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OBSERVATIONS OF THE NEAR-INFRARED SPECTRUM OF THE ZODIACAL LIGHT WITH CIBER

2010; IOP Publishing; Volume: 719; Issue: 1 Linguagem: Inglês

10.1088/0004-637x/719/1/394

1538-4357

Kohji Tsumura, J. Battle, J. J. Bock, Asantha Cooray, V. V. Hristov, Brian Keating, D. H. Lee, L. R. Levenson, P. Mason, Toshio Matsumoto, Shuji Matsuura, U. W. Nam, T. Renbarger, Ian Sullivan, K. Suzuki, Takehiko Wada, M. Zemcov,

Planetary Science and Exploration

Interplanetary dust (IPD) scatters solar radiation which results in the zodiacal light that dominates the celestial diffuse brightness at optical and near-infrared wavelengths. Both asteroid collisions and cometary ejections produce the IPD, but the relative contribution from these two sources is still unknown. The low resolution spectrometer (LRS) onboard the Cosmic Infrared Background ExpeRiment (CIBER) observed the astrophysical sky spectrum between 0.75 and 2.1 μm over a wide range of ecliptic latitude. The resulting zodiacal light spectrum is redder than the solar spectrum, and shows a broad absorption feature, previously unreported, at approximately 0.9 μm, suggesting the existence of silicates in the IPD material. The spectral shape of the zodiacal light is isotropic at all ecliptic latitudes within the measurement error. The zodiacal light spectrum, including the extended wavelength range to 2.5 μm using Infrared Telescope in Space (IRTS) data, is qualitatively similar to the reflectance of S-type asteroids. This result can be explained by the proximity of S-type asteroidal dust to Earth's orbit, and the relatively high albedo of asteroidal dust compared with cometary dust.