2004 FH is a micro-asteroid and near-Earth object of the Aten group, approximately 30 meters in diameter, that passed just 43,000 km (27,000 mi) above the Earth's surface on 18 March 2004, at 22:08 UTC. It was the 11th closest approach to Earth recorded as of 21 November 2008[update].[b] The asteroid was first observed on 16 March 2004, by astronomers of the Lincoln Near-Earth Asteroid Research at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico.
Flyby of asteroid 2004 FH [a]
|Discovery site||Lincoln Lab's ETS|
|Discovery date||16 March 2004|
|MPC designation||2004 FH|
|NEO · Aten |
|Orbital characteristics |
|Epoch 4 September 2017 (JD 2458000.5)|
|Uncertainty parameter 5|
|Observation arc||3 days|
|0.74 yr (270 days)|
|1° 19m 55.56s / day|
|Earth MOID||0.00002265 AU|
0.0088 LD · (3390 km)
|Dimensions||24 m (calculated)|
30 m (estimate)
|0.0504 h (3.02 min)|
Orbit and classificationEdit
2004 FH is an Aten asteroid. It passed 43,000 km from the Earth on 18 March 2004. For comparison, geostationary satellites orbit Earth at 35,790 kilometers. Despite its small size, it is still the fourth largest asteroid detected coming closer to the Earth than the Moon.
Had this object hit Earth, it would probably have detonated high in the atmosphere. It might have produced a blast measured in hundreds of kilotons of TNT, but may not have produced any effect on the ground. It could also have been an Earth-grazing fireball if it had been much closer but not close enough to impact.
On 17 March 2044 the asteroid will pass no closer than 0.0116 AU (1,740,000 km; 1,080,000 mi) from the Earth. 2004 FH also has the distinction of having the lowest inclination of any known near-Earth asteroids.
In March 2004, two rotational lightcurves of 2004 FH were obtained from photometric observations by astronomers Petr Pravec, Stefano Sposetti and Raoul Behrend. Lightcurve analysis gave a rotation period of 0.0504 hours (3.02 minutes) with a brightness amplitude of 1.16 and 0.75 magnitude, respectively (U=3/2+).
Diameter and albedoEdit
has been estimated to measure approximately 30 meters (100 feet) in diameter. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 24 meters based on an absolute magnitude of 25.7.
- Flyby of asteroid 2004 FH (center dot being followed by the sequence). The other object that flashes by is an artificial satellite. Images were taken by Stefano Sposetti and composited by Raoul Behrend of Geneva Observatory.
- Rankings depend on definitions of meteoroid and approach. The 2-10 m 1972 grazer was at 57 km, the 44 kg 1990 grazer was about 100 km, possible 2006 grazer size and altitude not available. See List of asteroid close approaches to Earth.
- "JPL Small-Body Database Browser: (2004 FH)" (2004-03-19 last obs.). Jet Propulsion Laboratory. Retrieved 23 November 2017.
- "2004 FH". Minor Planet Center. Retrieved 23 November 2017.
- "LCDB Data for (2004)". Asteroid Lightcurve Database (LCDB). Retrieved 23 November 2017.
- Steven R. Chesley; Paul W. Chodas (17 March 2004). "Recently Discovered Near-Earth Asteroid Makes Record-breaking Approach to Earth". NASA's Near Earth Object Program Office. Retrieved 23 November 2017.
- "JPL Close-Approach Data: (2004 FH)" (last observation: 2004-03-19; arc: 3 days; uncertainty: 3). Retrieved 23 March 2016.
- Behrend, Raoul. "Asteroids and comets rotation curves – (2004 FH)". Geneva Observatory. Retrieved 23 November 2017.
|Wikimedia Commons has media related to 2004 FH.|
- MPEC 2004-F24
- Images of 2004 FH at Klet
- Asteroid Lightcurve Database (LCDB), query form (info)
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- 2004 FH at the JPL Small-Body Database