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The Suborbital Particle Aggregation and Collision Experiment (SPACE): Studying the Collision Behavior of Submillimeter-Sized Dust Aggregates on the Suborbital Rocket Flight REXUS 12

机译:亚轨道粒子聚集和碰撞实验(spaCE):   亚毫米级粉尘聚集体碰撞行为的研究   亚轨道火箭飞行REXUs 12

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摘要

The Suborbital Particle Aggregation and Collision Experiment (SPACE) is anovel approach to study the collision properties of submillimeter-sized, highlyporous dust aggregates. The experiment was designed, built and carried out toincrease our knowledge about the processes dominating the first phase of planetformation. During this phase, the growth of planetary precursors occurs byagglomeration of micrometer-sized dust grains into aggregates of at leastmillimeters to centimeters in size. However, the formation of larger bodiesfrom the so-formed building blocks is not yet fully understood. Recentnumerical models on dust growth lack a particular support by experimentalstudies in the size range of submillimeters, because these particles arepredicted to collide at very gentle relative velocities of below 1 cm/s thatcan only be achieved in a reduced-gravity environment. The SPACE experiment investigates the collision behavior of an ensemble ofsilicate-dust aggregates inside several evacuated glass containers which arebeing agitated by a shaker to induce the desired collisions at chosenvelocities. The dust aggregates are being observed by a high-speed camera,allowing for the determination of the collision properties of theprotoplanetary dust analog material. The data obtained from the suborbitalflight with the REXUS (Rocket Experiments for University Students) 12 rocketwill be directly implemented into a state-of-the-art dust growth and collisionmodel.
机译:亚轨道粒子聚集与碰撞实验(SPACE)是研究亚毫米大小,高孔隙度尘埃聚集体碰撞特性的另一种方法。设计,建造和进行该实验是为了增加我们对主导行星形成第一阶段的过程的了解。在此阶段,行星前体的生长是通过将微米级的尘埃颗粒聚集成至少几毫米到几厘米大小的聚集体来实现的。然而,从如此形成的构造块形成更大的主体的方法尚未完全被理解。关于尘埃增长的最新数值模型在亚毫米大小范围内的实验研究中缺乏特别的支持,因为据预测这些颗粒将以低于1 cm / s的非常缓慢的相对速度碰撞,而这只能在重力降低的环境中才能实现。 SPACE实验研究了几个真空玻璃容器内一组硅酸盐-粉尘聚集体的碰撞行为,这些玻璃容器正被振荡器振动,以在选定的速度下引发所需的碰撞。高速照相机正在观察尘埃聚集物,从而可以确定原行星尘埃模拟材料的碰撞特性。使用REXUS(大学生火箭实验)12火箭从亚轨道飞行获得的数据将直接应用于最新的尘埃增长和碰撞模型。

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