NIX (MOON)
| Artist conception of Hydra (foreground), Pluto and Charon (background), and Nix (bright dot center left) | |
| Discovery | |
|---|---|
| Discovered by | Hubble Space Telescope Pluto Companion Search Team |
| Discovered in | June 2005 |
| Nictian orbital characteristics[1] | |
| Semi-major axisa | 48 675 ± 120 km |
| Eccentricity | 0.002 ± 0.002 |
| Orbital period | 24.856 ± 0.001 d |
| Inclinationb | 0.04° ± 0.22° |
| Parent body | Pluto |
| Physical characteristics | |
| Mean diameter | 44 − 130 km |
| Mass | 5×1016 − 2×1018 kg[2] |
| Mean density | ''unknown'' |
| Rotation period | ''unknown'' |
| Axial tilt | ''unknown'' |
| 'Albedo' | 0.04 − 0.35 (assumed) |
| Surface temp. | 33-55 K |
| Atmosphere | none |
| ---- | |
'Nix' ''(niks)'' is a natural satellite of Pluto. It was discovered along with Hydra in June 2005 by the Hubble Space Telescope Pluto Companion Search Team, composed of Hal A. Weaver, S. 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 May 15, 2005 and May 18, 2005; the moons were independently discovered by Max J. Mutchler on June 15, 2005 and Andrew J. Steffl on August 15, 2005. The discoveries were announced on October 31, 2005, after confirmation by precoveries from 2002. The moons were provisionally designated 'S/2005 P 1' (Hydra) and 'S/2005 P 2' (Nix).[3]
The moon follows a circular orbit in the same plane as Charon. Its orbital period of 24.9 days is close to a 1:4 orbital resonance with Charon, but the timing discrepancy is 2.7%, which suggests that there is no active resonance. A hypothesis explaining such a near-resonance is that it originated before the outward migration of Charon following the formation of all three known moons, and is maintained by the periodic local fluctuation of 9% in the Pluto-Charon gravitational field strength.
Although its size has not been directly measured, the moon is calculated to have a diameter of between 40 km (25 mi), if its reflectivity is similar to Charon's 35%, and 130 km (80 mi), if it has a reflectivity of 4%, like the darkest Kuiper Belt Objects. Nix is slightly fainter than Hydra, suggesting that it is somewhat smaller in size.
Early research appeared to show that Nix was reddish like Pluto and unlike the other moons, but more recent reports have been that it is grey like the remaining satellites.[4]
Nix is to be visited along with Pluto by the ''New Horizons'' mission in 2015.
The formal name "Nix", from the Greek goddess of darkness and night, and mother of Charon, was announced on June 21, 2006 on IAU Circular 8723,[5] where the designation 'Pluto II' is also given. Together with Hydra, Pluto's third moon, the initials are those of the ''New Horizons'' probe. The initial proposal was to use the Classical spelling Nyx, but to avoid confusion with the asteroid 3908 Nyx, this was changed to "the Egyptian spelling of the Greek name".[6]
| Contents |
| External links |
| References |
External links
★ Nix Profile by NASA's Solar System Exploration
★ Background Information Regarding Our Two Newly Discovered Satellites of Pluto – The discoverers' website
★ NASA's Hubble Reveals Possible New Moons Around Pluto – Hubble press release
★ Two More Moons Discovered Orbiting Pluto (SPACE.com)
★ Pluto's Newest Moons Named Hydra and Nix (SPACE.com)
References
1. ''Orbits and Photometry of Pluto's satellites: Charon, S/2005 P1, and S/2005 P2'' [sic], Buie, M. W., , , Astronomical Journal, 2006 (Final preprint)
2. Based on the range of diameters from Buie ''et al.'' (2006), and densities ranging from 1 g/cm³ (ice) to 2 g/cm³ (Pluto).
3. IAU Circular No. 8625 describing the discovery
4. ''The Positions, Colors, and Photometric Variability of Pluto's Small Satellites from HST Observations 2005-2006'', Stern, S. A., , , Astronomical Journal, 2006 (Final preprint)
5. IAU Circular No. 8723 naming the moons
6. Planet and Satellite Names and Discoverers
#
# The Discovery of Two New Satellites of Pluto, Weaver, H. A., , , Nature, 2006
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