Dysnomia (moon)

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Dysnomia
Eris and Dysnomia: artist's impression
Eris and Dysnomia: artist's impression
Discovery
Discovered by: M. E. Brown,
M. A. van Dam,
A. H. Bouchez,
D. Le Mignant[1]
Discovery date: September 10, 2005[1]
MPC designation: (136199) Eris I Dysnomia
Alternative names: S/2005 (2003 UB313) 1
Orbital characteristics [1]
Semi-major axis: 30,000 - 36,000 km
Eccentricity: 0?
Orbital period: ~14 d
Satellite of: Eris
Physical characteristics
Equatorial radius: ~150 km[2]

Dysnomia (IPA: [dɪsˈnoʊ.mi.ə]), officially designated (136199) Eris I Dysnomia, is a moon of the dwarf planet Eris. It was discovered in 2005 by Mike Brown and the laser guide star adaptive optics team at the W. M. Keck Observatory, and carried the provisional designation of S/2005 (2003 UB313) 1 until officially named Dysnomia[3] (from the Greek word Δυσνομία meaning "lawlessness") after the daughter of the Greek goddess Eris.

Contents

[edit] Discovery

During 2005, the adaptive optics team at the Keck telescopes in Hawaii carried out observations of the four brightest Kuiper belt objects (Pluto, 2005 FY9, 2003 EL61, and Eris), using the newly commissioned laser guide star adaptive optics system. Observations taken on 10 September revealed a moon in orbit around Eris, it was provisionally designated S/2005 (2003 UB313) 1. In keeping with the Xena nickname that was already in use for Eris, the moon was nicknamed "Gabrielle" by its discoverers, after the television warrior princess's sidekick. Also, Xena's character was played by actress Lucy Lawless, whereas Dysnomia is the Greek goddess of lawlessness.

[edit] Properties

The satellite is about 60 times fainter than Eris, and its diameter is estimated to be approximately eight times smaller.[2] With only a single observation, the satellite cannot yet be used to measure or constrain the mass of Eris, but likely orbital parameters were nevertheless estimated. One of these is its orbital period, thought to be about two weeks (14 days). Further observations made with the Keck telescopes in August and September 2006 have led to a much better measurement of the period. Once astronomers refine the period and the semimajor axis of the satellite's orbit (currently estimated at 36,000 km[1]), they will be able to determine the mass of the system.

[edit] Formation

Astronomers now know that three of the four brightest Kuiper belt objects (KBOs) have satellites, while among the fainter members of the belt only about 10% are known to have satellites. This is believed to imply that collisions between large KBOs have been frequent in the past. Impacts between bodies of the order of 1000 km across would throw off large amounts of material which would coalesce into a moon. A similar mechanism is believed to have led to the formation of Earth's own Moon when the Earth was struck by a giant impactor early in the history of the solar system.

[edit] Name

Mike Brown, the moon's discoverer, chose the name Dysnomia (Greek Δυσνομία) due to a number of resonances it possessed for him. Dysnomia, the daughter of Eris, fits the general historically established pattern of naming moons after lesser gods associated with the primary (hence, Jupiter's largest moons are named after lovers or servants of Jupiter, while Saturn's are named after his fellow Titans). Also, the English translation of "Dysnomia", "lawlessness," echoes Lucy Lawless, the actress famous for starring in Xena: Warrior Princess on television. Before receiving their official names, Eris and Dysnomia were known informally as "Xena" and "Gabrielle" respectively (Gabrielle being Xena's sidekick), and Brown decided to retain that honour.

Brown also notes that Pluto owes its name in part to its first two letters, which form the initials of its supposed discoverer, Percival Lowell. James Christy, who discovered Charon, followed the principle established with Pluto by choosing a name which shared its first four letters with his wife's name, Charlene. "Dysnomia", similarly, has the same first letter as Brown's wife, Diane.[4]

In addition, both Eris and Dysnomia, representing conflict, reflect the effect their existence had in the disputation on the definition of a planet, and specifically on Pluto's status as such.

[edit] References

  1. ^ a b c d Michael E. Brown; et al (2006). "Satellites of the largest Kuiper belt objects" (PDF). Astrophys.J. 639 (L43). arXiv:astro-ph/0510029. 
  2. ^ a b Eris' moon — includes section on Dysnomia's size.
  3. ^ IAU Circular 8747 - Official publication of the IAU reporting the naming of Eris and Dysnomia (PDF file)
  4. ^ Tytell, David. "All Hail Eris and Dysnomia", Sky & Telescope, September 14, 2006. Retrieved on 2006-12-30.


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