Porosity of phobos
WebPhobos, the 22-km diameter innermost moon of Mars, is a groovy body. ... Phobos has a near-surface porosity of at least 40%, so it seems impossible to sustain 2/5.
Porosity of phobos
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WebNov 23, 2015 · Its high porosity (for example, ref. 13) and hypothesized origin as a captured asteroid 69 or gravitational aggregate 51,70,71,72 imply Phobos is likely to be highly heterogeneous (possibly ... WebJan 1, 2024 · Phobos' spectra showed significant slope variation at shorter wavelengths (λ < 1.3 μm), suggesting surface heterogeneity possibly due to regolith's composition and grain size, and/or space weathering. Deimos' spectra indicated the presence of water/hydroxyl with a band depth at 2.90 μm of 4–5%.
WebOct 1, 2011 · Indeed, the density of Phobos, 1.87 +/- 0.02 g/cm [4,5], is lower than the density of presumed material analogs, suggesting that the interior of this small moon can contain … WebMay 7, 2010 · The porosity of Phobos is computed from its mass, its bulk density and known grain densities of the hydrous chondrites of the CM group and the Tagish-Lake meteorite …
WebAssuming Phobos is made of a mixture of poros- ity (macro-porosity or micro-porosity), Rosenblatt et al. (2011) have proposed models of heterogeneous internal mass distribu- tion inside Phobos, which can fit its bulk density and librational angle. Numerical models suggest that the formation of Stickney Table 1. WebJan 1, 2013 · Compositional interpretations of new spectral measurements of Phobos and Deimos from Mars Express/OMEGA and MRO/CRISM and density measurements from encounters by multiple spacecraft support refined estimates of the moons' porosity and internal structure. Phobos' estimated macroporosity of 12-20% is consistent with a …
Webspectral measurements of Phobos and Deimos from Mars Express/OMEGA and MRO/CRISM and density measurements from encounters by multiple spacecraft support refined estimates of the moons' porosity and internal structure. Phobos' estimated macroporosity of 12-20% is consistent with a fractured but coherent inte-
http://www.planetary.brown.edu/planetary/geo287/PhobosDeimos/papers/Criton2015Icarus-giantimpact.pdf pool deck with fire pitWebof them have significant fracture porosity, as well as evidence of internal voids manifested as chains of pit craters. These are probably formed by the drainage of ... Eros, 28 on (951) Gaspra and 57 on Phobos. The smallest subsidence craters are detected W.in (433) Eros, probably because the resolution Conferenceof the images used is much ... sharda the singerWebThe Phobos monolith is a large rock on the surface of Mars's moon Phobos. It is a boulder about 85 m (279 ft) across and 90 m (300 ft) tall. A monolith is a geological feature … sharda trading companyWebMar 15, 2024 · Mass heterogeneities correspond to either an excess of porosity or a compaction of material under Stickney , or a deficit of porosity in the upper layers of … sharda transportWebPhobos is the larger of the two moons, and is the closer of the two to Mars. Phobos has an average radius of 11 km, while Deimos has an average radius of 6 km. The origin of Mars' moons, Phobos and Deimos (pictured right), is unknown and remains controversial. One theory is that the moons are captured asteroids. shard at nightWebThe high porosity of the interior of Phobos (based on the density of 1.88 g/cm 3, voids are estimated to comprise 25 to 35 percent of Phobos's volume) is inconsistent with an … sharda tripathi google scholarWebspectral measurements of Phobos and Deimos from Mars Express/OMEGA and MRO/CRISM and density measurements from encounters by multiple spacecraft support refined … pool deck trench drain