Evidence for longitudinal variability of ethane ice on the surface of Pluto
@article{Holler2014EvidenceFL, title={Evidence for longitudinal variability of ethane ice on the surface of Pluto}, author={Bryan J. Holler and Leslie A. Young and William M. Grundy and Cathy B. Olkin and Jason C. Cook}, journal={arXiv: Earth and Planetary Astrophysics}, year={2014} }
19 Citations
Comparative Kbology: Using Surface Spectra of Triton, Pluto, and Charon to Investigate Atmospheric, Surface, and Interior Processes on Kuiper Belt Objects
- Physics
- 2016
We present the results of an investigation to determine the longitudinal (zonal) distributions and temporal evolution of ices on the surface of Triton. Between 2002 and 2014, we obtained 63 nights of…
The distribution of H2O, CH3OH, and hydrocarbon-ices on Pluto: Analysis of New Horizons spectral images
- PhysicsIcarus
- 2019
Physical state and distribution of materials at the surface of Pluto from New Horizons LEISA imaging spectrometer
- Environmental Science
- 2017
Triton’s surface ices: Distribution, temperature and mixing state from VLT/SINFONI observations
- Environmental ScienceIcarus
- 2018
Volatile Loss and Classification of Kuiper Belt Objects
- Physics, Environmental Science
- 2014
Observations indicate that some of the largest Kuiper Belt Objects (KBOs) have retained volatiles in the gas phase, which implies the presence of an atmosphere that can affect their reflectance…
Surface compositions across Pluto and Charon
- Physics, GeologyScience
- 2016
The New Horizons team presents the complex surface features and geology of Pluto and its large moon Charon, including evidence of tectonics, glacial flow, and possible cryovolcanoes, as well as their analysis of the encounter data downloaded so far.
General circulation models of the dynamics of Pluto’s volatile transport on the eve of the New Horizons encounter
- Environmental Science, Physics
- 2015
Pluto’s global surface composition through pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data
- Environmental Science, Physics
- 2017
An Atmospheric General Circulation Model for Pluto with Predictions for New Horizons
- Physics
- 2015
Results are presented from a 3-D Pluto general circulation model that includes a subsurface model and volatile cycle. Conductive heating and cooling, non-local thermodynamic equilibrium (non-LTE)…
References
SHOWING 1-10 OF 46 REFERENCES
Near-infrared spectral monitoring of Pluto’s ices: Spatial distribution and secular evolution
- Environmental Science, Physics
- 2013
Distribution and Evolution of CH4, N2, and CO Ices on Pluto's Surface: 1995 to 1998
- Physics, Environmental Science
- 2001
Abstract We present new near-infrared spectra of the planet Pluto obtained at Lowell Observatory on 83 nights during 1995–1998. The dense temporal sampling of our observations enables us to measure…
Ethane on Pluto and Triton
- Physics
- 2005
New spectra of Pluto were obtained with the Gemini Near-Infrared Spectrometer (GNIRS) on the Gemini South 8-m telescope covering the region 1.9-2.5 µm. We have analyzed these data and two spectra of…
Exploring the spatial, temporal, and vertical distribution of methane in Pluto's atmosphere
- Environmental Science, Physics
- 2015
Evidence for Methane Segregation at the Surface of Pluto
- Physics
- 2013
Abstract In May 1995, a set of spectrophotometric curves of the system Pluto–Charon were recorded with the UKIRT telescope equipped with the spectrometer CGS4. The spectra cover the near-infrared…
Near-Infrared Spectroscopy of Charon: Possible Evidence for Cryovolcanism on Kuiper Belt Objects
- Geology
- 2006
We present the first reported adaptive optics spectra of Charon in the H and K bands, which examine the anti-Pluto and sub-Pluto hemispheres. The ice temperature is estimated at 40-50 K, based on the…
Near-infrared spectral monitoring of Triton with IRTF/SpeX II: Spatial distribution and evolution of ices
- Physics, Environmental Science
- 2010
Pluto's Non-isothermal Surface
- Physics, Geology
- 2000
We report on repeated far-infrared photometric observations of the Pluto–Charon system conducted in 1997 with the Infrared Space Observatory (ISO). These observations have led to the first detection…