Discovery Announcement of Binary System 2020 BX12

Series of range-Doppler radar images of 2020 BX12 observed February 4, 2020.

Discovery Announcement of Binary System 2020 BX12

Arecibo, Puerto Rico - February 10th, 2020

Radar images obtained by the Arecibo Observatory on the 4th and 5th of February revealed that near-Earth asteroid 2020 BX12 is a binary asteroid. The detection of a satellite was made during the first planetary radar observations conducted at the observatory following a month-long shutdown of telescope operations caused by a series of earthquakes striking the southern part of the island of Puerto Rico. The primary asteroid was discovered on the 27th of January by the ATLAS survey on Mauna Loa in Hawaii and fits the definition of a potentially hazardous asteroid (PHA) due to its size and minimum orbit intersection distance (MOID) of 302,000 km (188,000 miles) from the Earth. While this means it could conceivably come closer to the Earth than the Moon, 2020 BX12 poses no danger at this time and is currently receding from Earth.

The Arecibo delay-Doppler radar images (2380 MHz, 12.6 cm) showing the asteroid and its satellite have a resolution of 7.5 meters/pixel in the vertical dimension and 0.075 Hz/pixel in the horizontal dimension (~5 mm/s). Preliminary analysis suggests that the primary asteroid is a round object at least 165 meters in diameter rotating approximately once every 2.8 hours or less. The satellite has a diameter of approximately 70 meters and rotates once every 49 hours or less. The distance between the two bodies is at least 360 m, as observed on February 5th. The movement of the satellite between the two observations, which were made ~23 hours apart, suggests a mutual orbital period of 45-50 hours and would be consistent with a tidally locked satellite. Due to projection effects, uncertainties remain on the rotation periods, and a shorter mutual orbital period of 15-16 hours has not yet been ruled out.

Range-Doppler radar images of binary near-Earth asteroid 2020 BX12 with range resolution of 7.5 m/pixel (vertical axis) and Doppler frequency resolution of 0.075 Hz/pixel (horizontal axis).

The secondary appears brighter than the primary body in the radar images, which is common for radar images of binaries. The horizontal axis in delay-Doppler images shows, in fact, the echo power per Doppler-shifted frequency, or in other words the surface area that has a specific radial velocity relative to the observer. This makes objects that rotate slower appear narrower in delay-Doppler images than objects that rotate faster. Because the secondary body rotates much slower than the primary, its echo power is distributed to fewer Doppler frequency bins than the echo power from the primary body, making the amount of echo power per pixel appear more intense.

The initial detection of the satellite was made during radar observations on 4 February 2020 conducted by Luisa Fernanda Zambrano-Marín, Sean Marshall, Anne Virkki, Dylan Hickson, Anna McGilvray, Johbany Lebron, and Israel Cabrera of the Arecibo Observatory (University of Central Florida/Yang Enterprises, Inc.).

The Arecibo Planetary Radar program and ATLAS are projects of the Near-Earth Object Observations Program in NASA’s Planetary Defense Coordination Office.

Dr. Tracy M. Becker, Technical Contact
Ricardo Correa, Arecibo Media Contact
Dr. Anne Virkki, Group Lead for Arecibo Planetary Radar

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