Planetary Science at the University of Kent

肯特小组专注于彗星、小行星、宇宙尘埃和撞击事件的研究，这样我们就可以更好地了解整个太阳系物质的起源、演化和分布。我们特别感兴趣的是：-复杂的有机材料--它们是如何进化的，它们是如何演变到今天的位置的；-彗星和小行星的内容和物理性质(它们是什么，它们的行为如何，它们是如何进化的)；-太阳光如何影响小行星等小型天体的物理性质和动力学；-各种大小的撞击事件(从小的尘埃撞击到可能损坏甚至分裂由岩石或冰组成的天体的更大撞击)；-寻找新的方法来收集到达地球表面的宇宙尘埃。我们将通过以下方式解决这些领域：在我们的撞击实验室进行实验，通过计算机模型研究撞击过程，使用来自太空任务、望远镜观测和建模的数据，研究来自太空任务的材料，研究我们正部署在世界偏远地区如中太平洋和南极的尘埃捕获仪器收集的样本。我们的实验工作包括在实验室创造我们自己的非常高速的撞击。然后，我们检查和分析受影响的材料，看看它们是否被更改过。我们的目标是确定我们发射的有机和矿物材料是否/如何转移到它们所影响的目标。我们的目标也是看看在撞击事件中，有机材料是否可以改变为更复杂的分子，成为生命的先驱。这将涉及到研究目标和上升到落点以上的羽流。目标也可能在撞击过程中解体。我们一般都知道这对可靠的目标是如何起作用的。但太阳系中有一些天体的表面覆盖着冰，覆盖在液态水的次表层海洋上。我们将在我们的实验室制造这样的物体，并用我们的枪撞击它们，看看它们是如何分解的。为了研究彗星，我们将检查NASA从太空中收集的81P/Wild 2彗星上的尘埃颗粒。我们将逐个颗粒地找出这颗彗星是由什么组成的，以及这些物质在形成彗星之前来自哪里。我们将在地球上搜寻来自太空的宇宙尘埃。它存在于我们周围的尘埃中，但当它从太空通过大气层落下时，它与我们自己来自地球的尘埃和人类的工业活动混合在一起，使得它很难识别。通过过滤器吸入空气，并在偏远地区(中太平洋或南极)进行这项工作，那里的大气干净，局部灰尘很少，我们将集中我们能找到的宇宙尘埃的数量。然后我们将研究这些样本，以更多地了解它们所来自的太阳系天体。我们还将观察太空中的小行星。YORP效应是小行星所经历的一种扭矩，主要是由太阳加热后其表面发出的热光子造成的。当这种情况发生时，小行星会经历微小的反冲效应，如果在任何给定的时刻，无数光子击中小行星的整个表面，这种效应可能会非常显著。YORP可以改变小行星的自转速度和自旋轴的方向，可能需要数百万年的时间。这一效应对太阳系天文学家来说至关重要，因为它可以解释小行星科学中观察到的许多现象。然而，尽管YORP效应很重要，但由于难以衡量其影响，只有少数情况下看到了YORP效应的作用。随着我们获得的新的望远镜数据，我们将在这一领域产生重大影响。我们的核心目标是在我们的小行星样本上实现更多的YORP探测，以进一步了解这一重要过程。这项研究还将为理论家提供实际测量数据，以校准他们的计算

The Kent group focusses on studies of comets, asteroids, cosmic dust and impact events so we can better understand the origin, evolution and distribution of material throughout the Solar System. We are particularly interested in:-complex organic materials - how they evolved and how they ended up where they are today;- the content and physical properties of comets and asteroids (what they are, how they behave and how they evolved);-how sun light influences the physical properties and dynamics of small bodies such as asteroids;-impact events at all sizes (from small dust impacts to larger impacts which can damage or even break apart bodies made of rock or ice);-finding new ways to collect cosmic dust arriving at the Earth's surface. We will address these areas by: performing experiments in our impact laboratory, studying impact processes through computer models, using data from space missions, telescope observations and modelling, studying materials from space missions and studying samples collected by dust capture instruments we are deploying in remote parts of the world such as the mid-Pacific and the Antarctic.Our experimental work involves creating our own very high speed impacts in the laboratory. We then examine and analyse the impacted materials to see if they have been altered. We aim to determine whether/how the organic and mineral materials that we fire transfer to targets they impact. We also aim to see if the organic materials can be changed during impact events into more complex molecules that are the precursors to life. This will involve studying both the targets and the plumes that rise above the impact point.The targets may also fall apart during impact. We generally know how this works for solid targets. But there are bodies in the Solar System which have ice covered surfaces, over a liquid water sub-surface ocean. We will make such objects in our laboratory and impact them in our gun to see how they break up. To study comets, we will examine dust grains collected in space by NASA from comet 81P/Wild 2. Grain by grain we will work out what the comet is made of and where these materials came from before they formed the comet. We will search here on Earth for cosmic dust from space. It is present in the dust around us, but as it falls from space through the atmosphere, it mixes with our own dust from Earth and mankind's industrial activities, making it hard to identify. By sucking air through filters, and doing this in remote places (mid-Pacific or the Antarctic) with clean atmospheres with little local dust, we will concentrate the amount of cosmic dust we can find. We will then study these samples to learn more about the Solar System bodies that they came from.We will also look at asteroids in space. The YORP effect is a torque experienced by small asteroids, and is caused mainly by thermal photons being emitted from their surfaces after being heated by the Sun. When this happens the asteroid experiences a tiny recoil effect, which can be significant if summed up over the entire surface with countless photons striking it at any given moment. YORP can modify how fast asteroids spin and the orientation of their spin-axis and can take millions of years. This effect is of fundamental importance to Solar System astronomers as it can explain many observed phenomena in asteroidal science. However, despite its importance, there have been only a few cases where the YORP effect has been seen in action, due to the difficulties in measuring the effect. With new telescope data we have obtained we will make significant impact in this field. Our core aim is to achieve additional YORP detections on our sample of small asteroids to further understand this important process. The study will also provide theoreticians with actual measurements to calibrate their calculations