http://vospace.esac.esa.int/vospace/sh/7a14a339d09a653f5ac4a7f0bb46d13b8788a7f7?dl=1 WebTwo distinct chemical basalt types have been sampled at the Apollo 17 landing site. Very high-titanium basalts (about 13 wt % TiO2) are the dominant type and display a …
Patrick Donohue - Kennewick, Washington, United States - LinkedIn
Web14 dic 2024 · Basalts in Mare Nectaris and Orientale are in the groups of very-low-titanium basalts and low-titanium basalts . Very-low-titanium and low-titanium basalts (<5 … WebThese basalts occur in two principal ways: as small rocks in the regolith from highland sites and as lithic fragments in highland breccias. The former occurrence of mare basalt is likely to result from the deposition of a ray from an impact crater on the distant maria, flung as ejecta to the highland site. porsche 911 informacje
Quantitative textural analysis of ilmenite in Apollo 17 high-titanium ...
WebCalculated values of log alpha SiO2 in lunar magmas range from approximately -0.8 to unity in the temperature range of 1100-1300 C. High-titanium mare basalts begin crystallizing at silica activities insufficient for orthopyroxene saturation; in contrast to terrestrial lavas, silica activities rise substantially with crystallization and cause silica saturation in the residuum. Web19 ott 2024 · The lithic clasts in the soils are composed of about 45% basalt and about 55% breccia. The breccia clasts are dominated by basalt fragments (more than 80%) with minor impact melt and agglutinate.... Web9 gen 2003 · Moreover, the depths of origin of these glasses can exceed 500 km (refs 27–29) and might share a mantle source with PKT basalts. If the high-titanium source region originally solidified at a ... porsche 911 indoor car cover