Definition
Irregular, shallow mare basin with relatively thin basalt fill.
Synonyms
Description
Tranquillitatis-type basins are noncircular in plan view and lack identifiable raised rings (Fig. 1).
References
De Hon RA (1979) Thickness of the western mare basalts. Proc Lunar Planet Sci Conf 10:2935–2955, Houston
De Hon RA, Waskom JD (1976) Geologic structure of the eastern mare basins. Proc Lunar Sci Conf 7:2729–2746, Houston
Hiesinger H, Head III JW (2003) Lunar south pole-aitken impact basin: clementine topography and implications for the interpretation of basin structure and stratigraphy. Microsymposium 38, MS101. Vernadsky Institute/Brown University, Moscow
Olson AB, Wilhelns DE (1974) Geologic map of the Undarum quadrangle of the moon. U.S. Geol Surv Misc Geol Inv Map I-837. U.S. Govt Printing Office, Washington, DC
Solomon SC, Comer RP, Head JW (1982) The evolution of impact basins’ viscous relaxation of topographic relief. JGR 87:3975–3992
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2014 Springer Science+Business Media New York
About this entry
Cite this entry
De Hon, R. (2014). Tranquillitatis-Type Mare Basin. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_593-1
Download citation
DOI: https://doi.org/10.1007/978-1-4614-9213-9_593-1
Received:
Accepted:
Published:
Publisher Name: Springer, New York, NY
Online ISBN: 978-1-4614-9213-9
eBook Packages: Springer Reference Earth and Environm. ScienceReference Module Physical and Materials ScienceReference Module Earth and Environmental Sciences