The maria likely formed several billion years ago when the Solar System was still in its turbulent formative years. Large meteors impacted the surface of the Moon, potentially causing it to crack open in isolated areas. This allowed hot magma to bubble up from below filling these impact zones with volcanic basalt that tends to be much darker. For a video of the Moon's evolution please see the link below.
Evolution of the Moon
The image below shows a picture I took of the moon on May 10, 2017. The prominent maria required for the Explore the Universe certification are labelled below. Two of the impact basins highlighted are not called maria. Oceanus Procellarum is so large it is referred to as an ocean. It also may be the largest impact crater in the Solar System. Sinus Iridum -- The Bay of Rainbows, is an offshoot of the larger Mare Imbrium.
Lunar Basins/Maria Observation Record |
Basin | Translation |
---|---|
Mare Crisium | Sea of Crises |
Mare Fecunditatis | Sea of Fertility |
Mare Tranquilitatis | Sea of Tranquility |
Mare Nectatis | Sea of Nectar |
Mare Frigoris | Sea of Cold |
Mare Serenitatis | Sea of Serenity |
Mare Imbrium | Sea of Showers |
Sinus Iridum | Bay of Rainbows |
Mare Vaporum | Sea of Vapors |
Oceanus Procellarum | Ocean of Storms |
Mare Nubium | Sea of Clouds |
Mare Humorum | Sea of Moisture |
At some point I will discuss each individual basin in separate blog posts. There is a more formal observing program specifically for the Moon that I intend to work on after the Explore the Universe certification.
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