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911 Agamemnon

Jupiter trojan


Jupiter trojan

FieldValue
minorplanetyes
background#C2FFFF
name911 Agamemnon
imageFile:911 Agamemnon.png
captionShape model of Agamemnon from its lightcurve
discovery_ref
discovererK. Reinmuth
discovery_siteHeidelberg Obs.
discovered19 March 1919
mpc_name(911) Agamemnon
alt_names1919 FD1937 QD
pronounced
adjectivesAgamemnonian
named_afterAgamemnon
(Greek mythology)
mp_categoryJupiter trojan
Greekbackground
orbit_ref
epoch23 March 2018 (JD 2458200.5)
uncertainty0
observation_arc97.93 yr (35,770 d)
aphelion5.6232 AU
perihelion4.9300 AU
semimajor5.2766 AU
eccentricity0.0657
period12.12 yr (4,427 d)
mean_anomaly236.05°
mean_motion/ day
inclination21.763°
asc_node338.01°
arg_peri80.874°
satellites1 (indirect observation)
jupiter_moid0.1064 AU
tisserand2.8530
dimensions
mean_diameter
rotation
albedo
spectral_typeD (Tholen)
D (S3OS2)
U–B
B–V
V–I
abs_magnitude7.89
8.27
magnitude14.7 to 16.1

(Greek mythology) Greekbackground

D (S3OS2) U–B
B–V
V–I
8.27

911 Agamemnon, provisional designation **, is a Jupiter trojan and a suspected binary asteroid from the Greek camp, approximately 168 km in diameter. It was discovered on 19 March 1919, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. The dark D-type asteroid is likely the second-largest Jupiter trojans and has a rotation period of 6.6 hours. It is named after the Greek King Agamemnon, a main character of the Iliad.

Orbit and classification

Agamemnon is a dark Jovian asteroid orbiting in the Greek camp at Jupiter's leading Lagrangian point, 60° ahead of its orbit in a 1:1 resonance . It is also a non-family asteroid in the Jovian background population.

It orbits the Sun at a distance of 4.9–5.6 AU once every 12 years and 1 month (4,427 days; semi-major axis of 5.28 AU). Its orbit has an eccentricity of 0.07 and an inclination of 22° with respect to the ecliptic. The body's observation arc begins at Heidelberg in October 1927, more than 8 years after its official discovery observation.

Physical characteristics

In the Tholen classification, Agamemnon is a dark D-type asteroid. It has also been characterized as a D-type in both the Tholen- and SMASS-like taxonomy of the Small Solar System Objects Spectroscopic Survey (S3OS2).

Rotation period

Photometric observations of this asteroid during 1997 were used to build a lightcurve showing a rotation period of hours with a brightness variation of magnitude. A 2009 study yielded a period of hours, in reasonable agreement with the previous result.

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Agamemnon measures between 131.04 and 185.30 kilometers in diameter, based on a common absolute magnitude of 7.89 and a surface albedo between 0.037 and 0.072. A concurring diameter estimate of kilometers from an occultation event (see below) has also been obtained. The Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, that is, an albedo of 0.0444 and a diameter of 166.66 kilometers based on an absolute magnitude of 7.89.

Shape and satellite

A 2012 stellar occultation produced a 2D shape model of roughly (with an irregular, skewed outline) and strong evidence of Agamemnon having a satellite of approximately kilometers in diameter orbiting at from the primary's center.

Naming

This minor planet named from Greek mythology after King Agamemnon, the leader of the Greeks in the Trojan War. He is a main character of Homer's Iliad. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 88).

Notes

References

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|access-date = 6 June 2018 |archive-date = 6 April 2023 |archive-url = https://web.archive.org/web/20230406204452/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=911+Agamemnon |url-status = dead

|access-date= 6 June 2018}}

|access-date = 4 March 2018 |archive-url = https://web.archive.org/web/20160303182918/http://www.asteroidoccultation.com/observations/Results/Data2012/20120119_AgamemnonProfilewithSatellite.gif |archive-date = 3 March 2016 |url-status = dead

|access-date = 14 June 2018}}

|display-authors = 6

|display-authors = 6 |doi-access= free

|access-date = 15 June 2018}}

|display-authors = 6

|display-authors = 6 |doi-access= free

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|access-date= 6 June 2018}}

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References

  1. Noah Webster (1884) ''A Practical Dictionary of the English Language''
  2. Browning (1877) ''The Agamemnon of Aeschylus''
  3. [https://ssd.jpl.nasa.gov/horizons_batch.cgi?batch=1&COMMAND=%27911%27&START_TIME=%272044-09-16%27&STOP_TIME=%272044-09-17%27&STEP_SIZE=%272%20day%27&QUANTITIES=%279,19,20,23,29%27 Perihelic opposition]
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