De Troianis: The Trojans in the Planetary System
暂无分享,去创建一个
Elisabetta Dotto | Dale P. Cruikshank | Alessandro Morbidelli | Maria Antonietta Barucci | J. Emery | M. Barucci | E. Dotto | D. Cruikshank | A. Morbidelli | J. P. Emery
[1] David Jewitt,et al. CCD spectra of asteroids. II - The Trojans as spectral analogs of cometary nuclei , 1990 .
[2] Joseph Veverka,et al. The composition of the Trojan asteroids , 1980, Nature.
[3] Barucci,et al. Physical Properties of Trojan and Centaur Asteroids , 2002 .
[4] L. McFadden,et al. CCD reflectance spectra of selected asteroids. I - Presentation and data analysis considerations , 1992 .
[5] F. Vilas,et al. CCD Reflectance Spectra of Selected Asteroids. II. Low-Albedo Asteroid Spectra and Data Extraction Techniques , 1993 .
[6] Emmanuel Lellouch,et al. The Spectrum of Comet Hale-Bopp (C/1995 O1) Observed with the Infrared Space Observatory at 2.9 Astronomical Units from the Sun , 1997, Science.
[7] R. Gomes. Dynamical Effects of Planetary Migration on the Primordial Asteroid Belt , 1997 .
[8] C. Barbieri,et al. Visible Spectroscopy of Dark, Primitive Asteroids , 1994 .
[9] Fernando Roig,et al. A Semianalytical Model for the Motion of the Trojan Asteroids: Proper Elements and Families , 2001 .
[10] K. Tsiganis,et al. Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets , 2005, Nature.
[11] D. Britt,et al. Asteroid Density, Porosity, and Structure , 2002 .
[12] D. Hamilton,et al. On the Origin of the Trojan Asteroids: Effects of Jupiter's Mass Accretion and Radial Migration , 2000, astro-ph/0007296.
[13] J. Brucato,et al. 308 Polyxo: ISO-SWS spectrum up to 26 micron , 2004 .
[14] K. Noll. Solar System binaries , 2005, Proceedings of the International Astronomical Union.
[15] Larry A. Lebofsky,et al. The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt , 1990 .
[16] Harold F. Levison,et al. From the Kuiper Belt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets☆ , 1997 .
[17] F. Roig,et al. Planetary Migration and the Effects of Mean Motion Resonances on Jupiter’s Trojan Asteroids , 2001 .
[18] Gabriele Arnold,et al. A Model of Spectral Albedo of Particulate Surfaces: Implications for Optical Properties of the Moon , 1999 .
[19] E. Cloutis,et al. Near-Infrared Spectroscopy of Primitive Solar System Objects , 1994 .
[20] M. A’Hearn,et al. Studies of proton-irradiated cometary-type ice mixtures , 1983 .
[21] C. Trujillo,et al. A Thick Cloud of Neptune Trojans and Their Colors , 2006, Science.
[22] Hans Rickman,et al. Nuclear magnitudes and the size distribution of Jupiter family comets , 2006 .
[23] B. Hapke,et al. Bidirectional reflectance spectroscopy. I - Theory. [of planetary surfaces , 1981 .
[24] T. Owen,et al. 10 Hygiea: ISO Infrared Observations , 2002 .
[25] Joshua Patrick Emery,et al. The surface composition of Trojan asteroids: constraints set by scattering theory , 2004 .
[26] T. Owen,et al. Near-Infrared Spectroscopy of Low-Albedo Surfaces of the Solar System: Search for the Spectral Signature of Dark Material , 1998 .
[27] B. Hapke. Theory of reflectance and emittance spectroscopy , 1993 .
[28] Hans Scholl,et al. Capture of Trojans by a Growing Proto-Jupiter , 1998 .
[29] Physical Properties of Trans-Neptunian Object (20000) Varuna , 2002, astro-ph/0201082.
[30] G. Strazzulla. Chemistry of Ice Induced by Bombardment with Energetic Charged Particles , 1998 .
[31] R. Duffard,et al. S3OS2: the visible spectroscopic survey of 820 asteroids , 2004 .
[32] Elisabetta Dotto,et al. Optical alteration of complex organics induced by ion-irradiation: 1. Laboratory experiments suggest unusual space weathering trend. , 2004 .
[33] F. Marzari,et al. The Role of Secular Resonances in the History of Trojans , 2000 .
[34] Dean C. Hines,et al. Spitzer Observations of the Dust Coma and Nucleus of 29P/Schwassmann-Wachmann 1 , 2004 .
[35] Paul J. Stomski,et al. A low density of 0.8 g cm-3 for the Trojan binary asteroid 617 Patroclus , 2006, Nature.
[36] F. Marzari,et al. The surface composition of Jupiter Trojans: Visible and near-infrared survey of dynamical families ☆ , 2006 .
[37] David Jewitt,et al. Spectroscopic Search for Water Ice on Jovian Trojan Asteroids , 2006 .
[38] Daniel D. Durda,et al. Asteroids Do Have Satellites , 2002 .
[39] M. Martino,et al. Spectroscopic observations of Jupiter Trojans , 2004 .
[40] K. Tsiganis,et al. Origin of the orbital architecture of the giant planets of the Solar System , 2005, Nature.
[41] Z. Ivezic,et al. Solar system objects observed in the Sloan Digital Sky Survey commissioning data , 2001 .
[42] Z. Ivezic,et al. The properties of Jovian Trojan asteroids listed in SDSS Moving Object Catalogue 3 , 2007, astro-ph/0703026.
[43] D. C. Jewitt,et al. Population and Size Distribution of Small Jovian Trojan Asteroids , 2000, astro-ph/0004117.
[44] Harold F. Levison,et al. Planetary migration in a planetesimal disk: why did Neptune stop at 30 AU? , 2004 .
[45] Julio A. Fernández,et al. Some dynamical aspects of the accretion of Uranus and Neptune: The exchange of orbital angular momentum with planetesimals , 1984 .
[46] Tjie SIIORT-PERJOD. The Kuiper Belt , 1997 .
[47] Jack J. Lissauer,et al. Formation of the Giant Planets by Concurrent Accretion of Solids and Gas , 1995 .
[48] L. Tannenbaum. Laboratory Studies , 2010, Pediatric Orthopaedics and Sports Injuries.
[49] 吉田 二美. Size and spatial distributions of sub-km main-belt asteroids , 2002 .
[50] Renu Malhotra,et al. The origin of Pluto's orbit: implications for the , 1994, astro-ph/9504036.
[51] David Jewitt,et al. The Albedo Distribution of Jovian Trojan Asteroids , 2003 .
[52] Neptune’s Migration into a Stirred-Up Kuiper Belt: A Detailed Comparison of Simulations to Observations , 2005, astro-ph/0507319.
[53] M. Moore,et al. Laboratory Studies of the Formation of Methanol and Other Organic Molecules by Water+Carbon Monoxide Radiolysis: Relevance to Comets, Icy Satellites, and Interstellar Ices , 1999 .
[54] W. R. Thompson,et al. Coloration and darkening of methane clathrate and other ices by charged particle irradiation: applications to the outer solar system. , 1987, Journal of geophysical research.
[55] K. Tsiganis,et al. Chaotic capture of Jupiter's Trojan asteroids in the early Solar System , 2005, Nature.
[56] Andrea Milani,et al. The Trojan asteroid belt: Proper elements, stability, chaos and families , 1993 .
[57] Faith Vilas,et al. Iron Alteration Minerals in the Visible and Near-Infrared Spectra of Low-Albedo Asteroids , 1994 .
[58] F. Marzari,et al. Visible spectroscopic and photometric survey of L5 Trojans: investigation of dynamical families , 2004 .
[59] W. Hartmann,et al. Trojan and Hilda asteroid lightcurves. I - Anomalously elongated shapes among Trojans (and Hildas?) , 1988 .
[60] Dale P. Cruikshank,et al. Thermal emission spectroscopy (5.2–38 μm) of three Trojan asteroids with the Spitzer Space Telescope: Detection of fine-grained silicates , 2006 .
[61] Robert H. Brown,et al. Constraints on the surface composition of Trojan asteroids from near-infrared (0.8–4.0 μm) spectroscopy , 2003 .
[62] Orbital Evolution of Planets Embedded in a Planetesimal Disk , 1999, astro-ph/9902370.
[63] J. Chambers,et al. The Primordial Excitation and Clearing of the Asteroid Belt , 2001 .
[64] E. M. Shoemaker,et al. Trojan asteroids - Populations, dynamical structure and origin of the L4 and L5 swarms , 1989 .
[65] P. Robutel,et al. The resonant structure of Jupiter's Trojan asteroids – I. Long‐term stability and diffusion , 2006 .
[66] A. Rivkin,et al. Spectroscopy and photometry of Mars Trojans , 2003 .
[67] S. Peale. The Effect of the Nebula on the Trojan Precursors , 1993 .
[68] Fumi Yoshida,et al. Size Distribution of Faint Jovian L4 Trojan Asteroids , 2005 .
[69] Charalampos Skokos,et al. Stability of the Trojan asteroids , 1997 .
[70] J. Dunlap,et al. Minor planets. III - Lightcurves of a Trojan asteroid. , 1969 .
[71] Alfred Edward Ringwood,et al. Origin of the Earth and Moon , 1979 .
[72] B. Hapke. Bidirectional reflectance spectroscopy: 1. Theory , 1981 .
[73] William K. Hartmann,et al. The Time-Dependent Intense Bombardment of the Primordial Earth/Moon System , 2000 .
[74] M J Gaffey,et al. Phyllosilicate Absorption Features in Main-Belt and Outer-Belt Asteroid Reflectance Spectra , 1989, Science.
[75] G. Wetherill. An alternative model for the formation of the asteroids , 1992 .
[76] Andrea Milani,et al. Asteroid Proper Elements and the Dynamical Structure of the Asteroid Main Belt , 1994 .
[77] Richard P. Binzel,et al. Trojan, Hilda, and Cybele asteroids: New lightcurve observations and analysis , 1992 .
[78] H. Scholla,et al. Dynamics of Mars Trojans , 2005 .
[79] K. J. Meech,et al. Spitzer Spectral Observations of the Deep Impact Ejecta , 2006, Science.
[80] H. Boehnhardt,et al. Aqueous altered silicates at the surface of two Plutinos , 2004 .
[81] E. Tedesco,et al. Compositional Structure of the Asteroid Belt , 1982, Science.
[82] F. De Luise,et al. Visible spectroscopic and photometric survey of Jupiter Trojans: Final results on dynamical families , 2007, 0704.0350.
[83] Analysis of the Rotational Properties of Kuiper Belt Objects , 2006, astro-ph/0601257.
[84] Renu Malhotra,et al. The origin of Pluto's peculiar orbit , 1995, Nature.
[85] A. Fitzsimmons,et al. A spectroscopic survey of D-type asteroids , 1994 .