World Library  
Flag as Inappropriate
Email this Article

Hydra (moon)

Article Id: WHEBN0003047717
Reproduction Date:

Title: Hydra (moon)  
Author: World Heritage Encyclopedia
Language: English
Subject: Pluto, Charon (moon), New Horizons, Natural satellite, Timeline of United States discoveries
Publisher: World Heritage Encyclopedia

Hydra (moon)

Image of Hydra taken by New Horizons on 14 July 2015
Discovered by Hubble Space Telescope
Pluto Companion Search Team
Discovery date 15 June 2005
Named after
Lernaean Hydra
(134340) Pluto III
Adjectives Hydrian
Orbital characteristics[1]
64738±3 km
Eccentricity 0.005862±0.000025
38.20177±0.00003 d
Inclination 0.242°±0.005°
Satellite of Pluto
Physical characteristics
Dimensions 43 km × 33 km (2D)[2]
Mean radius
20.5±0.5 km (projected 2D)
Mass (4.8±4.2)×1016 kg[2]
Albedo 0.51 average geometric
Temperature 33–55 K
22.9–23.3 (measured)[3]

Hydra is the outermost known natural satellite of Pluto. It was discovered along with Nix in June 2005, and was visited along with Pluto by New Horizons in July 2015. Hydra's surface is probably covered with water ice. Observed within Hydra's bright regions is a darker circular structure with a diameter of approximately 10 kilometers (5 miles). Hydra's reflectivity (the percentage of incident light reflected from the surface) is intermediate between those of Pluto and Charon.[4][5] Images taken by New Horizons should have a resolution of up to 780 meters per pixel.[6] This converts to a resolution of approximately 55 x 42 pixels.



Discovery images of Nix and Hydra

Hydra was discovered by the Hubble Space Telescope's "Pluto Companion Search Team", consisting of Hal A. Weaver, Alan Stern, Max J. Mutchler, Andrew J. Steffl, Marc W. Buie, William J. Merline, John R. Spencer, Eliot F. Young, and Leslie A. Young. The discovery images were taken on 15 May 2005, and 18 May 2005; Nix and Hydra were independently discovered by Max J. Mutchler on 15 June 2005, and Andrew J. Steffl on 15 August 2005. The discoveries were announced on 31 October 2005, after confirmation by precoveries from 2002. They were provisionally designated S/2005 P 1 (Hydra) and S/2005 P 2 (Nix).[7][8]


The name Hydra was announced on 21 June 2006, in IAU Circular 8723,[8] along with the formal designation Pluto III. The name is that of the Hydra, the nine-headed serpent that battled Hercules in Greek mythology. The nine heads of Hydra are a reference to Pluto's tenure as the ninth planet; its initial, H, refers to the Hubble Telescope, which discovered Hydra and, together with Nix, to the New Horizons mission whose safe passage was the motivation for taking the Hubble images.[9]

Orbital properties

Hydra orbits the barycenter of the system in the same plane as Charon and Nix, at a distance of about 65,000 km. Its eccentricity of 0.0059 is small, but significantly non-zero, and the largest of those of Pluto's small moons (slightly greater than that of Styx).

Hydra is in a 2:3 orbital resonance with Nix, and a 6:11 resonance with Styx (the ratios represent numbers of orbits completed per unit time; the period ratios are the inverses).[10][1] As a result of this "Laplace-like" 3-body resonance, it has conjunctions with Styx and Nix in a 5:3 ratio.

Its orbital period of 38.2 days is also close to a 1:6 orbital resonance with Charon, with the timing discrepancy being 0.3%. A hypothesis to explain the near-resonance is that it originated before the outward migration of Charon following the formation of all five known moons, and is maintained by the periodic local fluctuation of 5% in the Pluto–Charon gravitational field strength.

Like Saturn's moon Hyperion, Nix, and likely the other small Plutonian moons, Hydra rotates chaotically; its day length and rotational axis vary quickly over astronomical timescales, to the point that it regularly flips over. This is largely due to the aforementioned fluctuation of the Pluto-Charon gravitational field, as well as its irregular shape.

Physical properties

Hydra is irregular in shape, 55 × 40 km[11] in cross-section from one side. It is spectrally neutral like Charon and Nix (whereas Pluto is reddish) and is composed primarily of water ice,[12] probably ice XI.


The only detailed photographs of Hydra were taken by the New Horizons spacecraft from approximately 640,000 kilometres (400,000 mi) away during its historic flyby of the Pluto–Charon system on 14 July 2015. It also studied Hydra's surface composition, reflectivity and other basic physical properties. Hydra's reflectivity is estimated to be about 45 percent. More images and information will be downlinked from the spacecraft from 2015 to late 2016.


  1. ^ a b
  2. ^ a b The Pluto system: Initial results from its exploration by New Horizons
  3. ^ (Final preprint)
  4. ^
  5. ^
  6. ^ New Horizons flyby timeline
  7. ^ IAU Circular No. 8625 describing the discovery
  8. ^ a b IAU Circular No. 8723 naming the moons
  9. ^ Neil deGrasse Tyson, 2009, The Pluto Files
  10. ^
  11. ^
  12. ^
  • (Final preprint)

External links

  • Hydra Profile by NASA's Solar System Exploration
  • NASA's Hubble Reveals Possible New Moons Around Pluto – Hubble press release
  • Two More Moons Discovered Orbiting Pluto (
  • Pluto's Newest Moons Named Hydra and Nix (
  • Hydra at ESA/Hubble
This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.

Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.