Comprehensive Study of the Most Pristine Objects Known in the Outer Solar System

太阳系中形成的距离太阳最远的天体保持在这些位置，也是自形成以来在较长时间内变化最小的天体。他们可能仍然保留着太阳系形成时的条件的线索。这些情况也可能出现在其他行星系统中。这些天文学家将在研究期间观察其中约50个天体，以了解这些天体的特征，包括它们的形状、自转速度、颜色，以及两个天体是否形成得足够近，可以相互触摸。亚利桑那州和智利的望远镜将用于这项研究。这个项目服务于国家利益，因为它增加了我们对太阳系中最原始物体的科学知识。首席研究人员的家乡机构洛厄尔天文台将把结果包括在他们的公共推广计划中，该计划每年覆盖超过10万人。研究人员将对动态冷经典(CC)跨海王星天体(TNO)进行全面的观测研究，以了解它们的形成、演化、组成和旋转性质。他们将为天体测量、光曲线、颜色和双星物体研究建立一个广泛的可见光图像数据集。这些数据将被用来追踪这个原始种群的形成和演化。他们将定期使用4.3米的探索频道望远镜和6.5米的麦哲伦望远镜，并计划在感兴趣的目标情况下包括几个NOAO设施。所有大小范围内视觉星等高达23.5-24毫克的冷经典物体将成为目标，优先考虑可能接触双星的物体。研究人员计划每年确定15-20个CCS的特征，在项目结束时产生大约50个对象的样本。通过研究太阳系中这些最原始的天体，研究人员将确定对理解整个TNO种群至关重要的原始约束，进而确定我们自己的太阳系和其他行星系统的形成和演化。研究结果将被纳入洛厄尔天文台的外展项目，包括每年接待约10万名游客的游客中心，以及“会见天文学家”和“纳瓦霍-霍皮人外展”项目。

The Solar System objects that formed farthest away from the Sun and remained in these locations are also the objects least changed over the long period of time since they were formed. They likely still keep clues to the conditions at the time of the formation of the Solar System. These conditions could also be present in other planetary systems. These astronomers will observe about 50 of these objects over the life of the study to learn about the characteristics of the objects, including their shape, the rate they spin, their coloring, and whether two objects formed close enough to touch each other. Telescopes in Arizona and Chile will be used in the study. This project serves the national interest as it increases our scientific knowledge about the most pristine objects in the Solar System. The Principal Investigator's home institution, Lowell Observatory, will include the results in their public outreach programs, which reach well over 100,000 people per year.The investigators will conduct a comprehensive observational study of the dynamically Cold Classical (CC) trans-Neptunian objects (TNOs) to understand their formation, evolution, composition, and rotational properties. They will build an extensive data set of visible images for astrometry, lightcurve, color, and binary object study. These data will be used as tracers of the formation and evolution of this pristine population. They will regularly use the 4.3-m Discovery Channel Telescope and the 6.5-m Magellan Telescope and plan to include several NOAO facilities in case of interesting targets. Cold Classical objects with a visual magnitude up to 23.5 - 24 mag in all size ranges will be targeted, with priority given to objects that are potentially contact binaries. The investigators plan to characterize 15 - 20 CCs per year, resulting in a sample of about 50 objects at the end of the project. By studying these most pristine objects in the Solar System, the investigators will determine primordial constraints crucially needed to understand the entire TNO population, and, by extension, the formation and evolution of both our own Solar System and other planetary systems. Results from the research will be incorporated into Lowell Observatory outreach programs including the visitor center which receives about 100,000 visitors every year, as well as the "Meet An Astronomer" and the "Navajo-Hopi outreach" programs.