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We present a model confirming previous results regarding the presence of crystalline H2O and CH4 ice, as well as C 2H6 and organic materials, on the surface of this distant icy body. What we do. June 4 2002 Discoverer. You could also do it yourself at any point in time.It will enhance any encyclopedic page you visit with the magic of the WIKI 2 technology.According to Brown, Quaoar is correctly pronounced with three syllables. A.} We attempt a measurement of the temperature and find that stronger constraints on the composition are needed to obtain a precise determination. Irradiated crystalline H2O could be the source of small-grained amorphous H2O ice. Trujillo's website on Quaoar gives a three-syllable pronunciation, Polar dimension calculated by multiplying the measured equatorial diameter In the convention for minor planet provisional designations, the first letter represents the half-month of the year of discovery while the second letter and numbers indicate the order of discovery within that half-month. 50000 Quaoar. 285.97 Earth Years Discovery Date. We present new near-infrared (3.6 and 4.5 μm) photometric data obtained with the Spitzer Space Telescope.
Because of its distance from the Sun, Quaoar is expected to have preserved, to a degree, its original composition. Quaoar lies about 42 AU (6.5 billion kilometers) away from us, more distant than either Pluto or Neptune, and moves in a nearly circular orbit with an eccentricity of less than 0.04, meaning that its distance from the Sun changes by only about 8% over the course of a Quaoar year (equal to 285 Earth years). Model fits indicate that N2 may be a significant component, along with a component that is bright at < 3.3 μm, which we suggest at this time could be amorphous H2O ice in tiny grains or thin grain coatings. Conclusions. Because of its distance from the Sun, Quaoar is expected to have preserved, to a degree, its original composition.
The albedo and composition of Quaoar, in particular the presence of N2, if confirmed, make this TNO quite similar to Triton and Pluto.UR - http://www.scopus.com/inward/record.url?scp=67650931810&partnerID=8YFLogxKUR - http://www.scopus.com/inward/citedby.url?scp=67650931810&partnerID=8YFLogxK"We use cookies to help provide and enhance our service and tailor content.
50000 Quaoar – a cubewano and probable dwarf planet in the distant icy Kuiper Belt.
C. Morea Dalle Ore, M. A. Barucci, J. P. Emery, D. P. Cruikshank, L. V. Dalle Ore, F. Merlin, A. Alvarez-Candal, C. De Bergh, Aims.
Our goals are to determine to what degree this is true and to shed light on the chemical evolution of this icy body.Methods. In the case for These data complement high resolution, low signal-to-noise spectroscopic and photometric data obtained in the visible and near-infrared (0.4-2.3 μm) at VLT-ESO and provide an excellent set of constraints in the model calculation process. We also attempt to determine the temperature of H2O ice making use of the crystalline feature at 1.65 μm.
Our goals are to determine to what degree this is true and to shed light on the chemical evolution of this icy body.Methods. We perform spectral modeling of the entire wavelength range - from 0.3 to 4.5 μm by means of a code based on the Shkuratov radiative transfer formulation of the slab model. Conclusions.
We present a model confirming previous results regarding the presence of crystalline H2O and CH4 ice, as well as C 2H6 and organic materials, on the surface of this distant icy body. What we do. June 4 2002 Discoverer. You could also do it yourself at any point in time.It will enhance any encyclopedic page you visit with the magic of the WIKI 2 technology.According to Brown, Quaoar is correctly pronounced with three syllables. A.} We attempt a measurement of the temperature and find that stronger constraints on the composition are needed to obtain a precise determination. Irradiated crystalline H2O could be the source of small-grained amorphous H2O ice. Trujillo's website on Quaoar gives a three-syllable pronunciation, Polar dimension calculated by multiplying the measured equatorial diameter In the convention for minor planet provisional designations, the first letter represents the half-month of the year of discovery while the second letter and numbers indicate the order of discovery within that half-month. 50000 Quaoar. 285.97 Earth Years Discovery Date. We present new near-infrared (3.6 and 4.5 μm) photometric data obtained with the Spitzer Space Telescope.
Because of its distance from the Sun, Quaoar is expected to have preserved, to a degree, its original composition. Quaoar lies about 42 AU (6.5 billion kilometers) away from us, more distant than either Pluto or Neptune, and moves in a nearly circular orbit with an eccentricity of less than 0.04, meaning that its distance from the Sun changes by only about 8% over the course of a Quaoar year (equal to 285 Earth years). Model fits indicate that N2 may be a significant component, along with a component that is bright at < 3.3 μm, which we suggest at this time could be amorphous H2O ice in tiny grains or thin grain coatings. Conclusions. Because of its distance from the Sun, Quaoar is expected to have preserved, to a degree, its original composition.
The albedo and composition of Quaoar, in particular the presence of N2, if confirmed, make this TNO quite similar to Triton and Pluto.UR - http://www.scopus.com/inward/record.url?scp=67650931810&partnerID=8YFLogxKUR - http://www.scopus.com/inward/citedby.url?scp=67650931810&partnerID=8YFLogxK"We use cookies to help provide and enhance our service and tailor content.
50000 Quaoar – a cubewano and probable dwarf planet in the distant icy Kuiper Belt.
C. Morea Dalle Ore, M. A. Barucci, J. P. Emery, D. P. Cruikshank, L. V. Dalle Ore, F. Merlin, A. Alvarez-Candal, C. De Bergh, Aims.
Our goals are to determine to what degree this is true and to shed light on the chemical evolution of this icy body.Methods. In the case for These data complement high resolution, low signal-to-noise spectroscopic and photometric data obtained in the visible and near-infrared (0.4-2.3 μm) at VLT-ESO and provide an excellent set of constraints in the model calculation process. We also attempt to determine the temperature of H2O ice making use of the crystalline feature at 1.65 μm.
Our goals are to determine to what degree this is true and to shed light on the chemical evolution of this icy body.Methods. We perform spectral modeling of the entire wavelength range - from 0.3 to 4.5 μm by means of a code based on the Shkuratov radiative transfer formulation of the slab model. Conclusions.