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92 Undina

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
image92 Undina (orbit).gif
background#D6D6D6
name92 Undina
discovererC. H. F. Peters
discovery_siteLitchfield Obs.
discovered7 July 1867
mpc_name(92) Undina
pronounced
adjectiveUndinian
mp_categoryMain belt
observation_arc145.11 yr (53001 d)
orbit_ref
epoch31 July 2016 (JD 2457600.5)
uncertainty0
semimajor3.18800 AU
perihelion2.85654 AU
aphelion3.51946 AU
eccentricity0.10397
period5.69 yr (2079.1 d)
inclination9.92900°
asc_node101.588°
arg_peri239.494°
mean_anomaly6.12456°
mean_motion/ day
mean_diameter
124.44 ± 3.25 km
mass(4.43 ± 0.25) × 1018 kg
density4.39 ± 0.42 g/cm3
rotation15.941 h
spectral_typeM
abs_magnitude6.61
albedo
0.251
Note

asteroid (92) Undina

124.44 ± 3.25 km 0.251

92 Undina (from Latin Undīna) is a large main belt asteroid. The asteroid was discovered by Christian Peters on 7 July 1867 from the Hamilton College Observatory. It is named for the eponymous heroine of Undine, a popular novella by Friedrich de la Motte Fouqué.

This minor planet is orbiting at a distance of around 3 AU from the Sun, which is known for a concentration of Tholen M-type asteroids. Indeed, 92 Undina has an unusually high albedo of 0.25 and an M-type spectrum, or Xc-type on the Bus taxonomy. However, it displays absorption features at a wavelength of 3 μm, which is usually indicative of hydrated silicates on the surface. There is a faint band in the region of 9 μm that is typically attributed to a form of orthopyroxene having low levels of calcium and iron. The spectrum of 92 Undina closely resembles powdered material from the Esquel meteorite, although with a higher albedo.

Observations performed at the Palmer Divide Observatory in Colorado Springs, Colorado during 2007 produced a light curve with a period of 15.941 ± 0.002 hours with a brightness range of 0.20 ± 0.02 in magnitude. This matches a 15.94-hour period reported in 1979. Attempts in 2014 to model the spin axis and shape based on light curve information proved inconclusive, but did indicate that "the pole latitude is not far removed from the ecliptic plane and rotation is probably retrograde".

References

References

  1. Hunter, Roe & Hooker (1906) ''The New American Encyclopedic Dictionary''
  2. ''Readings: the poetics of Blanchot, Joyce, Kafka, Kleist, Lispector, and Tsvetayeva'' (1991) Cixous
  3. "Asteroid Data Sets".
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