尼古拉·叶夫多基莫夫(1868-1941):哈尔科夫天文台天体测量学研究的创始人

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2022-05-18 DOI:10.3103/S0884591322020027
M. A. Balyshev
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引用次数: 1

摘要

本文分析了乌克兰天文学家、天体测量专家尼古拉·叶夫多基莫夫所做的科学研究。这位天文学家的主要工作是用Repsold子午线圆来确定恒星的视差,黄道带和微弱的环极恒星的位置,以及大行星的位置。在哈尔科夫天文台,叶夫多基莫夫对下列物体和现象进行了系统的观测:日蚀和月食,包括在1914年和1936年日全食期间作为天文台的考察成员;彗星(哈雷彗星、德拉万彗星、斯特恩彗星、庞斯-温内克彗星);还有流星雨。他参与了确定小行星厄洛斯的参考恒星位置的工作。他对子午线圆进行了系统的研究,开发了新的天文仪器,在天文台组织了计时服务的运作,并通过桑德斯-雷蒙德法(使用子午线圆和凌日仪)测量了恒星对天顶距离的和和差,从而确定了恒星赤纬。
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Mykola Evdokymov (1868–1941): Founder of Astrometric Research at Kharkiv Astronomical Observatory

An analysis is presented of the scientific research accomplished by Ukrainian astronomer Mykola Evdokymov, a specialist in the field of astrometry. The astronomer’s main works, carried out using a Repsold meridian circle, are dedicated to determining stellar parallaxes, the positions of zodiacal and faint circumpolar stars, and the positions of large planets. At Kharkiv Astronomical Observatory, Evdokymov conducted systematic observations of the following objects and phenomena: solar and lunar eclipses, including as a member of the observatory’s expeditions during the total solar eclipses of 1914 and 1936; comets (Halley, Delavan, Stearns, Pons–Winnecke); and meteor showers. He participated in determining the positions of reference stars for the asteroid (433) Eros. He conducted systematic studies of the meridian circle, developed new astronomical instruments, organized the functioning of a time service at the observatory, and carried out the determination of star declinations by measuring the sums and differences of the zenith distances of star pairs by the Sanders–Raymond method (using a meridian circle and a transit instrument).

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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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