Gruithuisen Domes - Constellation Region of Interest

A small rille hugging the contours at the base of Gruithuisen Gamma, at the contact between the dome and the surrounding mare. Image is 1.6 km wide, illumination is from the left, NAC frame M104776541R [NASA/GSFC/Arizona State University].

The Gruithuisen Domes, a Constellation program region of interest, are located on the northeast border of Oceanus Procellarum at the highlands-mare boundary. The three Gruithuisen domes are named for nearby Gruithuisen crater. The two largest domes have been unofficially referred to for many years as Gruithuisen Gamma and Gruithuisen Delta, with the smallest dome called NW (for "northwest").

All three of the Gruithuisen domes and the surrounding terrain are shown in WAC frame M117752970. Image width is 64 km and illumination is from the left [NASA/GSFC/Arizona State University].

The Gruithuisen domes are classified by lunar scientists as "nonmare" volcanic domes.  This is because we know from Earth based telescopes, Lunar Prospector gamma-ray spectroscopy data, and Clementine multispectral data that the domes are composed of materials different from either the mare or highlands. The Gruithuisen Domes are characterized by a relatively high albedo and strong absorptions in the visible and ultraviolet, and the domes are low in iron and titanium compared to the volcanic deposits of the lunar mare. Previous studies of this region showed that Gruithuisen may represent a lunar analog to terrestrial rhyolites, dacites, or basaltic andesites, which are characterized by viscous lava and low extrusion rates. In comparison, mare volcanic domes (like the Marius Hills and Hortensius, also Constellation regions of interest) are similar to mare basalts in composition, and are generally flatter, smaller, as well as more common on the lunar surface.

Take out your 3D glasses and view this amazing anaglyph of Gruithuisen Gamma created using NAC stereo pairs! Image features NAC frames M104776541 and M104783697. The rille on the northeast edge of Gruithuisen Gamma is featured in the opening image [NASA/GSFC/Arizona State University].

Due to the unique nature of the Gruithuisen Domes, they are a high-priority target for future human lunar exploration. What geologic process created these domes here -- and when? How did the magmas that formed the Gruithuisen domes differ from the magmas that formed the highlands and the mare? Since significant scientific questions remain about the mechanics of lunar mare formation, understanding how the Gruithuisen Domes differ from typical mare basalts will enable us to answer these and other important questions about the formation and evolution of terrestrial planets. Data from LROC and the other instruments aboard LRO, as well as data from other recent lunar missions, are helping us address these questions, although a true understanding of the region will only come when astronauts can explore it directly.

Plan your own adventure to the Gruithuisen Domes!

For more information on LROC's observation campaign for the Constellation program regions of interest read this Lunar and Planetary Science Conference abstract, and visit the LRO Science Targeting Meeting website (look for the baseball card summary sheets for each site: part 1, part 2).

Published by Sarah Braden on 8 June 2010