scholarly journals Untying microscopic Gordian knots: The granular (zircon) details of impact basins

Geology ◽  
2019 ◽  
Vol 47 (8) ◽  
pp. 799-800
Author(s):  
Aaron J. Cavosie
Keyword(s):  
1982 ◽  
Vol 87 (B5) ◽  
pp. 3975 ◽  
Author(s):  
Sean C. Solomon ◽  
Robert P. Comer ◽  
James W. Head

Science ◽  
2010 ◽  
Vol 330 (6010) ◽  
pp. 1527-1530 ◽  
Author(s):  
William F. Bottke ◽  
Richard J. Walker ◽  
James M. D. Day ◽  
David Nesvorny ◽  
Linda Elkins-Tanton

Core formation should have stripped the terrestrial, lunar, and martian mantles of highly siderophile elements (HSEs). Instead, each world has disparate, yet elevated HSE abundances. Late accretion may offer a solution, provided that ≥0.5% Earth masses of broadly chondritic planetesimals reach Earth’s mantle and that ~10 and ~1200 times less mass goes to Mars and the Moon, respectively. We show that leftover planetesimal populations dominated by massive projectiles can explain these additions, with our inferred size distribution matching those derived from the inner asteroid belt, ancient martian impact basins, and planetary accretion models. The largest late terrestrial impactors, at 2500 to 3000 kilometers in diameter, potentially modified Earth’s obliquity by ~10°, whereas those for the Moon, at ~250 to 300 kilometers, may have delivered water to its mantle.


2010 ◽  
Vol 3 (8) ◽  
pp. 533-536 ◽  
Author(s):  
Satoru Yamamoto ◽  
Ryosuke Nakamura ◽  
Tsuneo Matsunaga ◽  
Yoshiko Ogawa ◽  
Yoshiaki Ishihara ◽  
...  

2003 ◽  
Vol 38 (4) ◽  
pp. 565-578 ◽  
Author(s):  
J. S. Halekas ◽  
R. P. Lin ◽  
D. L. Mitchell

1982 ◽  
Vol 87 (B9) ◽  
pp. 7763 ◽  
Author(s):  
Sean C. Solomon ◽  
Stuart K. Stephens ◽  
James W. Head

2017 ◽  
Vol 44 (20) ◽  
pp. 10,140-10,146 ◽  
Author(s):  
Katarina Miljković ◽  
Myriam Lemelin ◽  
Paul G. Lucey
Keyword(s):  

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