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9951 Tyrannosaurus

Asteroid


Asteroid

FieldValue
minorplanetyes
name9951 Tyrannosaurus
background#D6D6D6
imageAnimatedOrbitOf9951Tyrannosaurus.gif
caption
discovery_ref
discovered15 November 1990
discovererE. W. Elst
discovery_siteLa Silla Obs.
mpc_name(9951) Tyrannosaurus
alt_names
pronounced
named_afterTyrannosaurus
(theropod dinosaur)
mp_categorymain-belt(inner)
Vesta
orbit_ref
epoch4 September 2017 (JD 2458000.5)
uncertainty0
observation_arc42.53 yr (15,534 days)
aphelion2.7243 AU
perihelion2.1283 AU
semimajor2.4263 AU
eccentricity0.1228
period3.78 yr (1,380 days)
mean_anomaly155.31°
mean_motion/ day
inclination7.4000°
asc_node133.42°
arg_peri153.36°
dimensions17 km
spectral_typeS
abs_magnitude14.2

(theropod dinosaur) Vesta

9951 Tyrannosaurus, provisional designation , is a stony Vestian asteroid from the inner regions of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 15 November 1990, by Belgian astronomer Eric Elst at ESO's La Silla Observatory in northern Chile. It was named after Tyrannosaurus, a genus of dinosaurs.

Classification and orbit

Based on the Hierarchical Clustering Method, Tyrannosaurus is a member of the Vesta family (401), which is named after its parent 4 Vesta, the main belt's second-largest and second-most-massive body after Ceres.

Tyrannosaurus orbits the Sun in the inner main-belt at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,380 days). Its orbit has an eccentricity of 0.12 and an inclination of 7° with respect to the ecliptic. It was first identified as at El Leoncito in 1974, extending the body's observation arc by 16 years prior to its official discovery observation at La Silla.

Physical characteristics

Tyrannosaurus has been characterized as a common S-type asteroid. The overall spectral type for members of the Vesta family is that of a V-type. Vestian asteroids have a composition akin to cumulate eucrites (HED meteorites) and are thought to have originated deep within 4 Vesta's crust, possibly from the Rheasilvia crater, a large impact crater on its southern hemisphere near the South pole, formed as a result of a subcatastrophic collision.

Diameter and albedo

According to the survey carried out by the Infrared Astronomical Satellite IRAS, Tyrannosaurus measures 17 kilometers in diameter. Spectroscopic observations indicate that it is a stony S-type asteroid, the most abundant spectral class of asteroids in the inner main-belt. It has an absolute magnitude of 14.2.

Lightcurves

As of 2017, no rotational lightcurve of Tyrannosaurus has been obtained. The asteroid's rotation period, poles and shape remain unknown.

Naming

This minor planet was named for Tyrannosaurus, a large and heavy bipedal carnivorous dinosaur, that lived in the upper cretaceous. It was one of the most terrifying predators, with a large skull, massive jaws and sharp teeth. Adult individuals were 12 meters long and 4–7 meters high. Tyrannosaurus rex is the best known species of this genus. The official naming citation was published by the Minor Planet Center on 20 November 2002 (M.P.C. 47166).

References

References

  1. {{OED. Tyrannosaurus
  2. Tedesco E.F.. "The supplemental IRAS minor planet survey (SIMPS)".
  3. Gianluca Masi. "Search for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog".
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