General · EdgepediaOctober 21, 20263 min read

15977 Pyraechmes

15977 Pyraechmes (provisional designation 1998 MA₁₁) is a Jupiter Trojan asteroid, a roughly 44-kilometer body that shares Jupiter's orbit in a 1:1 mean-motion resonance from the L5 Lagrangian point, 60 degrees behind the planet. It was discovered on 19 June 1998 by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) program at the ETS site of Lincoln Laboratory near Socorro, New Mexico, in the United States.⁵

Key fact	Detail
Designations	15977 Pyraechmes = 1998 MA₁₁; alternate 1999 NG₂⁵
Discovery	19 June 1998, LINEAR, ETS of Lincoln Laboratory, near Socorro, New Mexico⁵
Orbit	Semimajor axis 5.18 AU; period 4,309 days (11 years 10 months); eccentricity 0.05; inclination 17°⁵
Naming	After Pyraechmes, Paeonian leader slain by Patroclus; name approved April 2025¹

Orbit and classification

It circles the Sun at a distance of 4.9 to 5.4 AU once every 11 years and 10 months (4,309 days; semimajor axis 5.18 AU). Its orbit has an eccentricity of 0.05 and an inclination of 17 degrees with respect to the ecliptic.⁶

Because the orbit never approaches Earth's, the asteroid is not classified as potentially hazardous; its closest possible distance to Earth's orbit is 3.96 AU.²

Discovery and precovery

The official discovery observation was made on 19 June 1998 by the LINEAR survey at Socorro.⁶

Numbering and naming

The name Pyraechmes was approved by the IAU Working Group Small Bodies Nomenclature and announced in its bulletin of 7 April 2025. The naming citation reads that Pyraechmes "was a leader of the Paeonian horsemen from Amydon. He was the first to be killed by Patroclus who fought while wearing Achilles armor," an episode from the Iliad.¹

Physical characteristics

Slow rotation. Robert Stephens of the Center for Solar System Studies observed Pyraechmes on three nights in 2013 but could not derive a meaningful rotational lightcurve, because the amplitude never changed appreciably.

Context among Jupiter's Trojans

The Trojans of Jupiter are asteroids sharing nearly the planet's own orbit, staying either ahead of or behind it in a co-orbital configuration at an angular separation of roughly 60 degrees.³ Their inclinations cover a fairly uniform range from 0° to 35° in both the L4 and L5 regions, with a median inclination of 10°, and their eccentricities tend to be below 0.15, values required to remain within the stable zones around the Lagrangian points.⁴ Pyraechmes fits this population: its 17° inclination is above the population median, and its eccentricity of 0.05 is well within the stable range.⁴

Dynamical studies indicate that most Trojans many tens of kilometers in diameter or larger are on stable orbits and can be treated as survivors of whatever processes created the Trojan population.⁴ The leading explanation for the Trojans' broad inclination distribution is that they formed in more distant regions and were captured into co-orbital motion with Jupiter during the migration of the giant planets, in a short period of chaos just after Jupiter and Saturn crossed their mutual 1:2 resonance.³

References

Topic: Encyclopedia › Places and geography › Extraterrestrial places › Small bodies of the Solar System › Jupiter Trojans and other dynamical groups › Trojan-camp Jupiter Trojans

Initially written Oct 21, 2026 · Edited: Oct 25, 2026

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