Cited by 19Astro and Planetary ScienceSpacecraft Dynamics and ControlSpace Satellite Systems and Control

A Kozai-resonating Earth quasi-satellite

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Connors, M.·2013·Monthly Notices of the Royal Astronomical Society: Letters

Abstract

The recently discovered asteroid 2013 LX28 is in 1:1 resonance with Earth, but has large eccentricity and inclination. These lead to unusual dynamics in which the Kozai resonance plays a large role on long time-scales, while interaction with the terrestrial planets causes shorter term orbital changes. For the nominal orbit, an interaction with Venus changed the nature of the Kozai resonance and injected the asteroid into resonance with Earth. Despite frequent planetary encounters, the nominal orbit shows remarkable stability. Recovery prospects for this object are excellent, so that investigation of its remarkable properties should be able to proceed on a firmer observational base in future.

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Crossref · 10.1093/mnrasl/slt147

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  • Earth has three temporary natural retrograde satellites or quasi-satellites: (164207) 2004 GU9, (277810) 2006 FV35, and 2013 LX28.

    “Our planet has one permanently bound satellite -the Moon-, a likely large number of minimoons or transient irregular natural satellites, and three temporary natural retrograde satellites or quasi-satellites. These quasi-moons -(164207) 2004 GU 9 , (277810) 2006 FV 35 and 2013 LX 28 - are unbound companions to the Earth.”

    From Asteroid 2014 OL339: yet another Earth quasi-satellite (2014) · cites this paper as Connors 2014

  • 2013 LX28 was proposed as a Kozai-resonating Earth quasi-satellite by Connors (2014), who pointed out its remarkable stability.

    “The object was proposed as a Kozai-resonating Earth quasi-satellite by Connors (2014), who pointed out its remarkable stability.”

    From Asteroid 2014 OL339: yet another Earth quasi-satellite (2014) · cites this paper as Connors (2014)

  • Although Connors (2014) classifies 2013 LX28 as quasi-satellite, this is incorrect in strict sense because its orbit is hybrid.

    “Although Connors (2014) classifies 2013 LX 28 as quasi-satellite, this is incorrect in strict sense because its orbit is hybrid.”

    From Asteroid 2014 OL339: yet another Earth quasi-satellite (2014) · cites this paper as Connors (2014)

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Authors
Connors, M.
Affiliations
Athabasca University (CA)
Corresponding author
Connors, M.
Venue
Monthly Notices of the Royal Astronomical Society: Letters
Published
2013-11
Volume
437
Issue
1
Pages
L85-L89
ISSN
  • 1745-3925 (ISSN-L)
  • 1745-3933
OpenAlex
W2006002644
Cited by
19
References
12
Citations by year
2026: 1 · 2025: 1 · 2024: 1 · 2023: 2 · 2021: 1 · 2020: 3 · 2018: 1 · 2017: 2 · 2016: 3 · 2015: 2 · 2014: 2
FWCI
1.26
Type
journal article
Language
en
Open access
Locations
Monthly Notices of the Royal Astronomical Society Letters (publishedVersion)
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
  • Physical Sciences › Engineering › Aerospace Engineering › Spacecraft Dynamics and Control
  • Physical Sciences › Engineering › Aerospace Engineering › Space Satellite Systems and Control
Keywords
Kozai resonance, 1:1 resonance, orbital stability, orbital injection

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