Craterra

LUNAR ATLAS · FAR SIDE BASIN

Mare Moscoviense: The Sea of Moscow on the Lunar Far Side

Centered within an ancient multi-ring impact basin on the lunar far side, Mare Moscoviense occupies an unusually thin crustal zone marked by a strong mascon.

Feature Profile & Selenographic Data

Feature type
mare
Coordinates
27.3° N · 147.9° E
Diameter
277 km
IAU approval
1961/01/01 00:00:00
LAC quadrangle
LAC-48 · Mare Moscoviense
Geological Period
Nectarian / Upper Imbrian

Geological Chronicle

Mare Moscoviense (Latin for 'Sea of Muscovy') is a lunar mare located within an impact basin on the far side of the Moon at 27.3° N, 147.9° E. The mare spans approximately 277 kilometers (172 miles) across, making it one of the few extensive volcanic plains on the lunar far hemisphere. Unlike the lunar near side, where volcanic plains cover wide regions, the far side has a thicker crust that generally prevented magma from reaching the surface. Mare Moscoviense formed where a deep basin penetrated an unusually thin crustal zone, allowing mantle material and basaltic lavas to emerge.

The underlying Moscoviense basin formed during the Nectarian epoch, while the subsequent volcanic basalt flows erupted during the Upper Imbrian epoch. Data from the Japanese SELENE (Kaguya) mission indicated that volcanic activity in the basin persisted for at least 1.5 billion years following its initial impact excavation. The basalt layer occupies the lower southwestern portion of the basin floor, surrounded by higher highland terrain. Doppler tracking by the Lunar Prospector spacecraft in 1998 detected a distinct mass concentration (mascon), marking a strong positive gravitational anomaly caused by dense basalt and mantle uplift.

Surrounding impact features include several named craters along the basin margin. The crater Titov lies within the northeastern section of the mare, while Tereshkova borders its northern rim. To the southeast lies the floor-fractured crater Komarov, alongside the larger Korolev basin. Just to the south sits the crater Leonov, named after Soviet cosmonaut Alexei Leonov. Farther east lies the ancient Freundlich-Sharonov Basin.

The mare was first discovered in October 1959 when the Soviet spacecraft Luna 3 returned the first photographs of the lunar far side. The Soviet Union proposed naming the feature after Moscow. In 1961, the International Astronomical Union (IAU) officially approved the designation after French astronomer Audouin Dollfus noted that Moscow was a state of mind, reconciling the choice with lunar naming conventions that typically use weather or abstract terms.

Chronology & Exploration

  1. Nectarian Epoch Moscoviense Basin Impact

    A major impact carves out the multi-ring Moscoviense basin on the northern far side of the Moon.

  2. Upper Imbrian Epoch Basalt Volcanism

    Volcanic lavas flood the low-elevation southwestern depression of the basin over an extended geological period.

  3. 1959 Luna 3 Discovery

    Soviet probe Luna 3 transmits the first photographic images of the lunar far side, identifying the dark plain.

  4. 1961 IAU Name Approval

    The International Astronomical Union formally ratifies the name Mare Moscoviense (Sea of Muscovy).

  5. 1998 Lunar Prospector Mascon Detection

    Doppler tracking data confirms a pronounced positive gravitational anomaly (mascon) beneath the basin floor.

Scientific Sources & References

Name Origin

"Sea of Muscovy."

Interactive Lunar Surface

Explore Mare Moscoviense in 3D

Inspect lunar elevation data and the official selenographic position.