The new map, created by the Gravity Recovery and Interior Laboratory (GRAIL) mission, is allowing scientists to learn about the Moon’s internal structure and composition in unprecedented detail. Data from the two washing-machine-sized spacecraft also will provide a better understanding of how Earth and other rocky planets in the solar system formed and evolved.
The gravity field map reveals an abundance of features never before seen in detail, such as tectonic structures, volcanic landforms, basin rings, crater central peaks, and numerous simple bowl-shaped craters. Data also show the Moon’s gravity field is unlike that of any terrestrial planet in our solar system.
“What this map tells us is that more than any other celestial body we know of, the Moon wears its gravity field on its sleeve,” said Maria Zuber of the Massachusetts Institute of Technology in Cambridge. “When we see a notable change in the gravity field, we can sync up this change with surface topography features such as craters, rilles, or mountains.”
According to Zuber, the Moon’s gravity field preserves the record of impact bombardment that characterized all terrestrial planetary bodies and reveals evidence for fracturing of the interior extending to the deep crust and possibly the mantle. This impact record is preserved, and now precisely measured, on the Moon.
The probes revealed the bulk density of the Moon’s highland crust is substantially lower than generally assumed. This low-bulk crustal density agrees well with data obtained during the final Apollo lunar missions in the early 1970s, indicating that local samples returned by astronauts are indicative of global processes.
“With our new crustal bulk density determination, we find that the average thickness of the Moon’s crust is between 21 and 27 miles (34 and 43 kilometers), which is about 6 to 12 miles (10 to 20km) thinner than previously thought,” said Mark Wieczorek at the Institut de Physique du Globe de Paris. “With this crustal thickness, the bulk composition of the Moon is similar to that of Earth. This supports models where the Moon is derived from Earth materials that were ejected during a giant impact event early in solar system history.”
The map was created by the spacecraft transmitting radio signals to define precisely the distance between them as they orbit the Moon in formation. As they fly over areas of greater and lesser gravity caused by visible features, such as mountains and craters and masses hidden beneath the lunar surface, the distance between the two spacecraft will change slightly.
“We used gradients of the gravity field in order to highlight smaller and narrower structures than could be seen in previous data sets,” said Jeff Andrews-Hanna from the Colorado School of Mines in Golden. “This data revealed a population of long, linear gravity anomalies, with lengths of hundreds of kilometers crisscrossing the surface. These linear gravity anomalies indicate the presence of dikes, or long, thin vertical bodies of solidified magma in the subsurface. The dikes are among the oldest features on the Moon, and understanding them will tell us about its early history.”
While results from the primary science mission are just beginning to be released, the collection of gravity science by the lunar twins continues. GRAIL’s extended mission science phase began August 30 and will conclude December 17. As the end of the mission nears, the spacecraft will operate at lower orbital altitudes above the Moon.
The new map, created by the Gravity Recovery and Interior Laboratory (GRAIL) mission, is allowing scientists to learn about the Moon’s internal structure and composition in unprecedented detail. Data from the two washing-machine-sized spacecraft also will provide a better understanding of how Earth and other rocky planets in the solar system formed and evolved.
The gravity field map reveals an abundance of features never before seen in detail, such as tectonic structures, volcanic landforms, basin rings, crater central peaks, and numerous simple bowl-shaped craters. Data also show the Moon’s gravity field is unlike that of any terrestrial planet in our solar system.
“What this map tells us is that more than any other celestial body we know of, the Moon wears its gravity field on its sleeve,” said Maria Zuber of the Massachusetts Institute of Technology in Cambridge. “When we see a notable change in the gravity field, we can sync up this change with surface topography features such as craters, rilles, or mountains.”
According to Zuber, the Moon’s gravity field preserves the record of impact bombardment that characterized all terrestrial planetary bodies and reveals evidence for fracturing of the interior extending to the deep crust and possibly the mantle. This impact record is preserved, and now precisely measured, on the Moon.
The probes revealed the bulk density of the Moon’s highland crust is substantially lower than generally assumed. This low-bulk crustal density agrees well with data obtained during the final Apollo lunar missions in the early 1970s, indicating that local samples returned by astronauts are indicative of global processes.
“With our new crustal bulk density determination, we find that the average thickness of the Moon’s crust is between 21 and 27 miles (34 and 43 kilometers), which is about 6 to 12 miles (10 to 20km) thinner than previously thought,” said Mark Wieczorek at the Institut de Physique du Globe de Paris. “With this crustal thickness, the bulk composition of the Moon is similar to that of Earth. This supports models where the Moon is derived from Earth materials that were ejected during a giant impact event early in solar system history.”
The map was created by the spacecraft transmitting radio signals to define precisely the distance between them as they orbit the Moon in formation. As they fly over areas of greater and lesser gravity caused by visible features, such as mountains and craters and masses hidden beneath the lunar surface, the distance between the two spacecraft will change slightly.
“We used gradients of the gravity field in order to highlight smaller and narrower structures than could be seen in previous data sets,” said Jeff Andrews-Hanna from the Colorado School of Mines in Golden. “This data revealed a population of long, linear gravity anomalies, with lengths of hundreds of kilometers crisscrossing the surface. These linear gravity anomalies indicate the presence of dikes, or long, thin vertical bodies of solidified magma in the subsurface. The dikes are among the oldest features on the Moon, and understanding them will tell us about its early history.”
While results from the primary science mission are just beginning to be released, the collection of gravity science by the lunar twins continues. GRAIL’s extended mission science phase began August 30 and will conclude December 17. As the end of the mission nears, the spacecraft will operate at lower orbital altitudes above the Moon.
