从空间碎片到近地天体,空间部门面临的一些重大挑战

G. Aglietti
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引用次数: 5

摘要

社会对空间资产的依赖已经发展到今天每个现代国家基础设施的一部分。空间技术提供的服务,例如全球导航卫星系统,对于从电信到运输到银行等各个部门的顺利运营至关重要(Hesse和Hornung, 2015年)。甚至一般公众也已经习惯使用卫星服务,如卫星电视或移动电话上的卫星导航。因此,对我们的空间资产的任何威胁都是一个非常重大的社会问题。截至2020年2月,太空中大约有5500颗卫星,但只有大约2300颗真正在运行,这意味着大约3200颗报废的卫星仍在绕地球轨道运行,其中包括火箭的上层和整流罩,以及由解体、爆炸、碰撞、退化或其他导致碎片产生的异常事件产生的各种较小物体。在空间碎片的统称下,这些物体的尺寸分布范围从大型完整物体(例如,尺寸大于10米,重量超过几吨的火箭或大型卫星的部件)到毫米大小的碎片,如油漆鳞片或冷却剂凝固液滴。2020年初的估计显示,超过10厘米的物体有3.4万个,大于1到10厘米的物体有90万个,大于1毫米到1厘米的物体有惊人的1.28亿个。鉴于它们的高速度和由此产生的高动能,即使是很小的碎片也会对正在运行的卫星构成重大威胁,因为它们可能给卫星造成灾难性后果,并可能丧失关键服务。与此同时,较大天体之间的高能碰撞可以产生真正的爆炸,产生数千个碎片。这些,反过来,可能会与其他轨道物体相撞,引发连锁反应和雪球效应,可能导致整个轨道无法使用。这种极端的情况(凯斯勒综合症),最初是由凯斯勒在70年代研究的(凯斯勒和courl - palais, 1978),离现实不远,因为已经发生了一些碰撞。也许最著名的是俄罗斯军用通信卫星Cosmos 2251与一颗铱星星座卫星之间的碰撞(Wang, 2010),这导致了碎片数量的逐步增加。随着越来越多的卫星应用正在开发,需要越来越多的卫星(例如,部署数百颗卫星的星座以提供全球连接或万维网),空间碎片问题变得越来越重要(Virgili et al., 2016)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
From Space Debris to NEO, Some of the Major Challenges for the Space Sector
Society’s reliance on space assets has grown to the point that today these are part of every modern country’s infrastructure. Services provided thanks to space technologies such as for example, Global Navigation Satellite Systems have become critical (Hesse and Hornung, 2015) for smooth operations in a variety of sectors, from telecommunications to transport to banking, and the list could continue. Even the general public has become accustomed to using satellite services like satellite television or the satnav on mobile phones. Hence, any threat to our space assets is a very significant issue for society. As of February 2020, there were about 5,500 satellites in space1 but only about 2,300 were actually functioning, which means about 3,200 defunct satellites are still orbiting Earth, together with upper stages and fairings of rockets and a variety of smaller objects produced by break-ups, explosions, collisions, degradation or other anomalous events that resulted in the production of fragments. Under the collective name of space debris, these objects have a size distribution that ranges from large intact bodies (e.g., parts of rockets or large satellites with a size larger than 10m and weight of several tons) down to millimeter-sized fragments like scales of paint or solidified droplets of coolant. Early 2020 estimates showed that there were 34,000 objects larger than 10 cm, 900,000 objects from >1 to 10 cm, and a staggering 128 million objects from >1mm to 1 cm. Given their high velocity and consequent high kinetic energy, even small pieces of debris pose a significant threat to operating satellites, as they could hit them with catastrophic consequences and the loss of potentially critical services. At the same time, high energy collisions between larger bodies can produce real explosions that can create thousands of fragments. These, in turn, can collide with other orbiting objects, triggering a chain reaction and a snowball effect that could render whole orbits unusable. This extreme scenario (Kessler Syndrome), initially studied by Kessler in the ’70s (Kessler and Cour-Palais, 1978), is not far from reality, as a handful of collisions have already happened. Perhaps the most famous is the one between Russian military communications satellite Cosmos 2,251 and a satellite of the Iridium constellation (Wang, 2010), which produced a step increase in the debris population. With more satellite applications currently being developed that demand a growing number of satellites (e.g., constellations of hundreds of satellites are being deployed to provide worldwide connectivity or a World Wide Web), the issue of space debris is becoming more significant (Virgili et al., 2016).
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