Space astrometry with Gaia: Advances in understanding our Galaxy

IF 27.5 1区 物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY
Physics Reports Pub Date : 2026-01-01 Epub Date: 2025-10-22 DOI:10.1016/j.physrep.2025.09.004
Michael Perryman
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引用次数: 0

Abstract

Gaia is a satellite mission of the European Space Agency which is creating a catalogue of extremely accurate positions, distances and space motions of two billion stars in our Galaxy, along with more than one hundred thousand solar system asteroids, and several million distant quasars, all on the same extragalactic reference system. Complementary information on each object’s multi-epoch photometry and spectra provides a vast and unprecedented data base of (model-dependent) fundamental physical quantities, such as each star’s mass, age, and chemical composition. I outline the field’s historical context, and explain the key principles involved in these space measurements. This is followed by a broad review of the many areas of solar system science, stellar structure and evolution, and topics in Galactic structure, evolution, and dynamics, that are being derived from these data.
盖亚的空间天体测量:了解银河系的进展
盖亚是欧洲航天局的一项卫星任务,它正在创建一个目录,其中包含我们银河系中20亿颗恒星的极其精确的位置、距离和空间运动,以及10万多颗太阳系小行星和数百万颗遥远的类星体,所有这些都在同一个星系外参考系统中。每个天体的多历元光度和光谱的补充信息提供了一个巨大的、前所未有的(依赖于模型的)基本物理量的数据库,比如每颗恒星的质量、年龄和化学成分。我概述了该领域的历史背景,并解释了这些空间测量所涉及的关键原则。接下来是对太阳系科学,恒星结构和演化的许多领域的广泛回顾,以及银河系结构,演化和动力学的主题,这些都是从这些数据中得出的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Reports
Physics Reports 物理-物理:综合
CiteScore
56.10
自引率
0.70%
发文量
102
审稿时长
9.1 weeks
期刊介绍: Physics Reports keeps the active physicist up-to-date on developments in a wide range of topics by publishing timely reviews which are more extensive than just literature surveys but normally less than a full monograph. Each report deals with one specific subject and is generally published in a separate volume. These reviews are specialist in nature but contain enough introductory material to make the main points intelligible to a non-specialist. The reader will not only be able to distinguish important developments and trends in physics but will also find a sufficient number of references to the original literature.
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