0:01 there's a mysterious Zone far out in our
0:04 solar system it's a region of ice worlds
0:08 some solitary some with
0:11 moons their names may be unfamiliar AIS
0:16 maake haa but they hold Clues to all our
0:20 Origins and the first of these worlds
0:23 and the one will reach in 2015 is the
0:26 king of the Kyper belt Pluto the long
0:30 journey of NASA's New Horizons Mission
0:32 began in 2006 aboard America's biggest
0:36 baddest rocket tricked out with every
0:38 conceivable booster we built a very
0:40 light spacecraft and bought a very large
0:42 launch vehicle and the combination is
0:44 ferocious but in some sense it All Began
0:47 in 1930 with Clyde tomall 24 years old
0:51 and fresh off a farm in Kansas but
0:53 willing to spend long hours scanning
0:56 starfields to find a moving point of
0:58 light he Humanity's first glimpse of
1:01 Pluto the dream of actually getting to
1:04 Pluto began with a 6-year-old boy in
1:06 love with science who grew up to lead a
1:09 team of brilliant researchers and
1:11 Engineers with dogged persistence
1:13 through Decades of Planning and Building
1:16 and testing a Race Against Time just to
1:19 get to the Launchpad exploring the outer
1:21 solar system because it so far takes a
1:25 lot of time it requires a lot of
1:27 patience a lot of dedication a lot of
1:29 perseverance
1:30 but it's a frontier assuming all goes
1:33 well at Pluto NASA may choose to extend
1:35 the adventure further out into the Kyper
1:38 belt the Solar System's mysterious third
1:40 Zone this is maybe the one chance in my
1:43 lifetime that we're going to get a
1:44 spacecraft out there and look up close
1:46 at one of these kelt objects December
1:49 6th 2014 we
1:53 have New Horizons wakes up for the last
1:56 time from hibernation New Horizons is
1:58 speeding towards Pluto at a phenomenal
2:01 rate and we can't wait for it to get
2:03 there January 27th 2015 6 months of
2:07 approach science begins July 14th
2:11 2015 New Horizon's Long Journey 3
2:15 billion miles 9 years in flight and 85
2:19 years of speculation about Pluto
2:22 climaxes in one day of close approach
2:25 and flyby you know we're rounding third
2:27 base and we're headed home the dream the
2:30 adventure the promise of Discovery
2:32 that's what makes 2015 the year of
2:39 [Music]
2:46 Pluto studying Pluto and its neighbors
2:48 from Earth is one of the toughest
2:50 challenges in
2:52 astronomy it takes the largest
2:55 telescopes and most advanced
2:57 instrumentation on the planet and and
2:59 it's tough even for the Hubble Space
3:03 Telescope and it takes time from the
3:06 discovery of Pluto in 1930 to NASA
3:09 approving the New Horizons mission in
3:11 2001 to arriving at the planet in 2015
3:16 it's been 85 years and time passing is
3:19 definitely an actor in our story but
3:22 it's the combination of human skill
3:24 Cutting Edge image processing and sheer
3:26 bloody-minded persistence that has
3:28 resulted in the most important
3:31 discoveries and that's a tale as true
3:33 today as back in 1930 when Pluto was
3:36 first found by Clyde
3:39 Tomba in 2011 at The seti Institute near
3:43 San Francisco Mark shalter used Hubble
3:46 data to discover two new moons around
3:48 Pluto although he was actually looking
3:51 for possible Rings Showalter has found
3:54 Rings associated with small moons around
3:56 other planets and that was kind of the
3:58 motivation for uh checking out Pluto
4:00 it's got two little satellites
4:02 satellites raise clouds of dust let's
4:04 see what might be there it's easy to
4:06 take artistic license to show what
4:08 Pluto's Rings might look like in reality
4:11 it's incredibly hard to see faint
4:13 objects against the dense background
4:15 Starfield and the glare from Pluto and
4:18 its large Moon Kon we came up with this
4:21 trick where you take the images and then
4:22 you rotate the camera 90° you take more
4:24 images and if you do that all just right
4:26 you can do this thing where all that
4:28 glare cancels out and what we're left
4:30 with is just the Rings we can think of
4:31 it as a stack of images think of it as
4:33 like a cube looking down so let's uh
4:35 let's turn it on its side so now if we
4:38 start peeling off the layers and looking
4:40 downward through the stack things
4:42 suddenly become much much cleaner for
4:44 example Hydra and Nyx show up very very
4:46 cleanly but the thing that immediately
4:48 caught my eye was this little dot right
4:50 there it's not a perfectly Sharp hot
4:52 pixel like over here and that's what
4:54 made it pretty convincing to me that we
4:56 had seen a very small moon of Pluto that
4:59 nobody had seen before to be sure you've
5:01 detected a real moon or Planet you have
5:04 to show it's moving unlike the
5:05 background Stars the thing that makes
5:07 moons distinctive is if we come back
5:09 later they'd all have shifted because
5:11 they all orbit the central Planet this
5:13 required a great deal of patience to
5:15 then wait about 6 days until we got our
5:17 next set of observations of the Pluto
5:19 system sure enough the object was still
5:21 there it had moved by just about the
5:23 right amount to be something orbiting
5:24 Pluto and we knew we had a moon next
5:27 year sh Walter and colleagues went back
5:29 and built on Lessons Learned to see what
5:32 else might be there summer
5:35 2012 now Mark had 15 more days of Hubble
5:38 observations now what you can see here
5:41 are three time steps each of those time
5:44 steps is actually about 45 minutes of
5:46 data does that means it's long enough
5:48 that the Little Moons move it's moving
5:50 back and forth in the three frame
5:51 sequence Hydra is moving NYX is moving I
5:54 mean it doesn't take a rocket scientist
5:56 to say that that looks like a little
5:57 moon of Pluto it's moving just the way
5:59 the other s are they're all going around
6:01 the planet in the same direction and so
6:03 was just a couple of weeks later that we
6:05 made the announcement that the fifth
6:06 Moon had been discovered patience
6:09 persistence Ingenuity that was exactly
6:12 what led to the discovery of Pluto back
6:14 in
6:15 1930 in Kansas in the 1920s Clyde Tomba
6:19 grew up in hard times and built
6:21 telescopes using leftover farm
6:24 implements to check the accuracy of his
6:27 best telescope he sent drawing of Mars
6:30 and Jupiter to the L observatory in
6:32 Flagstaff Arizona they were looking for
6:35 staff and he was hired along with
6:38 observing the Stars he stoked the
6:41 furnace and shoveled snow but one
6:44 assignment made history day after day
6:47 he'd use this machine known as a blink
6:50 comparator to look for anything in his
6:53 images that moved it was tedious
6:56 painstaking work but on plates taken on
6:58 January 23rd and 29th and analyzed in
7:02 February he saw a small dot that did
7:05 move against the fixed Stars announcing
7:09 the results after careful confirmation
7:11 The Observatory made it easy to find the
7:14 new planet by adding arrows this is an
7:17 incredible work of observational
7:19 astronomy and having done something
7:21 similar but with much more powerful
7:22 tools I can really appreciate his
7:24 achievement for decades Pluto remained
7:27 more or less a point of life light but
7:30 in the mid '70s Dale crook shank and
7:33 colleagues attached cameras with
7:34 infrared filters to a telescope at kit
7:38 Peak detectors or sensors had been
7:40 improved and larger telescopes had
7:43 become available well we did that work
7:46 in 1976 and found evidence for Frozen
7:48 methane on pluto surface it was several
7:51 years later that we found the evidence
7:53 for the other ises in 1978 astronomers
7:56 Jim Christie and Bob Harrington analyzed
7:59 new plates taken at the US Naval
8:01 Observatory and Flagstaff christe noted
8:04 an elongation to the north of Pluto 1
8:07 month later the bump had disappeared
8:10 from this and other evidence they
8:11 concluded that Pluto like Earth had a
8:14 moon Kon from eclipses between Pluto and
8:18 Kon occurring in the 1980s astronomers
8:21 calculated that the moon was almost half
8:23 the size of its parent body so large
8:26 that both objects spin around their
8:28 Mutual Center of gravity outside Pluto
8:32 Pluto and Kon were the first double
8:34 dwarf planet combo discovered in our
8:36 solar system using the basic physics of
8:39 their orbits and the distance between
8:40 them astronomers could calculate their
8:43 mass and size Pluto was a little smaller
8:46 than Earth's Moon about 1500 m in
8:49 diameter and had only one tenth its mass
8:52 between 1985 and 1990 astronomers were
8:55 in luck as Pluto and Karen orbited their
8:59 Mutual ual center of gravity each passed
9:01 in turn in front of the other the
9:03 so-called Mutual events allowed
9:06 astronomers like Mark buoy to capture
9:08 the changing patterns of light patiently
9:11 buoy created a map of Pluto Pluto turned
9:14 out to have one of the two most
9:16 contrasty surfaces in the entire solar
9:19 system in the mid90s buoy and Allan
9:22 Stern used the Hubble Space Telescope to
9:25 make the first direct images of Pluto's
9:27 surface and it's exciting to mark and I
9:29 and to our whole scientific team uh to
9:32 be able to see this object that no
9:34 humans really could Glimpse as a real
9:36 planet as a real object in the solar
9:39 system previously in 2005 Hal Weaver and
9:42 Allen Stern used the Hubble for another
9:44 close-up look at Pluto and Kon they
9:47 discovered two small dim moons where
9:49 only Kon had been seen before now we
9:52 know from Mark showalter's work that
9:55 there are two more moons making the
9:57 current total of five and that Pluto is
10:00 a genuine many planetary system from its
10:03 size and orbit astronomers estimated
10:05 that Pluto is perhaps 70% Rock and 30%
10:09 ice that makes it one of the largest of
10:11 a whole new class of objects the ice
10:14 dwarf planets making up what's known as
10:16 the Kyper belt this region is named for
10:18 Gerard Kyper a leading mid 20th century
10:21 planetary astronomer Kyper suggested
10:23 that the solar system didn't end with
10:26 Neptune and Pluto but that there should
10:28 be a dis of other other worlds Beyond
10:30 them in 1992 from a Mountaintop in
10:33 Hawaii David jitt and Jane Lou found the
10:36 first Kyer belt object they were using
10:39 new and highly sensitive ccds like the
10:41 sensors in a modern digital camera but
10:44 their technique was essentially an
10:46 updated version of tomba's work take
10:49 carefully registered images of a patch
10:51 of sky and see if anything moves against
10:54 the distant Stars this one qb1 did just
10:58 that it was only a few hundred km across
11:01 10 times smaller than Pluto but still
11:03 huge compared to a comet since then
11:07 teams of astronomers have found around
11:09 2,000
11:12 kbos informed by Cutting Edge astronomy
11:15 but with a fair dose of artistic license
11:17 let's take a trip through this third
11:19 zone of our solar system we used to
11:22 think of the solar system of consisting
11:25 of two different types of planets the
11:27 planets we call the terrestrial planets
11:29 which are earthlike planets that would
11:31 be Mercury Venus Earth and Mars next out
11:34 the asteroid belt fragments of Worlds
11:37 smashed to Pieces by gravitation and
11:39 collisions then come the four gas giants
11:44 Jupiter and its moons Saturn with its
11:47 magnificent Rings Uranus also ringed and
11:52 Neptune and then Pluto was this kind of
11:55 you know odd guy out it was this little
11:56 object at the edge of the solar system
11:59 and then when we found all these other
12:01 Qui rebelled objects this is kind of
12:03 almost a third type of object so for the
12:06 first time ever we'll be able to fly by
12:09 a brand new object an object that's been
12:13 forming for billions of years and
12:17 understand what outer parts of the solar
12:19 system are all about by July 2015 we'll
12:22 know for sure what Pluto and its moons
12:25 look like and that will provide
12:27 breakthrough information on all those
12:29 other ice dwarf planets the most
12:31 numerous planetary objects in the entire
12:34 solar system that make up the Kyper belt
12:37 actually the Kyper belt is more like a
12:39 dut bulging up above and down below the
12:42 ecliptic where most of the planets move
12:46 it's kind of like the asteroid belt but
12:48 much bigger it has hundreds of times
12:50 more objects in it than the asteroid
12:52 belt let's now visit five named kbos in
12:55 the exact positions they'll be in on
12:57 July 14th 20 5 the day when New Horizons
13:02 flies by Pluto quaa was one of the first
13:06 Kyper Bel objects to discovered it's
13:07 about 1,000 km in diameter a reddish
13:11 World covered in water ice methane and
13:14 ethane and like many kbos it has a tiny
13:17 Moon of its own way
13:21 what up above and down below the plane
13:24 of the solar system numerous kbos have
13:26 been flung about by Neptune's gravity
13:30 this region is known as the scattered
13:35 disc one of the largest of these kbos
13:38 aerys is close in size to Pluto and is
13:41 made of rock and methane
13:44 ice astronomers categorize kbos by the
13:48 tilt of their orbits relative to the
13:50 plane of the solar
13:53 system and one of the more highly
13:56 inclined orbits belongs to Mak Mak named
13:59 for a Hawaiian creation
14:01 deity some of these have methane or
14:04 water ice on their surfaces some of them
14:06 just seem to be covered in some brownish
14:08 Gunk there are gray objects out there
14:10 there are brown objects out there they
14:11 seem to be distinct
14:14 populations some of them seem to be very
14:17 spherical and so they probably have warm
14:19 interiors and then others are peculiar
14:21 shapes which suggest they're very cold
14:23 and
14:24 strong perhaps the most bizarre and
14:26 unexpected kbo is how AA a kbo shaped
14:31 like an American football made of rock
14:34 and Ice it's white with red splotches
14:37 and orbited by at least two moons one of
14:41 the strangest orbits of any kbo belongs
14:44 to sedna discovered in 2003 its orbit is
14:48 the most eccentric of any kbo now known
14:51 bringing it as close as 76 Au to the Sun
14:54 but then carrying it outward to
14:57 936 times the the Earth Sun distance
15:00 sedna's strange 11,000 year orbit seems
15:03 to link it to an even vaster cloud of
15:06 objects ready for exploration by Future
15:08 Generations the ort cloud is an immense
15:11 ice box of long period comets from 10 to
15:15 100 times more distant than the Kyper
15:17 belt surrounding All the known worlds of
15:19 our solar system there's a real record
15:21 of the early history of the solar system
15:23 out there in Cold Storage at the edge of
15:25 the solar system this is what was left
15:27 over Pluto is the first member of that
15:30 group but to begin Humanity's
15:32 exploration of the Kyper belt you first
15:35 have to get to Pluto and that means
15:37 getting a mission approved a spacecraft
15:40 designed and built and delivered to the
15:42 Launchpad on time and none of that was
15:46 [Music]
15:55 easy 2015 may be the year of Pluto but
15:59 getting there has taken many long years
16:02 of
16:02 effort and for New Horizons there's a
16:05 date when things got started
16:10 1989 it was the year when George Herbert
16:13 Walker Bush became president and the
16:15 Berlin Wall
16:17 fell far from Earth it was also the year
16:20 when NASA's Voyager spacecraft flew by
16:23 Neptune and returned the first images of
16:26 its Moon Triton
16:29 hairstyles of some New Horizon
16:31 scientists were very different but for
16:34 them May 5th 1989 was a most important
16:37 date that's the day that I marched into
16:40 the then division director for planetary
16:42 science at NASA headquarters Jeff Briggs
16:45 as a graduate student and asked him why
16:48 we aren't studying a mission to Pluto
16:50 and he responded because no one's ever
16:52 asked me before that seems like a
16:54 brilliant idea why don't we do that
16:57 space missions rely on hundreds if not
16:59 thousands of people but sometimes it
17:01 takes someone with passion and
17:04 persistence to make things happen and
17:06 for New Horizons that's Alan Stern I was
17:09 interested in this when I was a boy so
17:11 I've been somewhere between in the
17:12 groove and stuck in a rut for 40 years
17:14 there had been some thought about
17:16 sending one of the twin Voyager
17:17 spacecraft past Pluto to complete the
17:20 exploration of the known solar system
17:22 but in the '70s the scientific
17:24 establishment wasn't convinced Pluto was
17:26 all that interesting young grad students
17:28 mik Allen markk buoy and Fran bagenal
17:31 thought differently back in oh about
17:34 late 1989 or so there was a bunch of us
17:37 who were really Keen to go to Pluto and
17:39 the thing that Drew me to it the most
17:42 was the fact that we knew so little
17:44 here's the frontier so it was a bit of
17:46 an opportunity for young people to come
17:48 in and say hey where are we going to go
17:50 next what's the next great Frontier that
17:53 we should go explore and it was clear
17:55 out to the K Bel Allan Fram Mark and a
17:59 small band of enthusiasts became known
18:01 as the Pluto underground so we realized
18:05 to make this happen we had to get
18:06 together and Campaign hard to make the
18:09 case to go there and explore this little
18:12 planet with all its moons all through
18:14 the '90s there were many competing plans
18:17 for a Pluto mission like the Pluto fast
18:19 flyby the Pluto Kyper Express a Pluto
18:22 mission was on then off then on then off
18:25 the PLO Mission had been a cat it would
18:27 have been dead long ago because they
18:28 only get nine lives and we've had
18:30 significantly more than nine stoppages
18:33 and odd twists and turns what finally
18:36 turned the tide was the national
18:38 Academy's decadal survey a consensus
18:40 document from leading planetary
18:42 scientists that ranked a Kyper belt
18:44 Pluto mission highest in priority for
18:47 medium class budgets finally after
18:49 competitive proposals were evaluated New
18:52 Horizons which teamed alen Stern with
18:54 the Johns Hopkins Applied Physics
18:56 laboratory APL and several other in
18:58 institutions across the country was
19:00 selected by NASA on November 29th
19:04 2001 now plans on paper became metal in
19:08 clean rooms in 2004 lead scientist Alan
19:12 Stern described the mission's key
19:14 science objective well you know the key
19:16 to planetary science is um that you
19:19 really have to go places to get the
19:20 resolution to get up close enough to
19:22 really see what's going on we want to
19:24 get up close and personal the very best
19:26 resolution of current telescopes looking
19:28 at Pluto would give this kind of fuzzy
19:30 image of a much more familiar world but
19:33 here's what New Horizons would see if
19:36 flying over New York City lakes in
19:39 Central Park Wares on the Hudson River
19:43 your horizons is the first really of a
19:46 whole new breed of spacecraft that is
19:48 focusing on a very specific task for
19:51 this first mission to Pluto the
19:53 questions are basic what do Pluto and
19:56 Karen look like what are they made of
19:58 how do their atmospheres behave we have
20:01 to really be disciplined and say we
20:03 can't do everything let's focus on the
20:05 primary questions and design the
20:08 instruments to answer those primary
20:09 questions the long range imager lorri
20:12 will be used for navigation approaching
20:14 Pluto and close-up views during the
20:16 flyby the wide-angle camera Ralph has
20:19 both visible light and infrared sensors
20:21 to map Pluto and Caren and characterize
20:24 their icy surfaces there are two fields
20:27 and particles to detectors to probe the
20:30 solar wind at Pluto the large radio
20:33 antenna is an essential Communications
20:36 device but both Rex and Alice an
20:39 UltraViolet Imaging spectrometer are
20:41 part of experiments to analyze Pluto's
20:45 atmosphere and there's the Venicia
20:47 Bernie student dust counter built by
20:49 undergrads at UC Boulder and honoring
20:51 the school girl who named Pluto back in
20:54 1930 together the seven science
20:56 instruments comprise the most power
20:58 powerful set of detectors ever sent on a
21:01 first flyby of any world in our solar
21:03 system but their Innovative and highly
21:05 miniaturized design means that even when
21:08 all are operating they draw less power
21:11 than half a 60 W bulb and they're
21:13 intended to work together
21:17 seamlessly after building comes testing
21:21 but always with an eye on the clock and
21:23 the
21:24 calendar it's very very important that
21:26 we launch in either 2006 or 2007 we have
21:30 to make that deadline if you want to fly
21:32 to Pluto on the quickest route you need
21:35 Jupiter in position and that means we
21:37 have to launch in January of 2006 it
21:40 feels a little bit like being strapped
21:42 to a train going 500 mph the test
21:44 program involves teams of Engineers at
21:47 John's Hopkins APL and then at NASA's GD
21:50 space flight center once we launched
21:52 this we can't go after with a
21:54 screwdriver we can't go fix anything
21:56 that isn't working we make sure that we
21:58 carry plenty of spare equipment on board
22:00 the spacecraft if our main computer
22:01 breaks we have a backup if our main
22:04 transmitter breaks we have a backup one
22:06 of the things we do is we put the whole
22:07 spacecraft on a gigantic vibration table
22:11 a paint Shaker and shake it and and then
22:14 test it after that and shake it again
22:16 and test it again so that's what we're
22:18 doing from now until launch along with
22:20 testing the spacecraft New Horizons
22:22 needs to train and test its human
22:25 operators and for a mission planned to
22:27 reach Pluto in 2015 15 it's important to
22:30 have young people on board early so
22:32 they'll be around a close approach it's
22:35 good that we can do that so they will
22:38 have both the time the focus to stay
22:41 with the mission over this long period
22:43 of time many of the faces you see around
22:45 mission control in 2004 and 2005 are
22:48 young and enthusiastic spacecraft
22:50 Engineers normally we're focused on
22:53 subsystems and instruments in the
22:54 spacecraft surviving that duration but
22:57 you know for people we have to have a
22:59 longevity plan they'd be committing the
23:01 prime of their careers to this mission
23:03 to Pluto knowing they'd be a decade
23:06 older when New Horizons reaches its
23:09 primary target the ability to practice
23:11 things in those years far out there are
23:15 all part of the planning now to assure
23:17 Mission success then how old are you
23:19 going to be in
23:22 2015 I don't know something somewhere in
23:25 my 40s oh you're a youngster yes
23:29 in late 2005 the action shifts to Cape
23:32 Canaveral New Horizons may be light and
23:35 relatively small but launching it to
23:37 Pluto requires America's most powerful
23:41 rocket the atlas
23:43 5 New Horizons will be traveling so far
23:46 from the Sun that solar panels wouldn't
23:49 be sufficient so the department of
23:51 energy delivered an RTG that would power
23:54 the Pluto mission by turning heat from
23:56 the radioactive decay of pluton I onium
23:59 into
24:01 electricity working Round the Clock they
24:04 arrive at pad 41 Before Dawn on behalf
24:07 of NASA and the entire New Horizon's
24:10 team Stern wanted to be the last to bid
24:13 the spacecraft bonvoyage before closing
24:16 up the hatch on January 19th 2006 after
24:20 17 years of planning building and
24:22 testing a picture perfect launch that
24:25 thrilled onlookers in Florida and the
24:27 mission operations team back at John's
24:30 Hopkins in Maryland we
24:33 have
24:36 Horizon vo visit Pluto and then beyond
24:40 despite immense Technical and timetable
24:43 challenges the mission had made its
24:45 window and was on its way New Horizon's
24:49 velocity at launch was the fastest ever
24:51 traveling almost 60 times faster than a
24:54 jetliner in just 9 hours it passed the
24:57 orbit of of the Moon Apollo had taken
25:00 almost 10 times that long one year later
25:04 a slingshot gravity assist from the
25:06 giant planet Jupiter provided another 2
25:09 km/ second boost cutting travel time to
25:12 Pluto by three full years but this was
25:16 more than just a jump in speed the
25:18 Jupiter flyby was a scientific dress
25:21 rehearsal for Pluto New Horizon's
25:23 instruments returned detailed images of
25:26 Jupiter's clouds moons and
25:29 we got the night wow look at that then
25:32 it was off across the empty ocean of
25:34 space with no new land in sight till
25:38 Pluto in
25:40 2015 the spacecraft had been tested and
25:43 passed with flying colors now it was
25:46 time to test the humans and the ground
25:49 systems July 5th 2013 it's day one of a
25:53 9-day encounter rehearsal the main
25:56 success criteria for this rehearsal
25:58 is for the spacecraft to flawlessly
26:01 perform its activities as if it were a
26:04 pluta with everything the same except
26:06 the Pluto is not
26:07 there the dates in 2013 were carefully
26:11 chosen so that Earth received times
26:14 would be identical to those for the real
26:16 encounter in
26:19 2015 Mission managers wanted scientists
26:22 and Engineers to experience the stress
26:24 of time critical 247 operations EXP Ed
26:28 for July 2015 we're flying by an object
26:32 that is a huge distance from Earth and
26:34 we're trying to hit a box that's 100 by
26:36 150 km wide and that then leads into
26:39 maneuver planning and and trajectory
26:41 control needed to thread that that
26:43 needle and hit that small box it's way
26:45 the heck out there this rehearsal would
26:48 actually be uploading commands to New
26:50 Horizons to instruct the spacecraft to
26:53 run through the exact same set of
26:55 observations as in 2015 there definitely
26:59 is an element of risk involved but from
27:01 one standpoint if you didn't do any
27:03 simulation with the real spacecraft at
27:04 all you could argue that could POS more
27:06 risk because you don't want such a
27:08 critical activity only being done once
27:11 on flight those are all invaluable to
27:14 get us ready and and practiced for the
27:18 one and only shot we'll have to explore
27:21 the Pluto system we've been waiting uh
27:23 12 years since we wrote the proposals to
27:25 do this rehearsal it's the last big step
27:27 before we can do the encounter we think
27:30 that we are about 10 million miles out
27:33 from Pluto en closing but so far so good
27:37 we're off to the
27:39 [Music]
27:51 races today is our
27:54 2724 day in flight this has been a long
27:57 time coming literally I only want to say
27:59 thanks for all the work let them eat
28:02 [Music]
28:13 cake July 12th 2013 standing in for July
28:18 14th
28:20 2015 this is it a minute by minute
28:23 simulation of encounter day
28:28 it's maker
28:30 break well it's it's the most important
28:33 because we've best been spending the 24
28:35 hours of the most intense activities
28:37 that we've been running on the
28:37 spacecraft and this is the longest that
28:39 we've been out of contact since we've
28:41 entered encounter rehearsal this may be
28:43 a rehearsal but New Horizons has been
28:46 firing its thrusters and spinning in
28:48 space identical Maneuvers to those
28:51 planned for
28:52 2015 on encounter day the spacecraft
28:56 will be too busy taking data to send
28:58 back images that's why its first simple
29:01 I'm alive message will be so
29:05 important sometime within the next
29:07 minute DSS 43 should lock up on the
29:21 signal we're we're good we're nominal
29:23 spacecraft's nominal and it looks like
29:26 um all the observations that plan
29:28 between last track and this track
29:30 happened this gives us good confidence
29:32 that at least the spacecraft has been
29:34 performing all of those twists and turns
29:36 that we've been anticipating it to over
29:38 the last uh 7 days I like to say that at
29:41 the flyby I don't want to be learning
29:42 anything about the ground system or the
29:44 spacecraft of the team I want to be
29:46 learning only about the Pluto system no
29:48 spacecraft has ever been to Pluto or nor
29:50 will ever go back in our lifetime Pluto
29:52 is every child's favorite planet you
29:54 know you ask anyone under the age of six
29:56 they're going to say Pluto we don't
29:57 exactly know what Pluto looks like but
29:58 it looks very exciting from the images
30:01 we have from the Hubble Space Telescope
30:02 so far we really can't wait to get there
30:04 and see what it actually looks like so
30:07 if anybody says that Pluto is boring or
30:09 not important no way before New Horizons
30:13 arrives at Pluto most everything we
30:15 think we know about the planet and its
30:17 moons is up for grabs virtually every
30:20 place we've set a spacecraft on a first
30:22 reconnaissance mission like this that we
30:25 find out that our earth-based Notions
30:27 were flat wrong
30:28 so I'll tell you what we expect but I
30:32 before anything what we expect is to be
30:35 surprised from the 1990s through today
30:38 Stern has been consistent in avoiding
30:41 speculation you get the same answer
30:43 everybody's gotten from me for almost 20
30:47 years I don't make predictions except
30:50 for one my best guess is we're going to
30:53 find something wonderful but in the
30:55 final months leading up to the July 2015
30:58 encounter it's hard for most humans not
31:00 to imagine what we'll see many planetary
31:03 scientists like Paul shank base their
31:05 expectations and what we saw when
31:07 Voyager 2 reached Neptune and
31:10 specifically as it flew by its Moon
31:12 Triton Voyager was a 10e long
31:15 exploration of the outer solar system
31:17 and every time they got to a planet it
31:18 was basically the first time anybody had
31:21 really seen those bodies so when they
31:22 got to Jupiter they were greeted with
31:25 enormous surprises the erupting
31:26 volcanoes on on I were just completely
31:29 unexpected and so when they got to
31:31 Uranus there were more surprises the
31:33 Exotic trains of of Miranda and Ariel
31:35 for example were not expected so by the
31:37 time they got to Neptune they were kind
31:39 of accustomed to the idea that they were
31:41 going to be surprised and sure enough uh
31:43 Triton uh completely blew them away
31:46 Bonnie barate was at NASA's jet
31:48 propulsion lab as the first images of
31:50 Triton a moon of nearly 1,700 M diameter
31:54 came down Triton was almost a twin of
31:57 Pluto it's about the same size about the
31:59 same brightness originally Triton was
32:02 probably a Kyer belt object just like
32:04 Pluto floating around in space but then
32:06 it got too close to Neptune and it got
32:08 captured by Neptune's gravitational
32:10 field recently Paul shank enhanced the
32:14 original Voyager data to create this
32:16 detailed flyover of Triton it has odd
32:20 patches and odd blob like features kind
32:23 of like amibas crawling around on the
32:24 surface Triton has very few impact
32:27 crators it's surface is extremely young
32:29 geologically and it actually has ge's
32:33 spting Material off into space here is a
32:35 body that is hundreds of degrees below
32:39 zero so cold it's forlorn it's Barren we
32:43 just didn't expect to see this activity
32:46 on Triton it was quite a surprise if you
32:48 just assume that Pluto was going to look
32:50 exactly like Triton which is the most
32:52 similar object we know about then you
32:54 might expect to find a very interesting
32:56 body but Triton is not not the only
32:58 Dynamic ice world in the outer solar
33:00 system 16 years later the Cassini
33:03 spacecraft sent back images of Saturn's
33:05 moon Enceladus about 300 mes across this
33:09 is a tiny little Moon and Enceladus is
33:11 actually a winter wonderland it's very
33:14 bright it reflects almost all the
33:16 radiation that falls on it and it has
33:19 these huge ice volcanoes spewing out
33:22 from its s South Pole and Enceladus is
33:25 continuously giving off per of water
33:28 vapor and so if you start to see puffs
33:30 of water vapor coming off Pluto as newc
33:32 Horizons gets closer that would be
33:34 exceedingly interesting but what forces
33:37 can power volcanoes in the Deep Freeze
33:40 of the outer solar system Triton and
33:42 Pluto are both balls of ice with
33:45 presumably Rock in the center and so one
33:47 of the sources of energy is radioactive
33:50 decay inside the rock which gives off
33:52 heat just like the Earth is heated if
33:54 you just let Pluto sit there and pump
33:57 the heat out of the Rocks you you
33:59 generate enough energy to melt a couple
34:01 of hundred kmers worth of ice it's still
34:04 possible to have an ocean beneath a
34:06 relatively thick ice shell the ice shell
34:08 might be 100 miles thick or so over
34:11 billions of years the ice shell gets
34:14 thicker and thicker and thicker as Pluto
34:16 cools and as it does so it squeezes the
34:20 water underneath and if you squeeze the
34:22 water too much then it may well actually
34:24 create fractures and the water could jet
34:26 out to the surface when you're going out
34:27 to the edge of the solar system you kind
34:29 of have to expect some surprises and
34:31 we're going to see them at Pluto as well
34:33 just as tridon and Enceladus were mere
34:35 dots before spacecraft reached them
34:38 until now Pluto has been an astronomer's
34:41 Planet that's about the change we are
34:44 going to start off as astronomers and
34:46 we'll be using astronomical tools to um
34:50 try and sharpen up our images and pull
34:52 every last little bit of detail out of
34:54 these fuzzy blobs we gradually turn from
34:56 astronomers into GE ologists as we get
34:58 closer and it becomes a real world Jeff
35:01 Moore was in the room at JPL as those
35:03 Triton images came down but he also
35:05 enjoys field work and thinks we'll
35:08 recognize some similar planetary
35:10 processes at work on Pluto as back on
35:12 Earth so I'm a geologist and although we
35:14 don't expect to see oceans on Pluto
35:17 there are common processes which operate
35:20 on this planet which are likely to
35:22 operate also on Pluto and its moons
35:25 while the scales are very different
35:27 erosion shapes landforms here on Earth
35:30 and all across the solar system there
35:32 are these little finger-like projections
35:34 that are formed by the process of
35:36 erosion where wind and water have
35:39 sculpted this landscape by taking
35:41 advantage of small differences in the
35:43 strength of the original Rock creating
35:45 large huge fantastic Landscapes such as
35:48 on Jupiter's moon Kalisto and we can
35:51 anticipate that we may perhaps also see
35:53 Landscapes like this on Pluto and its
35:56 moons Pluto's 48-year orbit is more
36:00 eccentric than our Solar System's
36:02 terrestrial and gas giant planets
36:04 greatly varying its distance to the Sun
36:07 but it's typical of many other objects
36:09 in the Kyper belt and newly discovered
36:12 planets around other
36:13 stars that plus its highly angled polar
36:17 tilt combined to produce strong seasonal
36:20 effects in fact the seasons of Pluto are
36:22 amongst the most extreme of any seasons
36:24 on any world that we know of orbiting
36:26 the Sun and those extremes may be one
36:29 reason why its surface is also extremely
36:31 contrasty Pluto is props the most
36:34 intensely bright and dark place that
36:36 we've seen in the solar system this dark
36:38 surface collects more heat it warms up
36:40 like asphalt does on a sunny day here on
36:42 the earth and if there were Frost had
36:45 settled on this dark surface they're
36:47 being heated up and driven off and the
36:50 transportation of this material could
36:52 also be creating wind so you might see
36:54 small Dunes oriented along the periphery
36:57 of the dark surface showing this process
36:58 in action for planetary scientists color
37:01 can be a clue to the composition of
37:03 surfaces that can't be sampled directly
37:06 on the earth these kinds of colors from
37:08 red to uh dark gray are generated
37:11 entirely by the presence or absence of
37:13 rust on Pluto we see also these same
37:16 ranges of colors from Gray to bright
37:19 white to Yellow to Red to black but
37:22 there it must be due to a completely
37:24 different process at NASA's as research
37:26 center near San FRC Frisco longtime
37:28 Pluto researcher Dale Kook shank and
37:31 postto Chris mes conduct experiments to
37:34 see what processes might create the
37:36 colors we see on Pluto starting with
37:38 gases like methane and nitrogen and the
37:41 extreme low temperatures we know or
37:43 found there in our cold chamber we can
37:46 produce a thin film of ice and then
37:49 after that expose them to a beam of
37:52 electrons which are charged particles
37:54 comparable to what comes in to Pluto's
37:56 surface from space
37:58 we find that when we U shine ultraviolet
38:01 light or electrons on simple molecules
38:04 before too long the simple molecules are
38:07 broken apart and by natural processes
38:10 they reassemble into more complex
38:13 chemicals so far the colors we make in
38:15 the lab from radiating these IES is uh
38:18 is fairly close to what we see on Pluto
38:20 there are tones of yellow light brown up
38:24 through fairly dark red and if we care
38:27 the processing by ultraviolet light to
38:30 an extreme degree uh the material
38:32 actually turns black and this is almost
38:34 the color of of pure carbon seeing how
38:38 radiation transforms simple I into
38:40 complex and colorful organic molecules
38:43 should help interpret the close-up views
38:45 of Pluto's surface that'll be sent back
38:48 by New Horizons color translates to the
38:52 duration of the exposure of these
38:55 otherwise colorless IES over a year
38:58 10,000 years 10 million years that may
39:01 in turn tell us more about the nature of
39:05 the exposure of Pluto's surface and even
39:07 the age of Pluto's surface Dale
39:10 Crookshank began observing Pluto back in
39:13 1976 now 39 years later he's ready for
39:17 its closeup we can say that Pluto is
39:20 chemically active chemically Dynamic we
39:22 don't know yet if it's geologically
39:24 active and dynamic but that's what new
39:27 Horizons is going to tell us we've been
39:29 surprised in that way before as we've
39:31 passed other planetary bodies that we
39:34 had thought were totally cold dead um
39:37 inert worlds and find that there are
39:40 geysers there are ice flows there are
39:43 cracks and all kinds of evidence for
39:45 geological activity I can still remember
39:47 the first time I saw Pluto in a
39:49 telescope and it was just a little dot
39:51 that you could barely see it will be
39:54 amazing that within a period of hours it
39:56 will be transformed from this tiny dot
39:58 that I studied as an astronomer to this
40:01 huge geologic world that will be able to
40:04 see volcanoes and faults and ices and
40:06 mountains and craters I mean it will be
40:09 truly an amazing experience to see it
40:11 transformed so from sophisticated lab
40:14 experiments from exploring other worlds
40:16 and from applying insights from
40:18 terrestrial processes what should we
40:20 expect when we get to Pluto in July
40:24 2015 fact the only thing that would
40:26 surprise me would be if we turned out
40:27 not to be surprised but enjoying the
40:30 scientific surprises to come means
40:33 avoiding dangers on the last few million
40:36 miles to
40:37 Pluto that's
40:46 next December 6th
40:49 2014 in Mission Control Alice Bowman and
40:52 her team wait to get confirmation that
40:55 New Horizons has exited what's called
40:57 hibernation for 2/3 of its 3 billion
41:01 mile Journey most spacecraft systems
41:03 have been turned off saving wear and
41:05 tear on the science instruments New
41:08 Horizon sends a simple signal once a
41:10 week just to say I'm still AOK Alice's
41:14 team has a unique way of showing
41:16 spacecraft status when New Horizons is
41:19 hibernating their bare mascot is safely
41:22 asleep when the spacecraft wakes up they
41:25 put on its party hat if all goes well
41:28 this will be the 18th time spacecraft
41:31 and Bear have woken up but December 2014
41:34 is different VIPs from NASA are on hand
41:39 two film Crews document the action as
41:41 Allan explains the benefits of
41:43 hibernation um it lowers our cost
41:45 because we don't need to have people
41:47 babysitting the spacecraft 24/7 outside
41:50 interest in New Horizons is building if
41:53 all goes well New Horizons will stay
41:55 awake flying by Pluto and in July 2015
41:59 and then returning data until October
42:02 2016 copy that thank you
42:05 GNC tonight data trickles in and Alice
42:09 has to wait to be certain New Horizons
42:12 is fully awake we should be getting it
42:15 momentarily it should be any minute now
42:18 this is like watching paint dry I figure
42:20 if I stare at the screen hard enough
42:30 and packet five just came in there we go
42:32 go P PN mom on Pluto
42:37 1 we have a nominal wake up of the New
42:40 Horizon spacecraft on its way to
42:43 Pluto we're ready for our next leg of
42:46 the
42:50 journey was
42:52 awake ah our bear he's going to be here
42:55 for a while this is a shed day we have
42:58 completed the cruise across 3 billion
43:01 miles of space the spacecraft is now
43:04 awake finally after 9 years I'm glad to
43:07 see hibernation behind us and active Ops
43:10 ahead onto Pluto but there are still
43:13 hundreds of tasks to ensure a safe flyby
43:15 in July
43:17 2015 January 27th New Horizons has been
43:20 sending back technical data and all
43:22 seems fine but today is the first time
43:25 Hal Weaver and Andy Chen will be seeing
43:27 new science images I thought I saw it
43:29 pop up here let's try that again Chang
43:33 is lead scientist for the Lori camera
43:35 Lori is used for navigation to find the
43:38 targets and to correct the trajectory so
43:41 we get to the right place at the right
43:42 time voltages currents temperatures all
43:45 look normal uh no error messages this is
43:48 it uh let's let's check out the uh very
43:53 first images and then
43:55 Sharon right there Pete pixel
44:00 55
44:03 okay all right so there they are let's
44:06 look at the whole for project scientist
44:08 Hal Weaver even the jump in size from
44:11 one to two pixels was significant this
44:13 is a real milestone in the New Horizons
44:15 Mission the very first images of Pluto
44:17 in the Pluto encounter year uh hadn't
44:20 turned loran hadn't gotten any images
44:22 since last summer last July but this is
44:25 it this is the start of it AR she blue
44:28 we really don't know what we're going to
44:29 see that's what this mission is all
44:31 about what is the surface of Pluto
44:33 really like how big is it what are the
44:34 orbits really so it's nothing but
44:37 delightful surprises coming for us but
44:40 some of the surprises may not be quite
44:43 so welcome as New Horizons get still
44:46 closer to the Pluto system Lori will be
44:49 able to identify small moons and
44:51 possible rings that can't be seen from
44:55 Earth John Spencer is leading the uaz
44:59 campaign uaz stands for unknown hazards
45:03 we may found new moons or even rings
45:05 around Pluto and if we see anything like
45:07 that we're going to want to determine
45:10 whether it poses a threat to the
45:12 spacecraft because if it does if there's
45:15 debris that we might run into that might
45:18 damage or kill the spacecraft then we
45:19 want to uh evaluate that Hazard and
45:22 determine whether we should take any
45:24 evasive action to find out just how
45:27 vulnerable New Horizons might be to even
45:29 tiny dust particles the mission sent
45:31 samples of spacecraft components to the
45:33 White Sands test
45:36 range technicians at White Sands set up
45:39 gun tests to assess how vulnerable New
45:42 Horizon's outer covers and cables might
45:44 be we went to two facilities that could
45:49 shoot things into parts of models of the
45:53 spacecraft while the results might look
45:56 dangerous the Mission has options to
45:58 take evasive
46:00 action one of the backup strategies we
46:03 have if we feel we need give the
46:05 spacecraft Extra Protection is that we
46:07 Orient it so that the High Gain antenna
46:09 here which is um literally pretty
46:12 bulletproof and can protect the
46:13 spacecraft is going to be facing forward
46:16 in the ram Direction and this is ram in
46:19 the sense of battering ram it's a
46:21 direction in which stuff will be coming
46:22 at us and ramming into the spacecraft
46:25 and if that is facing forward then any
46:28 dust particles that hit the spacecraft
46:30 are most likely to hit that antenna
46:31 where they won't cause US problems and
46:33 only a small part of the spacecraft
46:35 around the edges is going to be exposed
46:37 to those particles that would protect
46:39 the guts of the spacecraft but limit the
46:42 pointing of the cameras the cameras are
46:44 fixed to the spacecraft so if the
46:46 spacecraft has to point in One Direction
46:48 the cameras can only point in a limited
46:51 range of directions this limits the
46:52 amount of times we can photograph the
46:54 system as we go past because we can only
46:56 photog objects when they're just in the
46:58 right angle that we can look at them
47:00 while protecting the spacecraft with the
47:02 main antenna another option is to take
47:04 different trajectories through the Pluto
47:06 system that's called the Shabbat play
47:10 Shabbat is the best acronym in the space
47:12 business it stands for Safe Haven by
47:15 other trajectory and it is is the word
47:19 we use to represent our backup plans at
47:21 Pluto the second Shabbat takes us much
47:24 closer to Pluto um into the region where
47:27 atmospheric drag uh depletes orbits of
47:30 any debris which we think would be uh
47:33 the safest Hail Mary pass that we could
47:35 fly if we have to do something different
47:37 than the nominal we are coming into the
47:38 Pluto system with the ability if we
47:41 learn something we don't expect to be
47:43 able to make uh a change and uh and get
47:46 the goods but those decisions can only
47:48 be made in the last month before closest
47:51 approach and there'll be limited time to
47:54 evaluate the best options so in February
47:56 20 2015 Spencer's uaz team including
48:00 ring specialist Mark shalter and postto
48:03 Simon Porter are running through a
48:05 Readiness test now they're on the clock
48:07 and being scored for whether they can
48:09 work through the calculations fast
48:11 enough to decide on a trajectory
48:13 correction maneuver that might prevent
48:15 loss of mission and that makes this
48:18 exercise more critical than any that
48:20 have gone before the difference between
48:24 this and previous operational Readiness
48:26 tests is is that this is where we have
48:28 to demonstrate to the project of NASA
48:30 that we can do this but the only test
48:32 that really matters comes on July 14th
48:36 2015 that one day will pay off 26 years
48:40 of dreams and 9 years in
48:48 [Music]
48:52 flight for the science team the year of
48:55 Pluto began with another meeting to
48:57 review the latest data on the Pluto
48:59 system and to hear updates on how the
49:01 spacecraft was performing Mission
49:04 manager Glenn Fountain who'd been with
49:06 the project from its start summarized
49:08 remaining risks red boxes are
49:11 possibilities that could kill the
49:13 mission but now in 2015 there are more
49:16 and more green boxes risks that have
49:19 been minimized something that we haven't
49:22 thought of still might happen but I'm
49:25 confident that whatever happens whatever
49:28 fate throws at us this team will be able
49:32 to resolve it and we'll go on to get
49:36 wonderful data when we get to Pluto we
49:38 have a fantastically talented team of
49:40 people who have worked very hard and
49:43 we've tested the sequences inside and
49:45 out and while there are always unknown
49:48 unknowns I'm very confident and really
49:51 looking forward to the curtain Rising
49:53 along with mindbending technical details
49:55 there also was a sense of history in the
49:58 making to document the long years of
50:00 effort to get this close to Pluto the
50:03 mission recreated a team photograph
50:05 taken in
50:07 2004 as Glenn Allan and Alice had
50:10 carefully planned back then many of the
50:12 scientists and Engineers were still
50:14 actively engaged in New Horizons and
50:17 looking forward to July
50:19 2015 we have worked hard to get a
50:23 coherent team because if you don't have
50:25 a good team to operate the spacecraft to
50:28 do the planning you will
50:31 fail and so we worked a plan early in
50:36 the mission to have younger people uh
50:40 with the right amount of
50:42 experience to be on the mission and it's
50:45 just like watching your kids grow it's
50:48 like all of a
50:49 sudden where did the time go you know
50:53 they are older they're more mature and
50:55 they're now the the very experienced
50:58 veterans but the hard work of mission
51:00 planning was by no means over even this
51:03 close to encounter day while exploring
51:06 Pluto in 2015 is exciting in itself New
51:09 Horizons was recommended in part as a
51:12 mission that might continue on farther
51:14 out into the Kyper belt that takes
51:16 identifying potential targets now for a
51:19 still more distant flyby should NASA
51:22 approve an extended Mission this
51:24 challenging task was assigned to John
51:26 Spencer Mark Buie and a team of young
51:29 posts and like everything else about
51:31 this Mission it wasn't easy Buie and
51:34 John Spencer had been using Earth's
51:36 largest telescopes in Hawaii and Chile
51:39 but even Earth's Best couldn't crack
51:41 this task but the basic problem is the
51:45 Earth's atmosphere is just a a mess at
51:47 these scales there's a limit and that's
51:50 what we've been beating our heads
51:51 against now with time running out we had
51:55 to turn to Hubble and so it's we sort of
51:57 not so jokingly talk about Hubble to the
51:59 rescue without Hubble we would not have
52:03 these objects Mark and his young
52:04 collaborators came up with Innovative
52:06 search techniques using custom software
52:08 what that does is makes the Stars smear
52:11 out and makes the Kyper Bel objects hold
52:13 still it's been a lot of work but to do
52:16 something as exciting as this has been
52:19 just so much fun I've been plugging
52:20 through the data today because it's
52:22 fresh data and I just really really
52:24 wanted to to know what the answer was
52:27 well we would have been in big trouble
52:28 if we didn't find the kbo in time so
52:31 there was this pressure but honestly we
52:34 had the best people in the world working
52:35 on the problem and we did it and we just
52:38 do the math write the software crunch
52:40 the pixels and then I create this
52:43 graphic and from that point on it's what
52:46 I call wetwear it's what you got in your
52:48 head in reality kbos are moving against
52:51 the fixed Stars Mark came up with a way
52:53 of making them more obvious by flipping
52:55 that around and making the stars appear
52:58 to move and any kbos stand still right
53:02 in the middle there's something that's
53:04 just holding dead
53:06 constant and that's the Kyper belt
53:09 option you can't argue with that it was
53:11 a high- tech variant of the approach
53:14 that had been instrumental in exploring
53:16 the Pluto system right from the start
53:18 but at the core it's a technique that
53:21 hasn't really changed since tombow's day
53:24 you have two pictures of the sky taken
53:26 in different times and you're looking
53:29 for the stuff that moves as soon as you
53:31 see something real there is absolutely
53:34 no question about it as soon as it
53:36 flashes on the screen in just a
53:39 millisecond there it is it's real and
53:42 you know I found another kyber bolt
53:44 object but finding a kbo is only half
53:47 the battle is it located where New
53:50 Horizons can reach it with available
53:52 fuel once you have the orbit then we and
53:54 we know where the spacecraft is and
53:57 where it's going to be we can figure out
53:59 how much fuel the spacecraft is going to
54:02 need to use to get to the these objects
54:05 with more Hubble time New Horizons got a
54:07 pleasant surprise it looked like we
54:09 might actually have to burn the engines
54:11 to miss the
54:13 object which was pretty exciting concept
54:16 you know it's good thing we looked cuz
54:18 you wouldn't want to run into one of
54:20 these things these cold classicals
54:21 they're pretty much as they were 4.5
54:25 billion years ago they're little fossils
54:28 that's incredible we have no idea what
54:31 they're going to look like so with
54:33 potential targets found at last it was
54:36 on the Pluto I'm feeling pretty
54:38 exhilarated at this point you know
54:40 you're at the top of the roller coaster
54:42 you were about to go down that dizzying
54:46 thrilling uh ride into the system just
54:49 seeing Pluto there getting bigger and
54:51 bigger it's gives me goosebumps today
54:53 we're only a few months away from the en
54:56 counter we're less than an astronomical
54:59 unit the distance between the Earth and
55:01 the Sun that distance away from this
55:03 fascinating object it's the last major
55:07 body in our solar system that we really
55:09 need to visit to be putting the Capstone
55:11 on the initial reconnaissance of the
55:13 solar system it's heartwarming and it it
55:17 feels like something that makes a career
55:19 worthwhile as spacecraft goes New
55:22 Horizons is a very small team but still
55:25 we've been working on this for over a
55:28 decade and you add it all up and it's
55:30 about 2 and 1/2 million work hours to
55:33 get ourselves to Pluto we have waited
55:37 first the four years that we couldn't
55:39 hardly think about because we were
55:40 running so fast and then it is oh we
55:44 wait and we wait and now we are ready to
55:48 begin the encounter we have had delayed
55:52 gratification the year of Pluto is you
55:54 know simultaneously a beginning and an
55:57 ending um it's an ending in that we are
56:00 uh completing our objective we're
56:02 accomplishing the flyby of the Pluto
56:04 system for the first time but it's also
56:07 the beginning of a whole new chapter for
56:09 science of really being able to explore
56:11 these objects as the data comes down
56:13 over a period of months you know in
56:15 bringing in postdocs and the younger
56:17 scientists who some of them were in high
56:19 school when we started this project and
56:21 now they have their phds and they are
56:23 spectacular experts and and very
56:25 talented at what they do I was in
56:28 preschool when Allan first started
56:31 talking about a Pluto mission and
56:34 finishing high school and starting
56:35 College when it was built and in grad
56:38 school for the cruise having young
56:40 people come into these programs gaining
56:43 The Experience they're going to be the
56:45 next generation of explorers we've never
56:48 been to a kbo we've never been anywhere
56:51 close to a kbo this this is the the most
56:54 unexplored area of the entire solar
56:57 system which is in other wayse saying
56:58 this is the most unknown area that we as
57:02 humans can reach with spacecraft we
57:04 can't wait to get to Pluto and to July
57:06 14th and see what the surface looks like
57:09 we're ready to go and it's showtime we
57:11 are capable of continuing an adventure
57:15 that Humanity began 100,000 years ago as
57:20 our ancestors Walked Out Of Africa and
57:24 we are continuing that
57:26 exploration and this country is in the
57:30 Forefront of doing that
57:35 [Music]