Arjuna asteroid

The Arjuna asteroids (also known as "Arjunas") are a dynamical group of asteroids in the Solar System. Arjunas are near-Earth objects (NEOs) whose orbits are very Earth-like in character, having low inclination, orbital periods close to one year, and low eccentricity. The group is named after Arjuna, a central hero in Hindu epic Mahabharata. The definition is somewhat vague and overlaps the definition of the four well-established Apollo, Amor, Aten and Atira groups. They constitute a dynamically cold group of small NEOs that experience repeated trappings in the 1:1 mean-motion resonance with the Earth.[1][2]

Members

Potential members of the Arjuna group with their Apollo (APO) or Aten (ATE) group classification in parenthesis, include:

gollark: Aha, it worked.
gollark: I'll get this eventually.
gollark: ++magic py `bot.get_channel(348702212110680064).fetch_message(811555849071886336).add_reaction("🐝")`
gollark: ++magic py `bot.get_channel(348702212110680064).get_message(811555849071886336).add_reaction("🐝")`
gollark: Just demote him to helper.

References

  1. de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (July 2013). "A resonant family of dynamically cold small bodies in the near-Earth asteroid belt". Monthly Notices of the Royal Astronomical Society: Letters. 434 (1): L1–L5. arXiv:1305.2825. Bibcode:2013MNRAS.434L...1D. doi:10.1093/mnrasl/slt062.
  2. de la Fuente Marcos, C.; de la Fuente Marcos, R. (January 2015). "Geometric characterization of the Arjuna orbital domain". Astronomische Nachrichten. 336 (1): 5. arXiv:1410.4104. Bibcode:2015AN....336....5D. doi:10.1002/asna.201412133.

Further reading


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