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 … Web5 apr 2024 · The in-form mare had a maintenance gallop to finalise her preparation. Matt Cumani runs Hanaady, who worked with James The Great on the hill track, their last 600m in 36.44.

Diverse Geological Evolution of Impact Basins on the Moon

WebСписок литературы. Барсуков В.Л., Сурков Ю.А., Москалева Л.П., Щеглов О.П. (1982) Геохимические ... Web2 giorni fa · In 1970, the Soviet robotic station Luna 16 landed in the northeastern portion of Mare Fecunditatis (Fig. 1 a) and returned a sample of lunar regolith to Earth [Vinogradov and Vinogradov, 1971].The drill system of Luna 16 penetrated 35 cm of the uppermost loose regolith, below which occurred the surface of a higher-strength material; the total weight … new jersey vs washington dc

Mare basalts from the Taurus-Littrow region of the Moon

WebThe high titanium basalts collected in the maria Tranquillitatis and Serenitatis crystallized 3.5-3.9 Ga ago. The ages of the low titanium rocks found in Oceanus Procellarum and on the eastern edge of mare Imbrium are lower, 3.1-3.4 Ga. There is, however, evidence that high-Ti basalts with lower ages and low-Ti basalts with higher ages occur on ... 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 … Web17 set 2016 · The last major phases of lunar volcanism occurred mainly in Oceanus Procellarum and Mare Imbrium and produced spectrally unique medium- and high … new jersey w2 forms