Understanding the birth of new elements by observing dying stars

我们周围的一切几乎都是由恒星内部产生的元素组成的。该项目旨在通过研究类太阳恒星在其生命的最后阶段之一喷射出的新物质来了解元素的起源。该项目预计将通过使用最先进的望远镜测量这些恒星产生的元素和同位素，并将其与理论模型预测进行比较，从而在恒星演化领域产生新的知识。预期成果包括更好地理解元素的产生、星系的化学富集以及中等质量恒星的首次质量估计。这将通过解决天文学中一个关键的悬而未决的问题而带来巨大的好处。

Almost everything around us is made up of elements that were created inside stars. This project aims to understand the origin of the elements by studying newly created material ejected by Sun-like stars during one of the final stages of their lives. This project expects to generate new knowledge in the field of stellar evolution by using state-of-the-art telescopes to measure the elements and isotopes produced by these stars and comparing them with theoretical model predictions. Expected outcomes include a better understanding of element creation, the chemical enrichment of galaxies, and the first mass estimates for intermediate-mass stars. This should provide significant benefits by addressing a key outstanding question in astronomy.