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442 Eichsfeldia

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Main-belt asteroid

442 Eichsfeldia
Discovery 
Discovered byM. Wolf
A. Schwassmann
Discovery siteHeidelberg Obs.
Discovery date15 February 1899
Designations
MPC designation(442) Eichsfeldia
Pronunciation/aɪksˈfɛldiə/
Named afterEichsfeld
Alternative designations1899 EE; A892 FA
Minor planet categorymain-belt
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc123.78 yr (45211 d)
Aphelion2.5112 AU (375.67 Gm)
Perihelion2.1796 AU (326.06 Gm)
Semi-major axis2.3454 AU (350.87 Gm)
Eccentricity0.070707
Orbital period (sidereal)3.59 yr (1312.0 d)
Mean anomaly185.97°
Mean motion0° 16 27.84 / day
Inclination6.0689°
Longitude of ascending node134.93°
Argument of perihelion85.047°
Earth MOID1.18144 AU (176.741 Gm)
Jupiter MOID2.47041 AU (369.568 Gm)
TJupiter3.550
Physical characteristics
Dimensions66.73±1.4 km
65.58±1.70 km
Mass1.95±0.20 × 10 kg
Mean density1.32±0.16 g/cm
Synodic rotation period11.871 h (0.4946 d)
Geometric albedo0.0386±0.002
Spectral typeBV = 0.692 mag
UB = 0.331 mag
tholen = C
SMASSII = Ch
Absolute magnitude (H)10.03 mag
9.94 mag

442 Eichsfeldia is a large main belt asteroid that was discovered by German astronomers Max Wolf and A. Schwassmann on 15 February 1899 in Heidelberg. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material.

Although Eichsfeldia has an orbit similar to the Vesta family asteroids, it was found to be an unrelated interloper on the basis of its non-matching spectral type.

References

  1. ^ "JPL Small-Body Database Browser: 442 Eichsfeldia (1899 EE)" (2015-09-27 last obs.). Jet Propulsion Laboratory. Retrieved 10 May 2016.
  2. ^ Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
  3. Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, vol. 34, pp. 113–119, Bibcode:2007MPBu...34..113W.

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