The New Horizons (NH) flyby of the Pluto–Charon binary planet and its system of four small
surrounding satellites in mid-2015 revolutionized our knowledge of this distant planet and its …

We provide the first solar system wide compendium of speleogenic processes and products.
An examination of 15 solar system bodies revealed that six cave‐forming processes occur …

The flyby of Pluto and Charon by the New Horizons spacecraft provided high-resolution
images of cratered surfaces embedded in the Kuiper belt, an extensive region of bodies …

Newly processed global imaging and topographic map** of Uranus's five major satellites
reveal differences and similarities to mid-sized satellites at Saturn and Pluto. Three modes of …

Pluto is thought to possess a present-day ocean beneath a thick ice shell. It has generally
been assumed that Pluto accreted from cold material and then later developed its ocean due …

A new global high-resolution stereogrammetric and photogrammetric topographic map and
updated 3-color global mosaic of Enceladus reveal that the shape of this active icy ocean …

We use an existing thermal evolution model to assess the plausibility of subsurface oceans
on the moons of Uranus. We adopt a conservative approach neglecting tidal heating and …

Abstract The New Horizons spacecraft returned images and compositional data showing
that terrains on Pluto span a variety of ages, ranging from relatively ancient, heavily cratered …

Context. The tenuous nitrogen (N 2) atmosphere on Pluto undergoes strong seasonal effects
due to high obliquity and orbital eccentricity, and has recently (July 2015) been observed by …

Abstract The New Horizons encounter with the Pluto system revealed Pluto to have an
extremely spatially variable surface with expansive dark, bright, and intermediate terrains …