Rotationally resolved spectroscopy of dwarf planet (136472) Makemake
arXiv:1504.02350 · doi:10.1051/0004-6361/201425575
Abstract
Context. Icy dwarf planets are key for studying the chemical and physical states of ices in the outer solar system. The study of secular and rotational variations gives us hints of the processes that contribute to the evolution of their surface. Aims. The aim of this work is to search for rotational variability on the surface composition of the dwarf planet (136472) Makemake Methods. We observed Makemake in April 2008 with the medium-resolution spectrograph ISIS, at the William Herschel Telescope (La Palma, Spain) and obtained a set of spectra in the 0.28 - 0.52 μm and 0.70 - 0.95 μm ranges, covering 82% of its rotational period. For the rotational analysis, we organized the spectra in four different sets corresponding to different rotational phases, and after discarding one with low signal to noise, we analyzed three of them that cover 71% of the surface. For these spectra we computed the spectral slope and compared the observed spectral bands of methane ice with reflectances of pure methane ice to search for shifts of the center of the bands, related to the presence of CH 4 /N 2 solid solution. Results. All the spectra have a red color with spectral slopes between 20%/1000 Å and 32%/1000 Å in accordance with previously reported values. Some variation in the spectral slope is detected, pointing to the possibility of a variation in the surface content or the particle size of the solid organic compound. The absorption bands of methane ice present a shift toward shorter wavelengths, indicating that methane (at least partially) is in solid solution with nitrogen. There is no variation within the errors of the shifts with the wavelength or with the depth of the bands, so there is no evidence of variation in the CH 4 /N 2 mixing ratio with rotation. By comparing with all the available data in the literature, no secular compositional variations between 2005 and 2008 is found.
References in corpus (13)
- "TNOs are Cool": A survey of the trans-Neptunian region X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations
- Discovery of a planetary-sized object in the scattered Kuiper belt
- The Compositions of Kuiper Belt Objects
- Pluto's lower atmosphere structure and methane abundance from high-resolution spectroscopy and stellar occultations
- Short-term variability of a sample of 29 trans-Neptunian objects and Centaurs
- Methane and Nitrogen Abundances On Pluto and Eris
- Visible spectroscopy of 2003 UB313: Evidence for N2 ice on the surface of the largest TNO?
- Optical Spectroscopy of the Large Kuiper Belt Objects 136472 (2005 FY9) and 136108 (2003 EL61)
- Evidence of N2-Ice On the Surface of the Icy Dwarf Planet 136472 (2005 FY9)
- Ice Mineralogy Across and Into the Surfaces of Pluto, Triton, and Eris
- The spectrum of (136199) Eris between 350 and 2350 nm: Results with X-Shooter
- Digging Into the Surface of the Icy Dwarf Planet Eris
- Estimating the Density of Intermediate Size KBOs from Considerations of Volatile Retention
Cited by in corpus (7)
- 1I/'Oumuamua as an N2 ice fragment of an exo-pluto surface. II. Generation of N2 ice fragments and the origin of 'Oumuamua
- Discovery of a satellite of the large trans-Neptunian object (225088) 2007OR10
- Moderate D/H Ratios in Methane Ice on Eris and Makemake as Evidence of Hydrothermal or Metamorphic Processes in Their Interiors: Geochemical Analysis
- Volatile evolution and atmospheres of Trans-Neptunian Objects
- Long-term photometric monitoring of the dwarf planet (136472) Makemake
- The Spectrum of Pluto, 0.40 - 0.93 m I. Secular and longitudinal distribution of ices and complex organics
- The Dwarf Planet Makemake as seen by X-Shooter