... M.C. and Ostro,, S.J., The Surface of Titan: Arecibo Radar Observations , in 33 rd ... O'Neil, K. and Bothun, G.D., Low Surface Brightness Galaxies and the Tully-Fisher ...
... sessions to determine the rotational dynamics of Mercury and Venus with a new radar ... the core-mantle and atmosphere-surface boundaries, and other geophysical phenomena ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/MargottagR1786tp.ps -- 91.1 Кб -- 19.04.2004 Похожие документы
... 1 Earth Ellipsoid "Mercury 1960", with semimajor axis 6378166 m and inverse ... 18 acres (73,000 sqare m) . Shape of surface . 70 spherical cap . ... Radius of curvature . 870 ft (265 m) . Surface accuracy . 2.2 mm rms . ...
... O'Neil, K., The Discovery of Red Low Surface Brightness Galaxies in The Low Surface Brightness Universe , IAU Colloq. 171, eds. J. Davies, M. Disney, S. Phillipps (San Francisco:ASP) (1999) . ...
... A. Taylor , and R.F. Jurgens, Near-Earth Asteroid Surface Roughness Depends on Compositional Class , Icarus 198, 294-304, 2008 ... Harmon, J.K. , Radar Imagery of the Southern Caloris Region, Mercury , Icarus 196, 298-301, 2008. ...
... Campbell, D.B., Analysis of Volcanic Surface Morphology on Venus from Comparison of ... J.K. and Slade, M.A., Radar Mapping of Mercury: Full-Disk Images and Polar Anomalies ...
... The Small Scale Environment of Low Surface Brightness Disk Galaxies , Astrophys ... Velez, R., Crespo, A., Dryer, M., New Radar Images of the Poles of Mercury , Bull ...
... One of Arecibo's main accomplishments has been to use active radar mapping to measure surface topographies and rotation rates of Mercury, Venus and the Moon. ...
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Ссылки http://www.naic.edu/~phil/misc/seniorReview06/AstSeniorReview.pdf -- 2058.1 Кб -- 03.11.2006 Похожие документы
... gas production rates for the properties of specific active regions on the surface ... be traced back to particular localities on the cometary surface (e.g. Belton et al ...
... The discovery of possible polar "ice caps" on Mercury with the Goldstone and Arecibo radar systems in 1991 initiated numerous studies of the stability of ice near the planet's poles, both sub-surface ice and ice on the permanently shaded floors of impact ...