Lunar lava tube
Lunar lava tubes are sub-surface tunnels on the Moon that are thought to have formed during basaltic lava flows. When the surface of a lava tube cools, it forms a hardened lid that contains the ongoing lava flow beneath the surface in a conduit-shaped passage. Once the flow of lava diminishes, the tunnel may drain, forming a hollow void. Lunar lava tubes are formed on surfaces that have a slope that ranges in angle from 0.4° to 6.5°. Lunar lava tubes may be as wide as 500 metres (1,600 ft) before they become unstable against gravitational collapse. However, stable tubes may still be disrupted by seismic events or meteoroid bombardment.
The existence of a lava tube is sometimes revealed by the presence of a "skylight", a place in which the roof of the tube has collapsed, leaving a circular hole that can be observed by lunar orbiters.
An area displaying a lava tube and rilles is the Marius Hills region. ( ) In 2008, an opening to a lava tube in this area may have been discovered by the Japanese Kaguya spacecraft. The skylight was photographed in more detail in 2011 by the Lunar Reconnaissance Orbiter, showing both the 65-meter wide pit and the floor of the cave about 36 meters below. The Hadley Rille may have been a partly roofed lava channel, some parts of which have since collapsed. There may also be lava tubes in the Mare Serenitatis.
The Lunar Reconnaissance Orbiter has imaged over 200 pits that show the signature of being skylights into subsurface voids or caverns, ranging in diameter from about 5 m (16 ft) to more than 900 m (3,000 ft), although some of these are likely to be post-flow features rather than volcanic skylights.
The Chandrayaan-1 orbiter imaged a lunar rille, formed by an ancient lunar lava flow, with an uncollapsed segment indicating the likely presence of a lava tube near the lunar equator, measuring about 2 km (1.2 mi) in length and 360 m (1,180 ft) in width.
Gravitometric observations by the GRAIL spacecraft suggest the presence of lunar lava tubes with widths of over 1 km. Assuming a width-to-height ratio of 3:1, such a structure can remain stable with a ceiling that is 2 m (6.6 ft) thick. Lava tubes at least 500 m underground can theoretically remain stable with widths of up to 5 km.
This section needs expansion. You can help by adding to it. (November 2017)
The "Moon Diver" mission led by Laura Kerber proposes to send the two-wheeled AXEL extreme-terrain rover developed at NASA-JPL into a lunar pit in order to investigate the history of the lunar mare and flood basalt eruptions.
Sites for human habitats
Lunar lava tubes may potentially serve as enclosures for human habitats. Tunnels larger than 300 metres (980 ft) in diameter may exist, lying under 40 metres (130 ft) or more of basalt with a stable temperature of −20 °C (−4 °F). These natural tunnels provide protection from cosmic radiation, solar radiation, meteorites, micrometeorites, and ejecta from impacts. They are shielded from the variations in temperature at the lunar surface, which would provide a stable environment for inhabitants. Lunar lava tubes are typically found along the boundaries between lunar mares and highland regions. This would give ready access to elevated regions for communications, basaltic plains for landing sites and regolith harvesting, and underground mineral resources.
- Greeley, Ronald (December 1971), "Lava Tubes and Channels in the Lunar Marius Hills", The Moon, 3 (3): 289–314, Bibcode:1971Moon....3..289G, doi:10.1007/BF00561842, hdl:2060/19710008532
- Cruikshank, D. P.; Wood, C. A. (March 1972), "Lunar Rilles and Hawaiian Volcanic Features: Possible Analogues", The Moon, 3 (4): 412–447, Bibcode:1972Moon....3..412C, doi:10.1007/BF00562463
- Huber, S. A.; et al. (2014), "Astrobotic Technology: Planetary Pits and Caves for Science and Exploration", Annual Meeting of the Lunar Exploration Analysis Group, abstract 3065 (PDF), retrieved 24 January 2016.
- Clark, Liat (9 February 2011), First underground cave photographed on the moon, Wired UK, archived from the original on 10 February 2011, retrieved 24 January 2016 Cite uses deprecated parameter
- Handwerk, Brian (October 26, 2009), First Moon "Skylight" Found -- Could House Lunar Base?, National Geographic, retrieved 2011-01-27
- "The Marius Hills hole is a possible skylight". Photojournal. Jet Propulsion Laboratory. Retrieved 28 June 2011.
- Greeley, Ronald (May 1971), "Lunar Hadley Rille: Considerations of Its Origin", Science, 172 (3984): 722–725, Bibcode:1971Sci...172..722G, doi:10.1126/science.172.3984.722, hdl:2060/19710005212, PMID 17780969
- Coombs, Cassandra R.; Hawke, B. Ray (September 1992), "A search for intact lava tubes on the Moon: Possible lunar base habitats", In NASA. Johnson Space Center, The Second Conference on Lunar Bases and Space Activities of the 21st Century (SEE N93-17414 05-91), 1, pp. 219–229, Bibcode:1992lbsa.conf..219C
- Scientists eye moon colonies — in the holes on the lunar surface, New York Daily News, retrieved 13 October 2011
- Plait, Phil (5 March 2010), Spelunking the Lunar Landscape, Discovery Magazine "Bad Astronomy" blog, retrieved 24 January 2016 Italic or bold markup not allowed in:
- Very Clever! LRO Views Huge Lava Tube Skylight in Mare Ingenii, Universe Today, retrieved 13 October 2011
- Dvorsky, George (October 18, 2014), "Could This Lunar Cave Provide Shelter for a Future Moon Colony?", io9/ Gizmodo.com, retrieved 24 January 2016.
- Wagner, Robert V.; Robinson, Mark S. (July 15, 2014), "Distribution, formation mechanisms, and significance of lunar pits", Icarus, 237: 52–60, Bibcode:2014Icar..237...52W, doi:10.1016/j.icarus.2014.04.002.
- Arya, A. S.; et al. (February 25, 2011), "Detection of potential site for future human habitability on the Moon using Chandrayaan-1 data", Current Science, 100 (4), retrieved 2016-12-19.
- "After water, now Indian scientists find cave on Moon", Silicon India News, February 8, 2010, retrieved 2016-01-24.
- Blair, David M.; et al. (January 15, 2017), "The structural stability of lunar lava tubes", Icarus, 282: 47–55, Bibcode:2017Icar..282...47B, doi:10.1016/j.icarus.2016.10.0081
- Ximenes, S. W.; Elliott, J. O.; Bannova, O. (2012). "Defining a Mission Architecture and Technologies for Lunar Lava Tube Reconnaissance". Earth and Space 2012. p. 344. doi:10.1061/9780784412190.038. ISBN 978-0-7844-1219-0.
- "Lecture: Moon Diver Mission Concept - Descending into a Moon Cave to Better Understand the Solar System's Largest Volcanic Eruptions". www.kiss.caltech.edu. Retrieved 2018-06-24.
- KISSCaltech (2018-04-03), Moon Diver Mission Concept, retrieved 2018-06-24
- O'Neill, Ian (October 27, 2009), "Living in Lunar Lava Tubes", Discover News, retrieved 1 January 2012.
- York, Cheryl Lynn; et al. (December 1992), "Lunar lava tube sensing", Lunar and Planetary Institute, Joint Workshop on New Technologies for Lunar Resource Assessment, pp. 51–52, Bibcode:1992ntlr.work...51Y
- De Angelis, G.; et al. (November 2001), "Lunar Lava Tubes Radiation Safety Analysis", Bulletin of the American Astronomical Society, 33: 1037, Bibcode:2001DPS....33.1003D
- Walden, Bryce E.; et al. (January 1998), "Utility of Lava Tubes on Other Worlds", Workshop on Using In Situ resources for Construction of Planetary Outposts, p. 16, Bibcode:1998uisr.work...16W