Namaka is the faint spot near the bottom of the photo, directly below Haumea (center), in this Keck telescope image.
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Discovery
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| Discovered by | Michael E. Brown, Chad Trujillo, David Rabinowitz, et al. |
| Discovery date | 30 June 2005 |
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Designations
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| MPC designation | Haumea II Namaka |
| Pronunciation | /nɑːˈmɑːkə/,[1] or as in Hawaiian Nāmaka [naːˈmɐkə] |
| Alternate name(s) | (136108) 2003 EL61 II, S/2005 (2003 EL61) 2 |
| Semi-major axis | 25657 ± 91 km[2] |
| Eccentricity | 0.249 (in 2009; variable) |
| Orbital period | 18 day[3] |
| Inclination | 13° relative to Hiʻiaka (in 2008; variable) |
| Satellite of | Haumea |
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Physical characteristics
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| Mean radius | ~85 km (if albedo is same as primary's 0.7±0.1) |
| Mass | 1.79 ± 1.48×1018 kg[2] (0.05% the mass of Haumea) |
| Mean density | (assumed to be near 1) |
| Rotation period | (unknown) |
| Axial tilt | (unknown) |
| Albedo | (unknown) |
| Temperature | 32±3 K |
| Apparent magnitude | 4.6 difference from primary's 17.3[4] |
Namaka is the smaller, inner moon of the dwarf planet Haumea. It is named after Nāmaka, one of the daughters of Haumea, the goddess of the sea in Hawaiian mythology.
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Contents
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Namaka was discovered on 30 June 2005 and announced on November 29, 2005.[5] It was nicknamed "Blitzen" by the discovery team before receiving an official name.
Namaka is only 1.5% as bright as its dwarf planet Haumea[6] and is about 0.05% its mass. If it turns out to have a similar albedo, it would be about 170 km in diameter.[4] Photometric observations indicate that its surface is made of water ice.[6]
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