433 Eros
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{{Minor Planet
| name=433 Eros | image= 433eros.jpg | caption= This picture of Eros shows the view looking from one end of the asteroid across the gouge on its underside and toward the opposite end. | discoverer=Carl Gustav Witt | discovery_date=August 13, 1898 | designations=1898 DQ; 1956 PC | category=Amor,
Mars-crosser asteroid | epoch=October 22, 2004 (JD 2453300.5) | semimajor=218.155 Gm (1.458 AU) | perihelion=169.548 Gm (1.133 AU) | aphelion=266.762 Gm (1.783 AU) | eccentricity=0.223 | period=643.219 d (1.76 a) | inclination=10.829° | asc_node=304.401° | arg_peri=178.664° | mean_anomaly=320.215° | speed=24.36 km/s | dimensions=13×13×33 km | mass=7.2×1015 kg | density=2.4 g/cm³ | gravity=0.0059 m/s² | escape_velocity=0.0103 km/s | rotation=0.2194 d (5 h 16 min) | spectral_class=S | abs_mag=11.16 | albedo=0.16 | temperature=~227 K}}
The asteroid 433 Eros (eer'-os) was named after the Greek god of love Eros. It is an S-type asteroid approximately 13 × 13 × 33 km in size, the second-largest near-Earth asteroid, belonging to the Amors. It is also a Mars-crosser asteroid.
Eros was visited by the NEAR Shoemaker probe, which orbited it, taking extensive photographs of its surface, and then, on February 12 2001 at the end of its mission, landed on the asteroid's surface using only its maneuvering jets.
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Physical characteristics
Surface gravity depends on the distance from a spot on the surface to the center of a body's mass. The Erotian surface gravity varies a lot, since Eros is not a sphere but an elongated peanut-shaped (or potato- or shoe-shaped) object. The daytime temperature on Eros hovers at about 100 °C and nighttime measurements at −150 °C. Eros's density is 2,400 kg/m3, about the same as the density of Earth's crust. It rotates once every 5.27 hours.
NEAR scientists have found that most of the larger rocks strewn across Eros were ejected from a single crater in a meteorite collision perhaps 1 Ga (1 billion years) ago. This impact may also be responsible for the 40 percent of the Erotian surface that is devoid of craters smaller than 0.5 kilometers across. It was originally thought that the debris thrown up by the collision filled in the smaller craters. An analysis of crater densities over the surface indicates that the areas with lower crater density are within 9 kilometers of the impact point. Some of the lower density areas were found on the opposite side of the asteroid but still within 9 kilometers.
It is theorized that seismic shockwaves propagated through the asteroid, shaking smaller craters into rubble. Since Eros is irregularly shaped, a 9 kilometer straight line through the asteroid can reach locations that would be further away if travelling across the surface, thus leading to the uneven pattern of crater density on the surface. (Thomas & Robinson, 2005)
Legal controversy
In an experimental legal case, Eros was claimed as property by Gregory W. Nemitz of OrbDev. According to the Homestead principle, Nemitz argued that he had the right to claim ownership of any celestial body that he made use of; he claimed he had designated Eros a spacecraft parking facility and wished to charge NASA a parking and storage fee of 20 cents per year for NEAR Shoemaker. Nemitz's case was dismissed and an appeal denied. [1]
Aspects
Stationary, retrograde | Opposition | Opposition distance | Maximum brightness | Stationary, prograde | Conjunction to sun |
---|---|---|---|---|---|
26 February, 2005 | 16 April, 2005 | 0.365 96 AU | 10.5 mag | 2 May, 2005 | 3 March, 2006 |
23 May, 2007 | 9 July, 2007 | 0.747 92 AU | 12 mag | 22 August, 2007 | 11 October, 2008 |
14 July, 2009 | 1 September, 2009 | 0.689 42 AU | 11.9 mag | 15 October, 2009 | 2 January, 2011 |
15 January, 2012 | 28 February, 2012 | 0.175 79 AU | 8.5 mag | 15 March, 2012 | 20 February, 2013 |
13 May, 2014 | 28 June, 2014 | 0.719 76 AU | 12.0 mag | 10 August, 2014 | 16 July, 2015 |
3 July, 2016 | 21 August, 2016 | 0.727 46 AU | 12.0 mag | 5 October, 2016 | 23 December, 2017 |
5 November, 2018 | 3 December, 2018 | 0.223 39 AU | 9.3 mag | 22 December, 2018 | 11 February, 2020 |
Eros in fiction
Eros is also mentioned in Orson Scott Card's novel Ender's Game (1985). It used to be an outpost for the aliens known as Formics who installed artificial gravity but was taken over by humans and a Command School was built there. This is where Ender was sent after he graduated from Battle School.
433 Eros also plays an important role in the future evolution of life on Earth in Stephen Baxter's novel Evolution (2003). Millions of years after being perturbed into a new orbit, the asteroid collides with Earth, bringing about another mass extinction. The micrometeoroid-ravaged shell of NEAR Shoemaker still stands on the surface of Eros until seconds before the impact.
See also
References
External links
- NEAR Shoemaker spacecraft
- NEAR image of the day archive
- Movie: NEAR Shoemaker spacecraft landing
- The Eros Project (OrbDev's attempts at litigation over their property claim)
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de:Eros (Asteroid) es:(433) Eros fr:(433) Éros ko:433 에로스 it:433 Eros la:433 Eros nl:Eros (planetoïde) ja:エロス (小惑星) nn:433 Eros pl:433 Eros pt:433 Eros sk:433 Eros fi:433 Eros zh:小行星433