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Orbital stability analysis and photometric characterization of the second Earth Trojan asteroid 2020 XL5

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  • T. Santana-Ros

    (Universidad de Alicante, Carr. de San Vicente del Raspeig
    Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB))

  • M. Micheli

    (ESA NEO Coordination Centre)

  • L. Faggioli

    (ESA NEO Coordination Centre)

  • R. Cennamo

    (ESA NEO Coordination Centre)

  • M. Devogèle

    (Arecibo Observatory, University of Central Florida)

  • A. Alvarez-Candal

    (Instituto de Astrofísica de Andalucía, CSIC
    Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, San Vicente del Raspeig
    Observatório Nacional / MCTIC)

  • D. Oszkiewicz

    (Astronomical Observatory Institute, Faculty of Physics, A. Mickiewicz University)

  • O. Ramírez

    (Solenix Deutschland GmbH)

  • P.-Y. Liu

    (Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, San Vicente del Raspeig)

  • P. G. Benavidez

    (Universidad de Alicante, Carr. de San Vicente del Raspeig
    Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, San Vicente del Raspeig)

  • A. Campo Bagatin

    (Universidad de Alicante, Carr. de San Vicente del Raspeig
    Instituto de Física Aplicada a las Ciencias y las Tecnologías, Universidad de Alicante, San Vicente del Raspeig)

  • E. J. Christensen

    (The University of Arizona, Lunar and Planetary Laboratory)

  • R. J. Wainscoat

    (Institute for Astronomy, University of Hawaii)

  • R. Weryk

    (The University of Western Ontario)

  • L. Fraga

    (Laboratório Nacional de Astrofísica LNA/MCTIC)

  • C. Briceño

    (Cerro Tololo Inter-American Observatory/NSF’s NOIRLab)

  • L. Conversi

    (ESA NEO Coordination Centre
    ESA ESRIN)

Abstract

Trojan asteroids are small bodies orbiting around the L4 or L5 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 TK7 has been the only known Earth Trojan thus far. Here we confirm that the recently discovered 2020 XL5 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 XL5 will remain in L4 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.

Suggested Citation

  • T. Santana-Ros & M. Micheli & L. Faggioli & R. Cennamo & M. Devogèle & A. Alvarez-Candal & D. Oszkiewicz & O. Ramírez & P.-Y. Liu & P. G. Benavidez & A. Campo Bagatin & E. J. Christensen & R. J. Wains, 2022. "Orbital stability analysis and photometric characterization of the second Earth Trojan asteroid 2020 XL5," Nature Communications, Nature, vol. 13(1), pages 1-11, December.
    • Handle: RePEc:nat:natcom:v:13:y:2022:i:1:d:10.1038_s41467-022-27988-4
    DOI: 10.1038/s41467-022-27988-4
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