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TIME-RESOLVED NEAR-INFRARED PHOTOMETRY OF EXTREME KUIPER BELT OBJECT HAUMEA

2009; Institute of Physics; Volume: 137; Issue: 2 Linguagem: Inglês

10.1088/0004-6256/137/2/3404

1538-3881

Pedro Lacerda,

Planetary Science and Exploration

We present time-resolved near-infrared (J and H) photometry of the extreme Kuiper belt object (136108) Haumea (formerly 2003 EL61) taken to further investigate rotational variability of this object. The new data show that the near-infrared peak-to-peak photometric range is similar to the value at visible wavelengths, ΔmR = 0.30 ± 0.02 mag. Detailed analysis of the new and previous data reveals subtle visible/near-infrared color variations across the surface of Haumea. The color variations are spatially correlated with a previously identified surface region, redder in B − R and darker than the mean surface. Our photometry indicates that the J − H colors of Haumea (J − H = −0.057 ± 0.016 mag) and its brightest satellite Hi'iaka (J − H = −0.399 ± 0.034 mag) are significantly (greater than 9σ) different. The satellite Hi'iaka is unusually blue in J − H, consistent with strong 1.5 μm water-ice absorption. The phase coefficient of Haumea is found to increase monotonically with wavelength in the range 0.4 < λ < 1.3. We compare our findings with other solar system objects and discuss implications regarding the surface of Haumea.