Near Earth Asteroids with measurable Yarkovsky effect
Davide Farnocchia,Steven R. Chesley,David Vokrouhlický,Andrea Milani,Federica Spoto,William F. Bottke +5 more
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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Gaia Data Release 2. Observations of solar system objects
Federica Spoto,Federica Spoto,Paolo Tanga,Francois Mignard,Jérôme Berthier,Benoit Carry,Benoit Carry,Alberto Cellino,Aldo Dell'Oro,Daniel Hestroffer,Karri Muinonen,Karri Muinonen,T. Pauwels,J. M. Petit,P. David,F. De Angeli,Marco Delbo,B. Frezouls,Laurent Galluccio,Mikael Granvik,Mikael Granvik,J. Guiraud,Jose M Hernandez,C. Ordénovic,Jordi Portell,E. Poujoulet,William Thuillot,G. Walmsley,A. G. A. Brown,Antonella Vallenari,T. Prusti,Jhj de Bruijne,C. Babusiaux,C. Babusiaux,C. A. L. Bailer-Jones,M. Biermann,D. W. Evans,L. Eyer,F. A. Jansen,Carme Jordi,Sergei A. Klioner,Uwe Lammers,Lennart Lindegren,Xavier Luri,C. Panem,Dimitri Pourbaix,Sofia Randich,P. Sartoretti,H. I. Siddiqui,Caroline Soubiran,F. van Leeuwen,Nicholas A. Walton,Frédéric Arenou,Ulrich Bastian,Mark Cropper,R. Drimmel,D. Katz,Mario G. Lattanzi,J. Bakker,Carla Cacciari,J. Castañeda,L. Chaoul,N. Cheek,C. Fabricius,Raphael Guerra,B. Holl,Eduard Masana,R. Messineo,Nami Mowlavi,Krzysztof Nienartowicz,P. Panuzzo,M. Riello,George M. Seabroke,F. Thévenin,G. Gracia-Abril,G. Comoretto,M. Garcia-Reinaldos,D. Teyssier,Martin Altmann,Martin Altmann,Rene Andrae,Marc Audard,I. Bellas-Velidis,Kevin Benson,R. Blomme,P. Burgess,G. Busso,Gisella Clementini,M. Clotet,O. L. Creevey,Michael Davidson,J. De Ridder,Ludovic Delchambre,C. Ducourant,J. Fernández-Hernández,Morgan Fouesneau,Yves Fremat,Miguel García-Torres,J. González-Núñez,J. González-Núñez,J. J. González-Vidal,Eric Gosset,Leanne P. Guy,J. L. Halbwachs,Nigel Hambly,D. L. Harrison,Simon Hodgkin,A. Hutton,Gérard Jasniewicz,A. Jean-Antoine-Piccolo,Stefan Jordan,Andreas Korn,Alberto Krone-Martins,A. C. Lanzafame,A. C. Lanzafame,T. Lebzelter,W. Loeffler,Minia Manteiga,P. M. Marrese,P. M. Marrese,J. M. Martín-Fleitas,André Moitinho,A. Mora,J. Osinde,Elena Pancino,Elena Pancino,Alejandra Recio-Blanco,P. J. Richards,Lorenzo Rimoldini,Annie C. Robin,L. M. Sarro,Christos Siopis,Mike Smith,Alessandro Sozzetti,M. Sueveges,J. Torra,W. van Reeven,Ummi Abbas,A. Abreu Aramburu,S. Accart,Conny Aerts,Conny Aerts,G. Altavilla,G. Altavilla,M. A. Álvarez,R Alvarez,João Alves,Richard I. Anderson,Richard I. Anderson,Alexandre Humberto Andrei,Alexandre Humberto Andrei,Alexandre Humberto Andrei,E. Anglada Varela,E. Antiche,Teresa Antoja,Teresa Antoja,Bernardino Arcay,Tri L. Astraatmadja,Tri L. Astraatmadja,N. Bach,S. G. Baker,L. Balaguer-Núñez,P. Balm,C. Barache,C. Barata,D. Barbato,D. Barbato,F. Barblan,Paul S. Barklem,David Barrado,M. Barros,Martin A. Barstow,S. Bartholomé Muñoz,J.-L. Bassilana,Ugo Becciani,Michele Bellazzini,A. Berihuete,Stefano Bertone,Stefano Bertone,Stefano Bertone,Luciana Bianchi,Olivier Bienaymé,Sergi Blanco-Cuaresma,Sergi Blanco-Cuaresma,Sergi Blanco-Cuaresma,T. Boch,C Boeche,Alex Bombrun,R. Borrachero,Diego Bossini,S. Bouquillon,G Bourda,Angela Bragaglia,L. Bramante,Maarten A. Breddels,Alessandro Bressan,N. Brouillet,T. Bruesemeister,E. Brugaletta,Beatrice Bucciarelli,A. Burlacu,Deborah Busonero,A. G. Butkevich,R. 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Orbit and bulk density of the OSIRIS-REx target Asteroid (101955) Bennu
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Asteroid families classification: Exploiting very large datasets
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Cohesive forces prevent the rotational breakup of rubble-pile asteroid (29075) 1950 DA
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TL;DR: In this article, the authors presented a new four-dimensional model of the near-Earth objects population that describes debiased steady-state distributions of semimajor axis, eccentricity, inclination, and absolute magnitude H in the range 17.962 − 56 + 52 + 52 ( 802 − 42 + 48 × 10 3 ) NEOs with H.
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