Relevant bibliographies by topics / Lunar megaregolith

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  1. Journal articles
  2. Dissertations / Theses

Academic literature on the topic 'Lunar megaregolith'

Author: Grafiati
Published: 4 June 2021
Last updated: 2 February 2022

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Journal articles on the topic "Lunar megaregolith"

1

Richardson, James E., and Oleg Abramov. "Modeling the Formation of the Lunar Upper Megaregolith Layer." Planetary Science Journal 1, no. 1 (2020): 2. http://dx.doi.org/10.3847/psj/ab7235.

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2

Cashore, Jac, and Alex Woronow. "A new Monte Carlo model of lunar megaregolith development." Journal of Geophysical Research 90, S02 (1985): C811. http://dx.doi.org/10.1029/jb090is02p0c811.

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Wiggins, Sean E., Brandon C. Johnson, Tim J. Bowling, H. Jay Melosh, and Elizabeth A. Silber. "Impact Fragmentation and the Development of the Deep Lunar Megaregolith." Journal of Geophysical Research: Planets 124, no. 4 (2019): 941–57. http://dx.doi.org/10.1029/2018je005757.

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4

Hartmann. "History of the Terminal Cataclysm Paradigm: Epistemology of a Planetary Bombardment That Never (?) Happened." Geosciences 9, no. 7 (2019): 285. http://dx.doi.org/10.3390/geosciences9070285.

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This study examines the history of the paradigm concerning a lunar (or solar-systemwide)terminal cataclysm (also called “Late Heavy Bombardment” or LHB), a putative, brief spikein impacts at ~3.9 Ga ago, preceded by low impact rates. We examine origin of the ideas, why theywere accepted, and why the ideas are currently being seriously revised, if not abandoned. Thepaper is divided into the following sections:1. Overview of paradigm.2. Pre-Apollo views (1949-1969).3. Initial suggestions of cataclysm (ca. 1974).4. Ironies.5. Alternative suggestions, megaregolith evolution (1970s).6. Impact melt
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PETRO, Noah E., and Carlé M. PIETERS. "The lunar-wide effects of basin ejecta distribution on the early megaregolith." Meteoritics & Planetary Science 43, no. 9 (2008): 1517–29. http://dx.doi.org/10.1111/j.1945-5100.2008.tb01025.x.

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6

Jackson, N. W., and B. D. Carter. "Global mapping of iron and titanium oxides in the lunar megaregolith and subsurface." Australian Journal of Earth Sciences 54, no. 6 (2007): 851–59. http://dx.doi.org/10.1080/08120090701392713.

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Hartmann, William K. "Megaregolith evolution and cratering cataclysm models-Lunar cataclysm as a misconception (28 years later)." Meteoritics & Planetary Science 38, no. 4 (2003): 579–93. http://dx.doi.org/10.1111/j.1945-5100.2003.tb00028.x.

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Hartmann, William K., and Alessandro Morbidelli. "Effects of early intense bombardment on megaregolith evolution and on lunar (and planetary) surface samples." Meteoritics & Planetary Science 55, no. 11 (2020): 2472–92. http://dx.doi.org/10.1111/maps.13595.

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Liu, Tiantian, Greg Michael, Kai Wünnemann, Harry Becker, and Jürgen Oberst. "Lunar megaregolith mixing by impacts: Spatial diffusion of basin melt and its implications for sample interpretation." Icarus 339 (March 2020): 113609. http://dx.doi.org/10.1016/j.icarus.2019.113609.

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10

Zhang, Nan, E. M. Parmentier, and Yan Liang. "Effects of lunar cumulate mantle overturn and megaregolith on the expansion and contraction history of the Moon." Geophysical Research Letters 40, no. 19 (2013): 5019–23. http://dx.doi.org/10.1002/grl.50988.

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Dissertations / Theses on the topic "Lunar megaregolith"

1

Jackson, Noel William. "A compositional study of the lunar global megaregolith using Clementine orbiter data a dissertation /." University of Southern Queensland, Faculty of Sciences, 2005. http://eprints.usq.edu.au/archive/00001452/.

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This thesis presents new information about the global megaregolith of the Moon, using 2059 craters (5 to 50 km diameter) as natural probes. Iron (FeO) and titanium (TiO2) concentrations were obtained from crater ejecta blanket data over an area between 600 North to 600 South latitude derived from the 1994 Clementine mission. The average iron and titanium weight percentages for lunar crater ejecta were calculated using the US Geological Survey's ISIS software, and used to determine the variation with depth of iron (FeO) and titanium (TiO2) in the highlands, mare areas and the South Pole Aitken
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