International audienceWhile major impacting bodies during accretion of a Mars type planet have very low velocities (<10 km/s), the characteristics of the shockwave propagation and, hence, the derived scaling laws are poorly known for these low velocity impacts. Here, we use iSALE-2D hydrocode simulations to calculate shock pressure and particle velocity in a Mars type body for impact velocities ranging from 4 to 10 km/s. Large impactors of 100–400 km in diameter, comparable to those impacted on Mars and created giant impact basins, are examined. To better represent the power law distribution of shock pressure and particle velocity as functions of distance from the impact site at the surface, we propose three distinct regions in the mantle: ...
We use scaling laws for impacts to estimate the differences in the effects on the interior of a plan...
New forms of empirical formulae that provide an approximate description of the decay of shock pressu...
Giant impacts have been suggested to explain various characteristics of terrestrial planets and thei...
International audienceWhile major impacting bodies during accretion of a Mars type planet have very ...
Co-auteur étrangerInternational audienceWhile major impacts during late accretion of a Mars type pla...
All planetary bodies with old surfaces exhibit planetary-scale impact craters: vast scars caused by ...
AbstractPlanetary impacts have shaped the surfaces and interiors of planets. They were particularly ...
We investigate the effects of planetary curvature and the crust-mantle boundary on the shock pressur...
Hypervelocity meteorite impacts on planets subject the target to very high shock pressures. The iso...
Abstract. Previous calculations indicate that the Earth suffered impacts from objects up to Mars siz...
International audienceThe accretion of the terrestrial planets from asteroid collisions and the deli...
Impact craters are numerous on planetary bodies and furnish important information about the composit...
[1] We investigate the direct thermal effects of giant impacts on the Martian core and its dynamo. S...
impactor with a given energy, s ize and composition into a given t a r g e t at a given gravi ty s t...
A geotechnical centrifuge was used to investigate large body impacts onto planetary surfaces. At ele...
We use scaling laws for impacts to estimate the differences in the effects on the interior of a plan...
New forms of empirical formulae that provide an approximate description of the decay of shock pressu...
Giant impacts have been suggested to explain various characteristics of terrestrial planets and thei...
International audienceWhile major impacting bodies during accretion of a Mars type planet have very ...
Co-auteur étrangerInternational audienceWhile major impacts during late accretion of a Mars type pla...
All planetary bodies with old surfaces exhibit planetary-scale impact craters: vast scars caused by ...
AbstractPlanetary impacts have shaped the surfaces and interiors of planets. They were particularly ...
We investigate the effects of planetary curvature and the crust-mantle boundary on the shock pressur...
Hypervelocity meteorite impacts on planets subject the target to very high shock pressures. The iso...
Abstract. Previous calculations indicate that the Earth suffered impacts from objects up to Mars siz...
International audienceThe accretion of the terrestrial planets from asteroid collisions and the deli...
Impact craters are numerous on planetary bodies and furnish important information about the composit...
[1] We investigate the direct thermal effects of giant impacts on the Martian core and its dynamo. S...
impactor with a given energy, s ize and composition into a given t a r g e t at a given gravi ty s t...
A geotechnical centrifuge was used to investigate large body impacts onto planetary surfaces. At ele...
We use scaling laws for impacts to estimate the differences in the effects on the interior of a plan...
New forms of empirical formulae that provide an approximate description of the decay of shock pressu...
Giant impacts have been suggested to explain various characteristics of terrestrial planets and thei...