{"id":62429,"date":"2024-08-05T08:40:43","date_gmt":"2024-08-05T08:40:43","guid":{"rendered":"http:\/\/0eea5e3b-fae1-4190-afae-922dee165dd6"},"modified":"2024-08-05T09:39:50","modified_gmt":"2024-08-05T09:39:50","slug":"lunar-maria-a-complete-guide-to-the-seas-of-the-moon","status":"publish","type":"rss_feed","link":"https:\/\/c01.purpledshub.com\/bbcskyatnight\/rss_feed\/lunar-maria-a-complete-guide-to-the-seas-of-the-moon\/","title":{"rendered":"Lunar maria: a complete guide to the seas of the Moon"},"content":{"rendered":"

All you need to know about the lunar maria, the seas of the Moon, including coordinates and facts about each mare. <\/p>

By Ezzy Pearson\n <\/p>

Published: Monday, 05 August 2024 at 08:40 AM<\/p>

\n\n

Lunar maria are the dark topographical features that can be observed on the lunar surface, covering about 15% of the Moon’s crust, and which have dazzled astronomers and moon-gazers for centuries.<\/p>

The maria, or \u2018seas\u2019, were named by early astronomers who mistook them for actual oceans on the Moon, but of course today we know that no such large bodies of liquid water exist on the lunar surface.<\/p>

The lunar maria are impact basins created by collisions with cosmic debris that filled with lava and other lunar material between 1-4 billion years ago.<\/p>

A mosaic image of the Moon captured by the Galileo spacecraft, showing colour on the lunar surface. On the upper left is Mare Imbrium; middle left is Mare Serenitatis; lower left is Mare Tranquillitatis, and the dark patch towards the bottom is Mare Crisium. Credit: Stocktrek Images<\/figcaption><\/figure>
Formation of the Moon<\/strong><\/h2>
By studying topographical features of the lunar landscape such as the highlands, maria and craters, astronomers have been able to piece together a history of the Moon as it formed and evolved over billions of years.<\/p>
One theory of how the Moon formed<\/a> says a large body collided with Earth about 4.5 billion years ago, and the debris from the wreckage coalesced over time to form a satellite in orbit around our planet.<\/p>
This early Moon was likely covered in molten magma, which then cooled to create the rugged, cold and lifeless rock that we know today.<\/p>
Over time, the lunar maria have been studied in great detail, both using ground-based telescopes, robotic probes and, of course, by human explorers during the Apollo missions.<\/p>
$\"Buzz$
Buzz Aldrin pictured in the Sea of Tranquility during Apollo 11. Credit: NASA \/ Neil A. Armstrong.<\/figcaption><\/figure>
Observing the lunar maria<\/strong><\/h2>
On a clear night, when the Moon is prominent in the night sky, it is one of the best objects to observe, and the lunar maria are among the easiest sights to see.<\/p>
While much can be seen on the Moon with the naked eye, a pair of modest binoculars will let you spot maria and craters on the lunar surface.<\/p>
For more on this, read our tutorial on how to observe the Moon<\/a>, or our beginners’ guide to stargazing with binoculars<\/a>.<\/p>
You might think that the ideal time to observe the lunar surface is during a full Moon or even a full supermoon<\/a>.<\/p>
Instead, find out when the Moon will next be visible in the night sky during its crescent or gibbous phase.<\/p>
This will enable you to spot the ‘terminator<\/a>‘, which is the line dividing the bright and dark portions of the Moon from our perspective.<\/p>
Learn more about this with our guide to the phases of the Moon<\/a>.<\/p>
$\"The$
The ‘terminator’ on the Moon is the line dividing the lit and unlit sections. Credit: William Ian Hamilton<\/figcaption><\/figure>
Looking along the terminator will enable you to use shadows to make out the Moon’s rugged surface much easier than when the Moon is full.<\/p>
And, because the Moon is tidally locked with Earth, meaning we always see the same side of the Moon<\/a>, you can track how the terminator changes night after night.<\/p>
We may not be able to see the far side of the Moon<\/a> directly from Earth, but you can catch a glimpse of what’s beyond the limb by studying and even photographing lunar libration<\/a>.<\/p>
In fact, one of the lunar seas, Mare Orientale<\/a>, can only be seen during a favourable libration.<\/p>
$\"mare$
Favourable lunar libration is required to see the Moon’s Mare Orientale region. Credit: Pete Lawrence<\/figcaption><\/figure>
**Observing the Moon online<\/strong><\/h2>**You can also explore the lunar surface online, either by using Google Moon<\/a>, by visiting the Lunar Reconnaissance Orbiter website<\/a> or by downloading the excellent JMars software<\/a> (used by actual NASA planetary scientists!)<\/p>
Below is our complete guide to the lunar seas, how big they are, where they\u2019re located, and facts about their interesting features.<\/p>
If you’re interested in trying to image them, read our guide on how to photograph the Moon<\/a>.<\/p>
**Lunar maria or seas<\/strong><\/h2>**
**Mare Anguis<\/strong><\/h3>**
$\"Mare$
Mare Anguis Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Serpent Sea<\/p>**
**Lat.<\/strong> 22.6 N<\/p>**
**Long.<\/strong> 67.7 E<\/p>**
**Diameter<\/strong> 150km<\/p>**
Located close to the edge of the lunar limb is Mare Anguis, which roughly shaped like an X. It lies near the rim of the much larger Mare Crisium, elevated 800m above. To its east is the 7km wide Eimmart A crater.<\/p>
**Mare Australe<\/strong><\/h3>**
$\"Mare$
Mare Australe Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Southern Sea<\/p>**
**Lat.<\/strong> 38.9 S<\/p>**
**Long.<\/strong> 93.0 E<\/p>**
**Diameter<\/strong> 603km<\/p>**
**Located on the very edge of the Moon, Mare Australe is only visible when** **libration<\/a> tips the Moon forward enough to see it. Unlike most of the other smooth maria, Australe is pockmarked by impact craters which then flooded with basaltic lava.<\/p>**
**Mare Cognitum<\/strong><\/h3>**
$\"Mare$
Mare Cognitum Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Known Sea<\/p>**
**Lat.<\/strong> 10.0 S<\/p>**
**Long.<\/strong> 23.1 W<\/p>**
**Diameter<\/strong> 376km<\/p>**
**In 1964, after years of trying, NASA finally succeeded in \u2018landing\u2019 on the Moon with their Ranger 7 impact probe. The Surveyor 3 soft lander would follow in 1967, paving the way for the** **Apollo 12<\/a> crew to arrive in 1969. Prior to the Ranger 7 landing, the region was unnamed, but was renamed to reflect its role in America\u2019s lunar plans.<\/p>**
**Mare Crisium<\/strong><\/h3>**
$\"Mare$
Mare Crisium, captured by the Lunar Reconnaissance Orbiter. Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Crises<\/p>**
**Lat.<\/strong> 17.0\u00b0 N<\/p>**
**Long.<\/strong> 59.1\u00b0 E<\/p>**
**Diameter<\/strong> 418km<\/p>**
**Unlike most of the other lunar seas,** Mare Crisium<\/a> is an isolated oval that doesn\u2019t merge with others. It\u2019s a large impact basin with visible walls in several places found to the northeast of Mare Tranquillitatis. With an area of 180,000km2, it’s around the same size as England.<\/p>
**Mare Fecunditatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Fecundity<\/p>**
**Lat.<\/strong> 7.8 S<\/p>**
**Long.<\/strong> 51.3 E<\/p>**
**Diameter<\/strong> 909km<\/p>**
**The main basin of** **Mare Fecunditatis<\/a> formed in the pre-Nectarian era \u2013 the earliest time period just after the Moon formed. However, material surrounding it dates from later eras.<\/p>**
The crater overlaps with surrounding Nectaris, Tranquillitatis and Crisium basins. It is unusual in that it has no \u2018mascons\u2019 \u2013 invisible concentrations of mass hidden below the surface of most lunar mare, which are great enough to pull orbiting spacecraft off course.<\/p>
**Mare Frigoris<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Cold<\/p>**
**Lat.<\/strong> 56.0\u00b0 N<\/p>**
**Long.<\/strong> 1.4\u00b0 E<\/p>**
**Diameter<\/strong> 1596km<\/p>**
**The northernmost sea, along the top of the Imbrium and Serenitatis basins,** **Mare Frigoris<\/a> has an intriguing elongated shape, averaging only 250m wide but stretching to over 1,400km in length.<\/p>**
$\"Craters$
Craters Aristoteles and Eudoxus by Avani Soares, Parsec Observatory, Canoas, Brazil. Equipment: C14 Edge, ASI 290, IR pass 685<\/figcaption><\/figure>
Notable features include ejecta from the 40km diameter Harpalus crater that covers a large portion of Frigoris\u2019s floor in the west and, on the south shore, the scars of 88km Aristoteles and 67km Eudoxus, both complex craters with terraced walls.<\/p>
**Mare Humboldtianum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Alexander von Humboldt<\/p>**
**Lat.<\/strong> 56.8 N<\/p>**
**Long.<\/strong> 81.5 E<\/p>**
**Diameter<\/strong> 273km<\/p>**
Located to the east of Frigoris, Mare Humboldtianum is right on the northeastern limb of the Moon. Due to the slight wobble of the Moon from Earth (an effect known as libration), the sea is sometimes hidden from view.<\/p>
The name is a reference to this location, bridging the gap between the known and the unknown, and so it was named after Alexander von Humboldt, a Prussian natural scientist born in 1769 who was famous for travelling the world and exploring places no European had visited before.<\/p>
**Mare Humorum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Moisture<\/p>**
**Lat.<\/strong> 24.4 S<\/p>**
**Long.<\/strong> 38.6 W<\/p>**
**Diameter<\/strong> 389km<\/p>**
**The lava layer of** Mare Humorum<\/a> is thought to exceed 3km in thickness at the basin\u2019s centre. It\u2019s also home to a major mascon, a mass concentration created by a collection of dense material below the surface that is large enough to affect the Moon\u2019s gravitational pull.<\/p>
For these reasons, it\u2019s an area of great scientific interest, allowing planetary scientists to study the relationship between lunar mare filling, basin tectonics and the thermal evolution of a major mascon maria.<\/p>
**Mare Imbrium<\/strong><\/h3>**
$\"Mare$
Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Showers<\/p>**
**Lat.<\/strong> 32.8 N<\/p>**
**Long.<\/strong> 15.6 W<\/p>**
**Diameter<\/strong> 1123km<\/p>**
**As the largest basin on the lunar nearside,** Mare Imbrium<\/a> requires a bit of mobility to explore properly and has been visited by three different rovers: the Soviet Union\u2019s Lunokhod 1 rover in 1970, NASA\u2019s Apollo 15 rover driven by David Scott and James Irwin in 1971, and the Chinese Chang\u2019e 3 lander<\/a> and its rover Yutu in 2013.<\/p>
**The basin is surrounded by a ring of mountains, rising up as much as 7km above the mare floor, and there are signs of ejecta radiating out as far as 800km from the crater.<\/p>**
**Mare Ingenii<\/strong><\/h3>**
$\"Mare$
Mare Ingenii Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Cleverness<\/p>**
**Lat.<\/strong> 33.7 S<\/p>**
**Long.<\/strong> 163.5 E<\/p>**
**Diameter<\/strong> 318km<\/p>**
**Located on the far side of the Moon, Mare Ingenii makes up part of the** **South Pole-Aitken basin<\/a> \u2013 a huge lunar feature that covers most of the southern hemisphere. The region contains the 112km wide Thomson crater.<\/p>**
The floor of Igenii is covered in dramatic swirls of light and dark volcanic material, the pattern of which is believed to reflect the localised magnetic field of the region back when the Moon’s lava was still molten.<\/p>
**Mare Insularum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Islands<\/p>**
**Lat.<\/strong> 7.5 N<\/p>**
**Long.<\/strong> 30.9 W<\/p>**
**Diameter<\/strong> 513km<\/p>**
**Insularum is hemmed in by the prominent Copernicus crater to the east, the Kepler crater to the west and joins up with the large Oceanus Procellarium in the southwest.<\/p>**
**The northern edge is bordered by the Montes Carpatus while the south merges into Mare Cognitum. It was only named in 1976.<\/p>**
**Mare Marginis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of the Edge<\/p>**
**Lat.<\/strong> 13.3 N<\/p>**
**Long.<\/strong> 86.1 E<\/p>**
**Diameter<\/strong> 420km<\/p>**
Located on the \u2018edge\u2019 of the lunar limb, Mare Marginis is unlike most of the nearside maria. It has an irregular outline, appears to be thinner and doesn\u2019t have an apparent impact crater associated with it.<\/p>
Instead, it seems to have been a region of the highlands that was low enough for lava to reach the surface. It is covered with swirls of lighter material most likely reflecting the magnetic field present when the lava formed.<\/p>
**Mare Moscoviense<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Moscow<\/p>**
**Lat.<\/strong> 27.3 N<\/p>**
**Long.<\/strong> 147.9 E<\/p>**
**Diameter<\/strong> 277km<\/p>**
One of the few lunar mare on the far side of the Moon, Moscoviense sits as a dark spot alone in the northern hemisphere. It was first seen in images from the Soviet Luna 3 spacecraft \u2013 the first spacecraft to return pictures of the lunar far side and was named after the nation\u2019s capital city.<\/p>
**Mare Nectaris<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Nectar<\/p>**
**Lat.<\/strong> 15.2 S<\/p>**
**Long.<\/strong> 35.5 E<\/p>**
**Diameter<\/strong> 333km<\/p>**
Mare Nectaris<\/a> is a small lunar mare just south of Mare Tranquillitatis, and bordered by the Montes Pyrenaeus along its eastern edge. The region is in a wider impact basin measuring 860km across (it was this impact that created the Pyrenaeus), but the lava that created the mare didn\u2019t flood the basin until some time later, as is apparent from the lack of impact craters in the region.<\/p>
**Mare Nubium<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Clouds<\/p>**
**Lat.<\/strong> 21.3 S<\/p>**
**Long.<\/strong> 16.6 W<\/p>**
**Diameter<\/strong> 715km<\/p>**
Located to the southeast of Oceanus Procellarum, Mare Nubium is part of the pre-nectarian system, meaning it dates back to the earliest eras of the lunar surface. To the west lies the prominent Bullialdus crater.<\/p>
**Nubium\u2019s northern portion is split in two by a spur of higher ground known as the Fra Mauro highlands, the location of the Apollo 14 landings.<\/p>**
**Mare Orientale<\/strong><\/h3>**
$\"Mare$
Mare Orientale, as seen by NASA’s Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Eastern Sea<\/p>**
**Lat.<\/strong> 19.4 S<\/p>**
**Long.<\/strong> 92.8 W<\/p>**
**Diameter<\/strong> 327km<\/p>**
Mare Orientale is located in the basin created by an ancient meteor impact. The region wasn\u2019t as flooded by lava as other such basins, meaning the multi-ring structure of the basin floor created as the spacerock rebounded after the impact is still clearly visible.<\/p>
**Oceanus Procellarum<\/strong><\/h3>**
$\"Oceanus$ <\/figure>
**English name<\/strong> Ocean of Storms<\/p>**
**Lat.<\/strong> 18.4 N<\/p>**
**Long.<\/strong> 57.4 W<\/p>**
**Diameter<\/strong> 2,568km<\/p>**
Due to its huge size, Procellarum isn\u2019t just a sea \u2013 but an ocean! Its large size suggests it was created by more than a single asteroid impact, but might have been effected by the Moon\u2019s own early geological processes.<\/p>
The GRAIL mission found several large rift valleys created by tectonic faults cracking the land before being flooded with lava. However, these are all buried beneath a remarkably featureless surface that is only peppered with small craters and only one large rayed crater, Kepler, at its centre.<\/p>
**Mare Serenitatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Serenity<\/p>**
**Lat.<\/strong> 28.0 N<\/p>**
**Long.<\/strong> 17.5 E<\/p>**
**Diameter<\/strong> 707km<\/p>**
One of the more prominent seas on the lunar near side, Mare Serenitatis<\/a> is very circular in shape, usually forming the left eye of the \u2018 man in the Moon<\/a>\u2019. Mare Serenitatis was visited both by the crew of NASA\u2019s Apollo 17 in 19XX and by the Soviet Union\u2019s Lunokhod 2 rover in 19XX (also known as Luna 21).<\/p>
Rock samples returned by the Apollo 17 crew revealed that surface of the mare formed 3.8 to 3.9 billion years ago. Almost 50 years later, the Israel Aerospace Industries’ Beresheet lander attempted to land in the sea, but crashed shortly before landing.<\/p>
**Mare Smythii<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Smyth\u2019s Sea<\/p>**
**Lat.<\/strong> 1.3 N<\/p>**
**Long.<\/strong> 87.5 E<\/p>**
**Diameter<\/strong> 373km<\/p>**
In reality, Mare Smythii is circular, but it is so near the lunar limb that from Earth it appears elliptical. In fact, some of the mare curves around onto the far side. The craters within the mare appear to have a large number of fractured floors, most likely caused by lava rising up from underneath.<\/p>
**Mare Spumans<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Foaming Sea<\/p>**
**Lat.<\/strong> 1.1 N<\/p>**
**Long.<\/strong> 65.1 E<\/p>**
**Diameter<\/strong> 139km<\/p>**
Mare Supmans is one of the smaller seas located on the raised edge of the Crisium basin, surrounding the larger Mare Crisium. It is just to the south of Mare Undarum. On its western rim is the bright white Petit crater, surrounded by bright rays of ejecta.<\/p>
**Mare Tranquillitatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Tranquility<\/p>**
**Lat.<\/strong> 8.5 N<\/p>**
**Long.<\/strong> 31.4 E<\/p>**
**Diameter<\/strong> 873km<\/p>**
**Made famous as the location where Neil Armstrong took \u2018one small step for man\u2019 during the** **Apollo 11<\/a> landing, Mare Tranquillitatis<\/a> is a very flat region, with only 500m elevation difference between the highest and lowest points in the basin.<\/p>**
The mare has an irregular edge, which it shares with the basins of Serenitatis and Nectaris. It has a higher metal content than surrounding lunar rock giving it a blue tinge – not to be confused with a ‘blue Moon<\/a>‘, however! – , though this only really stands out in heavily processed images.<\/p>
**If you’d like to try and spot this region for yourself, read our guide on how to find Apollo 11’s landing site<\/a>.<\/p>**
**Mare Undarum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Waves<\/p>**
**Lat.<\/strong> 6.8 N<\/p>**
**Long.<\/strong> 68.4 E<\/p>**
**Diameter<\/strong> 243km<\/p>**
Mare Undarum is an irregular shaped sea without the smooth surface seen in many other maria. In the early 1800s, when lunar astronomer Johann M\u00e4dler was surveying the region, he discovered dark streaks throughout the region and speculated that they might be caused by vegetation growing across the surface: a forgivable conclusion considering he was looking through an early 95mm refractor.<\/p>
**Mare Vaporum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Vapors<\/p>**
**Lat.<\/strong> 13.3 N<\/p>**
**Long.<\/strong> 3.6 E<\/p>**
**Diameter<\/strong> 245km<\/p>**
Near the centre of the Moon\u2019s visible face lies the circular Mare Vaporum. It\u2019s bordered to the north by several mountain ranges, including the impressive Apennine\u2019s which tower 5,000m over the floor of the crater. The mare contains only one significant crater, the 39km wide Manilium.<\/p>
***What are your favourite lunar maria? Share your thoughts and images with us by emailing*** ***contactus@skyatnightmagazine.com<\/a><\/em><\/strong><\/p> <\/body><\/html>\n***
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A mosaic image of the Moon captured by the Galileo spacecraft, showing colour on the lunar surface. On the upper left is Mare Imbrium; middle left is Mare Serenitatis; lower left is Mare Tranquillitatis, and the dark patch towards the bottom is Mare Crisium. Credit: Stocktrek Images<\/figcaption><\/figure>
Formation of the Moon<\/strong><\/h2>
By studying topographical features of the lunar landscape such as the highlands, maria and craters, astronomers have been able to piece together a history of the Moon as it formed and evolved over billions of years.<\/p>
One theory of how the Moon formed<\/a> says a large body collided with Earth about 4.5 billion years ago, and the debris from the wreckage coalesced over time to form a satellite in orbit around our planet.<\/p>
This early Moon was likely covered in molten magma, which then cooled to create the rugged, cold and lifeless rock that we know today.<\/p>
Over time, the lunar maria have been studied in great detail, both using ground-based telescopes, robotic probes and, of course, by human explorers during the Apollo missions.<\/p>
$\"Buzz$
Buzz Aldrin pictured in the Sea of Tranquility during Apollo 11. Credit: NASA \/ Neil A. Armstrong.<\/figcaption><\/figure>
Observing the lunar maria<\/strong><\/h2>
On a clear night, when the Moon is prominent in the night sky, it is one of the best objects to observe, and the lunar maria are among the easiest sights to see.<\/p>
While much can be seen on the Moon with the naked eye, a pair of modest binoculars will let you spot maria and craters on the lunar surface.<\/p>
For more on this, read our tutorial on how to observe the Moon<\/a>, or our beginners’ guide to stargazing with binoculars<\/a>.<\/p>
You might think that the ideal time to observe the lunar surface is during a full Moon or even a full supermoon<\/a>.<\/p>
Instead, find out when the Moon will next be visible in the night sky during its crescent or gibbous phase.<\/p>
This will enable you to spot the ‘terminator<\/a>‘, which is the line dividing the bright and dark portions of the Moon from our perspective.<\/p>
Learn more about this with our guide to the phases of the Moon<\/a>.<\/p>
$\"The$
The ‘terminator’ on the Moon is the line dividing the lit and unlit sections. Credit: William Ian Hamilton<\/figcaption><\/figure>
Looking along the terminator will enable you to use shadows to make out the Moon’s rugged surface much easier than when the Moon is full.<\/p>
And, because the Moon is tidally locked with Earth, meaning we always see the same side of the Moon<\/a>, you can track how the terminator changes night after night.<\/p>
We may not be able to see the far side of the Moon<\/a> directly from Earth, but you can catch a glimpse of what’s beyond the limb by studying and even photographing lunar libration<\/a>.<\/p>
In fact, one of the lunar seas, Mare Orientale<\/a>, can only be seen during a favourable libration.<\/p>
$\"mare$
Favourable lunar libration is required to see the Moon’s Mare Orientale region. Credit: Pete Lawrence<\/figcaption><\/figure>
**Observing the Moon online<\/strong><\/h2>**You can also explore the lunar surface online, either by using Google Moon<\/a>, by visiting the Lunar Reconnaissance Orbiter website<\/a> or by downloading the excellent JMars software<\/a> (used by actual NASA planetary scientists!)<\/p>
Below is our complete guide to the lunar seas, how big they are, where they\u2019re located, and facts about their interesting features.<\/p>
If you’re interested in trying to image them, read our guide on how to photograph the Moon<\/a>.<\/p>
**Lunar maria or seas<\/strong><\/h2>**
**Mare Anguis<\/strong><\/h3>**
$\"Mare$
Mare Anguis Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Serpent Sea<\/p>**
**Lat.<\/strong> 22.6 N<\/p>**
**Long.<\/strong> 67.7 E<\/p>**
**Diameter<\/strong> 150km<\/p>**
Located close to the edge of the lunar limb is Mare Anguis, which roughly shaped like an X. It lies near the rim of the much larger Mare Crisium, elevated 800m above. To its east is the 7km wide Eimmart A crater.<\/p>
**Mare Australe<\/strong><\/h3>**
$\"Mare$
Mare Australe Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Southern Sea<\/p>**
**Lat.<\/strong> 38.9 S<\/p>**
**Long.<\/strong> 93.0 E<\/p>**
**Diameter<\/strong> 603km<\/p>**
**Located on the very edge of the Moon, Mare Australe is only visible when** **libration<\/a> tips the Moon forward enough to see it. Unlike most of the other smooth maria, Australe is pockmarked by impact craters which then flooded with basaltic lava.<\/p>**
**Mare Cognitum<\/strong><\/h3>**
$\"Mare$
Mare Cognitum Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Known Sea<\/p>**
**Lat.<\/strong> 10.0 S<\/p>**
**Long.<\/strong> 23.1 W<\/p>**
**Diameter<\/strong> 376km<\/p>**
**In 1964, after years of trying, NASA finally succeeded in \u2018landing\u2019 on the Moon with their Ranger 7 impact probe. The Surveyor 3 soft lander would follow in 1967, paving the way for the** **Apollo 12<\/a> crew to arrive in 1969. Prior to the Ranger 7 landing, the region was unnamed, but was renamed to reflect its role in America\u2019s lunar plans.<\/p>**
**Mare Crisium<\/strong><\/h3>**
$\"Mare$
Mare Crisium, captured by the Lunar Reconnaissance Orbiter. Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Crises<\/p>**
**Lat.<\/strong> 17.0\u00b0 N<\/p>**
**Long.<\/strong> 59.1\u00b0 E<\/p>**
**Diameter<\/strong> 418km<\/p>**
**Unlike most of the other lunar seas,** Mare Crisium<\/a> is an isolated oval that doesn\u2019t merge with others. It\u2019s a large impact basin with visible walls in several places found to the northeast of Mare Tranquillitatis. With an area of 180,000km2, it’s around the same size as England.<\/p>
**Mare Fecunditatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Fecundity<\/p>**
**Lat.<\/strong> 7.8 S<\/p>**
**Long.<\/strong> 51.3 E<\/p>**
**Diameter<\/strong> 909km<\/p>**
**The main basin of** **Mare Fecunditatis<\/a> formed in the pre-Nectarian era \u2013 the earliest time period just after the Moon formed. However, material surrounding it dates from later eras.<\/p>**
The crater overlaps with surrounding Nectaris, Tranquillitatis and Crisium basins. It is unusual in that it has no \u2018mascons\u2019 \u2013 invisible concentrations of mass hidden below the surface of most lunar mare, which are great enough to pull orbiting spacecraft off course.<\/p>
**Mare Frigoris<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Cold<\/p>**
**Lat.<\/strong> 56.0\u00b0 N<\/p>**
**Long.<\/strong> 1.4\u00b0 E<\/p>**
**Diameter<\/strong> 1596km<\/p>**
**The northernmost sea, along the top of the Imbrium and Serenitatis basins,** **Mare Frigoris<\/a> has an intriguing elongated shape, averaging only 250m wide but stretching to over 1,400km in length.<\/p>**
$\"Craters$
Craters Aristoteles and Eudoxus by Avani Soares, Parsec Observatory, Canoas, Brazil. Equipment: C14 Edge, ASI 290, IR pass 685<\/figcaption><\/figure>
Notable features include ejecta from the 40km diameter Harpalus crater that covers a large portion of Frigoris\u2019s floor in the west and, on the south shore, the scars of 88km Aristoteles and 67km Eudoxus, both complex craters with terraced walls.<\/p>
**Mare Humboldtianum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Alexander von Humboldt<\/p>**
**Lat.<\/strong> 56.8 N<\/p>**
**Long.<\/strong> 81.5 E<\/p>**
**Diameter<\/strong> 273km<\/p>**
Located to the east of Frigoris, Mare Humboldtianum is right on the northeastern limb of the Moon. Due to the slight wobble of the Moon from Earth (an effect known as libration), the sea is sometimes hidden from view.<\/p>
The name is a reference to this location, bridging the gap between the known and the unknown, and so it was named after Alexander von Humboldt, a Prussian natural scientist born in 1769 who was famous for travelling the world and exploring places no European had visited before.<\/p>
**Mare Humorum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Moisture<\/p>**
**Lat.<\/strong> 24.4 S<\/p>**
**Long.<\/strong> 38.6 W<\/p>**
**Diameter<\/strong> 389km<\/p>**
**The lava layer of** Mare Humorum<\/a> is thought to exceed 3km in thickness at the basin\u2019s centre. It\u2019s also home to a major mascon, a mass concentration created by a collection of dense material below the surface that is large enough to affect the Moon\u2019s gravitational pull.<\/p>
For these reasons, it\u2019s an area of great scientific interest, allowing planetary scientists to study the relationship between lunar mare filling, basin tectonics and the thermal evolution of a major mascon maria.<\/p>
**Mare Imbrium<\/strong><\/h3>**
$\"Mare$
Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Showers<\/p>**
**Lat.<\/strong> 32.8 N<\/p>**
**Long.<\/strong> 15.6 W<\/p>**
**Diameter<\/strong> 1123km<\/p>**
**As the largest basin on the lunar nearside,** Mare Imbrium<\/a> requires a bit of mobility to explore properly and has been visited by three different rovers: the Soviet Union\u2019s Lunokhod 1 rover in 1970, NASA\u2019s Apollo 15 rover driven by David Scott and James Irwin in 1971, and the Chinese Chang\u2019e 3 lander<\/a> and its rover Yutu in 2013.<\/p>
**The basin is surrounded by a ring of mountains, rising up as much as 7km above the mare floor, and there are signs of ejecta radiating out as far as 800km from the crater.<\/p>**
**Mare Ingenii<\/strong><\/h3>**
$\"Mare$
Mare Ingenii Credit: NASA \/ Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Sea of Cleverness<\/p>**
**Lat.<\/strong> 33.7 S<\/p>**
**Long.<\/strong> 163.5 E<\/p>**
**Diameter<\/strong> 318km<\/p>**
**Located on the far side of the Moon, Mare Ingenii makes up part of the** **South Pole-Aitken basin<\/a> \u2013 a huge lunar feature that covers most of the southern hemisphere. The region contains the 112km wide Thomson crater.<\/p>**
The floor of Igenii is covered in dramatic swirls of light and dark volcanic material, the pattern of which is believed to reflect the localised magnetic field of the region back when the Moon’s lava was still molten.<\/p>
**Mare Insularum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Islands<\/p>**
**Lat.<\/strong> 7.5 N<\/p>**
**Long.<\/strong> 30.9 W<\/p>**
**Diameter<\/strong> 513km<\/p>**
**Insularum is hemmed in by the prominent Copernicus crater to the east, the Kepler crater to the west and joins up with the large Oceanus Procellarium in the southwest.<\/p>**
**The northern edge is bordered by the Montes Carpatus while the south merges into Mare Cognitum. It was only named in 1976.<\/p>**
**Mare Marginis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of the Edge<\/p>**
**Lat.<\/strong> 13.3 N<\/p>**
**Long.<\/strong> 86.1 E<\/p>**
**Diameter<\/strong> 420km<\/p>**
Located on the \u2018edge\u2019 of the lunar limb, Mare Marginis is unlike most of the nearside maria. It has an irregular outline, appears to be thinner and doesn\u2019t have an apparent impact crater associated with it.<\/p>
Instead, it seems to have been a region of the highlands that was low enough for lava to reach the surface. It is covered with swirls of lighter material most likely reflecting the magnetic field present when the lava formed.<\/p>
**Mare Moscoviense<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Moscow<\/p>**
**Lat.<\/strong> 27.3 N<\/p>**
**Long.<\/strong> 147.9 E<\/p>**
**Diameter<\/strong> 277km<\/p>**
One of the few lunar mare on the far side of the Moon, Moscoviense sits as a dark spot alone in the northern hemisphere. It was first seen in images from the Soviet Luna 3 spacecraft \u2013 the first spacecraft to return pictures of the lunar far side and was named after the nation\u2019s capital city.<\/p>
**Mare Nectaris<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Nectar<\/p>**
**Lat.<\/strong> 15.2 S<\/p>**
**Long.<\/strong> 35.5 E<\/p>**
**Diameter<\/strong> 333km<\/p>**
Mare Nectaris<\/a> is a small lunar mare just south of Mare Tranquillitatis, and bordered by the Montes Pyrenaeus along its eastern edge. The region is in a wider impact basin measuring 860km across (it was this impact that created the Pyrenaeus), but the lava that created the mare didn\u2019t flood the basin until some time later, as is apparent from the lack of impact craters in the region.<\/p>
**Mare Nubium<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Clouds<\/p>**
**Lat.<\/strong> 21.3 S<\/p>**
**Long.<\/strong> 16.6 W<\/p>**
**Diameter<\/strong> 715km<\/p>**
Located to the southeast of Oceanus Procellarum, Mare Nubium is part of the pre-nectarian system, meaning it dates back to the earliest eras of the lunar surface. To the west lies the prominent Bullialdus crater.<\/p>
**Nubium\u2019s northern portion is split in two by a spur of higher ground known as the Fra Mauro highlands, the location of the Apollo 14 landings.<\/p>**
**Mare Orientale<\/strong><\/h3>**
$\"Mare$
Mare Orientale, as seen by NASA’s Lunar Reconnaissance Orbiter<\/figcaption><\/figure>
**English name<\/strong> Eastern Sea<\/p>**
**Lat.<\/strong> 19.4 S<\/p>**
**Long.<\/strong> 92.8 W<\/p>**
**Diameter<\/strong> 327km<\/p>**
Mare Orientale is located in the basin created by an ancient meteor impact. The region wasn\u2019t as flooded by lava as other such basins, meaning the multi-ring structure of the basin floor created as the spacerock rebounded after the impact is still clearly visible.<\/p>
**Oceanus Procellarum<\/strong><\/h3>**
$\"Oceanus$ <\/figure>
**English name<\/strong> Ocean of Storms<\/p>**
**Lat.<\/strong> 18.4 N<\/p>**
**Long.<\/strong> 57.4 W<\/p>**
**Diameter<\/strong> 2,568km<\/p>**
Due to its huge size, Procellarum isn\u2019t just a sea \u2013 but an ocean! Its large size suggests it was created by more than a single asteroid impact, but might have been effected by the Moon\u2019s own early geological processes.<\/p>
The GRAIL mission found several large rift valleys created by tectonic faults cracking the land before being flooded with lava. However, these are all buried beneath a remarkably featureless surface that is only peppered with small craters and only one large rayed crater, Kepler, at its centre.<\/p>
**Mare Serenitatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Serenity<\/p>**
**Lat.<\/strong> 28.0 N<\/p>**
**Long.<\/strong> 17.5 E<\/p>**
**Diameter<\/strong> 707km<\/p>**
One of the more prominent seas on the lunar near side, Mare Serenitatis<\/a> is very circular in shape, usually forming the left eye of the \u2018 man in the Moon<\/a>\u2019. Mare Serenitatis was visited both by the crew of NASA\u2019s Apollo 17 in 19XX and by the Soviet Union\u2019s Lunokhod 2 rover in 19XX (also known as Luna 21).<\/p>
Rock samples returned by the Apollo 17 crew revealed that surface of the mare formed 3.8 to 3.9 billion years ago. Almost 50 years later, the Israel Aerospace Industries’ Beresheet lander attempted to land in the sea, but crashed shortly before landing.<\/p>
**Mare Smythii<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Smyth\u2019s Sea<\/p>**
**Lat.<\/strong> 1.3 N<\/p>**
**Long.<\/strong> 87.5 E<\/p>**
**Diameter<\/strong> 373km<\/p>**
In reality, Mare Smythii is circular, but it is so near the lunar limb that from Earth it appears elliptical. In fact, some of the mare curves around onto the far side. The craters within the mare appear to have a large number of fractured floors, most likely caused by lava rising up from underneath.<\/p>
**Mare Spumans<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Foaming Sea<\/p>**
**Lat.<\/strong> 1.1 N<\/p>**
**Long.<\/strong> 65.1 E<\/p>**
**Diameter<\/strong> 139km<\/p>**
Mare Supmans is one of the smaller seas located on the raised edge of the Crisium basin, surrounding the larger Mare Crisium. It is just to the south of Mare Undarum. On its western rim is the bright white Petit crater, surrounded by bright rays of ejecta.<\/p>
**Mare Tranquillitatis<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Tranquility<\/p>**
**Lat.<\/strong> 8.5 N<\/p>**
**Long.<\/strong> 31.4 E<\/p>**
**Diameter<\/strong> 873km<\/p>**
**Made famous as the location where Neil Armstrong took \u2018one small step for man\u2019 during the** **Apollo 11<\/a> landing, Mare Tranquillitatis<\/a> is a very flat region, with only 500m elevation difference between the highest and lowest points in the basin.<\/p>**
The mare has an irregular edge, which it shares with the basins of Serenitatis and Nectaris. It has a higher metal content than surrounding lunar rock giving it a blue tinge – not to be confused with a ‘blue Moon<\/a>‘, however! – , though this only really stands out in heavily processed images.<\/p>
**If you’d like to try and spot this region for yourself, read our guide on how to find Apollo 11’s landing site<\/a>.<\/p>**
**Mare Undarum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Waves<\/p>**
**Lat.<\/strong> 6.8 N<\/p>**
**Long.<\/strong> 68.4 E<\/p>**
**Diameter<\/strong> 243km<\/p>**
Mare Undarum is an irregular shaped sea without the smooth surface seen in many other maria. In the early 1800s, when lunar astronomer Johann M\u00e4dler was surveying the region, he discovered dark streaks throughout the region and speculated that they might be caused by vegetation growing across the surface: a forgivable conclusion considering he was looking through an early 95mm refractor.<\/p>
**Mare Vaporum<\/strong><\/h3>**
$\"Mare$ <\/figure>
**English name<\/strong> Sea of Vapors<\/p>**
**Lat.<\/strong> 13.3 N<\/p>**
**Long.<\/strong> 3.6 E<\/p>**
**Diameter<\/strong> 245km<\/p>**
Near the centre of the Moon\u2019s visible face lies the circular Mare Vaporum. It\u2019s bordered to the north by several mountain ranges, including the impressive Apennine\u2019s which tower 5,000m over the floor of the crater. The mare contains only one significant crater, the 39km wide Manilium.<\/p>
***What are your favourite lunar maria? Share your thoughts and images with us by emailing*** ***contactus@skyatnightmagazine.com<\/a><\/em><\/strong><\/p> <\/body><\/html>\n***
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