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McEachern, Firth M. Dynamical evolution of the Hungaria Asteroids. 2009.

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Book chapters on the topic "Asteroid Dynamics"

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Michalak, Grzegorz. "Determination of Masses of Six Asteroids from Close Asteroid—Asteroid Encounters." In Dynamics of Natural and Artificial Celestial Bodies. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1327-6_40.

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Cellino, A., and A. dell’Oro. "Asteroid Dynamical Families." In Dynamics of Small Solar System Bodies and Exoplanets. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-04458-8_3.

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Dikova, S. "Statistical Challenges in Asteroid Dynamics." In Statistical Challenges in Modern Astronomy II. Springer New York, 1997. http://dx.doi.org/10.1007/978-1-4612-1968-2_48.

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Sansaturio, M. E., Andrea Milani, and A. La Spina. "The Asteroid Identification Problem." In Impact of Modern Dynamics in Astronomy. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4527-5_38.

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Glikson, Andrew Y. "Impact and Cratering Dynamics." In The Asteroid Impact Connection of Planetary Evolution. Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-6328-9_4.

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Tupikova, I. V., A. A. Vakhidov, and M. Soffel. "Explicit Semianalytical Theory of Asteroid Motion." In Impact of Modern Dynamics in Astronomy. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4527-5_9.

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Ostro, Steven J. "Radar Contributions to Asteroid Astrometry and Dynamics." In Dynamics and Astrometry of Natural and Artificial Celestial Bodies. Springer Netherlands, 1997. http://dx.doi.org/10.1007/978-94-011-5534-2_10.

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Nesvorný, D., and A. Morbidelli. "Mean Motion Resonances in the Asteroid Belt." In Impact of Modern Dynamics in Astronomy. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4527-5_46.

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Šidlichovský, Miloš. "On Stable Chaos in the Asteroid Belt." In Impact of Modern Dynamics in Astronomy. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4527-5_8.

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Vakhidov, Akmal. "Asteroid Orbits in Some Three-Body Resonances." In Dynamics of Natural and Artificial Celestial Bodies. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1327-6_39.

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Conference papers on the topic "Asteroid Dynamics"

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Al Hameli, Fatema, Jeremy Knittel, Jeffrey Parker, and Mohamed Salem. "The Emirates Mission to the Asteroid Belt: An Overview of the Flight Dynamics System." In IAF Space Exploration Symposium, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078357-0108.

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Yamaguchi, Kohei, Xinbo Gu, Takaya Inamori, and Ji Hyun Park. "Near-Earth Asteroid Capture Mission Design Method Based on the Orbital Dynamics in the Planar-Circular Restricted Three-body Problem." In IAF Symposium on Planetary Defense and Near-Earth Objects, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078387-0026.

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Venditti, Flaviane, and Marcelo Lisboa Mota. "The Dynamical Environment of Potentially Hazardous Binary Asteroid (285263) 1998 QE2." In IAF Symposium on Planetary Defense and Near-Earth Objects, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078387-0005.

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Lobanova, K., and A. Melnikov. "The influence of uncertainty in the shape of an asteroid on the estimate of perturbation magnitudes in its rotational dynamics when approaching the Earth." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.148.

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The shape of the vast majority of small asteroids is unknown. There are only estimates of the average diameter obtained for them on the basis of absolute magnitude and albedo under a number of assumptions. To estimate the magnitude of perturbations in the rotational dynamics of an asteroid that arise when approaching the Earth by means of numerical modeling, it is necessary to know its moments of inertia, determined, among other things, by the shape of the asteroid. By conducting massive numerical experiments to simulate a close approach of an asteroid to the Earth, the influence of the figure
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Melnikov, A., and K. Lobanova. "Perturbations in the rotational dynamics." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.151.

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Using numerical modeling, perturbations that occur in the rotational motion of small (10--50 m in diameter) asteroids during their close approaches to the Earth (at distances of the order of several Earth radii) are considered. For a number of asteroids (Duende, 2012\,TC4 and 2023 BU), estimates of possible changes in the rotational period $P$ and the orientation of the rotational axis due to approach to the Earth were obtained. It has been established that in the case of fast rotation of an asteroid ($P &lt; 1$~h), perturbations in its rotational motion that arise during approach are negligib
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Pavlov, S., Yu Medvedev, T. Galushina, and A. Baturin. "Accuracy of orbits of small celestial bodies obtained using different software." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.153.

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The threat of a collision with a potentially hazardous object (PHO) and smaller asteroids requires the ability to reliably calculate the orbits of celestial bodies. The quality of the determined orbit depends on both the accuracy and intervals of observations and on the method of their processing: the completeness of the dynamic model, the method of numerical integration, calculation errors, etc. The practical implementation of the orbit determination algorithm is associated with the peculiarities of taking into account the above factors. To assess the accuracy of motion prediction using orbit
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Kuznetsov, S. Yu. "Dust injection into the plasma sheath near the surface of active asteroids’261." In 51-st All-Russian with international participation student scientific conference "Physics of Space". Ural University Press, 2024. http://dx.doi.org/10.15826/b978-5-7996-3848-1.52.

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This article is devoted to the analysis of the dynamics of submicron-sized dust particles near the surface of active asteroids. The Sun plays an important role in the passing of an asteroid near perihelion. In addition to the main role in the sublimation of particles under the action of radiation, the Sun makes a significant contribution to the evolution of the motion of dust particles. Streams of ionized plasma interact with the surface of the asteroid, forming an electrostatic field that allows particles to levitate above the surface.
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Scheeres, Daniel J., Daniel Wibben, Peter G. Antreasian, et al. "The Dynamics about Asteroid (101955) Bennu." In AIAA SCITECH 2022 Forum. American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-2468.

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Melnikov, A., M. Khovrichev, I. Balyaev, and K. Lobanova. "Tidal changes in the rotational state of asteroids asevolution factor of the magnitude of the Yarkovsky effect." In Modern astronomy: from the Early Universe to exoplanets and black holes. Special Astrophysical Observatory of the Russian Academy of Sciences, 2024. https://doi.org/10.26119/vak2024.150.

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We examined possible tidal-induced leaps in the rotational state parameters of the asteroids during their planet approaches. These dramatic changes in the rotational period and obliquity lead to significant changes in orbital dynamics due to the corresponding Yarkovsky acceleration $A_2$ leap. Our numerical simulations of asteroid rotational parameters evolution due to their planet encounters support the conclusion that significant $A_2$ changes can happen when planetocentric distance is less than ten planetary radii. We have found nine asteroids with anomalous $A_2$ values. However, there is
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Shi, Y., and X. Wu. "Global mapping analysis tools for asteroid exploration." In 1st International Conference on Mechanical System Dynamics (ICMSD 2022). Institution of Engineering and Technology, 2022. http://dx.doi.org/10.1049/icp.2022.1886.

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Reports on the topic "Asteroid Dynamics"

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King, P. K. Gas Dynamics Near and Far: Observational Magnetohydrodynamics of Interstellar Molecular Clouds and X-Ray Ablation of Asteroids for the Earth's Defense. Office of Scientific and Technical Information (OSTI), 2019. http://dx.doi.org/10.2172/1544929.

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