Lunar Polar Ice Everywhere, but Only on Surface

An international team of Chinese, American, and Russian scientists may have conducted the most extensive study of lunar Permanently Shadowed Region (PSR) ice yet performed. By comparing the reflections from flat surfaces in major PSRs to those of adjacent non-PSRs, they determined that the vast majority contain ice. However, the ice appears to be restricted to the uppermost surface.

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Why the Lunar South Pole?

NASA was recently directed to return to the Moon by 2024, an announcement first made in remarks given by Vice President Mike Pence at the 5th meeting of the National Space Council on March 26th. However this huge announcement and acceleration in schedule also came with another set of exciting details. He stated, the “lunar South Pole holds great scientific, economic, and strategic value” and that “when the first American astronauts return to the lunar surface, that they will take their first steps on the Moon’s South Pole.” But why the focus on the Moon’s south pole? He explored that as well, saying that we will “mine oxygen from lunar rocks” and “use nuclear power to extract water from the permanently shadowed craters of the South Pole”. These statements are exciting because they specifically include the use of in-situ resource utilization on the Moon, and select human landing locations near the South Pole due to proximity to those resources.

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Adam Hugomoon, nasa, isru, waterComment
Lunar Lava Tube Exploration

Lava tubes on the Moon represent an enticing location for establishing lunar habitats. In addition to providing protection from radiation and meteorites, lunar lava tubes have a stable temperature range compared to surface conditions. These characteristics will allow the building of safe, yet economical habitats in lava tubes. However, we must first explore and categorize lava tubes before establishing the first settlements in them. One likely platform for enabling this exploration is via the Moon Diver mission and the tethered Axel rover.

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Surface Strength of PSRs

Although multiple landers and rovers have touched down on the Moon, no vehicle has visited the Permanently Shadowed Regions (PSRs) at the lunar poles. Water ice has been observed within some PSRs, and therefore represents an ideal target for future lunar missions. An important unknown to study before the first PSR mission is understanding the surface environment, including how much mass the PSR regolith can support. It is critical that rover wheels and landing pads don’t sink into the regolith. To study this, a recent analysis used boulder tracks to evaluate the bearing capacity of regolith in these areas.

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The Space Resource Newsletter - March 2019

Welcome to The Space Resources monthly newsletter for March 2019. We have seen exciting news related to evidence of groundwater on Mars, hydrated minerals on Bennu, and NASA being challenged to return astronauts to the Moon by 2024. However, the Indian anti-satellite test and failure of UN talks to create a space disarmament treaty place a dark cloud on the horizon.

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More Questions than Answers at Bennu

After less than three months in orbit, the NASA OSIRIS-REx mission has already made several discoveries about the Near Earth Asteroid (NEA) Bennu. Most promising for resource utilization is the presence of water-bearing (hydrated) materials. However, the environment is dangerous with particle ejections from unknown sources, many large boulders, and an ever accelerating rotation rate. Asteroid exploration and processing missions are in for a challenge!

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Impacting Lunar Polar Ice

The permanently shadowed regions (PSRs) at the lunar poles represent prime locations for finding high concentrations of water bearing material on the Moon. Even though PSRs have been remotely observed for the past few decades, much is still unknown about these areas. Key questions include the origin of the ice, how extensive it is, and how it changes over time. A recent model addresses some of these questions by predicting how long near-surface ice should exists before being sublimated away.

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Advanced Composite Habitats

Extraterrestrial habitats are required for sustained human exploration of space. The trade-off between mass, size, and safety is a concern for all proposed systems. The goal is to provide a low mass system that is easy to transport, while providing maximum space to astronauts and protection from the harsh environment. In addition to large temperature swings, structures need to survive multiple g’s during transportation, radiation, and micrometeorite impacts.

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Modeling Ice in Asteroids

A key appeal for processing water from asteroids as opposed to the Moon is the low delta-V required to get to and from them. However, this assumes that water rich asteroids come near Earth. Scientists from the Planetary Science Institute have recently developed an analytical model that can help estimate if some near-Earth objects (NEOs) contain water ice.

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Ryugu's Visitor

The quiet, everlasting vacuum has been a steady companion. After millions of years, a new visitor emerged from the darkness. Normally visitors come barreling in and cause a significant disturbance. Unusually, this visitor remained in a cautious orbit for a few months. Out of nowhere, this new companion approached with a strange appendage and fired a metal slug into the surface. Materials ejected were collected in a surgical fashion before the visitor retreated back to a safe distance. Quietness once again enveloped the scene.

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What are China's Moon Plans?

With the China National Space Administration (CNSA) successfully landing their Chang’e 4 lander and Yutu-2 rover in January 2019, China has now had two successful landings on the Moon. Their first successful landing with Chang’e 3 was also the first soft landing on the lunar surface since the Soviet Luna 24 in 1976. China’s most recent landing with Chang’e 4 is an even greater accomplishment as it is the first time any spacecraft has landed on the Moon’s far side. These missions are just the start of China’s ultimate goals for lunar exploration.

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Adam Hugomoon, chinaComment
Surviving the Temperamental Moon

As indicated by the title of Robert Heinlein's 1966 novel The Moon is a Harsh Mistress, the Moon is a harsh environment to operate in. There is a scant atmosphere, abrasive dust, and extreme temperature ranges to deal with. Observed temperatures range from a blistering 127 C (260 F) in equatorial sunlight down to a frosty -238 C (-397 F) in the permanently shadowed regions of the poles. Designing missions to survive these conditions pushes current technology to its limits.

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The Importance of Lunar Landing Ejecta and Emissions

There are many exciting opportunities to be found as gradual progress is made to return humans to the Moon to stay in the coming years. With these opportunities there are also various challenges to overcome related to an increasing frequency of landed missions. When spacecraft land they emit large quantities of gases and displace significant amounts of regolith. Because of the Moon’s low gravity and thin atmosphere relative to the Earth, both of these actions have magnified effects.

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Adam Hugomoon, ejecta Comment