Solar-Radiation Heating Effects on 3200 Phaethon
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Makoto Yoshikawa | Takashi Ito | Daisuke Kinoshita | Sunao Hasegawa | Aiko Nakato | Tomoki Nakamura | D. Kinoshita | M. Yoshikawa | S. Hasegawa | Tomoki Nakamura | A. Nakato | Takashi Ito | K. Ohtsuka | Katsuhito Ohtsuka
[1] Elisabetta Dotto,et al. Optical alteration of complex organics induced by ion-irradiation: 1. Laboratory experiments suggest unusual space weathering trend. , 2004 .
[2] M. Houde,et al. An upper limit on gas production from 3200 Phaethon , 2008, 0801.0793.
[3] M. Miyamoto. Thermal Metamorphism of CI and CM Carbonaceous Chondrites: an Internal Heating Model , 1991 .
[4] Richard P. Binzel,et al. Keck observations of near-Earth asteroids in the thermal infrared , 2003 .
[5] S. Price,et al. Midcourse Space Experiment Observations of Small Solar System Bodies , 2005 .
[6] Richard P. Binzel,et al. Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes , 2004 .
[7] D. Jewitt,et al. Search for Activity in 3200 Phaethon , 2005 .
[8] D. Kinoshita,et al. Surface heterogeneity of 2005 UD from photometric observations , 2007 .
[9] A. J. Meadows,et al. Infrared observations of the extinct cometary candidate minor planet (3200) 1983TB , 1985 .
[10] G. Ryabova. Mathematical modelling of the Geminid meteoroid stream , 2007 .
[11] Benefits of an impact mission to 3200 Phaethon: nature of the extinct comet and artificial meteor shower , 2006 .
[12] Richard P. Binzel,et al. Spectral Properties of Near-Earth Objects: Palomar and IRTF Results for 48 Objects Including Spacecraft Targets (9969) Braille and (10302) 1989 ML , 2001 .
[13] M. Barucci,et al. VISIBLE SPECTROSCOPY OF POSSIBLE COMETARY CANDIDATES , 1996 .
[14] T. Mukai,et al. Dust trails along asteroid 3200 Phaethon's orbit , 2002 .
[15] William F. Bottke,et al. THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics , 2006 .
[16] Tomoki Nakamura. Yamato 793321 CM chondrite: Dehydrated regolith material of a hydrous asteroid , 2006 .
[17] Hiroshi Terada,et al. Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target 162173 1999 JU3 from AKARI , 2008 .
[18] A. Harris,et al. New findings on asteroid spin-vector distributions , 2007 .
[19] Uwe Fink,et al. THE UNUSUAL SPECTRA OF 15 NEAR-EARTH ASTEROIDS AND EXTINCT COMET CANDIDATES , 1998 .
[20] T. Kasuga,et al. Creating an artificial Geminid meteor shower: Correlation between ejecta velocity and observability , 2007 .
[21] R. Jedicke,et al. Debiased Orbital and Absolute Magnitude Distribution of the Near-Earth Objects , 2002 .
[22] David Jewitt,et al. Charge-coupled device spectra of asteroids. I. Near-earth and 3:1 resonance asteroids , 1990 .
[23] A. Cochran,et al. Minor planet 1983TB: A dead comet? , 1984 .
[24] P. Babadzhanov,et al. Evolution of short period meteoroid streams , 1992 .
[25] M. Zolensky,et al. Aqueous alteration on the hydrous asteroids - Results of EQ3/6 computer simulations , 1989 .
[26] Alan W. Harris,et al. A Thermal Model for Near-Earth Asteroids , 1998 .
[27] W. Bottke,et al. Oxygen and Asteroids , 2008 .
[28] R. Clayton,et al. Oxygen isotope studies of carbonaceous chondrites , 1999 .
[29] M. Zolensky,et al. Thermal metamorphism of the C, G, B, and F asteroids seen from the 0.7 μm, 3 μm, and UV absorption strengths in comparison with carbonaceous chondrites , 1996 .
[30] T. Kasuga,et al. Thermal desorption of Na in meteoroids Dependence on perihelion distance of meteor showers , 2006 .
[31] A. Chamberlin,et al. 4015 Wilson-Harrington, 2201 Oljato, and 3200 Phaethon: Search for CN Emission , 1996 .
[32] Stefano Mottola,et al. Thermal inertia of near-Earth asteroids and implications for the magnitude of the Yarkovsky effect , 2007, 0704.1915.
[33] D. Jewitt,et al. OBSERVATIONS OF 1999 YC AND THE BREAKUP OF THE GEMINID STREAM PARENT , 2008, 0805.2636.
[34] M. Yoshikawa,et al. Near-misses in orbital motion of asteroids , 1994 .
[35] W. Delamere,et al. Surface temperature of the nucleus of Comet 9P/Tempel 1 , 2007 .
[36] G. Neukum,et al. The Near-Earth Objects Follow-up Program. IV. CCD Photometry in 1996-1999 , 2002 .
[37] M. Zolensky,et al. Evidence of Thermal Metamorphism on the C, G, B, and F Asteroids , 1993, Science.
[38] D. Jewitt,et al. Physical Observations of 2005 UD: A Mini-Phaethon , 2006 .
[39] N. Mcbride,et al. Thermal infrared and optical observations of four near-Earth asteroids , 2008 .
[40] F. Vilas,et al. Are Low-Albedo Asteroids Thermally Metamorphosed? , 1996 .
[41] Michael J. S. Belton,et al. Deep Sub-Surface Exploration of Cometary Nuclei , 1999 .
[42] J. Licandro,et al. The nature of comet-asteroid transition object (3200) Phaethon , 2007 .
[43] D. Kinoshita,et al. Apollo asteroid 2005 UD : split nucleus of (3200) Phaethon? , 2006 .
[44] Harry Y. McSween,et al. Meteorites and the early solar system II , 2006 .
[45] Alain Doressoundiram,et al. The puzzling case of the Nysa-Polana family finally solved ? , 1998 .
[46] Tomoki Nakamura,et al. Evaluation of dehydration mechanism during heating of hydrous asteroids based on mineralogical and chemical analysis of naturally and experimentally heated CM chondrites , 2008 .
[47] A. Vitagliano. Numerical integration for the real time production of fundamental ephemerides over a wide time span , 1996 .
[48] E. Anders,et al. Meteorites and the Early Solar System , 1971 .
[49] Richard J. Rudy,et al. A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas , 1986 .
[50] H. McSween,et al. Water and the thermal evolution of carbonaceous chondrite parent bodies , 1989 .