S / 2005 (29314) 1

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(29314) Eurydamas I (S / 2005 (29314) 1)
Provisional or systematic name S / 2005 (29314) 1
Central body (29314) Eurydamas
Properties of the orbit
Major semi-axis 41 km
Periapsis unknown
Apoapsis unknown
Orbital time 0.62646 ± 0.00030 d
Physical Properties
Albedo ≈ 0.140 ± 0.039
Medium diameter 16.0 km
surface 800 km 2
Medium density ≈ 0.59 ± 0.06 g / cm 3
discovery
Explorer
Date of discovery August 14, 2003

S / 2005 (29314) 1 is a moon of the L 5 - Jupiter Trojan (29314) Eurydamas . Its mean diameter is 16 kilometers.

Discovery and naming

S / 2005 (29314) 1 was discovered on August 14, 2003 by Rita K. Mann, David C. Jewitt and Pedro Lacerda through light curve observations. The discovery was announced on June 1, 2007; the moon was given the provisional designation S / 2005 (29314) 1 . An official naming by the IAU is still pending.

Track properties

Orbit

S / 2005 (29314) 1 orbits Eurydamas in an orbit at an average distance of 41 kilometers from its center (about 3.8 Eurydamas radii). The orbital eccentricity and inclination are not yet determined.

The orbit time of S / 2005 (29314) 1 is 15 hours and 2.1 minutes. The orbit of S / 2001 (47171) 1 is well within Eurydamas' Hill radius of 9,800 km.

rotation

Since the orbital time is equal to the rotation time of the main body of Eurydama's, it is most likely a double- bound rotation . This means that both bodies always face the same side. The prerequisite for this is a similar mass ratio and a narrow orbit of the two bodies.

Physical Properties

size

According to current data, S / 2005 (29314) 1 has a diameter of 16 km (about 3/4 of the central body), based on Eurydamas' estimated density of 0.59 g / cm 3 and the corresponding assumed equal reflectivity of 14%.

Assuming an average diameter of 16 km, this results in a surface of around 804 km 2 , which corresponds to the area of ​​the Swiss canton of Neuchâtel .

Determination of the diameter for S / 2005 (29314) 1

year Dimensions km source
2007 24 Man u. a.
2012 16 Grav u. a.

The most precise determination is marked in bold .

internal structure

The unusually low mean density of 0.59 g / cm 3 is an indication that it is not a compact body, but that the object is likely to be a rubble pile , an accumulation of dust and rocks interspersed with cavities .

See also

Web links

Individual evidence

  1. ^ Rita K. Mann et al: Fraction of contact binary asteroids (September 2007) (PDF). Retrieved September 18, 2017 .
  2. T. Grav et al .: WISE / NEOWISE Observations of the Jovian Trojan Population: Taxonomy (November 2012). Retrieved September 18, 2017 .