Media Information

 
 
 
Collection:
NASA Solarsystem Collection
title:
Lunar Maria
description:
The smooth dark areas on the Moon's surface are called maria (plural for mare; Latin for seas). These volcanic plains are made up of a rock type known as basalt, similar in composition to the rocks found in Hawaii. They cover 17% of the surface area of the Moon. The maria contain physical features such as pits and channels, but lack large volcanos.

Features visible in this image of the western part of the lunar nearside include Mare Imbrium, Mare Humorum, Mare Nubium, and the craters Copernicus and Kepler. Copernicus is the most prominent crater with its bright rays composed of ejecta material.

This image was taken by one of NASA's Lunar Orbiters in 1967.

*Image Credit*: NASA
keywords:
Solar System Exploration
keywords:
SSE
keywords:
Space
keywords:
NASA
keywords:
National Aeronautics and Space Administration
keywords:
JPL
keywords:
Jet Propulsion Laboratory
keywords:
Planets
facet_what:
Crater
facet_what:
Moon
facet_where:
Jet Propulsion Laboratory
facet_where:
Hawaii
facet_where:
Jet Propulsion Laboratory (JPL)
facet_when:
1967
facet_when_year:
1967
UID:
SPD-SLRSY-800
original url:

Lunar Maria