Observations of small and low elongation near-Earth asteroids

1Vovk, VS, 1Kulichenko, MO, 1Kozyryev, ES, 1Sybiriakova, ES, 1Shulga, OV
1Research Institute "Mykolaiv Astronomical Observatory", Mykolaiv, Ukraine
Kinemat. fiz. nebesnyh tel (Online) 2015, 31(3):73-
Start Page: Positional and Theoretical Astronomy
Language: Russian
Abstract: 

We present some results of observations of small near Earth asteroids (NEAs) and NEAs observed in low solar elongation. All the results are obtained in the Research Institute «Nikolaev Astronomical Observatory» with the use of the combined observation method and time delay and integration operation mode of CCD.

Keywords: asteroid, Earth, solar elongation
References: 

1.E. S. Kozyrev, E. S. Sibiryakova, and A. V. Shul’ga, “Estimation of astrometric reduction accuracy for the combined method of celestial object observations,” Kosm. Nauka Tekhnol. 16(5), 71–76 (2010).

2.E. S. Sibiryakova, E. S. Kozyrev, and A. V. Shul’ga, “The results of coordinate observations of the asteroids approaching Earth using a combined method of observation,” Izv. Krym. Astrofiz. Obs. 109(1), 103–108 (2013).

3.A. V. Shul’ga, E. S. Kozyrev, E. S. Sibiryakova, et al., “The mobile telescope complex of RI MAO for observation of near-Earth space objects,” Kosm. Nauka Tekhnol. 18(4), 52–58 (2012).

4.D. Bancelin, D. Hestroffer, and W. Thuillot, “Near Earth Asteroids Astrometry with GAIA,” in Proc. Gaia Follow-up Network for Solar System Objects Workshop held at IMCCE-Paris Observatory, Paris, Nov. 29–Dec. 1, 2010 (Inst. de Mecanique Celeste et de Calcul des Ephemerides, Paris, 2010), pp. 47–50.

5.O. P. Popova, P. Jenniskens, Y. Emel’yanenko, et al., “Chelyabinsk airburst, damage assessment, meteorite recovery, and characterization,” Science 342(6162), 1069–1073 (2013).
https://doi.org/10.1126/science.1242642

6.O. Shulga, Y. Kozyryev, and Y. Sybiryakova, “Observation of NEO Having High Apparent Rates with Mobitel Telescope,” in Proc. Gaia Follow-up Network for Solar System Objects Workshop held at IMCCE-Paris Observatory, Paris, Nov. 29–Dec. 1, 2010 (Inst. de Mecanique Celeste et de Calcul des Ephemerides, Paris, 2010), pp. 97–100.