Martian meteorite launch: high-speed ejecta from small craters.
نویسندگان
چکیده
We performed high-resolution computer simulations of impacts into homogeneous and layered martian terrain analogs to try to account for the ages and characteristics of the martian meteorite collection found on Earth. We found that craters as small as approximately 3 kilometers can eject approximately 10(7) decimeter-sized fragments from Mars, which is enough to expect those fragments to appear in the terrestrial collection. This minimum crater diameter is at least four times smaller than previous estimates and depends on the physical composition of the target material. Terrain covered by a weak layer such as an impact-generated regolith requires larger, therefore rarer, impacts to eject meteorites. Because older terrain is more likely to be mantled with such material, we estimate that the martian meteorites will be biased toward younger ages, which is consistent with the meteorite collection.
منابع مشابه
Transfer of mercurian impact ejecta to Earth and implications for mercurian meteorites
Introduction: The existence of lunar and especially martian meteorites in our collections proves that escape from the gravitational well of Mercury (with escape speed of about 4.2 km/sec, less than that of Mars) should be possible, presumably via impact of asteroids or comets into the mercurian surface. Once impact ejecta is liberated from Mercury, it finds itself in orbit around the Sun. What ...
متن کاملRole of Volatiles in the Emplacement of Ejecta Deposits around Martian Impact Craters
Introduction: Impact craters are a dominant geological landform on Mars, the most Earth-like planet in the Solar System. The martian impact cratering record is more diverse than for Earth and the other terrestrial planets [e.g., 1]. Of particular interest is the presence of multiple layers of lobate or fluidized proximal ejecta deposits surrounding martian impact craters. These are collectively...
متن کاملMartian Impact Craters: the Normal and the Unusual
Introduction: Our group has conducted a number of studies investigating the characteristics of martian impact craters. Many of these studies have provided insights into the normal characteristics of martian impact craters, such as their ejecta extents, ratio of central pit diameters to crater diameters, and the distributions of specific ejecta and interior morphologies. Other characteristics ar...
متن کاملQuantifying the Amount of Impact Ejecta at the Mer Landing Sites and Potential Paleolakes in the Southern Martian Highlands
Introduction: Martian paleolakes have been offered as landing sites for in situ and sample-return missions because of their high probability of containing climatic and hydrologic records and potential biomarkers. Prospective paleolake sites are identified in closed craters primarily based on discrepancies between the craters' expected and measured depths and interpretation of associated fluvial...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید
ثبت ناماگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید
ورودعنوان ژورنال:
- Science
دوره 298 5599 شماره
صفحات -
تاریخ انتشار 2002