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All exposures are specified with a single integration. Poston, M. Walsh, K. In addition, the density of Haumea and Quaoar is best explained in a scenario where they suffered from a high-speed collision after they differentiated and had their icy mantle fragmented Barr and Schwamb, Fraser, W. Vilenius, E. The transneptunian region has proven to be a valuable probe to test models of the formation and evolution of the solar system. Hapke, B. This is however important to pursue because it may lift some degeneracies existing among broadband color measurements several compounds may be responsible for the same color. AREPS 40, —
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For example, Barr and Schwamb suggest that two different types of collisions may explain the properties of large TNOs. These may be linked to different initial compositions. Figure 3. Lacerda, P. Jewitt, D. Barucci, M. Morbidelli Tucson: University of Arizona Press, —
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Frontiers JWST/NIRSpec Prospects on Transneptunian Objects Astronomy and Space Sciences
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A portrait of Plutino Orcus. Wavelet theory applied to the study of spectra of trans-Neptunian objects. Marsset, M.
JWST will be commissioned to observe moving solar system targets starting at the beginning of science operations in Cycle 1. In addition, Brown suggests there may be an inherent change of surface composition for objects larger than — km, possibly due to different physical processes dominating their evolution. As helpful as broadband photometry may be, it remains a proxy in terms of providing constraints of TNOs' surface composition.
Passive cooling of the telescope will be handled by a large sunshield that must be directed at the Sun at all times.
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|Statistical study of the early solar system's instability with four, five, and six giant planets.
Quaoar: a rock in the Kuiper Belt.
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Rotationally resolved spectroscopy of Varuna in the near-infrared. Colors and albedos have been the best way so far to classify and study the surface properties of a large number TNOs. We thus briefly detail this program Table 2 : because of the flux difference between both objects, the observing strategy we chose for each is different.
These compounds, however, have different diagnostic absorption features beyond 3 microns, which will be accessible from NIRSpec.