Moons of Jupiter Codexery

Harpalyke (moon)

A small retrograde irregular moon of Jupiter in the Ananke group.

Harpalyke (moon)

Harpalyke, designated Jupiter XXII and originally S/2000 J 5, is a small moon of Jupiter. It belongs to the planet's collection of irregular moons, which travel in distant, highly tilted, and elongated orbits. Discovered by Scott S. Sheppard on November 23, 2000, the moon was later named for Harpalyce, the daughter of Clymenus.

The moon moves around Jupiter in a retrograde direction—meaning it orbits opposite to the planet's spin—at an average distance of 21.0 million kilometers. Its orbital path is similar to that of the larger irregular moon Ananke, placing Harpalyke in the Ananke group. Scientists think the moons in this group are remnants of an asteroid or trans-Neptunian object that Jupiter captured with its gravity and that broke apart in a collision billions of years ago.

Most of Harpalyke's physical traits remain unknown. It is estimated to be about 4 kilometers in diameter, and its surface is probably dark and gray. The moon was discovered in November 2000 alongside ten other Jovian moons by a University of Hawaiʻi team led by Scott S. Sheppard, receiving the temporary designation S/2000 J 5. In October 2002, it was named after Harpalyce, the incestuous daughter of Clymenus, who in some stories was also a lover of Zeus (Jupiter).

Harpalyke orbits Jupiter at a mean distance of 21,280,180 km, completing one revolution in 634.19 days. Its orbit has an inclination of 148° relative to the ecliptic and an eccentricity of 0.160. This orbit constantly changes due to gravitational disturbances from the Sun and other planets.

As a member of the Ananke group, Harpalyke shares orbital characteristics with other retrograde irregular moons. These moons orbit Jupiter at distances of roughly 19 to 22 million km, with inclinations between 144° and 156° and eccentricities from 0.10 to 0.30. The group is thought to be fragments of a captured asteroid or trans-Neptunian object shattered by a collision billions of years ago.

Because of its small size, Harpalyke is very faint from Earth, with a visual apparent magnitude around 22.2, visible only through large, sensitive telescopes. Assuming a low geometric albedo of 0.04, like other irregular moons, its diameter is estimated at 4 km. Its shape is unknown, but given its small size, it is likely irregular, similar to other small irregular moons.

Quick Facts

Pronounced
h · ɑːr · ˈ · p · æ · l · ə · k · iː
Adjective
Harpalykean h · ɑːr · p · ə · l · ə · ˈ · k · iː · ə · n
Named After
Ἁρπαλύκη Harpălykē
Mpc Name
Jupiter XXII
Discoverer
Scott S. Sheppard / David C. Jewitt / Yanga R. Fernandez / Eugene A. Magnier
Discovery Site
Mauna Kea Observatory
Discovered
23 November 2000
Satellite Of
Jupiter
Group
Ananke group
Epoch
17 December 2020 (JD 2459200.5)
Observation Arc
2000 · 2024 / 2024-12-02 (last obs)
Semimajor
0.1422492 AU

Facts from the source article.

Lore & Background

Harpalyke was discovered in November 2000, along with ten other Jovian moons by a team of astronomers from the University of Hawaiʻi led by Scott S. Sheppard and given the temporary designation S/2000 J 5. In October 2002, the moon was named after Harpalyce, the incestuous daughter of Clymenus, who in some accounts was also a lover of Zeus (Jupiter).

The satellite orbits Jupiter in the retrograde direction at a mean distance of 21,280,180 km and completes one orbit in 634.19 days. Its orbit has an inclination of 148° relative to the ecliptic and an eccentricity of 0.160, and is subject to continuous changes due to gravitational perturbation from the Sun and the other planets. Harpalyke belongs to the Ananke group, a group of irregular retrograde Jovian moons that orbit Jupiter at distances of approximately 19 to 22 million km, with orbital inclinations ranging from 144° to 156° and eccentricities between 0.10 and 0.30. The moons of the Ananke group are believed to be fragments of an asteroid or trans-Neptunian object that was gravitationally captured by Jupiter and destroyed by a collision several billion years ago.

Due to its small size, Harpalyke appears very faint from Earth with a visual apparent magnitude of around 22.2, so it can only be observed by very large, sensitive telescopes. Assuming Harpalyke has a low geometric albedo of 0.04 like other irregular moons, its diameter has been estimated to be 4 km. The shape of the moon is currently unknown, but given its small size, it is likely to have an irregular shape, similar to other small irregular moons. The satellite appears grey (color index R-V=0.43), similar to C-type asteroids.

Reader's Guide

Harpalyke is notable as a member of the Ananke group, a collection of irregular retrograde moons believed to be remnants of a captured asteroid or trans-Neptunian object that was shattered by a collision billions of years ago. Its discovery in November 2000 by Scott S. Sheppard and his team added to the growing catalog of Jupiter's irregular satellites, which provide insights into the dynamical history of the Jovian system. The moon's orbit, with a mean distance of about 21 million km and an inclination of 148°, is subject to gravitational perturbations from the Sun and other planets, illustrating the complex gravitational environment of the outer solar system. Although most of its physical properties are unknown, its estimated diameter of 4 km and grey color suggest it is a small, irregular, C-type asteroid-like body. Harpalyke has not been imaged up close by a space probe, but it is planned to be a distant observation target for the European Space Agency's Jupiter Icy Moons Explorer (Juice) mission, which will measure the rotation periods and shapes of Jupiter's irregular moons by watching their brightness change over time.

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