Dozens of virtual impactor orbits eliminated by the EURONEAR VIMP DECam data mining project

¹ Isaac Newton Group of Telescopes, Apto. 321, 38700 Santa Cruz de la Palma, Canary Islands, Spain
e-mail: ovidiu.vaduvescu@gmail.com
² Instituto de Astrofisica de Canarias (IAC), C/Via Lactea s/n, 38205 La Laguna, Tenerife, Spain
³ University of Craiova, Str. A. I. Cuza nr. 13, 200585 Craiova, Romania
⁴ EURONEAR member, Brasov, Romania
⁵ Astronomical Institute of the Romanian Academy, 5 Cutitul de Argint, 040557 Bucharest, Romania
⁶ Astronomical Observatory Cluj-Napoca, Romanian Academy, 15 Ciresilor Street, 400487 Cluj-Napoca, Romania
⁷ Department of Physics, Babes-Bolyai University, Kogalniceanu Street, 400084 Cluj-Napoca, Romania
⁸ EURONEAR collaborator, Bucharest, Romania

Received: 15 June 2020
Accepted: 27 July 2020

Abstract

Context. Massive data mining of image archives observed with large etendue facilities represents a great opportunity for orbital amelioration of poorly known virtual impactor asteroids (VIs). There are more than 1000 VIs known today; most of them have very short observed arcs and many are considered lost as they became extremely faint soon after discovery.

Aims. We aim to improve the orbits of VIs and eliminate their status by data mining the existing image archives.

Methods. Within the European Near Earth Asteroids Research (EURONEAR) project, we developed the Virtual Impactor search using Mega-Precovery (VIMP) software, which is endowed with a very effective (fast and accurate) algorithm to predict apparitions of candidate pairs for subsequent guided human search. Considering a simple geometric model, the VIMP algorithm searches for any possible intersection in space and time between the positional uncertainty of any VI and the bounding sky projection of any image archive.

Results. We applied VIMP to mine the data of 451,914 Blanco/DECam images observed between 12 September 2012 and 11 July 2019, identifying 212 VIs that possibly fall into 1286 candidate images leading to either precovery or recovery events. Following a careful search of candidate images, we recovered and measured 54 VIs in 183 DECam images. About 4,000 impact orbits were eliminated from both lists, 27 VIs were removed from at least one list, while 14 objects were eliminated from both lists. The faintest detections were around V ∼ 24.0, while the majority fall between 21 <  V <  23. The minimal orbital intersection distances remains constant for 67% detections, increasing for eight objects and decreasing for ten objects. Most eliminated VIs (70%) had short initial arcs of less than five days. Some unexpected photometric discovery has emerged regarding the rotation period of 2018 DB, based on the close inspection of longer trailed VIs and the measurement of their fluxes along the trails.

Conclusions. Large etendue imaging archives represent great assets to search for serendipitous encounters of faint asteroids and VIs.