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  • Orbital stability analysis ...
    Santana-Ros, T.; Micheli, M.; Faggioli, L.; Cennamo, R.; Devogèle, M.; Alvarez-Candal, A.; Oszkiewicz, D.; Ramírez, O.; Liu, P.-Y.; Benavidez, P. G.; Campo Bagatin, A.; Christensen, E. J.; Wainscoat, R. J.; Weryk, R.; Fraga, L.; Briceño, C.; Conversi, L.

    Nature communications, 02/2022, Volume: 13, Issue: 1
    Journal Article

    Abstract Trojan asteroids are small bodies orbiting around the L 4 or L 5 Lagrangian points of a Sun-planet system. Due to their peculiar orbits, they provide key constraints to the Solar System evolution models. Despite numerous dedicated observational efforts in the last decade, asteroid 2010 TK 7 has been the only known Earth Trojan thus far. Here we confirm that the recently discovered 2020 XL 5 is the second transient Earth Trojan known. To study its orbit, we used archival data from 2012 to 2019 and observed the object in 2021 from three ground-based observatories. Our study of its orbital stability shows that 2020 XL 5 will remain in L 4 for at least 4 000 years. With a photometric analysis we estimate its absolute magnitude to be $${H}_{r}=18.5{8}_{-0.15}^{+0.16}$$ H r = 18.5 8 − 0.15 + 0.16 , and color indices suggestive of a C-complex taxonomy. Assuming an albedo of 0.06 ± 0.03, we obtain a diameter of 1.18 ± 0.08 km, larger than the first known Earth Trojan asteroid.