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(612901) 2004 XP14

Near-Earth asteroid

(612901) 2004 XP14

Near-Earth asteroid

FieldValue
minorplanetyes
background#FFC2E0
name
image2004 XP14 radar.jpg
captionimaged by the Goldstone Solar System Radar in 2006
discovererLINEAR
discovered10 December 2004
mp_categoryNEOApolloPHA
orbit_ref
observation_arc1007 days (2.76 yr)
uncertainty0
epoch13 January 2016 (JD 2457400.5)
semimajor1.05156 AU
perihelion0.884900 AU
aphelion1.21822 AU
eccentricity0.158488
period1.08 yr (393.87 d)
inclination32.9505°
asc_node281.045°
arg_peri273.695°
mean_anomaly10.1555°
mean_motion/day
moid0.00316799 AU
mean_diameter
300–800 m
rotation100 h
abs_magnitude19.4

300–800 m

**** is a sub-kilometer asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Apollo group. It was first observed by the LINEAR project on 10 December 2004.

Description

14}} as seen from France during its closest approach to Earth on 3 July 2006

Although initially there were concerns that it might possibly impact Earth later in the 21st century and thus merit special monitoring, further analysis of its orbit has since ruled out any such collision, at least in the foreseeable future.

The size of is not precisely known. Based on optical measurements, the object is between 300 and 800 meters in diameter. Radar observations place a lower bound of about 260 m.

's closest pass by Earth was above the west coast of North America at 04:25 UTC on 3 July 2006.

The asteroid's distance from Earth's center of mass at that moment was 0.0028906 AU, or just 1.1 times the Moon's average distance from Earth. It was observed immediately after this close approach by radar from three locations, from Goldstone in the Mojave Desert in the US, from Sicily, and from Yevpatoria RT-70 radio telescope, Ukraine, as well as optically from other observatories and amateurs.

It was removed from the Sentry Risk Table on 17 March 2005.

AsteroidDateNominal approach distance (LD)Min. distance (LD)Max. distance (LD)Absolute magnitude (H)Size (meters)
1914-12-310.6060.6040.60819.4279–900
1918-09-170.9110.9090.91317.9556–1795
1925-08-300.9030.9010.90518.5*443–477*
[69230 Hermes](69230-hermes)1937-10-301.9261.9261.92717.5668–2158
69230 Hermes1942-04-261.6511.6511.65117.5668–2158
1975-01-311.7621.7611.76218.1507–1637
2002-08-181.3711.3711.37119.0335–1082
** ****2006-07-03****1.125****1.125****1.125****19.3****292–942**
2015-10-311.2661.2661.26620.0211–682
2027-08-071.0141.0101.01917.9556–1793
2028-06-260.6470.6470.64718.2*921–943*
[99942 Apophis](99942-apophis)2029-04-130.09810.09630.100019.7*310–340*
2072-07-261.2161.2152.75918.8367–1186
2072-10-171.8751.8651.88619.6254–820
2080-08-311.6551.6541.65618.5*443–477*
[(416801) 1998 MZ](416801-1998-mz)2116-11-261.0681.0681.06919.2305–986
2140-12-010.6340.6310.63719.3*427–593*
2172-02-081.7831.7751.79218.7385–1242
[(290772) 2005 VC](290772-2005-vc)2198-05-051.9511.7912.13417.6638–2061

References

|archive-url=https://web.archive.org/web/20020602101400/http://neo.jpl.nasa.gov/risk/removed.html |url-status=dead |archive-date=2002-06-02

References

  1. "Absolute Magnitude (H)". NASA/JPL.
  2. (2006). "Asteroid fly-by eludes study". Nature.
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