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3753 Cruithne

Aten asteroid co-orbital with Earth


Aten asteroid co-orbital with Earth

FieldValue
minorplanetyes
background#FFC2E0
name3753 Cruithne
imageCruithne.jpg
discovererDuncan Waldron
discovered10 October 1986
mpc_name(3753) Cruithne
alt_names1983 UH; 1986 TO
named_afterCruthin
pronounced
mp_category{{Ubl
Aten&thinsp;<ref namejpldata/
orbit_ref
epoch4 September 2017 (JD 2458000.5)
observation_arc16087 days (44.04 yr)
uncertainty0
aphelion1.5114 AU
perihelion0.48405 AU
semimajor0.99774 AU
eccentricity0.51485
(213000 wrt Earth)
period1.00 yr (364.02 d)
inclination19.805°
asc_node126.23°
arg_peri43.831°
mean_anomaly257.46°
mean_motion/ day
moid0.07119 AU
avg_speed27.73 km/s
mean_diameter~5 km
mass
rotation27.30990 h
albedo0.15
spectral_typeQ
abs_magnitude15.6

| NEO | Aten  | horseshoe | Venus-crosser | Mars-crosser (213000 wrt Earth)

3753 Cruithne is a Q-type, Aten asteroid in orbit around the Sun in 1:1 orbital resonance with Earth, making it a co-orbital object. It is an asteroid that, relative to Earth, orbits the Sun in a bean-shaped orbit that effectively describes a horseshoe, and that can change into a quasi-satellite orbit. Cruithne does not orbit Earth and at times it is on the other side of the Sun, placing Cruithne well outside of Earth's Hill sphere. Its orbit takes it near the orbit of Mercury and outside the orbit of Mars. Cruithne orbits the Sun in about one Earth year, but it takes 770 years for the series to complete a horseshoe-shaped movement around Earth.

The asteroid takes its name from the Cruithne, a people mentioned in early Irish annals.

Discovery

Cruithne was discovered on 10 October 1986 by Duncan Waldron on a photographic plate taken with the UK Schmidt Telescope at Siding Spring Observatory, Coonabarabran, Australia. A 1983 precovery (1983 UH) is credited to Giovanni de Sanctis and Richard M. West of the European Southern Observatory in Chile.

It was not until 1997 that its unusual orbit was determined by Paul Wiegert and Kimmo Innanen, working at York University in Toronto, and Seppo Mikkola, working at the University of Turku in Finland.

Dimensions and orbit

Cruithne appears to make a bean-shaped orbit from the perspective of Earth.
3753 Cruithne}}

Cruithne is approximately 5 km in diameter, and its closest approach to Earth is 12 e6km, approximately thirty times the separation between Earth and the Moon. From 1994 through 2015, Cruithne made its annual closest approach to Earth every November.

Although Cruithne's orbit is not thought to be stable over the long term, calculations by Wiegert and Innanen showed that it has probably been synchronized with Earth's orbit for a long time. There is no danger of a collision with Earth for millions of years, if ever. Its orbital path and Earth's do not cross, and its orbital plane is currently tilted to that of Earth by 19.8°. Cruithne, having a maximum near-Earth magnitude of +15.8, is fainter than Pluto and would require at least a 12.5 in reflecting telescope to be seen.

Cruithne is in a normal elliptic orbit around the Sun. Its period of revolution around the Sun, approximately 364 days in the early 21st century, is almost equal to that of Earth. Because of this, Cruithne and Earth appear to "follow" each other in their paths around the Sun. This is why Cruithne is sometimes called "Earth's second moon". However, it does not orbit Earth and is not a moon. In 2058, Cruithne will come within 0.09 AU (13.6 e6km) of Mars.

Due to a high orbital eccentricity, Cruithne's distance from the Sun and orbital speed vary a lot more than Earth's, so from Earth's point of view Cruithne actually follows a kidney-bean-shaped horseshoe orbit ahead of Earth, taking slightly less than one year to complete a circuit of the "bean". Because it takes slightly less than a year, Earth "falls behind" the bean a little more each year, and so, from the point of view of an observer on Earth, the circuit is not quite closed, but rather like a spiral loop that moves slowly away from Earth.

After many years, Earth will have fallen so far behind that Cruithne will then actually be "catching up" on Earth from "behind". When it eventually does catch up, Cruithne will make a series of annual close approaches to Earth and gravitationally exchange orbital energy with Earth; this will alter Cruithne's orbit by a little over half a million kilometres—while Earth's orbit is altered by about 1.3 cm—so that its period of revolution around the Sun will then become slightly more than a year. The kidney bean will then start to migrate away from Earth again in the opposite direction—instead of Earth "falling behind" the bean, it is "pulling away from" the bean. The next such series of close approaches will be centred on the year 2292—in July of that year, Cruithne will approach Earth to about 12.5 e6km.

After 380 to 390 years or so, the kidney-bean-shaped orbit approaches Earth again from the other side, and Earth, once more, alters the orbit of Cruithne so that its period of revolution around the Sun is again slightly less than a year (this last happened with a series of close approaches centered on 1902, and will next happen with a series centered on 2676). The pattern then repeats itself.

Similar minor planets

More near-resonant near-Earth objects (NEOs) have since been discovered. These include 54509 YORP, , , and which exist in resonant orbits similar to Cruithne's. is the first identified Earth trojan (out of only two known ).

Other examples of natural bodies known to be in horseshoe orbits (with respect to each other) include Janus and Epimetheus, natural satellites of Saturn. The orbits these two moons follow around Saturn are much simpler than the one Cruithne follows, but operate along the same general principles.

Mars has four known co-orbital asteroids (5261 Eureka, , , and , all at the Lagrangian points), and Jupiter has many (an estimated one million greater than 1 km in diameter, the Jovian trojans); there are also other small co-orbital moons in the Saturnian system: Telesto and Calypso with Tethys, and Helene and Polydeuces with Dione. However, none of these follow horseshoe orbits.

References

References

  1. (2011). "A long-lived horseshoe companion to the Earth". [[Monthly Notices of the Royal Astronomical Society]].
  2. [http://www.wwu.edu/depts/skywise/a101_cruithne.html Cruithne: Asteroid 3753] {{Webarchive. link. (2012-03-02 . Western Washington University Planetarium. Retrieved 27 January 2011.)
  3. Wiegert, Paul A.. (June 1998). "The Orbital Evolution of Near-Earth Asteroid 3753". The Astronomical Journal.
  4. Wiegert, Paul A.. (12 June 1997). "An asteroidal companion to the Earth (letter)". Nature.
  5. "JPL Close-Approach Data: 3753 Cruithne (1986 TO)".
  6. "This month Pluto's apparent magnitude is m=14.1. Could we see it with an 11" reflector?". Singapore Science Centre.
  7. "The astronomical magnitude scale.". The ICQ Comet Information Website.
  8. Lloyd, Robin. "More Moons Around Earth?". [[Space.com]].
  9. Meeus, reference above, writes "we may not deduce that Cruithne is a "companion" of the Earth, as some authors wrote, and certainly it is not a satellite! The object simply ''cannot'' be a satellite of the Earth, as it moves from nearly the orbit of Mercury to outside that of Mars, and because sometimes it is in ''superior'' conjunction, at the far side of the Sun as seen from the Earth".
  10. (2022-12-28). "3753 Cruithne, la «deuxième Lune» dont vous ignoriez l'existence".
  11. "QI: Season 1, Episode 2 script {{!}} Subs like Script".
  12. "QI: Season 11, Episode 7 script {{!}} Subs like Script".
  13. ''Astonishing X-Men'' vol. 3 #31
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