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(419624) 2010 SO16

Asteroid


Asteroid

FieldValue
minorplanetyes
name
background#FFC2E0
image2010SO16-orbit.png
captionOrbit with inner solar system
discovery_ref
discovererWISE
discovery_site*Low Earth orbit*
discovered17 September 2010
mpc_name(419624)
alt_names
named_after
mp_categoryApolloNEOPHA
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc5.28 yr (1,928 days)
aphelion1.0785 AU
perihelion0.9272 AU
semimajor1.0028 AU
eccentricity0.0754
period1.00 yr (367 days)
mean_anomaly173.30°
mean_motion/ day
inclination14.520°
asc_node40.397°
arg_peri108.99°
moid0.0299 AU (11.6 LD)
mean_diameterkm
albedo
abs_magnitude20.5

**** is a sub-kilometer asteroid in a co-orbital configuration with Earth, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. It was discovered by the Wide-field Infrared Survey Explorer space telescope (WISE) on 17 September 2010.

Description

The orbit was described by Apostolos Christou and David Asher at the Armagh Observatory in Northern Ireland. The object has an absolute magnitude of 20.5. Observations by the discovering WISE telescope give a diameter of 357 meters and an albedo of 0.084.

has a horseshoe orbit that allows it to stably share Earth's orbital neighborhood without colliding with it. It is one of a handful of known asteroids with an Earth-following orbit, a group that includes 3753 Cruithne, and the only known asteroid in an horseshoe orbit with Earth. It is, however, neither an Aten asteroid nor an Apollo asteroid because the semi-major axis of its orbit is neither less than nor greater than 1 AU, but oscillates between approximately 0.996 and 1.004 AU, with a period of about 350 years. In its ~350 yr horseshoe cycle, it never approaches Earth more closely than about 0.15 AU, alternately trailing and leading.

According to various simulations will remain in this orbit for at least 120,000 years and possibly for more than a million years, which is unusually stable compared to other similar objects. One reason for this stability is its low orbital eccentricity, .

A precovery of may have been located in a 2005 Spitzer Space Telescope image.

References

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References

  1. [http://www.technologyreview.com/blog/arxiv/26608/Earth-Companion Asteroid Discovered in Horseshoe-Shaped Orbit], The Physics arXiv Blog, ''[[Technology Review]]'', 4/05/2011
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