Pluto
Hubble observations record strong large-scale brightness differences across Pluto's surface at unprecedented spatial resolution.
Follow Marc Buie through 9 dated historical records for United States of America.
A chronological timeline drawn from matching World History Database records.
Hubble observations record strong large-scale brightness differences across Pluto's surface at unprecedented spatial resolution.
The Hubble surface map confirms a dark equatorial belt and bright polar regions on Pluto.
Hubble images of the Pluto system provide an earlier comparison epoch later used in searches for faint satellites.
Hubble completes a series of observations later combined into detailed maps showing changes in Pluto's surface appearance.
New Hubble maps assembled from 2002-2003 observations reveal measurable changes in Pluto's surface color and brightness patterns.
Buie identifies the object later named Arrokoth in Hubble images obtained for the New Horizons target search.
Buie helps lead a Hubble search for small Kuiper Belt objects reachable by New Horizons after its Pluto encounter.
The Hubble search identifies three Kuiper Belt objects with trajectories potentially reachable by New Horizons after Pluto.
Buie helps lead stellar-occultation observations that constrain the size and shape of 2014 MU69 before the New Horizons flyby.
These dates and descriptions come from the historical_events database. Exact duplicate records have been collapsed. Names are grouped by the country, Name 2 and Name 1 fields; records with missing Name 2 cannot be reliably assigned to an individual biography. Check the underlying sources before formal citation.