Results 1 to 10 of about 14,933 (266)

Parameter Estimation of Lunar Regolith from Lunar Penetrating Radar Data. [PDF]

open access: goldSensors (Basel), 2018
Parameter estimation of the lunar regolith not only provides important information about the composition but is also critical to quantifying potential resources for lunar exploration and engineering for human outposts.
Zhang L   +6 more
europepmc   +4 more sources

Vapor Deposits in the Lunar Regolith [PDF]

open access: bronzeScience, 1994
Since the Apollo missions, we have emphasized the following points, which are based on theoretical calculations and on laboratory studies of the properties of evaporated silicate deposits and of lunar samples. The mass of vapor generated by impacts on the lunar surface is comparable in magnitude to the mass of impact melt glasses; the physics of impact
Bruce Hapke   +2 more
  +11 more sources

Phosphorus-solubilizing bacteria improve the growth of Nicotiana benthamiana on lunar regolith simulant by dissociating insoluble inorganic phosphorus. [PDF]

open access: yesCommun Biol, 2023
In-situ utilization of lunar soil resources will effectively improve the self-sufficiency of bioregenerative life support systems for future lunar bases.
Xia Y, Yuan Y, Li C, Sun Z.
europepmc   +2 more sources

Thermal Extraction of Volatiles from Lunar and Asteroid Regolith in Axisymmetric Crank-Nicholson Modeling [PDF]

open access: hybridJ. Aerospace Engineering 33, no.6 (Nov. 2020): 04020075, 2023
A physics-based computer model has been developed to support the development of volatile extraction from regolith of the Moon and asteroids. The model is based upon empirical data sets for extraterrestrial soils and simulants, including thermal conductivity of regolith and mixed composition ice, heat capacity of soil and mixed composition ice, hydrated
Philip T. Metzger   +2 more
arxiv   +3 more sources

Experiments Indicate Regolith is Looser in the Lunar Polar Regions than at the Lunar Landing Sites [PDF]

open access: greenarXiv, 2018
Since the Apollo program or earlier it has been widely believed that the lunar regolith was compacted through vibrations including nearby impact events, thermal stress release in the regolith, deep moon quakes, and shallow moon quakes. Experiments have shown that vibrations both compact and re-loosen regolith as a function of depth in the lunar soil ...
Philip T. Metzger   +2 more
arxiv   +3 more sources

In-Situ Radar Observation of Shallow Lunar Regolith at the Chang’E-5 Landing Site: Research Progress and Perspectives [PDF]

open access: goldRemote Sensing, 2023
China accomplished a historic milestone in 2020 when the mission Chang’e-5 (CE-5) to the Lunar’s surface was successfully launched. An extraordinary component of this mission is the “Lunar Regolith Penetrating Radar” (LRPR) housed within its lander ...
Feiyang Fang   +5 more
doaj   +2 more sources

The Lunar Regolith Structure and Electromagnetic Properties of Chang’E-5 Landing Site [PDF]

open access: goldRemote Sensing, 2022
On 1 December 2020, China’s Chang’E-5 (CE-5) probe successfully landed in the northeastern Oceanus Procellarum. This work mainly presents the results of Lunar Regolith Penetrating Radar (LRPR) equipped on the CE-5 Lander.
Yuxi Li   +8 more
doaj   +2 more sources

Matrix transformation of lunar regolith and its use as a feedstock for additive manufacturing. [PDF]

open access: yesiScience, 2023
Summary: Building a sustainable human habitat on the Moon requires advances in excavation, paving, and additive manufacturing to construct landing pads, surface transportation arteries, resilient shelters, and scientific outposts.
Cool NI   +12 more
europepmc   +2 more sources

Telomere dynamics and oxidative stress in Arabidopsis grown in lunar regolith simulant. [PDF]

open access: yesFront Plant Sci
NASA envisions a future where humans establish a thriving colony on the Moon by 2050. Plants will be essential for this endeavor, but little is known about their adaptation to extraterrestrial bodies.
Barcenilla BB   +10 more
europepmc   +2 more sources

Automated Mineralogy Analysis of the Apollo 17 73002 Continuous Core Thin Sections Using QEMSCAN Mapping Techniques. [PDF]

open access: yesJ Geophys Res Planets
Abstract The Apollo 17 73001/73002 double drive tube, collected at the base of the South Massif in the Taurus‐Littrow Valley, was opened in 2019 as part of the Apollo Next Generation Sample Analysis program (ANGSA). A series of continuous thin sections were prepared capturing the full length of the upper portion of the double drive tube (73002).
Bell SK   +7 more
europepmc   +2 more sources

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