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* The crustal density and porosity were determined.<ref name=":4">{{Cite journal|last1=Wieczorek|first1=M. A.|last2=Neumann|first2=G. A.|last3=Nimmo|first3=F.|last4=Kiefer|first4=W. S.|last5=Taylor|first5=G. J.|last6=Melosh|first6=H. J.|last7=Phillips|first7=R. J.|last8=Solomon|first8=S. C.|last9=Andrews-Hanna|first9=J. C.|last10=Asmar|first10=S. W.|last11=Konopliv|first11=A. S.|display-authors=9|date=2013|title=The Crust of the Moon as Seen by GRAIL|journal=Science|language=en|volume=339|issue=6120|pages=671–675|doi=10.1126/science.1231530|issn=0036-8075|pmc=6693503|pmid=23223394|bibcode=2013Sci...339..671W}}</ref> The crust was fragmented by large ancient impacts. |
* The crustal density and porosity were determined.<ref name=":4">{{Cite journal|last1=Wieczorek|first1=M. A.|last2=Neumann|first2=G. A.|last3=Nimmo|first3=F.|last4=Kiefer|first4=W. S.|last5=Taylor|first5=G. J.|last6=Melosh|first6=H. J.|last7=Phillips|first7=R. J.|last8=Solomon|first8=S. C.|last9=Andrews-Hanna|first9=J. C.|last10=Asmar|first10=S. W.|last11=Konopliv|first11=A. S.|display-authors=9|date=2013|title=The Crust of the Moon as Seen by GRAIL|journal=Science|language=en|volume=339|issue=6120|pages=671–675|doi=10.1126/science.1231530|issn=0036-8075|pmc=6693503|pmid=23223394|bibcode=2013Sci...339..671W}}</ref> The crust was fragmented by large ancient impacts. |
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* Long narrow linear features were found that are interpreted to be ancient tabular intrusions or dikes formed by magma.<ref>{{Cite journal|last1=Andrews-Hanna|first1=J. C.|last2=Asmar|first2=S. W.|last3=Head|first3=J. W.|last4=Kiefer|first4=W. S.|last5=Konopliv|first5=A. S.|last6=Lemoine|first6=F. G.|last7=Matsuyama|first7=I.|last8=Mazarico|first8=E.|last9=McGovern|first9=P. J.|last10=Melosh|first10=H. J.|last11=Neumann|first11=G. A.|display-authors=9|date=2013|title=Ancient Igneous Intrusions and Early Expansion of the Moon Revealed by GRAIL Gravity Gradiometry|url=https://www.science.org/doi/10.1126/science.1231753|journal=Science|language=en|volume=339|issue=6120|pages=675–678|doi=10.1126/science.1231753|pmid=23223393|bibcode=2013Sci...339..675A|s2cid=18004181|issn=0036-8075}}</ref> |
* Long narrow linear features were found that are interpreted to be ancient tabular intrusions or dikes formed by magma.<ref>{{Cite journal|last1=Andrews-Hanna|first1=J. C.|last2=Asmar|first2=S. W.|last3=Head|first3=J. W.|last4=Kiefer|first4=W. S.|last5=Konopliv|first5=A. S.|last6=Lemoine|first6=F. G.|last7=Matsuyama|first7=I.|last8=Mazarico|first8=E.|last9=McGovern|first9=P. J.|last10=Melosh|first10=H. J.|last11=Neumann|first11=G. A.|display-authors=9|date=2013|title=Ancient Igneous Intrusions and Early Expansion of the Moon Revealed by GRAIL Gravity Gradiometry|url=https://www.science.org/doi/10.1126/science.1231753|journal=Science|language=en|volume=339|issue=6120|pages=675–678|doi=10.1126/science.1231753|pmid=23223393|bibcode=2013Sci...339..675A|s2cid=18004181|issn=0036-8075}}</ref> |
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*Combining gravity and [[Lunar Laser Ranging experiment|Lunar Laser Ranging]] data gives the 3 principal moments of inertia.<ref>{{Cite journal|last1=Williams|first1=James G.|last2=Konopliv|first2=Alexander S.|last3=Boggs|first3=Dale H.|last4=Park|first4=Ryan S.|last5=Yuan|first5=Dah-Ning|last6=Lemoine|first6=Frank G.|last7=Goossens|first7=Sander|last8=Mazarico|first8=Erwan|last9=Nimmo|first9=Francis|last10=Weber|first10=Renee C.|last11=Asmar|first11=Sami W.|display-authors=9|date=2014|title=Lunar interior properties from the GRAIL mission|journal=Journal of Geophysical Research: Planets|language=en|volume=119|issue=7|pages=1546–1578|doi=10.1002/2013JE004559|bibcode=2014JGRE..119.1546W|s2cid=7045590 |doi-access=free}}</ref> The moments indicate that a dense core is small. |
*Combining gravity and [[Lunar Laser Ranging experiment|Lunar Laser Ranging]] data gives the 3 principal moments of inertia.<ref>{{Cite journal|last1=Williams|first1=James G.|last2=Konopliv|first2=Alexander S.|last3=Boggs|first3=Dale H.|last4=Park|first4=Ryan S.|last5=Yuan|first5=Dah-Ning|last6=Lemoine|first6=Frank G.|last7=Goossens|first7=Sander|last8=Mazarico|first8=Erwan|last9=Nimmo|first9=Francis|last10=Weber|first10=Renee C.|last11=Asmar|first11=Sami W.|display-authors=9|date=2014|title=Lunar interior properties from the GRAIL mission|url=http://doi.wiley.com/10.1002/2013JE004559|journal=Journal of Geophysical Research: Planets|language=en|volume=119|issue=7|pages=1546–1578|doi=10.1002/2013JE004559|bibcode=2014JGRE..119.1546W|s2cid=7045590 |doi-access=free}}</ref> The moments indicate that a dense core is small. |
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*Combining gravity and lunar [[Topography of the Moon|Topography]], 74 circular impact basins were identified.<ref>{{Cite journal|last1=Neumann|first1=Gregory A.|last2=Zuber|first2=Maria T.|last3=Wieczorek|first3=Mark A.|last4=Head|first4=James W.|last5=Baker|first5=David M. H.|last6=Solomon|first6=Sean C.|last7=Smith|first7=David E.|last8=Lemoine|first8=Frank G.|last9=Mazarico|first9=Erwan|last10=Sabaka|first10=Terence J.|last11=Goossens|first11=Sander J.|display-authors=9|date=2015|title=Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements|journal=Science Advances|language=en|volume=1|issue=9|pages=e1500852|doi=10.1126/sciadv.1500852|issn=2375-2548|pmc=4646831|pmid=26601317|bibcode=2015SciA....1E0852N}}</ref> Strong increases in gravity that are associated with circular impact basins are [[Mass concentration (astronomy)|mascons]] discovered by Muller and Sjogren.<ref>{{Cite journal|last1=Muller|first1=P. M.|last2=Sjogren|first2=W. L.|date=1968|title=Mascons: Lunar Mass Concentrations|url=https://www.science.org/doi/10.1126/science.161.3842.680|journal=Science|language=en|volume=161|issue=3842|pages=680–684|doi=10.1126/science.161.3842.680|pmid=17801458|bibcode=1968Sci...161..680M|s2cid=40110502|issn=0036-8075}}</ref> The strongest gravity anomalies are from basins filled with dense mare material, but the strong gravity also requires that the boundary between the crust and denser mantle be warped upward. Where the crust is thicker, there may be no mare fill but the crust-mantle boundary is still warped upward. |
*Combining gravity and lunar [[Topography of the Moon|Topography]], 74 circular impact basins were identified.<ref>{{Cite journal|last1=Neumann|first1=Gregory A.|last2=Zuber|first2=Maria T.|last3=Wieczorek|first3=Mark A.|last4=Head|first4=James W.|last5=Baker|first5=David M. H.|last6=Solomon|first6=Sean C.|last7=Smith|first7=David E.|last8=Lemoine|first8=Frank G.|last9=Mazarico|first9=Erwan|last10=Sabaka|first10=Terence J.|last11=Goossens|first11=Sander J.|display-authors=9|date=2015|title=Lunar impact basins revealed by Gravity Recovery and Interior Laboratory measurements|journal=Science Advances|language=en|volume=1|issue=9|pages=e1500852|doi=10.1126/sciadv.1500852|issn=2375-2548|pmc=4646831|pmid=26601317|bibcode=2015SciA....1E0852N}}</ref> Strong increases in gravity that are associated with circular impact basins are [[Mass concentration (astronomy)|mascons]] discovered by Muller and Sjogren.<ref>{{Cite journal|last1=Muller|first1=P. M.|last2=Sjogren|first2=W. L.|date=1968|title=Mascons: Lunar Mass Concentrations|url=https://www.science.org/doi/10.1126/science.161.3842.680|journal=Science|language=en|volume=161|issue=3842|pages=680–684|doi=10.1126/science.161.3842.680|pmid=17801458|bibcode=1968Sci...161..680M|s2cid=40110502|issn=0036-8075}}</ref> The strongest gravity anomalies are from basins filled with dense mare material, but the strong gravity also requires that the boundary between the crust and denser mantle be warped upward. Where the crust is thicker, there may be no mare fill but the crust-mantle boundary is still warped upward. |
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*The radius, density, and rigidity of interior layers is inferred.<ref>{{Cite journal|last1=Matsuyama|first1=Isamu|last2=Nimmo|first2=Francis|last3=Keane|first3=James T.|last4=Chan|first4=Ngai H.|last5=Taylor|first5=G. Jeffrey|last6=Wieczorek|first6=Mark A.|last7=Kiefer|first7=Walter S.|last8=Williams|first8=James G.|date=2016|title=GRAIL, LLR, and LOLA constraints on the interior structure of the Moon|url=http://doi.wiley.com/10.1002/2016GL069952|journal=Geophysical Research Letters|language=en|volume=43|issue=16|pages=8365–8375|doi=10.1002/2016GL069952|bibcode=2016GeoRL..43.8365M|hdl=10150/621595|s2cid=36834256 |hdl-access=free}}</ref> |
*The radius, density, and rigidity of interior layers is inferred.<ref>{{Cite journal|last1=Matsuyama|first1=Isamu|last2=Nimmo|first2=Francis|last3=Keane|first3=James T.|last4=Chan|first4=Ngai H.|last5=Taylor|first5=G. Jeffrey|last6=Wieczorek|first6=Mark A.|last7=Kiefer|first7=Walter S.|last8=Williams|first8=James G.|date=2016|title=GRAIL, LLR, and LOLA constraints on the interior structure of the Moon|url=http://doi.wiley.com/10.1002/2016GL069952|journal=Geophysical Research Letters|language=en|volume=43|issue=16|pages=8365–8375|doi=10.1002/2016GL069952|bibcode=2016GeoRL..43.8365M|hdl=10150/621595|s2cid=36834256 |hdl-access=free}}</ref> |
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