کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1781490 1022283 2012 8 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Hydrocode simulations of the largest crater on asteroid Lutetia
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات فیزیک زمین (ژئو فیزیک)
پیش نمایش صفحه اول مقاله
Hydrocode simulations of the largest crater on asteroid Lutetia
چکیده انگلیسی

The flyby of the Main Belt asteroid Lutetia by the Rosetta spacecraft allows the camera OSIRIS to obtain very good images of about half of the body at the maximum resolution of 60 m per pixel. From the images and radio-science experiment, a density of about (3.4±0.3) g/cm3 has been inferred for the asteroid.Many impact craters have been observed on the surface of Lutetia and the largest, named Massilia, has a diameter of about 55 km. Relative to the size of Lutetia (the longest axis is approximately 126 km) the crater represents one of the dominating features on its surface. Whether or not the impact that formed Massilia affected the entire asteroid can be only evaluated via numerical modeling, with hydrocodes, of the impact process. The results of a suite of iSALE simulations are compared with the crater profile derived from the Digital Terrain Model of the observed surface. The best match to the DTM of the crater with hydrocode simulations has allowed to determine a value of 7.5 km for the impactor diameter, which suggests a primordial origin of Lutetia due to the low probability of such an impact event.A second interesting impact structure has been identified nearby Massilia within the North Pole Crater Cluster. The crater has a diameter of 24 km and it lies over a larger crater of the North Pole Crater Cluster. This is strongly suggestive of a very young structure on Lutetia. The numerical simulations of this feature constrain the impactor to be 3.8 km in diameter, assuming the same material properties for target and impactor as in the model of the formation of Massilia.


► Hydrocode iSALE simulations of the largest crater on the asteroid Lutetia.
► iSALE simulations of one component of the North Polar Crater Cluster having the diameter of 24 km.
► The largest crater of 55 km has been simulated with an impactor of 7.5 km and the 24 km with an impactor of 3.8 km.
► The hydrocode fit the two craters diameter/depth without assuming a crust.
► A pre-fracturated layer could have been created in the largest crater generation.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Planetary and Space Science - Volume 66, Issue 1, June 2012, Pages 147–154
نویسندگان
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