Evaluation of short-term temporal evolution of Pluto's surface composition from 2014-2017 with APO/TripleSpec

In this work we present the results of a spectral observing campaign of Pluto to search for temporal changes in surface composition on 1- to 3-year timescales. Near-infrared spectra of Pluto were obtained from June 2014 to August 2017 with the TripleSpec cross-dispersed spectrograph at the Apache Point Observatory's 3.5-meter Astrophysical Research Consortium (ARC) telescope. Observations were requested in order to obtain spectra of approximately the same sub-observer hemisphere \(\sim\)14 months apart, thus removing the effects of viewing geometry and rotation phase. Comparison of the CH\(_4\) (methane) band areas and band center shifts between each component of these "matched pairs" revealed a surface in transition. Band areas for the 1.66 and 1.72 \(\mu\)m CH\(_4\) absorption features exhibited a \(>\)5-\(\sigma\) increase between 2014-06-17 and 2015-08-19, corresponding to a sub-observer hemisphere centered at \(\sim\)280\(^{\circ}\)E, with the latter date only 1 month after the New Horizons flyby of Pluto. The majority of matched pairs were obtained of the anti-Charon hemisphere, home to the bright, volatile-rich Sputnik Planitia, and did not present statistically significant changes in CH\(_4\) band areas. CH\(_4\) band center shifts, which provide information on the mixing state of CH\(_4\) and N\(_2\) in solid solution, were calculated between components of each matched pair, with no significant band shifts detected. The favored explanation for these combined results is the sublimation of more-volatile N\(_2\) from the northern latitudes of Pluto in the lead-up to northern hemisphere summer solstice in 2029, leading to an increase in CH\(_4\) concentration.