Moon-forming impactor as a source of Earth’s basal mantle anomalies
Qian Yuan, Mingming Li, Steven J. Desch, Byeongkwan Ko, Hongping Deng,
Edward J. Garnero, Travis S. J. Gabriel, Jacob A. Kegerreis, Yoshinori Miyazaki, Vincent Eke & Paul D. Asimow
Abstract
Seismic images of Earth’s interior have revealed two continent-sized anomalies with low seismic velocities, known as the large low-velocity provinces (LLVPs), in the lowermost mantle. The LLVPs are often interpreted as intrinsically dense heterogeneities that are compositionally distinct from the surrounding mantle. Here we show that LLVPs may represent buried relics of Theia mantle material (TMM) that was preserved in proto-Earth’s mantle after the Moon-forming giant impact. Our canonical giant-impact simulations show that a fraction of Theia’s mantle could have been delivered to proto-Earth’s solid lower mantle. We find that TMM is intrinsically 2.0–3.5% denser than proto-Earth’s mantle based on models of Theia’s mantle and the observed higher FeO content of the Moon. Our mantle convection models show that dense TMM blobs with a size of tens of kilometres after the impact can later sink and accumulate into LLVP-like thermochemical piles atop Earth’s core and survive to the present day. The LLVPs may, thus, be a natural consequence of the Moon-forming giant impact. Because giant impacts are common at the end stages of planet accretion, similar mantle heterogeneities caused by impacts may also exist in the interiors of other planetary bodies.
https://www.nature.com/articles/s41586-023-06589-1
There is also an article on the subject here:
Scientists say they’ve finally found remnants of Theia, an ancient planet that collided with Earth to form the moon
JACKIE WATTLES CNN
Figure 3 … the anomalies viewed (a) from the North pole and (b) from the South pole. These plots emphasize the larger size of the African anomalies compared to the Pacific anomalies. Surface topography is projected onto the CMB for reference. See also the Supporting Information.
https://www.aol.com/news/collision-forme...16923.html
Qian Yuan, Mingming Li, Steven J. Desch, Byeongkwan Ko, Hongping Deng,
Edward J. Garnero, Travis S. J. Gabriel, Jacob A. Kegerreis, Yoshinori Miyazaki, Vincent Eke & Paul D. Asimow
Abstract
Seismic images of Earth’s interior have revealed two continent-sized anomalies with low seismic velocities, known as the large low-velocity provinces (LLVPs), in the lowermost mantle. The LLVPs are often interpreted as intrinsically dense heterogeneities that are compositionally distinct from the surrounding mantle. Here we show that LLVPs may represent buried relics of Theia mantle material (TMM) that was preserved in proto-Earth’s mantle after the Moon-forming giant impact. Our canonical giant-impact simulations show that a fraction of Theia’s mantle could have been delivered to proto-Earth’s solid lower mantle. We find that TMM is intrinsically 2.0–3.5% denser than proto-Earth’s mantle based on models of Theia’s mantle and the observed higher FeO content of the Moon. Our mantle convection models show that dense TMM blobs with a size of tens of kilometres after the impact can later sink and accumulate into LLVP-like thermochemical piles atop Earth’s core and survive to the present day. The LLVPs may, thus, be a natural consequence of the Moon-forming giant impact. Because giant impacts are common at the end stages of planet accretion, similar mantle heterogeneities caused by impacts may also exist in the interiors of other planetary bodies.
https://www.nature.com/articles/s41586-023-06589-1
There is also an article on the subject here:
Scientists say they’ve finally found remnants of Theia, an ancient planet that collided with Earth to form the moon
JACKIE WATTLES CNN
Figure 3 … the anomalies viewed (a) from the North pole and (b) from the South pole. These plots emphasize the larger size of the African anomalies compared to the Pacific anomalies. Surface topography is projected onto the CMB for reference. See also the Supporting Information.
https://www.aol.com/news/collision-forme...16923.html
Paper Trail: 42% English, 31.5% Scottish, 12.5% Irish, 6.25% German, 6.25% Sicilian & 1.5% French.
LDNA©: Britain & Ireland: 89.3% (51.5% English, 37.8% Scottish & Irish), N.W. Germanic: 7.8%, Europe South: 2.9% (Southern Italy & Sicily)
BigY 700: I1-Z141 >F2642 >Y3649 >Y7198 (c.349 AD) >Y168300 (c.385 AD) >A13248 (c.867 AD) >A13252 (c.1046 AD) >FT81015 (c.1277 AD) >A13243 (c.1620 AD) >FT80854 (c.1700 AD) >FT80630 (1893 AD).
LDNA©: Britain & Ireland: 89.3% (51.5% English, 37.8% Scottish & Irish), N.W. Germanic: 7.8%, Europe South: 2.9% (Southern Italy & Sicily)
BigY 700: I1-Z141 >F2642 >Y3649 >Y7198 (c.349 AD) >Y168300 (c.385 AD) >A13248 (c.867 AD) >A13252 (c.1046 AD) >FT81015 (c.1277 AD) >A13243 (c.1620 AD) >FT80854 (c.1700 AD) >FT80630 (1893 AD).