activity
20142026
most citedThe Pluto system: Initial results from its exploration by New Horizons

485 citations · 1.2k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2026

TNFlow: Amortized Posterior Inference for Trans-Neptunian Object Surface Composition

Agastya Gaur, Cristina M. Dalle Ore, Alessandra Ricca

We present TNFlow, a transformer and normalizing flow architecture for inferring the surface composition of Trans-Neptunian Objects (TNOs) from their reflectance spectra. TNFlow is…

astro-ph.EP2023★ 7 cited

Surface Composition of Pluto's Kiladze Area and Relationship to Cryovolcanism

A. Emran, C. M. Dalle Ore, D. P. Cruikshank +1

A link between exposures of water (HO) ice with traces of an ammoniated compound (e.g., a salt) and the probable effusion of a water-rich cryolava onto the surface of Pluto…

astro-ph.EP2023

Pluto's Surface Mapping using Unsupervised Learning from Near-Infrared Observations of LEISA/Ralph

A. Emran, C. M. Dalle Ore, C. J. Ahrens +3

We map the surface of Pluto using an unsupervised machine learning technique using the near-infrared observations of the LEISA/Ralph instrument onboard NASA's New Horizons spacecra…

astro-ph.EP2020★ 175 cited

Initial results from the New Horizons exploration of 2014 MU69, a small Kuiper Belt Object

S. A. Stern, H. A. Weaver, J. R. Spencer +202

The Kuiper Belt is a distant region of the Solar System. On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU69, a Cold Classical Kuiper Belt Object, a cla…

astro-ph.EP2020★ 86 cited

Color, Composition, and Thermal Environment of Kuiper Belt Object (486958) Arrokoth

W. M. Grundy, M. K. Bird, D. T. Britt +46

The outer Solar System object (486958) Arrokoth (provisional designation 2014 MU) has been largely undisturbed since its formation. We study its surface composition using da…

astro-ph.EP2016★ 291 cited

Surface Compositions Across Pluto and Charon

W. M. Grundy, R. P. Binzel, B. J. Buratti +32

The New Horizons spacecraft mapped colors and infrared spectra across the encounter hemispheres of Pluto and Charon. The volatile ices CH, CO, and N, that dominate Pluto's…

astro-ph.EP2016★ 94 cited

The Small Satellites of Pluto as Observed by New Horizons

H. A. Weaver, M. W. Buie, B. J. Buratti +48

The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of 40…

astro-ph.EP2016★ 32 cited

Saturn's icy satellites investigated by Cassini - VIMS. IV. Daytime temperature maps

Gianrico Filacchione, Emiliano D'Aversa, Fabrizio Capaccioni +13

The spectral position of the 3.6 micron continuum peak measured on Cassini-VIMS I/F spectra is used as a marker to infer the temperature of the regolith particles covering the surf…

astro-ph.EP2015★ 485 cited

The Pluto system: Initial results from its exploration by New Horizons

S. A. Stern, F. Bagenal, K. Ennico +148

The Pluto system was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015. Pluto's surface displays diverse landforms, terrain ages, albedos…

astro-ph.EP2014★ 11 cited

Rotationally resolved spectroscopy of (20000) Varuna in the near-infrared

V. Lorenzi, N. Pinilla-Alonso, J. Licandro +2

Models of the escape and retention of volatiles by minor icy objects exclude any presence of volatile ices on the surface of TNOs smaller than ~1000km in diameter at the typical te…