Moons of Haumea
The
Haumea's moons are unusual in a number of ways. They are thought to be part of its extended collisional family, which formed billions of years ago from icy debris after a large impact disrupted Haumea's ice mantle. Hiʻiaka, the larger, outermost moon, has large amounts of pure water ice on its surface, which is rare among Kuiper belt objects.[1] Namaka, about one tenth the mass, has an orbit with surprising dynamics: it is unusually eccentric and appears to be greatly influenced by the larger satellite.
History
Two small
The permanent names of these moons were announced, together with that of 2003 EL61, by the
In her legend, Haumea's many children came from different parts of her body.[7] The dwarf planet Haumea appears to be almost entirely made of rock, with only a superficial layer of ice; most of the original icy mantle is thought to have been blasted off by the impact that spun Haumea into its current high speed of rotation, where the material formed into the small Kuiper belt objects in Haumea's collisional family. There could therefore be additional outer moons, smaller than Namaka, that have not yet been detected. However, HST observations have confirmed that no other moons brighter than 0.25% of the brightness of Haumea exist within the closest tenth of the distance (0.1% of the volume) where they could be held by Haumea's gravitational influence (its Hill sphere).[8] This makes it unlikely that any more exist.
Surface properties
Hiʻiaka is the outer and, at roughly 310 km in diameter, the larger and brighter of the two moons.[9] Strong absorption features observed at 1.5, 1.65 and 2 µm in its infrared spectrum are consistent with nearly pure crystalline water ice covering much of its surface. The unusual spectrum, and its similarity to absorption lines in the spectrum of Haumea, led Brown and colleagues to conclude that it was unlikely that the system of moons was formed by the gravitational capture of passing Kuiper belt objects into orbit around the dwarf planet: instead, the Haumean moons must be fragments of Haumea itself.[10]
The sizes of both moons are calculated with the assumption that they have the same infrared albedo as Haumea, which is reasonable as their spectra show them to have the same surface composition. Haumea's albedo has been measured by the Spitzer Space Telescope: from ground-based telescopes, the moons are too small and close to Haumea to be seen independently.[11] Based on this common albedo, the inner moon, Namaka, which is a tenth the mass of Hiʻiaka, would be about 170 km in diameter.[12]
The Hubble Space Telescope (HST) has adequate angular resolution to separate the light from the moons from that of Haumea. Photometry of the Haumea triple system with HST's NICMOS camera has confirmed that the spectral line at 1.6 µm that indicates the presence of water ice is at least as strong in the moons' spectra as in Haumea's spectrum.[11]
The moons of Haumea are too faint to detect with telescopes smaller than about 2 metres in aperture, though Haumea itself has a visual magnitude of 17.5, making it the third-brightest object in the Kuiper belt after Pluto and Makemake, and easily observable with a large amateur telescope.
Orbital characteristics
Hiʻiaka orbits Haumea nearly circularly every 49 days.[9] Namaka orbits Haumea in 18 days in a moderately elliptical, non-Keplerian orbit, and as of 2008 was inclined 13° with respect to Hiʻiaka, which perturbs its orbit.[4] Because the impact that created the moons of Haumea is thought to have occurred in the early history of the Solar System,[13] over the following billions of years it should have been tidally damped into a more circular orbit. Namaka's orbit has likely been disturbed by orbital resonances with the more-massive Hiʻiaka due to converging orbits as they moved outward from Haumea due to tidal dissipation.[4] They may have been caught in and then escaped from orbital resonance several times; they currently are in or at least close to an 8:3 resonance.[4] This resonance strongly perturbs Namaka's orbit, which has a current precession of its argument of periapsis by about −6.5° per year, a precession period of 55 years.[8]
At present, the orbits of the Haumean moons appear almost exactly edge-on from Earth, with Namaka having periodically
Label [note 1] |
Name ( pronunciation )
|
Mean diameter (km) |
Mass (×1018 kg) |
Semi-major axis (km) |
Orbital period (days) |
Eccentricity | Inclination (°)[note 2] | Discovery date | |
---|---|---|---|---|---|---|---|---|---|
(ring) | ≈ 70 | 2285±8[20] | 0.489438±0.000012[20][a] | [approximately same as Haumea's equator] | January 2017 | ||||
II | Namaka | /nɑːˈmɑːkə/ | ≈ 170? | 1.79±1.48[8] (≈ 0.05% Haumea) |
25657±91[8] | 18.2783±0.0076[8][note 3] | 0.249±0.015[8][note 4] | 113.013±0.075[8] (13.41±0.08 from Hiʻiaka)[note 4] |
June 2005 |
I | Hiʻiaka | /hiːʔiːˈɑːkə/ | ≈ 310 | 17.9±1.1[8] (≈ 0.5% Haumea) |
49880±198[8] | 49.462±0.083[8][note 3] | 0.0513±0.0078[8] | 126.356±0.064[8] | January 2005 |
Notes
- ^ Label refers to the Roman numeral attributed to each moon in order of their discovery.[19]
- ^ Orbital inclinations of Namaka and Hiʻiaka are with respect to Haumea's orbit.
- ^ a b Using Kepler's third law.
- ^ a b As of 2008: Namaka's eccentricity and inclination are variable due to perturbation.
- ^ Based on a 3:1 resonance with Haumea's rotation period.
References
- S2CID 17831967.
- S2CID 119408563.
- New York Times. Retrieved 12 October 2008.
- ^ a b c d e D. Ragozzine; M. E. Brown; C. A. Trujillo; E. L. Schaller. "Orbits and Masses of the 2003 EL61 Satellite System". AAS DPS conference 2008. Archived from the original on 18 July 2013. Retrieved 17 October 2008.
- ^ "News Release – IAU0807: IAU names fifth dwarf planet Haumea". International Astronomical Union. 17 September 2008. Retrieved 18 September 2008.
- ^ "Dwarf Planets and their Systems". US Geological Survey Gazetteer of Planetary Nomenclature. Retrieved 17 September 2008.
- ^ ISBN 1-57607-894-9.
- ^ S2CID 15310444.
- ^ S2CID 2578831. Retrieved 19 October 2011.
- ^ Michael E. Brown. "The largest Kuiper belt objects" (PDF). Caltech. Retrieved 19 September 2008.
- ^ S2CID 119273925.
- ^ "(136108) Haumea, Hi'iaka, and Namaka". Johnstonsarchive.net. Retrieved 1 February 2009.
- S2CID 4430027.
- ^ "IAU Circular 8949". International Astronomical Union. 17 September 2008. Archived from the original on 11 January 2009. Retrieved 6 December 2008.
- ^ Brown, M. "Mutual events of Haumea and Namaka". Retrieved 18 February 2009.
- ISBN 978-0-12-088589-3. Retrieved 17 October 2008.
- ^ Bibcode:2008DPS....40.3608F.
- ^ Mike Brown (18 May 2008). "Moon shadow Monday (fixed)". Mike Brown's Planets. Retrieved 27 September 2008.
- ^ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 23 June 2022.
- ^ S2CID 205260767.