The DOI matches its Crossref record.
Geologic map of the near side of the Moon
Open accessAbstract
RATIONALE, METHODS, AND FORMATthe Moon and produced a workable nearside stratigraphy (Shoemaker and Hackman, 1962; McCauley, 1967b; Wilhelms, 1970b).Prior to the Lunar Orbiters, telescopic resolution limitations dictated emphasis on the grosser aspects of lunar geology: the structures and ejecta blankets associated with the multiringed basins, the major craters, and the stratigraphic relations between the generally younger maria and older terrae.The main products of the telescopic work were 36 1:1 ,000,000-scale geologic quadrangle maps (those marked "T" in table 1) and a 1 :5,000,000-scale preliminary map of the region 32°N.to 32°S.and 70°E.to 70°W.(Wilhelms, Trask, and Keith, 1965).Before the systematic program began, Hackman and Mason (1961) produced a set of three nearside maps at a scale of 1:3,800,000 from telescopic data; these maps emphasized the geology, physiography and ray-crater distribution.The chief purpose of the 1 :5,000,000-scale map is to summarize the current state of lunar geologic knowledge as developed from the U.S. Geological Survey's systematic lunar mapping program, which began in 1960.Like terrestrial synoptic maps it provides a stratigraphic framework to be used for developing new theory and for determining the regional significance of surface exploration results.The geologic summary which accompanies the map gives the major genetic and historical conclusions which stem from the work.The map explanation provides the descriptive details that led to these conclusions.This pamphlet discusses the rationale methods, and nomenclature of lunar stratigraphy: specifically for those interested in why and how the map was produced.The work is based both on results of the telescopic mapping program and on data from the unmanned lunar exploration program, particularly the regional coverage of Lunar Orbiter IV 1 The early telescopic studies established the geologic heterogeneity of 1 U.s e f u I .c .oII e c t ions of photographs from a II Orbtter ~tsstons, accompanied by geologically oriented explanatiOns, appear in Lowman ( 1969) and Kosofsky and El-Baz (1970).
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cited by
Major lunar crustal terranes: Surface expressions and crust‐mantle origins
Jolliff, B. L., Gillis, J. J., Haskin, L. A., Korotev, R. L., & Wieczorek, M. A. (2000) · Journal of Geophysical Research: Planets · doi:10.1029/1999je001103 · Cited by 939
Geology and distribution of impact craters on Venus: What are they telling us?
Schaber, G. G., Strom, R. G., Moore, H. J., Soderblom, L. A., Kirk, R. L., Chadwick, D. J., Dawson, D. D., Gaddis, L. R., Boyce, J. M., & Russell, J. (1992) · Journal of Geophysical Research: Planets · doi:10.1029/92je01246 · Cited by 473
Radial thickness variation in impact crater ejecta: implications for lunar basin deposits
McGetchin, T. R., Settle, M., & Head, J. W. (1973) · Earth and Planetary Science Letters · doi:10.1016/0012-821x(73)90162-3 · Cited by 425
Evidence for negative charging of the lunar surface in shadow
Halekas, J. S., Mitchell, D. L., Lin, R. P., Hood, L. L., Acuña, M. H., & Binder, A. B. (2002) · Geophysical Research Letters · doi:10.1029/2001gl014428 · Cited by 125
Metadata
- Publisher
- US Geological Survey
- Published
- 1971
- DOI
- 10.3133/i703
- OpenAlex
- W1581373985
- Cited by
- 247
- References
- 0
- Type
- report
- Language
- en
- Open access
- gold
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: Geologic map of the near side of the Moon. https://app.cochat.ai/papers/10.3133/i703
- The paper
- Geologic map of the near side of the Moon. (1971). https://doi.org/10.3133/i703
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.