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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.
The team reported two weeks ago that the first attempts at observing 2014 MU69 were unsuccessful. But in their third try, on July 17, astronomers in Argentina saw the telltale sign of MU69's presence: a stellar wink.
What's ahead for our intrepid space explorers in 2017? It'll be the end of Cassini, but not before the mission performs great science close to the rings. OSIRIS-REx will fly by Earth, and Chang'e 5 will launch to the Moon, as a host of other spacecraft continue their ongoing missions.
Cassini is going to make a major change to its orbit, getting much close to Saturn, setting up 20 "F-ring" orbits. ExoMars will get two science orbits before beginning aerobraking. Long March 5 will have its first launch, while many Earth-observing missions, including Himawari-9 and GOES-R, will go up. But Juno science is on hold.
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.
As Director of Space Policy, Casey leads the strategic planning and implementation of the Society's policy- and advocacy-related efforts. He works closely with the Society's leadership, the Board of Directors, and other policy experts to craft the organizational positions and generate ideas about the future of space exploration.
Emily Lakdawalla, Planetary Society blogger, podcaster, webcaster, Twitterer, et cetera. Emily is considered one of the most influential and passionate space bloggers around. Emily is a planetary geologist with a unique way of blending science facts and space news with a sense of whimsy, and, yes, lots of pretty pictures!
This high-resolution swath of Pluto sweeps over the cratered plains at the west of the New Horizons’ encounter hemisphere and across numerous prominent faults, skimming the eastern margin of the dark, forbidding region informally known as Cthulhu Regio, and finally passing over the mysterious, possibly cryovolcanic edifice Wright Mons, before reaching the terminator or day-night line. Among the many notable details shown are the overlapping and infilling relationships between units of the relatively smooth, bright volatile ices from Sputnik Planum (at the edge of the mosaic) and the dark edge or “shore” of Cthulhu. The pictures in this mosaic were taken by the Long-Range Reconnaissance Imager (LORRI) in “ride-along” mode with the LEISA spectrometer, which accounts for the ‘zigzag’ or step pattern. Taken shortly before New Horizons’ July 14, 2015 closest approach to Pluto, details as small as 500 meters can be seen. (NOTE: Click on the image and ZOOM IN for optimal viewing.)
This recently received panchromatic image of Pluto’s small satellite Nix taken by the Multispectral Visible Imaging Camera (MVIC) aboard New Horizons is one of the best images of Pluto’s third-largest moon generated by the NASA mission. Taken on July 14, 2015 at a range of about 23,000 kilometers from Nix, the illuminated surface is about 19 kilometers by 47 kilometers. The unique perspective of this image provides new details about Nix’s geologic history and impact record.
On July 17, 2017 at 03:50 UTC, members of the New Horizons science team successfully observed Kuiper belt object 2014 MU69 passing in front of a background star in the constellation Sagittarius. The 24 frames in this animation were separated by 0.2 seconds apiece. In each 0.2 seconds, the shadow of 2014 MU69 passed 4 kilometers across Earth's surface. Observations like these will allow the team to constrain the size and position of the New Horizons mission's flyby target, improving the precision of their encounter planning. This animation has been processed from the originally published version to reduce noise and align the star field.
On February 28, 2007, New Horizons took this picture of Jupiter with MVIC, its color imaging instrument. Due to the nature of these observations, the Red, Blue, and NIR channels were completely saturated (they appeared bright white with no detail), but the narrow-band methane channel was well-exposed. As part of some instrument calibration work, New Horizons team member Alex Parker re-processed this archival Jupiter data using the latest approaches we developed after studying the Pluto flyby data. The new processing approach results in substantial detail enhancement.