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9694 Lycomedes

Asteroid


Asteroid

FieldValue
minorplanetyes
name9694 Lycomedes
background#C2FFFF
image009694-asteroid shape model (9694) Lycomedes.png
captionShape model of Lycomedes from its lightcurve
discovery_ref
discovererC. J. van Houten
I. van Houten-G.
T. Gehrels
discovery_sitePalomar Obs.
discovered26 September 1960
mpc_name(9694) Lycomedes
alt_names6581 P-L
pronounced
named_afterLycomedes
(Greek mythology)
mp_categoryJupiter trojan
Greekbackground
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc57.65 yr (21,058 d)
aphelion5.2852 AU
perihelion4.9135 AU
semimajor5.0993 AU
eccentricity0.0364
period11.52 yr (4,206 d)
mean_anomaly226.07°
mean_motion/ day
inclination4.9436°
asc_node350.07°
arg_peri53.908°
jupiter_moid0.019 AU
tisserand2.9920
mean_diameter
(calculated)
rotation
albedo(assumed)
spectral_typeC (assumed)
abs_magnitude10.60
10.7

I. van Houten-G. T. Gehrels (Greek mythology) Greekbackground (calculated)

10.7

9694 Lycomedes is a Jupiter trojan from the Greek camp, approximately 32 km in diameter. It was discovered during the Palomar–Leiden survey at the Palomar Observatory in 1960 and later named after Lycomedes from Greek mythology. The dark Jovian asteroid is likely elongated in shape and has a rotation period of 18.2 hours.

Discovery

Lycomedes was discovered on 26 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by astronomer Tom Gehrels at the Palomar Observatory in California. The body's observation arc begins the night after its official discovery observation at Palomar.

Palomar–Leiden survey

The survey designation "P-L" stands for "Palomar–Leiden", named after Palomar and Leiden observatories, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroids.

Naming

This minor planet was named from Greek mythology after Lycomedes, the Greek king of Scyros. At the request of Thetis, he concealed her son Achilles dressed in girl's clothes among his own daughters to save him from the Trojan War until Odysseus drew him out of his disguise. The official naming citation was published by the Minor Planet Center on 2 April 1999 (M.P.C. 34355).

Orbit and classification

As all Jupiter trojans, Lycomedes is in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's Lagrangian point, 60° ahead on its orbit .

It orbits the Sun at a distance of 4.9–5.3 AU once every 11 years and 6 months (4,206 days; semi-major axis of 5.1 AU). Its orbit has an eccentricity of 0.04 and an inclination of 5° with respect to the ecliptic.

Physical characteristics

Lycomedes is an assumed C-type asteroid, while most larger Jupiter trojans are D-types.

Rotation period

In October 2010, a first rotational lightcurve of Lycomedes was obtained from photometric observations by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of hours with a brightness amplitude of 0.38 magnitude ().

In November 2011, follow-up observations over two consecutive nights were made by Daniel Coley at the Goat Mountain Astronomical Research Station in California. It gave a concurring rotation period of hours with a high brightness amplitude of 0.55 magnitude, indicative of a non-spherical shape ().

Diameter and albedo

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Lycomedes measures between 31.736 and 31.74 kilometers in diameter and its surface has an albedo, while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 40.33 kilometers based on an absolute magnitude of 10.7.

Notes

References

References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. (July 2012). "Photometry of 17 Jovian Trojan Asteroids". Minor Planet Bulletin. link
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