Lacus Felicitatis
An academic exploration of a unique lunar mare, detailing its geological characteristics, location, and associated craters.
Explore Lacus Felicitatis 🔭 Discover Craters craterDive in with Flashcard Learning!
🎮 Play the Wiki2Web Clarity Challenge Game🎮
Overview
Definition and Nature
Lacus Felicitatis, translating from Latin to "Lake of Happiness," is a distinct geological feature on the Moon's surface. It represents a region that has been inundated by basaltic lava flows, a process common in the formation of lunar maria. This volcanic resurfacing has resulted in a relatively smooth, level terrain with a lower albedo (reflectivity) compared to the surrounding, more ancient lunar highlands.[1]
Significance in Lunar Geology
As a relatively small mare, Lacus Felicitatis offers valuable insights into the later stages of lunar volcanic activity. Its unique morphology and composition, particularly its lower albedo, suggest specific lava flow characteristics and potential differences in mineralogy compared to larger maria. Studying such features helps refine our understanding of the Moon's thermal history and geological evolution.
Location and Topography
Geographical Context
Lacus Felicitatis is situated within the continental region designated as Terra Nivium. It lies to the north of the larger lunar mare, Mare Vaporum. Its geographical context is further defined by its proximity to the Montes Haemus mountain range, located approximately 70 to 80 kilometers to the northeast, and its position along the southwestern margin of Mare Serenitatis.
Morphological Characteristics
The formation exhibits a characteristic bent or irregular morphology, comprising a discernible northwestern lobe and an eastern extension. Its perimeter is notably uneven, bordered by the more rugged and ancient lunar highlands. This irregular boundary is a testament to the complex interplay between the lava flows and the pre-existing lunar topography.
Dimensions and Coordinates
Precise Location
The selenographic coordinates, which specify locations on the Moon's surface relative to its center, for the center of Lacus Felicitatis are approximately 18.5° North latitude and 5.4° East longitude (18°30′N 5°24′E).
Extent of the Feature
The feature possesses a maximum extent of approximately 98 kilometers (61 miles) in diameter. This measurement reflects the overall dimensions of the lava-inundated area.
Key Features
Albedo Variation
A defining characteristic of Lacus Felicitatis is its lower albedo compared to the surrounding terrain. This reduced reflectivity suggests a different surface composition, likely due to the specific mineralogy of the basaltic lavas that formed the mare. Understanding these variations is crucial for remote sensing analysis of lunar surfaces.
Evidence of Recent Activity?
Within Lacus Felicitatis lies the crater Ina, a unique geological formation. Ina is a semi-circular depression, approximately 30 meters deep, which is notoriously difficult to image clearly from Earth. In 2006, scientific hypotheses suggested that Ina might be the result of a relatively recent gas eruption, potentially occurring within the last ten million years. This possibility indicates that some lunar geological processes may have continued more recently than previously assumed.
Designated Craters
IAU Nomenclatures
Three small craters within the boundaries of Lacus Felicitatis have been officially named by the International Astronomical Union (IAU). These designations aid in precise astronomical observation and cartography.
Teacher's Corner
Edit and Print this course in the Wiki2Web Teacher Studio

Click here to open the "Lacus Felicitatis" Wiki2Web Studio curriculum kit
Use the free Wiki2web Studio to generate printable flashcards, worksheets, exams, and export your materials as a web page or an interactive game.
True or False?
Test Your Knowledge!
Gamer's Corner
Are you ready for the Wiki2Web Clarity Challenge?
Unlock the mystery image and prove your knowledge by earning trophies. This simple game is addictively fun and is a great way to learn!
Play now
References
References
Feedback & Support
To report an issue with this page, or to find out ways to support the mission, please click here.
Disclaimer
Important Notice
This page has been generated by Artificial Intelligence and is intended for informational and educational purposes exclusively. The content is derived from a snapshot of publicly available data, primarily from Wikipedia, and may not represent the most current or complete scientific understanding.
This is not professional scientific advice. The information provided herein is not a substitute for expert consultation in planetary science, geology, or astronomy. Always refer to peer-reviewed scientific literature and consult with qualified professionals for specific research or academic inquiries.
The creators of this page are not responsible for any inaccuracies, omissions, or for any actions taken based on the information presented.