Water on terrestrial planets of the Solar System Water on terrestrial planets of the Solar System The origin and development of water on terrestrial planets, Venus, Earth, Mars, and the closely related Earth's Moon, varies with each planetary body, with the exact origins remaining unclear. Additionally, the terrestrial dwarf planet, Ceres is known to have water ice on its surface. A significant amount of surface hydrogen has been observed globally by the Mars Odyssey GRS. Stoichiometrically estimated water mass fractions indicate that—when free of carbon dioxide—the near surface at the poles consists almost entirely of water covered by a thin veneer of fine material. This is reinforced by
First Suite in E-flat for Military Band shelf listing is as follows: Add. MS 47824. GUSTAV HOLST COLLECTION. Vol. XXI (ff. 37). First Suite in E flat for military band, op. 28, no. 1, consisting of Chaconne, Intermezzo and March. [1909.] Full score. Autograph. With various notes on f.1 relating to ad lib. parts, etc. Published by Boosey & Co., 1921, in Boosey's Military Journal, 142nd Series, No. 2. [I. Holst, no. 105.] The original title of the suite was simply "Suite in E for Military Band by Gustav von Holst". Holst's birthname had actually been Gustavus Theodore von Holst (he had German, Russian, Latvian and Swedish