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Journal articles on the topic 'Geology of the Moon'

Author: Grafiati

Published: 24 April 2022

Last updated: 30 July 2025

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1

Marvin, Ursula B. "Meteorites, the Moon and the History of Geology." Journal of Geological Education 34, no. 3 (1986): 140–65. http://dx.doi.org/10.5408/0022-1368-34.3.140.

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2

Rynott, Tim. "Fly Me to the Moon." Mountain Geologist 60, no. 4 (2023): 197–205. http://dx.doi.org/10.31582/rmag.mg.60.3.197.

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On August 16th, 1960, sitting in an open-air gondola at 103,000’ carefully suspended by a 200’ tall helium balloon, U.S. Air Force Captain Joe Kittinger peers upon cobalt blue skies and the blackest of black (Figure 1). The avant-garde astronaut gets word from the ground crew, “Jump!”, triggering a free fall from 103,000’ and setting the record for the highest skydive ever by any living being (Kittinger, 1961; Kindy, 2023). Captain Joe blazed the trail for the likes of Sheppard, Grissom, and Glenn, testing the limits of the human body. A mere nine years later helium – a relative newcomer to th

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3

Yang, Zhen, Guiqin Wang, Yuming Xu, Yuling Zeng, and Zhaofeng Zhang. "A Review of the Lunar 182Hf-182W Isotope System Research." Minerals 12, no. 6 (2022): 759. http://dx.doi.org/10.3390/min12060759.

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In recent years, the extinct nuclide 182Hf-182W system has been developed as an essential tool to date and trace the lunar origin and evolution. Despite a series of achievements, controversies and problems exist. As a review, this paper details the application principles of the 182Hf-182W isotope system and summarizes the research development on W isotopes of the Moon. A significant radiogenic ε182W excess of 0.24 ± 0.01 was found in the lunar mantle, leading to heated debates. There are three main explanations for the origin of the excess, including (1) radioactive origin; (2) the mantle of t

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4

Rader, Matthew. "Atmospheric Moon River." Canada and Beyond: A Journal of Canadian Literary and Cultural Studies 12 (October 20, 2023): 165–67. http://dx.doi.org/10.14201/candb.v12i165-167.

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These two long poems address both embodied and encultured experiences of climate change in the Kelowna region of the Okanagan Valley and the Salmon Arm region of the Shuswap in the British Columbia southern interior. Both poems grapple with the fear of future-oriented thinking in a time of climate catastrophe while registering the long historical dimensions that inform that present fear. “Atmospheric Moon River” examines desire and beauty in the context of torrential rain and flooding that resulted in the deaths of several humans and many hundreds of farm animals. The poem updates old qu

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5

Xing, Lin. "Lunar explorer." Physics World 35, no. 6 (2022): 10i—11i. http://dx.doi.org/10.1088/2058-7058/35/06/14.

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6

Reuver, M., R. J. de Meijer, I. L. ten Kate, and W. van Westrenen. "Boundary conditions for the formation of the Moon." Netherlands Journal of Geosciences - Geologie en Mijnbouw 95, no. 2 (2015): 131–39. http://dx.doi.org/10.1017/njg.2015.24.

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AbstractRecent measurements of the chemical and isotopic composition of lunar samples indicate that the Moon's bulk composition shows great similarities with the composition of the silicate Earth. Moon formation models that attempt to explain these similarities make a wide variety of assumptions about the properties of the Earth prior to the formation of the Moon (the proto-Earth), and about the necessity and properties of an impactor colliding with the proto-Earth. This paper investigates the effects of the proto-Earth's mass, oblateness and internal core-mantle differentiation on its moment

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7

Foing, B. H., C. Stoker, and P. Ehrenfreund. "Astrobiology field research in Moon/Mars analogue environments." International Journal of Astrobiology 10, no. 3 (2011): 137–39. http://dx.doi.org/10.1017/s1473550411000139.

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AbstractExtreme environments on Earth often provide similar terrain conditions to landing/operation sites on Moon and Mars. Several field campaigns (EuroGeoMars2009 and DOMMEX/ILEWG EuroMoonMars from November 2009 to March 2010) were conducted at the Mars Desert Research Station (MDRS) in Utah. Some of the key astrobiology results are presented in this special issue on ‘Astrobiology field research in Moon/Mars analogue environments’ relevant to investigate the link between geology, minerals, organics and biota. Preliminary results from a multidisciplinary field campaign at Rio Tinto in Spain a

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8

Wood, Charles. "Scientific Knowledge of the Moon, 1609 to 1969." Geosciences 9, no. 1 (2018): 5. http://dx.doi.org/10.3390/geosciences9010005.

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Discoveries stemming from the Apollo 11 mission solved many problems that had vexed scientists for hundreds of years. Research and discoveries over the preceding 360 years identified many critical questions and led to a variety of answers: How did the Moon form, how old is its surface, what is the origin of lunar craters, does the Moon have an atmosphere, how did the Moon change over time, is the Moon geologically active today, and did life play any role in lunar evolution? In general, scientists could not convincingly answer most of these questions because they had too little data and too lit

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9

Sharkov, E. V., and O. A. Bogatikov. "Tectonomagmatic evolution of the Earth and Moon." Geotectonics 44, no. 2 (2010): 85–101. http://dx.doi.org/10.1134/s0016852110020019.

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10

Jaumann, R., H. Hiesinger, M. Anand, et al. "Geology, geochemistry, and geophysics of the Moon: Status of current understanding." Planetary and Space Science 74, no. 1 (2012): 15–41. http://dx.doi.org/10.1016/j.pss.2012.08.019.

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11

Talwani, Manik. "The Apollo 17 gravity measurements on the moon." Leading Edge 22, no. 8 (2003): 786–89. http://dx.doi.org/10.1190/1.1605083.

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12

Hammond, Noah P., and Amy C. Barr. "Global resurfacing of Uranus’s moon Miranda by convection." Geology 42, no. 11 (2014): 931–34. http://dx.doi.org/10.1130/g36124.1.

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13

Simms, Michael J. "Meteorites and the Moon." Geology Today 37, no. 6 (2021): 231–36. http://dx.doi.org/10.1111/gto.12373.

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14

Huang, Yuetong. "Building Beyond Earth: Creating a Scientific Facility on the Moon." Highlights in Business, Economics and Management 47 (February 8, 2025): 229–35. https://doi.org/10.54097/d0p9eq45.

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The Earth’s resources are now being further complicated to an engineer by climate change and population growth. As such, the quest for alternative habitats is more than ever before necessary. In this paper, we discuss the plausibility of a sustainable human habitat on the Moon with special reference to Moon Village Project for a collaborative effort toward lunar colonization. We go on to describe, in detail, the enormous challenges that would be met in erecting a structure on the Moon with respect to the highly laminar environmental situation, the scarcity of resources, as well as the plight o

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15

McKinnon, William B., and Randy L. Korotev. "The geology of multi-ring impact basins: The moon and other Planets." Geochimica et Cosmochimica Acta 58, no. 20 (1994): 4532–33. http://dx.doi.org/10.1016/0016-7037(94)90357-3.

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16

Radhakrishna, B. P. "40th anniversary of Mankind’s Great Voyage to the Moon." Journal of the Geological Society of India 74, no. 3 (2009): 287–89. http://dx.doi.org/10.1007/s12594-009-0131-8.

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17

Vanyo, J. P., and S. M. Awramik. "Stromatolites and earth—sun—moon dynamics." Precambrian Research 29, no. 1-3 (1985): 121–42. http://dx.doi.org/10.1016/0301-9268(85)90064-6.

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18

Braun, Alexander, Mark Panning, Sean Gulick, and Yongyi Li. "Introduction to this special section: Planetary geophysics." Leading Edge 41, no. 10 (2022): 670–71. http://dx.doi.org/10.1190/tle41100670.1.

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While geophysical exploration of Earth is well established as a critical method for understanding planetary processes, many current and planned missions offer great opportunities for geophysicists to apply their skills and expertise to space exploration. Programs such as NASA's Artemis aiming to bring humans back to the moon and the James Webb Space Telescope for deep space imaging, the 10-year extension plan for the Chinese Lunar Exploration Program's Chang'e missions, the Japanese Aerospace Exploration Agency's Martian Moons eXploration program, and the European Space Agency's European Large

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19

Stewart, Robert R. "President's Page." Leading Edge 38, no. 9 (2019): 666–67. http://dx.doi.org/10.1190/tle38090666.1.

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Most people love a little traveling, but this year we celebrate the anniversaries of some of the greatest voyages of exploration. It was 50 years ago on 20 July 1969 that mankind, in the person of Neil Armstrong, first walked on another celestial body, the Moon, with the Apollo 11 mission — certainly a pinnacle step in human accomplishment. We anticipate that a woman, hopefully a geoscientist (such as Harrison Schmitt, the second-to-last man on the Moon), soon will accomplish a similar feat. Perhaps, less well remembered is 500 years ago on 20 September 1519 when Ferdinand Magellan began in Sp

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20

Boyce, Joseph M., Thomas Giguere, Peter Mouginis-Mark, Timothy Glotch, and G. Jeffrey Taylor. "Geology of Mairan middle dome: Its implication to silicic volcanism on the Moon." Planetary and Space Science 162 (November 2018): 62–72. http://dx.doi.org/10.1016/j.pss.2017.12.009.

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21

Martinot, M., S. Besse, J. Flahaut, C. Quantin-Nataf, L. Lozac'h, and W. van Westrenen. "Mineralogical Diversity and Geology of Humboldt Crater Derived Using Moon Mineralogy Mapper Data." Journal of Geophysical Research: Planets 123, no. 2 (2018): 612–29. http://dx.doi.org/10.1002/2017je005435.

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22

Schneer, Cecil. "Geology, Time and History." Earth Sciences History 8, no. 2 (1989): 103–5. http://dx.doi.org/10.17704/eshi.8.2.n871088718k50220.

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There is evidence of consciousness of natural time as far back as the Early Ice Age in recorded observations of the recurrent and successive appearances of the moon. The idea of geologic time was broached as part of the 17th century scientific revolution in the same milieu as the ideal time of rational mechanics, but the sense of time drawn from observations of the earth transcended the limitations of ideal physical law. Inapplicable to "…an unlimited assemblage of local instabilities…" (Maxwell, 1877 p. 14), the laws of physics by definition are independent of the very particulars of time and

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23

Rutherford, Malcolm J., and Paolo Papale. "Origin of basalt fire-fountain eruptions on Earth versus the Moon." Geology 37, no. 3 (2009): 219–22. http://dx.doi.org/10.1130/g25402a.1.

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24

Emmermann, Axel. "For a piece of the moon." Geology Today 18, no. 5 (2002): 186–94. http://dx.doi.org/10.1046/j.0266-6979.2003.00368.x.

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25

Radebaugh, Jani, Dario Ventra, Ralph D. Lorenz, et al. "Alluvial and fluvial fans on Saturn's moon Titan reveal processes, materials and regional geology." Geological Society, London, Special Publications 440, no. 1 (2016): 281–305. http://dx.doi.org/10.1144/sp440.6.

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26

Watters, Thomas R., Mark S. Robinson, Geoffrey C. Collins, et al. "Global thrust faulting on the Moon and the influence of tidal stresses." Geology 43, no. 10 (2015): 851–54. http://dx.doi.org/10.1130/g37120.1.

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27

Jara-Orué, H. M., and B. L. A. Vermeersen. "Tides on Jupiter's moon Ganymede and their relation to its internal structure." Netherlands Journal of Geosciences - Geologie en Mijnbouw 95, no. 2 (2016): 191–201. http://dx.doi.org/10.1017/njg.2015.23.

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AbstractOne of the major scientific objectives of ESA's JUICE (JUpiter ICy moons Explorer) mission, which is scheduled for launch in 2022 and planned to arrive at the Jovian system in 2030, is to characterise the internal water ocean and overlying ice shell of Jupiter's largest moon Ganymede. As part of the strategy developed to realise this objective, the tidal response of Ganymede's interior will be constrained by JUICE's measurements of surface displacements (by the Ganymede Laser Altimeter (GALA) instrument) and variations in the gravitational potential (by the 3GM radio science package) d

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28

Kagan, Boris A. "Earth—Moon tidal evolution: model results and observational evidence." Progress in Oceanography 40, no. 1-4 (1997): 109–24. http://dx.doi.org/10.1016/s0079-6611(97)00027-x.

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29

Schenk, Paul, Chloe Beddingfield, Tanguy Bertrand, et al. "Triton: Topography and Geology of a Probable Ocean World with Comparison to Pluto and Charon." Remote Sensing 13, no. 17 (2021): 3476. http://dx.doi.org/10.3390/rs13173476.

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The topography of Neptune’s large icy moon Triton could reveal important clues to its internal evolution, but has been difficult to determine. New global digital color maps for Triton have been produced as well as topographic data for <40% of the surface using stereogrammetry and photoclinometry. Triton is most likely a captured Kuiper Belt dwarf planet, similar though slightly larger in size and density to Pluto, and a likely ocean moon that exhibited plume activity during Voyager 2′s visit in 1989. No surface features or regional deviations of greater than ±1 km amplitude are found. Volat

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30

Bland, M. T., L. A. Weller, D. P. Mayer, and B. A. Archinal. "A GLOBAL SHAPE MODEL FOR SATURN’S MOON ENCELADUS FROM A DENSE PHOTOGRAMMETRIC CONTROL NETWORK." ISPRS Annals of Photogrammetry, Remote Sensing and Spatial Information Sciences V-3-2020 (August 3, 2020): 579–86. http://dx.doi.org/10.5194/isprs-annals-v-3-2020-579-2020.

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Abstract. A planetary body’s global shape provides both insight into its geologic evolution, and a key element of any Planetary Spatial Data Infrastructure (PSDI). NASA’s Cassini mission to Saturn acquired more than 600 moderate- to high-resolution images (<500 m/pixel) of the small, geologically active moon Enceladus. The moon’s internal global ocean and intriguing geology mark it as a candidate for future exploration and motivates the development of a PSDI. Recently, two PSDI foundational data sets were created: geodetic control and orthoimages. To provide the third foundational data set,

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31

Wormnes, Kjetil, William Carey, Thomas Krueger, et al. "ANALOG-1 ISS – The first part of an analogue mission to guide ESA’s robotic moon exploration efforts." Open Astronomy 31, no. 1 (2022): 5–14. http://dx.doi.org/10.1515/astro-2022-0002.

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Abstract The European Space Agency’s ANALOG-1 experiment is the culmination of 12 distinct METERON experiments carried out since 2011. These all address aspects of teleoperating a robotic asset from an orbital platform, i.e., technical implementation, user interfaces, autonomy and operations. The ANALOG-1 technology demonstration and operations concept experiment is based upon the surface mission scenario segment of the notional EL3 sample return mission. This segment focuses on the control of a lunar surface robotic asset from the Earth and from the Lunar Gateway. The experiment is taking pla

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32

Pettinelli, Elena, Barbara Cosciotti, Sebastian Emanuel Lauro, and Elisabetta Mattei. "An overview of GPR subsurface exploration of planets and moons." Leading Edge 41, no. 10 (2022): 672–80. http://dx.doi.org/10.1190/tle41100672.1.

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Geophysical techniques were first tested beyond Earth during the Apollo program. Of those examined, radio-wave propagation methods appeared to be the most suitable for the moon and other solar system bodies. This was due to the electromagnetic characteristics of planetary subsurfaces and the possibility to remotely perform measurements on board spacecrafts and rovers. After the first successful experiment on the moon, more than 20 years passed before ground-penetrating radar (GPR) was included in the payload of a planetary mission. Technological advancements in GPR design and successful result

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33

Ashley, J. W., M. S. Robinson, B. R. Hawke, et al. "Geology of the King crater region: New insights into impact melt dynamics on the Moon." Journal of Geophysical Research: Planets 117, E12 (2012): n/a. http://dx.doi.org/10.1029/2011je003990.

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34

Gillis, Jeffrey J., and Paul D. Spudis. "Geology of the Smythii and Marginis region of the Moon: Using integrated remotely sensed data." Journal of Geophysical Research: Planets 105, E2 (2000): 4217–33. http://dx.doi.org/10.1029/1999je001111.

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35

Messeri, Lisa. "Earth as Analog: The Disciplinary Debate and Astronaut Training that Took Geology to the Moon." Astropolitics 12, no. 2-3 (2014): 196–209. http://dx.doi.org/10.1080/14777622.2014.964131.

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36

Clark, P. E., and B. R. Hawke. "The relationship between geology and geochemistry in the Undarum/Spumans/Balmer region of the Moon." Earth, Moon and Planets 38, no. 2 (1987): 97–112. http://dx.doi.org/10.1007/bf00119678.

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37

Przylibski, Tadeusz A., Mateusz Szczęśniewicz, and Konrad Blutstein. "Czy na Dolnym Śląsku występują naturalne analogi skał księżycowych?" Przegląd Geologiczny 72, no. 1 (2024): 26–46. http://dx.doi.org/10.7306/2024.2.

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38

Lu, Yunfan, Yifan Hu, Jun Xiao, Lupeng Liu, Long Zhang, and Ying Wang. "Three-Dimensional Model of the Moon with Semantic Information of Craters Based on Chang’e Data." Sensors 21, no. 3 (2021): 959. http://dx.doi.org/10.3390/s21030959.

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China’s Chang’e lunar exploration project obtains digital orthophoto image (DOM) and digital elevation model (DEM) data covering the whole Moon, which are critical to lunar research. The DOM data have three resolutions (i.e., 7, 20 and 50 m), while the DEM has two resolutions (i.e., 20 and 50 m). Analysis and research on these image data effectively help humans to understand the Moon. In addition, impact craters are considered the most basic feature of the Moon’s surface. Statistics regarding the size and distribution of impact craters are essential for lunar geology. In existing works, howeve

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39

Doyle, Peter. "The Apollo missions and Moon rocks, 1969-1972." Geology Today 33, no. 4 (2017): 142–47. http://dx.doi.org/10.1111/gto.12192.

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40

Antonov, Yury V., and Irina Yu Antonova. "ON THE POSSIBLE INFLUENCE OF THE MOON AND THE SUN ON SEISMIC AND GRAVIMETRIC MEASUREMENTS." Вестник ВГУ Серия Геология, no. 1 (2023): 89–96. http://dx.doi.org/10.17308/geology/1609-0691/2023/1/89-96.

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41

Holmström, M., S. Fatemi, Y. Futaana, and H. Nilsson. "The interaction between the Moon and the solar wind." Earth, Planets and Space 64, no. 2 (2012): 237–45. http://dx.doi.org/10.5047/eps.2011.06.040.

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42

HUSSAIN, Ahlam A., Ebtesam F. KANGER, and Ban S. ISMAEEL. "USING A NEW HYBRID SEGMENTATION TECHNIQUE TO SEGMENT LUNAR CRATERS AND DETERMINE ITS DIAMETER." MINAR International Journal of Applied Sciences and Technology 03, no. 02 (2021): 144–51. http://dx.doi.org/10.47832/2717-8234.2-3.18.

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Segmentation method is the process of partition digital image into parts depending to color, texture, and intensity. There are many segmentation methods used in different fields according to the purpose of application. In this study the global thresholding and proposed hybrid method were used to segment lunar craters. Craters on Moon's surface caused by collision between Moon and celestial objects as comet, meteorite, asteroids and others. Due to the Moon has no atmosphere, the lunar surface covered by a huge number of craters different in their size and depth depending on velocity and size of

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43

Singh, Tanu, and Neeraj Srivastava. "Geology of Grimaldi Basin on the Moon: Evidence for volcanism and tectonism during the Copernican period." Icarus 351 (November 2020): 113921. http://dx.doi.org/10.1016/j.icarus.2020.113921.

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44

Fields, Brian D., and Anton Wallner. "Deep-Sea and Lunar Radioisotopes from Nearby Astrophysical Explosions." Annual Review of Nuclear and Particle Science 73, no. 1 (2023): 365–95. http://dx.doi.org/10.1146/annurev-nucl-011823-045541.

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Live (not decayed) radioisotopes on the Earth and Moon are messengers from recent nearby astrophysical explosions. Measurements of 60Fe in deep-sea samples, Antarctic snow, and lunar regolith reveal two pulses about 3 Myr and 7 Myr ago. Detection of 244Pu in a deep-sea crust indicates a recent r-process event. We review the ultrasensitive accelerator mass spectrometry techniques that enable these findings. We then explore the implications for astrophysics, including supernova nucleosynthesis, particularly the r-process, as well as supernova dust production and the formation of the Local Bubble

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45

Cross, Matthew, Melissa Battler, Volker Maiwald, et al. "Operational Lessons Learnt from the 2013 ILEWG EuroMoonMars-B Analogue Campaign for Future Habitat Operations on the Moon and Mars." Acta Futura, no. 10 (December 14, 2016): 61–73. https://doi.org/10.5281/zenodo.202179.

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This paper discusses operational lessons learnt from the 2013 Euro\-Moon\-Mars-B (MDRS crew 125) analogue campaign for future habitat operations on the Moon and Mars. The two-week campaign conducted a series of geologic, technological, operational, and human factors research toward the goals of the International Lunar Exploration Working Group (ILEWG). The results from those operations provide recommendations for future crewed expeditions for increasing the science return based on improved resource allocation and crew habitation.  

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46

Thompson, Thomas W., Bruce A. Campbell, Rebecca R. Ghent, and B. Ray Hawke. "Rugged crater ejecta as a guide to megaregolith thickness in the southern nearside of the Moon." Geology 37, no. 7 (2009): 655–58. http://dx.doi.org/10.1130/g25565a.1.

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47

Hansen, H. J., R, Gwozdz, R, G, Bromley, E. W. Vogensen, and K. L. Rasmussen. "Cretaceous-Tertiary boundary spherules from Denmark, New Zealand and Spain." Bulletin of the Geological Society of Denmark 35 (October 29, 1986): 75–82. http://dx.doi.org/10.37570/bgsd-1986-35-09.

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Spherules from the Cretaceous-Tertiary boundary layers in Denmark, New Zealand and Spain have been studied with respect to their content of organic material. After dissolution in HC! and HF, organic spheres were found, According to their morphology and structure they belong to the green algal group Prasi- nophyta. The mineralogical composition of the spherules is dominated by goethite in the Danish and New Zealand examples while those from Spain show a combination of sanidine and goethite. It is concluded that the spherules are the result of diagenetic infill of prasinophyte algae and are unre

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48

Williams, George E. "Precambrian tidal and glacial clastic deposits: implications for Precambrian Earth–Moon dynamics and palaeoclimate." Sedimentary Geology 120, no. 1-4 (1998): 55–74. http://dx.doi.org/10.1016/s0037-0738(98)00027-x.

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49

Banks, Michael. "China releases most detailed geological map of the Moon to date." Physics World 35, no. 7 (2022): 12ii. http://dx.doi.org/10.1088/2058-7058/35/07/14.

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50

Granier, Bruno, and Philippe Lapointe. "The Kalkowsky Project - Chapter II. Wobbly ooids in a stromatolite from the Yacoraite Formation (Argentina)." Carnets de géologie (Notebooks on geology) 22, no. 3 (2021): 111–17. http://dx.doi.org/10.2110/carnets.2022.2203.

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Eccentric ooids are described from a brackish Maastrichtian paleolake in NW Argentina. The first report of such atypical coated grains was from marine Upper Jurassic strata in SE Poland. Because their growth pattern is not likely to be confused with that of other "eccentric" ooids, such as asymmetric ooids, hiatus ooids, half-moon ooids, or "broken" ooids, it is suggested here to name them "wobbly ooids".

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