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2010 TD54

Near-Earth micro-asteroid


Near-Earth micro-asteroid

FieldValue
minorplanetyes
name
background#FFC2E0
imageAsteroid 2010TD54 orbit.jpg
captionOrbital diagram of during its near-Earth encounter on 12 Oct 2010
discovery_ref
discovererMount Lemmon Srvy.
discovery_siteMount Lemmon Obs.
discovered9 October 2010
mpc_name
mp_categoryNEOApollo
orbit_ref
epoch21 November 2025 (JD 2461000.5)
uncertainty6
observation_arc3 days
aphelion3.2371 AU
perihelion0.7053 AU
semimajor1.9712 AU
eccentricity0.6422
period2.77 yr (1,011 days)
mean_anomaly147.92°
mean_motion/ day
inclination4.2945°
asc_node18.123°
arg_peri76.641°
moid0.001444 AU
0.562 LD
dimensions5 m
5–10 m
rotation0.01167 h (dated)
0.0229317 h
albedo0.20 (assumed)
spectral_typeSrv
abs_magnitude28.9

0.562 LD 5–10 m 0.0229317 h

**** is a tiny asteroid and fast rotator, classified as a near-Earth object of the Apollo group, approximately 5 meters in diameter. It was first observed by the Mount Lemmon Survey in October 2010, when the asteroid crossed through the Earth-moon system and had a close encounter with Earth.

Orbit and classification

orbits the Sun at a distance of 0.7–3.2 AU once every 2 years and 9 months (1,011 days). Its orbit has an eccentricity of 0.64 and an inclination of 4° with respect to the ecliptic.

The body's observation arc begins with its first observations by the Mount Lemmon Survey and only spans over a period of 3 days until 12 October 2010. It has been observed since then.

Close approach

made its closest approach at 10:51, 12 October 2010 UTC (6:51 EDT a.m.) at 0.000346 AU. It is one of the closest known approaches of an asteroid to Earth, at which time the object appeared at a magnitude of 14. It was first observed by of the Catalina Sky Surveys telescopes north of Tucson, Arizona on 9 October 2010.

It has an Earth minimum orbit intersection distance of 0.00144418 AU, which corresponds to 0.562 lunar distance. It was removed from the Sentry Risk Table on 11 October 2010. The asteroid may have passed 0.0009 AU from Earth in October 1979, but the nominal orbit suggests it passed millions of kilometres from Earth in 1979.

Physical characteristics

is a stony asteroid, characterized as a Srv subtype.

Rotation period

In November 2010, a rotational light curve of was obtained from photometric observations, which showed that the asteroid is a fast rotator. Light curve analysis gave a well-defined rotation period of 0.0229317 hours (1 minute and 23 seconds) with a brightness amplitude of 0.92 magnitude (). A high amplitude typically indicates that the body has an irregular, elongated rather than spherical shape. This result supersedes a previously obtained lightcurve with a shorter period of 0.01167 hours ().

Diameter and albedo

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 5 m based on an absolute magnitude of 28.9. NASA's press release gave an estimated diameter of 5 to.

Notes

References

Info: Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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