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60 Echo

Main-belt asteroid

60 Echo

Summary

Main-belt asteroid

FieldValue
minorplanetyes
image60Echo (Lightcurve Inversion).png
captionThree-dimensional model of 60 Echo created based on light-curve
background#D6D6D6
name60 Echo
discovererJames Ferguson
discoveredSeptember 14, 1860
mpc_name(60) Echo
pronounced
adjectivesEchoian
named_afterEcho
mp_categoryMain belt
epochDecember 31, 2006 (JD 2454100.5)
semimajor2.394 AU
perihelion1.958 AU
aphelion2.830 AU
eccentricity0.182
period1353.002 days
inclination3.602°
asc_node191.803°
arg_peri270.477°
mean_anomaly91.065°
dimensions60.2 km{{cite web
id2011-08-14 last obs
titleJPL Small-Body Database Browser: 60 Echo
urlhttps://ssd.jpl.nasa.gov/sbdb.cgi?sstr=60
publisherJet Propulsion Laboratory
access-date2012-01-27}}
mass(3.15 ± 0.32) × 1017 kg
density2.78 ± 0.33 g/cm3
rotation25.2 hr
spectral_typeS
abs_magnitude8.21
albedo0.254

|access-date=2012-01-27}}

60 Echo is a quite large main-belt asteroid. It was discovered by James Ferguson of the United States Naval Observatory in Washington D.C., on September 14, 1860. It was his third and final asteroid discovery. It is named after Echo, a nymph in Greek mythology. James Ferguson had initially named it "Titania", not realizing that name was already used for a satellite of Uranus.

Orbit

This object is orbiting the Sun with a period of 1353.002 days, a semimajor axis of , and an eccentricity of 0.18. Its orbital plane is at an inclination of 3.6° to the plane of the ecliptic. This is a stony S-type asteroid with a cross-sectional size of 60.2 km that is spinning with a rotation period of 25.2 hr. Echo has been studied by radar.{{cite web |access-date=2012-01-23}} It is not known to be a member of any asteroid family.

References

References

  1. "Asteroid Data Sets".
  2. (1863). "Appletons' annual cyclopaedia and register of important events of the year: 1862". [[D. Appleton & Company]].
Wikipedia Source

This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.

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