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- Q723802 subject Q15264787.
- Q723802 subject Q6746745.
- Q723802 subject Q6935928.
- Q723802 subject Q7685539.
- Q723802 subject Q8736907.
- Q723802 abstract "A lunar dome is a type of shield volcano that is found on the surface of the Earth's Moon. They are typically formed by highly viscous, possibly silica-rich lava, erupting from localized vents followed by relatively slow cooling. Lunar domes are wide, rounded, circular features with a gentle slope rising in elevation a few hundred meters to the midpoint. They are typically 8–12 km in diameter, but can be up to 20 km across. Some of the domes contain a small craterlet at the peak.Some of the domes have been shown to consist of the same materials as the lunar maria. Thus they could be created by some mechanism that differs from the mare-forming flows. It is thought that these domes are formed from a smaller magma chamber that is closer to the surface than is the case for a mare. This results in a lower pressure, and so the lava flows more slowly. The magma wells up through a crack in the surface, but the flow eventually concentrates through one primary vent. This concentration can then result in a vent crater at the peak of the dome.The cluster of lunar domes at the Marius Hills was considered as a possible landing site of Apollo 15. There are concentrations of lunar domes near the craters Hortensius, and T. Mayer, across the top of Mons Rümker, and in Mare Fecunditatis. Solitary lunar domes are also found, including Kies Pi (π), Milichius Pi (π), Mons Gruithuisen Gamma (γ) and Delta (δ), and domes near the craters Gambart C, Beer, and Capuanus. Omega Cauchy (ω) and Tau Cauchy (τ) form a pair of domes near the crater Cauchy. Likewise near Arago are the domes Arago Alpha (α) and Arago Beta (β). There are two domes south of Mons Esam.".
- Q723802 thumbnail Milichius_Pi_4133_h2.jpg?width=300.
- Q723802 wikiPageExternalLink gibbidomine.
- Q723802 wikiPageExternalLink lunar_domes.htm.
- Q723802 wikiPageExternalLink 2002JE001909.shtml.
- Q723802 wikiPageExternalLink lunar.html.
- Q723802 wikiPageExternalLink 978-88-470-2636-0.
- Q723802 wikiPageExternalLink lunar_dome.html&date=2009-10-26+01:15:34.
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- Q723802 wikiPageWikiLink Q6746745.
- Q723802 wikiPageWikiLink Q6935928.
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- Q723802 wikiPageWikiLink Q7685539.
- Q723802 wikiPageWikiLink Q814070.
- Q723802 wikiPageWikiLink Q8736907.
- Q723802 comment "A lunar dome is a type of shield volcano that is found on the surface of the Earth's Moon. They are typically formed by highly viscous, possibly silica-rich lava, erupting from localized vents followed by relatively slow cooling. Lunar domes are wide, rounded, circular features with a gentle slope rising in elevation a few hundred meters to the midpoint. They are typically 8–12 km in diameter, but can be up to 20 km across.".
- Q723802 label "Lunar dome".
- Q723802 depiction Milichius_Pi_4133_h2.jpg.