Characteristics of small-sized space debris objects using Terskol observatory measurements

被引：2

作者：

Bakhtigaraev, N. S. ^{[1
]}

Levkina, P. A. ^{[1
]}

Rykhlova, L. V. ^{[1
]}

Chazov, V. V. ^{[2
]}

Sergeev, A. V. ^{[3
]}

Karpov, N. V. ^{[3
]}

机构：

[1] Russian Acad Sci, Inst Astron, Ul Pyatnitskaya 48, Moscow 119017, Russia

[2] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Skii Pr 13, Moscow 119991, Russia

[3] Natl Acad Sci, Int Ctr Astron & Medicoecol Res, Ul Akad Zabolotnoho 27, UA-03680 Kiev, Ukraine

来源：

KINEMATICS AND PHYSICS OF CELESTIAL BODIES | 2016年 / 32卷 / 05期

关键词：

D O I：

10.3103/S0884591316050056

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Zeiss-2000 telescope of the International Center for Astronomic and Medico-Ecological Research, National Academy of Sciences of Ukraine (Terskol observatory), with a 2-meter aperture is the largest optical instrument in Europe that is regularly used for investigating space debris in the vicinity of the geostationary orbit. One of the main objectives is to detect and characterize small fragments of space debris that are difficult to approach for other telescopes. During each photometric night, we usually detect four to five unknown fragments of 17th to 20th magnitude. This article provides orbital parameters and physical characteristics of several small-sized fragments of space debris that were detected during observations at Terskol observatory in 2014-2015.

引用

页码：233 / 236

页数：4

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