Comet science: Rosetta and beyond

彗星科学：罗塞塔及其他

• 批准号: ST/L004569/2
• 负责人: Colin Snodgrass
• 金额: $ 9.43万
• 依托单位: University of Edinburgh
• 依托单位国家: 英国
• 项目类别: Fellowship
• 财政年份: 2018
• 资助国家: 英国
• 起止时间: 2018 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FL004569%2F2
• 关键词: Comet; science; Rosetta; beyond

Comets have fascinated, and terrified, people throughout recorded history. The unpredictable appearances of bright comets, even in times when the motions of the "wandering stars" (planets) were well understood, meant that they were treated with suspicion. Today, our knowledge of comets has come a long way, but there are still many puzzles left to solve. As I write this, telescopes and spacecraft scattered all over the solar system are tracking comet ISON as it plunges toward the Sun, but we still cannot predict whether it will light up the sky as a "Great comet" or fizzle out before it arrives.Nowadays we are interested in comets not as harbingers of doom, but because we can use them to learn about the disc of rock and ice that formed the planets. Comets and asteroids are the leftover "building blocks" from the early days of the solar system; the survivors that didn't get incorporated into one of the planets, crash into the Sun, or get thrown out of the system altogether. The next few years will be an exciting time in cometary science, as the ESA mission "Rosetta" will be exploring comet 67P/Churyumov-Gerasimenko in great detail. This audacious mission will, for the first time ever, rendezvous with a comet and follow it on its orbit around the Sun. Its array of scientific instruments will watch as the activity of the comet evolves. This mission will not only get closer to a comet than any previous spacecraft (down to only a few km from the surface, flying deep within jets of gas and dust), and be the first to spend an extended period of time watching changes on the comet; it will also land a probe on the surface, to find out exactly what the comet is made of.I will work on the data that will be returned by Rosetta, especially through the camera system OSIRIS, and also by parallel ground-based observations of the comet. Such ground-based context observations are of critical importance: While the spacecraft will return very detailed information about the nucleus and inner coma of one particular comet, we need to be able to see how these details correspond to the large-scale activity that can be observed with telescopes in order to relate this to comets in general. I am coordinating a campaign of observations from telescopes worldwide. This will include a significant contribution from amateur astronomers, and from UK schools via the Faulkes Telescope project, when the comet is bright enough. Together, these data will reveal how cometary activity works.In addition to 67P, I will also observe other comets for comparison. These will include those of the same class, the short-period "Jupiter family" comets, and also other types such as main belt and long-period comets, including comet ISON. The interaction between the Sun and comets like ISON, which get very close to the solar surface, not only tells us about how highly active comets behave under extreme heating conditions, but can also reveal new information about the Sun itself and the environment around it. Main belt comets are at the other end of the cometary activity scale: They are a recently discovered missing link between icy comets and rocky asteroids, with asteroid-like orbits but weak comet-like activity. They are also a potential source of Earth's water: It is much easier to have delivered water from the outer asteroid belt to the early Earth than it is to account for all of it from the impact of "normal" comets. My work will look at the differences in the activity of the three classes of comet (high-activity near-Sun comets, medium-activity Jupiter family comets, and low-activity main belt comets), and the question of whether the variation is due to the different source regions they come from, or due to the environment in which they are active now. This "nature vs. nurture" question for comets will provide clues about the properties of different areas of the planet-forming disc, and the evolution of icy bodies over the age of the solar system.

纵观历史，彗星既让人着迷，也让人恐惧。明亮的彗星的不可预测的出现，即使是在“流浪恒星”（行星）的运动被很好地理解的时候，也意味着它们被怀疑。今天，我们对彗星的了解已经有了很大的进展，但仍有许多谜题有待解决。就在我写这篇文章的时候，散布在太阳系各处的望远镜和航天器都在追踪彗星ISON向太阳俯冲的轨迹，但我们仍然无法预测它是会作为一颗“大彗星”照亮天空，还是在它到来之前就消失了。如今，我们对彗星感兴趣，不是因为它是末日的预兆，而是因为我们可以利用它们来了解形成行星的岩石和冰盘。彗星和小行星是太阳系早期遗留下来的“积木”；那些没有被合并到其中一颗行星上，没有撞向太阳，或者被完全扔出太阳系的幸存者。未来几年将是彗星科学的激动人心的时刻，因为欧洲航天局的“罗塞塔”任务将对67P/丘留莫夫-格拉西门科彗星进行详细探索。这一大胆的任务将是有史以来第一次与一颗彗星会合，并跟踪它绕太阳运行的轨道。它的一系列科学仪器将观察彗星的活动演变。这次任务不仅将比以往任何航天器都更接近彗星（距离彗星表面只有几公里，在气体和尘埃喷流的深处飞行），而且是第一个花更长的时间观察彗星变化的航天器；它还将在彗星表面着陆一个探测器，以找出彗星的确切成分。我将处理罗塞塔号传回的数据，尤其是通过OSIRIS相机系统传回的数据，以及对彗星的平行地面观测数据。这种基于地面的背景观测是至关重要的：虽然航天器将返回关于一颗特定彗星的核心和内部彗发的非常详细的信息，但我们需要能够看到这些细节如何与望远镜可以观察到的大规模活动相对应，以便将其与彗星联系起来。我正在协调一项全球望远镜观测活动。这将包括业余天文学家的重要贡献，以及英国学校通过福克斯望远镜项目，当彗星足够亮的时候。总之，这些数据将揭示彗星活动是如何运作的。除了67P，我还会观察其他彗星进行比较。这将包括那些同类型的，短周期的“木星家族”彗星，以及其他类型的，如主带彗星和长周期彗星，包括ISON彗星。太阳和像ISON这样的彗星之间的相互作用，非常接近太阳表面，不仅告诉我们高度活跃的彗星在极端加热条件下的行为，而且还可以揭示关于太阳本身及其周围环境的新信息。主带彗星处于彗星活动规模的另一端：它们是最近发现的冰彗星和岩石小行星之间缺失的一环，具有类似小行星的轨道，但类似彗星的活动较弱。它们也是地球水的潜在来源：将水从外层小行星带输送到早期的地球要比从“正常”彗星的撞击中解释所有的水容易得多。我的工作将着眼于三类彗星（高活动的近太阳彗星、中等活动的木星家族彗星和低活动的主带彗星）活动的差异，以及这种变化是由于它们来自不同的来源区域，还是由于它们现在活动的环境。对于彗星来说，这个“先天vs后天”的问题将为我们提供有关行星形成盘不同区域特性的线索，以及太阳系中冰体的演化。

项目成果

Phase-curve analysis of comet 67P/Churyumov-Gerasimenko at small phase angles

67P/Churyumov-Gerasimenko 彗星小相位角下的相位曲线分析

• DOI: 10.1051/0004-6361/201834845
• 发表时间: 2019
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Masoumzadeh N

Monitoring of the optical spectrum of comet 2I/Borisov at the VLT

在 VLT 上监测 2I/鲍里索夫彗星的光谱

• DOI: 10.5194/epsc2020-653
• 发表时间: 2020
• 作者: Jehin E

Properties of the Bare Nucleus of Comet 96P/Machholz 1

96P/Machholz 1 彗星裸核的性质

• DOI: 10.3847/1538-3881/ab0f42
• 发表时间: 2019
• 期刊: The Astronomical Journal
• 作者: Eisner N

Detection of CN Gas in Interstellar Object 2I/Borisov

• DOI: 10.3847/2041-8213/ab49fc
• 发表时间: 2019-11-01
• 期刊: ASTROPHYSICAL JOURNAL LETTERS
• 影响因子: 7.9
• 作者: Fitzsimmons, Alan;Hainaut, Olivier;Snodgrass, Colin
• 通讯作者: Snodgrass, Colin

Physical modelling of YORP-evolved NEA (23187) 2000 PN9 from optical and radar observations

根据光学和雷达观测对 YORP 演化的 NEA (23187) 2000 PN9 进行物理建模

• DOI: 10.5194/epsc2020-825
• 发表时间: 2020
• 作者: Dover L