2020 BX<sub>12</sub>—The Last Binary Asteroid Discovered at Arecibo

Abstract Radar observations of 2020 BX 12 conducted with the S -band planetary radar system (2380 MHz, 12.6 cm) at the Arecibo Observatory on 2020 February 4 and 5 revealed that this potentially hazardous asteroid is a binary system. Spectroscopic observations with the 10.4 m Gran Telescopio Canarias on 2024 February 16 indicate that 2020 BX 12 is an S-complex asteroid (Bus–DeMeo taxonomy). We present the results of shape modeling and orbit fitting based on the radar observations. The system consists of a primary of a diameter ∼205 m and a ∼50 m secondary revolving around their common center of mass. This size places the system among the smallest 10% of known binary asteroid systems. The orbital period of the system is &gt;40 hr. The semimajor axis is &gt;375 m. This binary system, like many other binary near-Earth asteroids, features a spheroidal primary spinning near the breakup point, indicating likely formation through spin-up and fission and migration from the main belt. 2020 BX 12 was the last binary asteroid discovered at Arecibo.

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Publication Details

Journal
The Planetary Science Journal
Published
2025-04-01
DOI
https://doi.org/10.3847/psj/adbe39
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00

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article

2020 BX12—The Last Binary Asteroid Discovered at Arecibo

S. Marshall, N. Pinilla-Alonso, Flaviane Venditti, E. S. Howell et al.
The Planetary Science Journal
Astro and Planetary Science
article

2020 BX12—The Last Binary Asteroid Discovered at Arecibo

S. Marshall, N. Pinilla-Alonso, Flaviane Venditti, E. S. Howell, Jon D. Giorgini, Luisa Fernanda Zambrano-Marin, J. de León, Anne Virkki
article en

Abstract

Abstract Radar observations of 2020 BX 12 conducted with the S -band planetary radar system (2380 MHz, 12.6 cm) at the Arecibo Observatory on 2020 February 4 and 5 revealed that this potentially hazardous asteroid is a binary system. Spectroscopic observations with the 10.4 m Gran Telescopio Canarias on 2024 February 16 indicate that 2020 BX 12 is an S-complex asteroid (Bus–DeMeo taxonomy). We present the results of shape modeling and orbit fitting based on the radar observations. The system consists of a primary of a diameter ∼205 m and a ∼50 m secondary revolving around their common center of mass. This size places the system among the smallest 10% of known binary asteroid systems. The orbital period of the system is &gt;40 hr. The semimajor axis is &gt;375 m. This binary system, like many other binary near-Earth asteroids, features a spheroidal primary spinning near the breakup point, indicating likely formation through spin-up and fission and migration from the main belt. 2020 BX 12 was the last binary asteroid discovered at Arecibo.

The Planetary Science JournalVol. 6(4)
University of Central Florida (US), Jet Propulsion Laboratory (US), University of Helsinki (FI), University of Arizona (US), Universidad de Oviedo (ES), Universidad de Granada (ES), Helsinki Institute of Physics (FI), Instituto de Astrofísica de Canarias (ES), Instituto Nacional de Silicosis (ES)
National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, University of Central Florida, Nuclear Safety and Security Commission, Universidad de Granada, Jet Propulsion Laboratory
Openalex Percentile: Top 95%
Astro and Planetary Science
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