Near Earth Asteroids with measurable Yarkovsky effect
Davide Farnocchia,Steven R. Chesley,David Vokrouhlický,Andrea Milani,Federica Spoto,William F. Bottke +5 more
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TLDR
In this article, the Yarkovsky effect among near Earth asteroids (NEAs) was investigated by measuring the YARKovsky-related orbital drift from the orbital fit using a high precision dynamical model, including the Newtonian attraction of 16 massive asteroids and the planetary relativistic terms.About:
This article is published in Icarus.The article was published on 2013-05-01 and is currently open access. It has received 140 citations till now. The article focuses on the topics: Yarkovsky effect & Near-Earth object.read more
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Yarkovsky Drift Detections for 247 Near-Earth Asteroids
TL;DR: Greenberg et al. as mentioned in this paper analyzed both optical and radar astrometry for 600 near-Earth asteroids (NEAs) for the purpose of detecting and quantifying the Yarkovsky effect.
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Constraints on the near-Earth asteroid obliquity distribution from the Yarkovsky effect
Chiara Tardioli,Davide Farnocchia,Ben Rozitis,D. Cotto-Figueroa,Steven R. Chesley,T. S. Statler,Massimiliano Vasile +6 more
TL;DR: In this paper, the authors tried to constrain the spin axis obliquity distribution of near-Earth asteroids by leveraging the Yarkovsky effect and its dependence on an asteroid's oblivity.
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Detecting the Yarkovsky effect among near-Earth asteroids from astrometric data
TL;DR: In this paper, the authors presented an updated set of near-Earth asteroids with a Yarkovsky-related semimajor axis drift detected from the orbital fit to the astrometry.
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Detailed Analysis of the Asteroid Pair (6070) Rheinland and (54827) 2001 NQ8
David Vokrouhlický,Petr Pravec,Josef Ďurech,Kamil Hornoch,Peter Kusnirak,Adrian Galad,J. Vrastil,Hana Kučáková,J. T. Pollock,Jose Luis Ortiz,Nicolás Morales,N. M. Gaftonyuk,Donald P. Pray,Yurij N. Krugly,R. Inasaridze,V. R. Ayvazian,Igor Molotov,C. Colazo +17 more
TL;DR: In this paper, the authors used optical photometry to determine the rotational state and convex shape of the (6070) Rheinland and (54827) 2001 NQ8 pairs.
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Nongravitational perturbations and virtual impactors: the case of asteroid (410777) 2009 FD
Federica Spoto,Andrea Milani,Davide Farnocchia,Steven R. Chesley,Marco Micheli,Giovanni B. Valsecchi,Giovanni B. Valsecchi,Davide Perna,Olivier Hainaut +8 more
TL;DR: In this article, the authors used the available physical characterization of 2009 FD and general properties of the near Earth asteroid population to compute the Yarkovsky effect by using a Monte Carlo approach.
References
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Theory and Experiment in Gravitational Physics
TL;DR: In this paper, the authors provide a complete treatment of techniques for analyzing gravitation theory and experience, taking into account the Dicke framework, basic criteria for the viability of a gravitation theories, experimental tests of the Einstein equivalence principle, Schiff's conjecture, and a model theory devised by Lightman and Lee (1973).
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Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects
William F. Bottke,Alessandro Morbidelli,Robert Jedicke,Jean-Marc Petit,Harold F. Levison,Patrick Michel,Travis S. Metcalfe +6 more
TL;DR: In this article, a best-fit model of the near-Earth objects (NEOs) population is presented, which is fit to known NEs discovered or accidentally rediscovered by Spacewatch.
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THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics
TL;DR: The Yarkovsky and YORP effects are thermal radiation forces and torques that cause small objects to undergo semimajor axis drift and spin vector modifications, respectively, as a function of their spin, orbit, and material properties as discussed by the authors.
Application of photometric models to asteroids.
TL;DR: In this paper, the brightness of a rough and porous surface is parameterized in terms of the optical properties of individual particles, by shadowing between particles, and by the way in which light is scattered among collections of particles.
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TL;DR: In this paper, the authors present algorithms for computing ET-TAI, including the calculation of precision light times and quasar delays, as well as partial derivatives of light times.