Skip to content
BY 4.0 license Open Access Published by De Gruyter Open Access October 22, 2020

Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2015–2018

  • Ireneusz Wlodarczyk EMAIL logo , Kazimieras Černis and Ilgmars Eglitis
From the journal Open Astronomy

Abstract

This paper is devoted to the discovery of 37 asteroids at the Baldone Astrophysical Observatory (MPC 069) from 2015 to 2018, and one of dynamically interesting Mars-crosser (MC) observed at the Baldone Astrophysical Observatory, namely 2008 LX16. In Baldone Observatory, was independently discovered the Near-Earth Object 2018 GE3 on the image of 13 April 2018. Also, the NEO 2006 VB14 was observed doing its astrometry and photometry. Moreover, we observed asteroids 1986 DA and 2014 LJ1. We computed orbits and analyzed the orbital evolution of these asteroids. 566 positions and photometric observations of NEO objects 345705 (2006 VB14) and 6178 (1986 DA) were obtained with Baldone Schmidt telescope in 2018 and 2019. We detected their rotation period and other physical characteristics. Also, a Fourier transform was applied to determine the rotation period of asteroid 6178 (1986 DA). Value (3.12 ± 0.02)h was obtained. Our observations confirm the previously obtained rotation periodP=3.25hfor2006VB14.

References

Chesley SR, Baer J, Monet DG. 2010. Treatment of star catalog biases in asteroid astrometric observations. Icar. 210(1):158–181.Search in Google Scholar

Chesley SR, Farnocchia D, Nolan MC, Vokrouhlický D, Chodas PW, Milani A, et al. 2014. Orbit and bulk density of the OSIRIS-REx target Asteroid (101955) Bennu. Icar. 235(5):5-22.Search in Google Scholar

Černis K, Wlodarczyk I, Eglitis I. 2015. Observational data and orbits of the asteroids discovered at the Baldone Observatory in 2008—2013. BaltA. (24): 251-262.10.1515/astro-2017-0226Search in Google Scholar

Eglitis I. 2019. Investigation of NEO asteroids 2006 VB14 and 1986 DA. OAP. 32(0):146–147.10.18524/1810-4215.2019.32.181826Search in Google Scholar

Farnocchia D, Chesley SR, Vokrouhlický D, Milani A, Spoto F, Bottke WF. 2013a. Near Earth Asteroids with measurable Yarkovsky effect. Icar. 224(1):1–13.10.1016/j.icarus.2013.02.004Search in Google Scholar

Farnocchia D, Chesley SR, Chodas PW, Micheli M, Tholen DJ, Milani A, et al. 2013b. Yarkovsky-driven impact risk analysis for asteroid (99942) Apophis. Icar. 224(1):192–200.10.1016/j.icarus.2013.02.020Search in Google Scholar

Farnocchia D, Chesley SR, Chamberlin AB, Tholen DJ. 2015. Star catalog position and proper motion corrections in asteroid astrometry. Icar. 245:94–111.10.1016/j.icarus.2014.07.033Search in Google Scholar

Levison HF, Duncan MJ. 1994. The Long-Term Dynamical Behavior of Short-Period Comets. Icar. 108(1):18–36.Search in Google Scholar

Milani A, Chesley SR, Sansaturio ME, Tommei G, Valsecchi GB. 2005a. Nonlinear impact monitoring: line of variation searches for impactors. Icar. 173(2):362–384.10.1016/j.icarus.2004.09.002Search in Google Scholar

Milani A, Sansaturio ME, Tommei G, Arratia O, Chesley SR. 2005b. Multiple solutions for asteroid orbits: Computational procedure and applications. A&A. 431:729-74610.1051/0004-6361:20041737Search in Google Scholar

Neslusan L., Svoren J., Porubcan V. 1998. A computer program for calculation of a theoretical meteor-stream radian. A&A. 331:411-413Search in Google Scholar

Skiff BA, Bowell E, Koehn BW, Sanborn JJ, McLelland KP, Warner BD. 2012. Lowell Observatory Near-Earth Asteroid Photometric Survey (NEAPS) - 2008 May through 2008 December. MPBu. 39:111–130.Search in Google Scholar

Vereš P, Farnocchia D, Chesley SR, Chamberlin AB. 2017. Statistical analysis of astrometric errors for the most productive asteroid surveys. Icar. 296:139–149.10.1016/j.icarus.2017.05.021Search in Google Scholar

Wlodarczyk I. 2015. The Potentially Hazardous Asteroid (410777) 2009 FD. AcA. 65:215–231.Search in Google Scholar

Wlodarczyk I. 2019a. Some parameters of selected NEAs. BlgAJ. 30: 44-59.10.5455/ajvs.1922Search in Google Scholar

Wlodarczyk, I. 2019b. The potentially hazardous NEA 2001 BB1. Open Astronomy. 28:180–190.10.1515/astro-2019-0016Search in Google Scholar

Received: 2020-01-01
Accepted: 2020-06-30
Published Online: 2020-10-22

© 2020 Ireneusz Wlodarczyk et al., published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

Downloaded on 26.4.2024 from https://www.degruyter.com/document/doi/10.1515/astro-2020-0017/html
Scroll to top button