Ludwig von Struve (1858–1920): Development of Positional Astronomy at the Kharkiv Astronomical Observatory

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2021-10-13 DOI:10.3103/S0884591321050032
M. Balyshev
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引用次数: 2

Abstract

An overview is given of the research work by Prof. Gustav Wilhelm Ludwig von Struve (in Russian, Lyudvig Ottovich Struve), a representative of the world-famous Struve dynasty of scholars. His work pertains to astrometry, a subfield of positional astronomy, traditionally studied by the Struves. Ludwig von Struve’s works on lunar eclipses and binary stars (in particular, the systems of η Cassiopeia and Procyon), their proper motions and positional determinations, stand out for their extraordinary methodicalness and meticulous processing. The greatest value is attached to those works by Struve where he calculates (being one the first researchers to do so) the speed of rotation of the Milky Way, refines the constant of precession, and determines the coordinates of the solar apex. At the Kharkiv Astronomical Observatory, Struve determined the positions of reference stars for the asteroid Eros, carries out long-term observations of circumpolar stars, and contributed to compiling a catalog of 779 zodiacal stars. He also organized an expedition of Kharkiv astronomers to observe the total solar eclipse of 1914. Struve’s works have been distinguished twice by the Russian Astronomical Society.

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路德维希·冯·斯特鲁夫(1858-1920):哈尔科夫天文台位置天文学的发展
本文概述了世界著名的斯特鲁维王朝学者代表古斯塔夫·威廉·路德维希·冯·斯特鲁维教授的研究工作。他的工作涉及天体测量学,这是位置天文学的一个分支,传统上由斯特鲁夫夫妇研究。路德维希·冯·斯特鲁夫关于月食和双星(特别是η仙后座和双星系统)的著作,它们的适当运动和位置决定,以其非凡的有条不紊和细致的处理而引人注目。最具价值的是斯特鲁夫的作品,他计算出了银河系的自转速度(他是第一批这样做的研究人员之一),精炼了进动常数,并确定了太阳顶点的坐标。在哈尔科夫天文台,斯特鲁夫为小行星厄洛斯确定了参考恒星的位置,对环极恒星进行了长期观测,并为编制779颗黄道带恒星的目录做出了贡献。他还组织了一支由哈尔科夫天文学家组成的探险队,观察1914年的日全食。斯特鲁夫的作品曾两次获得俄罗斯天文学会的认可。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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