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69 Hesperia

Main-belt asteroid


Main-belt asteroid

FieldValue
minorplanetyes
background#D6D6D6
name69 Hesperia
image69Hesperia (Lightcurve Inversion).png
captionA three-dimensional model of 69 Hesperia based on its light curve.
discovererG. Schiaparelli
discoveredApril 29, 1861
mpc_name(69) Hesperia
pronounced
adjectiveHesperian
named_afterHesperia
mp_categoryMain belt
epoch(absent)
semimajor2.980 AU
perihelion2.489 AU
aphelion3.471 AU
eccentricity0.165
period1879 d
inclination8.59°
asc_node184.99°
arg_peri288.8°
dimensions138 km (IRAS)
110 ± 15 km
mass
density
rotation5.655 h
spectral_typeM
abs_magnitude7.05
albedo0.140

110 ± 15 km

69 Hesperia is a large, M-type main-belt asteroid. It was discovered by the Italian astronomer Giovanni Schiaparelli on April 29, 1861 from Milan, while he was searching for the recently discovered 63 Ausonia. It was his only asteroid discovery. Schiaparelli named it Hesperia in honour of Italy (the word is a Greek term for the peninsula). The asteroid is orbiting the Sun with a period of 1879 d, a semimajor axis of , and eccentricity of 0.165. The orbital plane is inclined by an angle of 8.59° to the plane of the ecliptic.

Hesperia was observed by Arecibo radar in February 2010. Radar observations combined with lightcurve-based shape models, lead to a diameter estimate of 110 +/-. The radar albedo is consistent with a high-metal M-type asteroid. In the near infrared, a weak absorption feature near a wavelength of 0.9 μm can be attributed to orthopyroxenes on the surface. A meteorite analogue of the reflectance spectra from 69 Hesperia is the Hoba ataxite.

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. {{OED. Hesperian
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