We are pleased to provide comprehensive multimedia resources to support your New Horizons reporting process. Please find and use the following resources in our digital media kit: articles, biographies, video, high-resolution photography for print and online purposes, and background information.
In addition to these resources, interviews with Planetary Society spokespeople are available upon request. To schedule an interview, or to be added to our media mailing list, please contact our Director of Communications Erin Greeson at email@example.com or +1-626-793-5100.
All press materials are provided by The Planetary Society, unless otherwise credited.
Nearly ten years after its launch, the New Horizons spacecraft will reach its closest encounter with Pluto on July 14, 2015. NASA and the world science community will celebrate the landmark at the Applied Physics Laboratory (APL) at Johns Hopkins University, as well as at “PlutoPalooza” events around the world.
Three months ago, I posted an article explaining what to expect during the flyby. This is a revised version of the same post, with some errors corrected, the expected sizes of Nix and Hydra updated, and times of press briefings added.
Pluto is reluctant to give up its secrets. Last week at the American Geophysical Union meeting I attended sessions featuring results from the New Horizons mission, and most of the presentations could be summed up thusly: the data sets are terrific, but there are still a lot of Pluto features that have scientists scratching their heads.
For my first post on results from the Division for Planetary Sciences meeting, I'm going to tell you about Pluto's small moons: Styx, Nix, Kerberos, and Hydra, their bright colors and wacky rotation states.
New Horizons—what will be NASA’s greatest success of 2015—was cancelled multiple times in its early life, and many times before that in its previous incarnations. A mission to Pluto was not inevitable, despite the overwhelming scientific and public excitement.
Casey is the public face of The Planetary Society's efforts to advance planetary exploration, planetary defense, and the search for life. He is a trusted expert in space policy and works to demystify the political and policy processes behind space exploration.
The Long-Range Reconnaissance Imager (LORRI) took this photo of 2014 MU69 on 1 January 2019 at 5:01 UT, just 30 minutes before closest approach, from a range of 28,000 kilometers, with an original scale of 140 meters per pixel. It has been sharpened and enlarged.
This photo combines a color image taken by New Horizons' Ralph MVIC instrument with a LORRI image taken near the same time. It is an enhanced color image, featuring infrared, red, and blue channels. It was taken at a distance of 137,000 kilometers on 1 January 2019 at 04:08 UT, slightly more than an hour before closest approach. Note the reduced red coloring at the neck of the object.
Binary systems formed when aggregates of pebbles accreted into separated binaries under the force of gravity. Eventually, the orbit destabilized and the two pieces came into contact at a very slow speed of 80 centimeters per second or so.