The near-infrared spectrum of (50000) Quaoar obtained at the Keck Observatory shows distinct absorption features of crystalline water ice, solid methane, and ethane, and possibly other higher order hydrocarbons. Quaoar is only the fifth Kuiper Belt object (KBO) on which volatile ices have been detected. The small amount of methane on an otherwise water ice-dominated surface suggests that Quaoar is a transition object between the dominant volatile-poor small KBOs and the few volatile-rich large KBOs such as Pluto and Eris
The dark, reddish tinged surfaces of icy bodies in the outer solar system are usually attributed to ...
We report the detection of crystalline water ice on the surface of 2003 EL_(61). Reflectance spectra...
Orcus is an intermediate-size 1000 km-scale Kuiper belt object (KBO) in 3:2 mean-motion resonance w...
The near-infrared spectrum of (50000) Quaoar obtained at the Keck Observatory shows distinct absorpt...
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significa...
Recent discoveries have shown that the very largest Kuiper Belt objects—Eris, 2005 FY9, and Sedna—ar...
(50000) Quaoar, one of the largest Trans-neptunian objects, is comparable in size to Pluto's moon Ch...
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significa...
International audienceAims: The objective of this work is to investigate the physical properties of ...
Visible and near-IR observations of the Kuiper Belt Object (136472) 2005 FY_9 have indicated the pre...
We present high signal precision optical reflectance spectra of the large Kuiper belt objects 2005 F...
We present high signal precision optical reflectance spectra of the large Kuiper Belt objects 2005 F...
The surprisingly complex dynamical distribution of small bodies among and beyond the orbits of the p...
International audienceOrcus is an intermediate-size 1000 km-scale Kuiper belt object (KBO) in 3:2 me...
The dark, reddish tinged surfaces of icy bodies in the outer solar system are usually attributed to ...
We report the detection of crystalline water ice on the surface of 2003 EL_(61). Reflectance spectra...
Orcus is an intermediate-size 1000 km-scale Kuiper belt object (KBO) in 3:2 mean-motion resonance w...
The near-infrared spectrum of (50000) Quaoar obtained at the Keck Observatory shows distinct absorpt...
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significa...
Recent discoveries have shown that the very largest Kuiper Belt objects—Eris, 2005 FY9, and Sedna—ar...
(50000) Quaoar, one of the largest Trans-neptunian objects, is comparable in size to Pluto's moon Ch...
We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significa...
International audienceAims: The objective of this work is to investigate the physical properties of ...
Visible and near-IR observations of the Kuiper Belt Object (136472) 2005 FY_9 have indicated the pre...
We present high signal precision optical reflectance spectra of the large Kuiper belt objects 2005 F...
We present high signal precision optical reflectance spectra of the large Kuiper Belt objects 2005 F...
The surprisingly complex dynamical distribution of small bodies among and beyond the orbits of the p...
International audienceOrcus is an intermediate-size 1000 km-scale Kuiper belt object (KBO) in 3:2 me...
The dark, reddish tinged surfaces of icy bodies in the outer solar system are usually attributed to ...
We report the detection of crystalline water ice on the surface of 2003 EL_(61). Reflectance spectra...
Orcus is an intermediate-size 1000 km-scale Kuiper belt object (KBO) in 3:2 mean-motion resonance w...