کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
8138592 1523559 2014 7 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Survival of water ice in Jupiter Trojans
ترجمه فارسی عنوان
زنده ماندن یخ آب در مشتری تروجان ها
کلمات کلیدی
سیارک های تروجان، دنباله دار تاریخچه حرارتی، ایسس،
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم فضا و نجوم
چکیده انگلیسی
Jupiter Trojans appear to be a key population of small bodies to study and test the models of the Solar System formation and evolution. Because understanding the evolution of Trojans can bring strong and unique constraints on the origins of our planetary system, a significant observational effort has been undertaken to unveil their physical characteristics. The data gathered so far are consistent with Trojans having volatile-rich interiors (possibly water ice) and volatile-poor surfaces (fine grained silicates). Since water ice is not thermodynamically stable against sublimation at the surface of an object located at ∼5 AU, such layering seems consistent with past outgassing. In this work, we study the thermal history of Trojans after the formation of a dust mantle by possible past outgassing, so as to constrain the depth at which water ice could be stable. We find that it could have survived 100 m below the surface, even if Trojans orbited close to the Sun for ∼10,000 years, as suggested by the most recent dynamical models. Water ice should be found ∼10 m below the surface in most cases, and below 10 cm in the polar regions in some cases.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Icarus - Volume 231, 1 March 2014, Pages 232-238
نویسندگان
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