  The New Horizons spacecraft provided near global observations of Pluto that
far exceed the resolution of Earth-based data sets. Most Pluto New Horizons
analysis hitherto has focused on the encounter hemisphere of Pluto (i.e., the
antiCharon hemisphere containing Sputnik Planitia). In this work, we summarize
and interpret data on the far side (i.e., the non-encounter hemisphere),
providing the first integrated New Horizons overview of the far side terrains.
We find strong evidence for widespread bladed deposits, evidence for an impact
crater about as large as any on the near side hemisphere, evidence for complex
lineations approximately antipodal to Sputnik Planitia that may be causally
related, and evidence that the far side maculae are smaller and more structured
than the encounter hemisphere maculae.
