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- Q180874 subject Q6933080.
- Q180874 subject Q7485015.
- Q180874 abstract "The lunar maria /ˈmɑːriə/ (singular: mare /ˈmɑːreɪ/) are large, dark, basaltic plains on Earth's Moon, formed by ancient volcanic eruptions. They were dubbed maria, Latin for "seas", by early astronomers who mistook them for actual seas. They are less reflective than the "highlands" as a result of their iron-rich compositions, and hence appear dark to the naked eye. The maria cover about 16 percent of the lunar surface, mostly on the side visible from Earth. The few maria on the far side are much smaller, residing mostly in very large craters. The traditional nomenclature for the Moon also includes one oceanus (ocean), as well as features with the names lacus (lake), palus (marsh), and sinus (bay). The last three are smaller than maria, but have the same nature and characteristics.The names of maria generally call up psychic states of mind, with a few exceptions. For example, Mare Humboldtianum and Mare Smythii were established long before the nomenclature was accepted and do not follow this pattern. When Mare Moscoviense was discovered by the Luna 3, and the name was proposed by the Soviet Union, it was only accepted by the International Astronomical Union with the justification that Moscow is the state of mind.".
- Q180874 thumbnail Moon_names.svg?width=300.
- Q180874 wikiPageExternalLink id26.htm.
- Q180874 wikiPageExternalLink expmoon.
- Q180874 wikiPageExternalLink basaltFragments.html.
- Q180874 wikiPageExternalLink Archive-Moon.html.
- Q180874 wikiPageExternalLink highTi.html.
- Q180874 wikiPageExternalLink MoonVolcanics.html.
- Q180874 wikiPageExternalLink lunarMaria.html.
- Q180874 wikiPageExternalLink moon.
- Q180874 wikiPageExternalLink lunar_atlases.
- Q180874 wikiPageWikiLink Q109144.
- Q180874 wikiPageWikiLink Q116681.
- Q180874 wikiPageWikiLink Q1409625.
- Q180874 wikiPageWikiLink Q142616.
- Q180874 wikiPageWikiLink Q1648514.
- Q180874 wikiPageWikiLink Q165.
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- Q180874 wikiPageWikiLink Q168032.
- Q180874 wikiPageWikiLink Q168398.
- Q180874 wikiPageWikiLink Q17159.
- Q180874 wikiPageWikiLink Q178733.
- Q180874 wikiPageWikiLink Q178977.
- Q180874 wikiPageWikiLink Q190444.
- Q180874 wikiPageWikiLink Q2.
- Q180874 wikiPageWikiLink Q2106459.
- Q180874 wikiPageWikiLink Q214753.
- Q180874 wikiPageWikiLink Q2366717.
- Q180874 wikiPageWikiLink Q318438.
- Q180874 wikiPageWikiLink Q3208478.
- Q180874 wikiPageWikiLink Q320936.
- Q180874 wikiPageWikiLink Q326868.
- Q180874 wikiPageWikiLink Q397.
- Q180874 wikiPageWikiLink Q405.
- Q180874 wikiPageWikiLink Q43338.
- Q180874 wikiPageWikiLink Q43653.
- Q180874 wikiPageWikiLink Q487895.
- Q180874 wikiPageWikiLink Q488299.
- Q180874 wikiPageWikiLink Q49055.
- Q180874 wikiPageWikiLink Q567788.
- Q180874 wikiPageWikiLink Q590245.
- Q180874 wikiPageWikiLink Q674.
- Q180874 wikiPageWikiLink Q6867.
- Q180874 wikiPageWikiLink Q6933080.
- Q180874 wikiPageWikiLink Q693461.
- Q180874 wikiPageWikiLink Q703.
- Q180874 wikiPageWikiLink Q7485015.
- Q180874 wikiPageWikiLink Q782867.
- Q180874 wikiPageWikiLink Q8072.
- Q180874 wikiPageWikiLink Q816838.
- Q180874 wikiPageWikiLink Q877100.
- Q180874 wikiPageWikiLink Q930183.
- Q180874 wikiPageWikiLink Q936117.
- Q180874 wikiPageWikiLink Q942814.
- Q180874 type Thing.
- Q180874 comment "The lunar maria /ˈmɑːriə/ (singular: mare /ˈmɑːreɪ/) are large, dark, basaltic plains on Earth's Moon, formed by ancient volcanic eruptions. They were dubbed maria, Latin for "seas", by early astronomers who mistook them for actual seas. They are less reflective than the "highlands" as a result of their iron-rich compositions, and hence appear dark to the naked eye. The maria cover about 16 percent of the lunar surface, mostly on the side visible from Earth.".
- Q180874 label "Lunar mare".
- Q180874 depiction Moon_names.svg.