Астронет: С. С. Наумов/МГУ Особенности астероида 433 Эрос http://www.variable-stars.ru/db/msg/1198835/bibl.html |
ЛИТЕРАТУРА
Acuna, M. H., Anderson, B. J., Russell, C. T., Wasilewski, P., Kletetshka, G., Zanetti, L., Omidi, N., 2002. NEAR magnetic field observations at 433 Eros: first measurements from the surface of an asteroid. Icarus 155, 220-228.
Bell III, J. F., Izenberg, N. I., Lucey, P. G., Clark, B. E., Peterson, C., Gaffey M. J., Joseph J., Carcich, B., Harch, A., Bell, M. E., Warren, J., Martin, P. D., McFadden,љL. A., Wellnitz, D., Murchie, S., Winter, M., Veverka, J., Thomas, T., Robinson, M. S., Malani, M., Cheng, A., 2002. Near-IR reflectance spectroscopy of 433 Eros from the NIS instrument on the NEAR mission, I. Low phase angel observations. Icarus 155, 119-144.
Britt, D.T., Yeomans, D., Housen, K., Consolmagno, G., 2002. Asteroid density, porosity and structure. In Bottke, W.F., Cellino, A., Paolicchi, P., Binzel, R.P., Asteroids III. University of Arizona Press, Tucson, 485-500.
Carrier, W. D., Olhoeft, G. R., Wendell, W., 1991. Physical properties of the lunar surface. In Lunar Sourcebook (Heiken, G. H., Vaniman, D. T., French, B. M., Eds.). Cambridge Univ. Press, Cambridge, UK. 475-594.
Chapman, C. R., 1978. Asteroid collisions, craters, regoliths, and lifetimes. NASA Conf. Publ. 2053, 145-160.
Chapman, C. R., Merline, W. J., Thomas, P. C., Joseph, J., Cheng, A. F., Izenberg,љN., 2002. Impact history of Eros: craters and boulders. Icarus 155, 104118.
Cheng, A. F., Izenberg, N., Chapman, C. R., Zuber, M. T., 2002. Ponded deposits on asteroid 433 Eros. Meteoritics & Planetary Science 37, 1095-1105.
Cheng, A., Izenberg, N., Malin, M., Chapman, C., McFadden, L. A., Kirk, R., Gaffey, M., Lucey, P. G., 2002. Eros: shape, topography, and slope processes. Icarus 155, 18-37.
Davis, D. R., Chapman, C. R., Greenberg, R., Weidenschilling, S. J., Harris,љA.љW., 1979. Collisional evolution of asteroids: Populations, rotations, and velocities.љInљAsteroidsљ(Gehrels,љT.,љEd),љUniv.љofљArizonaљPress,љTucson,љ528557
Estimating the mass of Asteroid 433 Eros during the NEAR spacecraft flyby. Science 285, 560-561.
Grimm, R. E., 1985. Penecontemporaneous metamorphism, fragmentation, and reassembly of ordinary chondrite bodies. J. Geophys. Res 90, 2022-2028.
Herndon, J. M., and Herndon, M. A., 1977. Aluminum-26 as a planetoid heat source in the early Solar System. Meteoritics 12, 459-465.
Lee, P., 1996. Dust levitation on asteroids. Icarus 124. 181-194.
Mantz, A., Sullivan, R., Veverka, J., 2004. Regolith transport in craters on Eros. Icarus 167, 197-203.
McCoy, T. J., Taylor, G. J., Scott, E. R. D., Keil, K., 1990. Metallographic cooling rates correlated with petrologic type in LL3.0-4 chondrites: Implications for parent body structures. Lunar Planet. Sci. Conf. 21, 749-750 (abstract).
Miller, J. K., Antreasian, P. G., Gasskell, R. W., Giorgini, J. D., Helfrich, C. E., Owen, W. M., Williams, B. G., Yeomans, D. K., 1999. Determination of Eros physical parameters for Near Earth Asteroid Rendezvous orbit phase navigation. AAS Paper 99-463, presented at AAS/AIAA Astrodynamics Specialist Conference, Girdwood, Alaska.
Miller, J. K., Konopliv, A.S., Antreasian, P. G., Bordi, J. J., Chesley, S., Helfrich,љC. E., Owen, W. M., Wang, T. C., Williams, B. G., Yeomans, D. K., 2002. Determination of shape, gravity, and rotational state of asteroid 433 Eros. Icarus 155, 3-17.
Minster, J. F., and Allegre, C., 1979. 87Rb-87Sr chronology of H chondrites: Constraint and speculations on the early evolution of their parent body. Earth Planet. Sci. Lett. 42, 333-347.
Miyamoto, M., and Futjii, N., 1980. A model of ordinary chondrite parent body: An external heating model. Mem. NIPR 17, 291-298.
Miyamoto, M., Fujii, N., Tekada, H., 1981. Ordinary chondrite parent body: An internal heating model. Proc. Lunar Planet. Sci. Conf. 12B, 1145-1152.
Murchie, S. L. and Pieters, C. M., 1996. Spectral properties and rotation spectral heterogeneity of 433 Eros. J. Geophys. Res. 101, 2201-2214.
Pellas, P., and Strorzer, D., 1981. 244Pu fission track thermometry and its application to stony meteorites. Proc. R. Soc. London A374, 253-270.
Pettijohn, F. J., 1957. Sedimentary rocks. Harper and Row, New York.
Prockter, L., Thomas, P., Robinson, M., Joseph, J., Milne, A., Bussey, B., Veverka, J., Cheng, F., 2002. Surface expressions of structural features on Eros. Icarus 155, 75-93.
Robinson, M. S., Thomas, P. C., Veverka, J., Murchie, S., Carcich, B., 2001. The nature of ponded deposits on Eros. Nature 413, 396-399.
Scott, E. R. D., and Rajan, R. S., 1981. Metallic minerals, thermal histories, and parent bodies of some xenolithic, ordinary chondrite meteorites. Geochim. Cosmochim. Acta 45, 53-67.
Souchay, J., Kinoshita, H., Nakai, H., Roux, S., 2003. A precise modeling of Eros 433 rotation. Icarus 166, 285-296.
Taylor, G. J., Scott, R. D., Rubin, A. E., Maggiore, P., Keil, K., 1982. Structure and fragmentation of the parent asteroids of ordinary chondrites. Lunar Planet. Sci. 13, 799-800 (Abstract).
The NEAR Earth Asteroid Rendezvous. A Guide to the Mission, the Spacecraft, and the People. (NEAR Press Kit) (Johns Hopkins University Applied Physics Laboratory, 1998), 10.
Thomas, P. C., Veverka, J., Bell III, J. F., Clark, B. E., Carcich, B., Joseph, J., Robinson, M., McFadden, L. A., Malin, M. C., Chapman, C. R., Merline, W., Murchie, S., 1999. Mathilde: Size, shape, and geology. Icarus 140, 17-27.
Thomas, P. C., Joseph, J., Carcich, B., Veverka, J., Clark, B. E., Bell III, J. F., Byrd, A. W., Chomko, R., Robinson, M. S., Murchie, S. L., Prockter, L. M., Cheng, A., Izenberg, N., Malin, M., Chapman, C., McFadden, L. A., Kirk, R., Gaffey, M., Lucey, P. G., 2002. Eros: shape, topography, and slope processes. Icarus 155, 18-37.
Trombka, J. I., Squyres, S. W., Bruckner, J., Boynton, W. V., Reedy, R. C., McCoy, T. J., Gorenstein, P., Evans, L., G., Arnold, J. R., Starr, R. D., Nittler,љL.љR., Murphy, M. E., Mikheeva, I., McNutt Jr., R., L., McClanahan, T. P., McCartney, E., Goldsten, J. O., Gold, R. E., Floyd, S. R., Clark, P. E., Burbine,љT.љH., Bhangoo, J. S., Bailey, S. H., Pataev, M., 2000. The elemental composition of asteroid 433 Eros: results of NEAR-Shoemaker X-ray spectrometer. Science 289, 2101-2105.
Veverka, J., Robinson, M., Thomas, P., Murchie, S., Bell III, J. F., Izenberg, N., Chapman, C., Harch, A., Bell, M., Carcich, B., Cheng, A., Clark, B., Dominigue,љD., Dunham, D., Farquhar, R., Gaffey, M. J., Hawkins, E., Joseph, J., Kirk, R., Li, H., Lucey, P., Malin, M., Martin, P., McFadden, L., Merline, W. J., Miller, J. K., Owen Jr., W. M., Peterson, C., Prockter, L., Warren, J., Wellnitz, D., Williams, B. G., Yeomans, D. K., 2000. NEAR at Eros: Imaging and spectral results. Science 289, 2088-2097.
Wetherill, G. W., and Chapman, C. R., 1988. Asteroids and meteorites. In meteorites and the early Solar System (Kerridge, J. F. and Matthews, M. S., Eds.), Univ. of Arizona Press, Tucson, 35-67.
Wilkison, S. L., Robinson, M. S., Thomas, P. C., Veverka, J., McCoy, T. J., Murchie, S. L., Prockter, L. M., Yeomans, D. K., 2002. An estimate of Eros's porosity and implications for internal structure. Icarus 155, 94-103.
Yeomans, D. K., Antreasian, P. G., Barriot, J., Chesley, S., Dunham, D., Farquhar,љR., Giorgini, J., Helfrich, C., Konopliv, A., McAdams, J., Miller, J., Owen, W., Scheeres, D., Thomas, P., Veverka, J., Williams, B., 2000. Radio science results during the NEAR-Shoemaker spacecraft rendezvous with Eros. Science 289, 2085-2088.
<< Глава 3. Плоскодонные кратеры ... | Оглавление |