All language subtitles for The.New.Frontier.S03E06.1080p.AMZN.WEB-DL.DDP2.0.H.264-ISA_track3_[eng]

af Afrikaans
ak Akan
sq Albanian
am Amharic
ar Arabic
hy Armenian
az Azerbaijani
eu Basque
be Belarusian
bem Bemba
bn Bengali
bh Bihari
bs Bosnian
br Breton
bg Bulgarian
km Cambodian
ca Catalan
ceb Cebuano
chr Cherokee
ny Chichewa
zh-CN Chinese (Simplified)
zh-TW Chinese (Traditional)
co Corsican
hr Croatian
cs Czech
da Danish
nl Dutch
en English
eo Esperanto
et Estonian
ee Ewe
fo Faroese
tl Filipino
fi Finnish
fr French
fy Frisian
gaa Ga
gl Galician
ka Georgian
de German
gn Guarani
gu Gujarati
ht Haitian Creole
ha Hausa
haw Hawaiian
iw Hebrew
hi Hindi
hmn Hmong
hu Hungarian
is Icelandic
ig Igbo
id Indonesian
ia Interlingua
ga Irish
it Italian
ja Japanese
jw Javanese
kn Kannada
kk Kazakh
rw Kinyarwanda
rn Kirundi
kg Kongo
ko Korean
kri Krio (Sierra Leone)
ku Kurdish
ckb Kurdish (Soranî)
ky Kyrgyz
lo Laothian
la Latin
lv Latvian
ln Lingala
lt Lithuanian
loz Lozi
lg Luganda
ach Luo
lb Luxembourgish
mk Macedonian
mg Malagasy
ms Malay
ml Malayalam
mt Maltese
mi Maori
mr Marathi
mfe Mauritian Creole
mo Moldavian
mn Mongolian
my Myanmar (Burmese)
sr-ME Montenegrin
ne Nepali
pcm Nigerian Pidgin
nso Northern Sotho
no Norwegian
nn Norwegian (Nynorsk)
oc Occitan
or Oriya
om Oromo
ps Pashto
fa Persian
pl Polish
pt-BR Portuguese (Brazil)
pt Portuguese (Portugal)
pa Punjabi
qu Quechua
ro Romanian
rm Romansh
nyn Runyakitara
ru Russian
sm Samoan
gd Scots Gaelic
sr Serbian
sh Serbo-Croatian
st Sesotho
tn Setswana
crs Seychellois Creole
sn Shona
sd Sindhi
si Sinhalese
sk Slovak
sl Slovenian
so Somali
es Spanish
es-419 Spanish (Latin American)
su Sundanese
sw Swahili
sv Swedish
tg Tajik
ta Tamil
tt Tatar
te Telugu
th Thai
ti Tigrinya
to Tonga
lua Tshiluba
tum Tumbuka
tr Turkish
tk Turkmen
tw Twi
ug Uighur
uk Ukrainian
ur Urdu
uz Uzbek
vi Vietnamese
cy Welsh
wo Wolof
xh Xhosa
yi Yiddish
yo Yoruba
zu Zulu
Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:04,950 --> 00:00:06,500 - [Narrator] The Soviet era Luna Three 2 00:00:06,500 --> 00:00:08,960 was the first spacecraft to use gravity 3 00:00:08,960 --> 00:00:12,273 to change course to photograph the dark side of the Moon. 4 00:00:13,320 --> 00:00:15,820 The NASA Mariner 10 mission used the technique 5 00:00:15,820 --> 00:00:18,053 to swing by Venus to target Mercury. 6 00:00:18,910 --> 00:00:21,385 The gravity assist or a sling shot maneuver 7 00:00:21,385 --> 00:00:24,557 has become a standard for navigating the solar system 8 00:00:24,557 --> 00:00:27,440 with our probes reaching further, faster, 9 00:00:27,440 --> 00:00:29,563 and more accurately than ever before. 10 00:00:30,710 --> 00:00:33,460 (dramatic music) 11 00:01:05,879 --> 00:01:09,100 The Voyager mission started by chance over 40 years ago 12 00:01:09,100 --> 00:01:11,912 when Michael Minovitch, a mathematical PHD student 13 00:01:11,912 --> 00:01:15,800 decided to tackle celestial mechanics holy grail. 14 00:01:15,800 --> 00:01:19,430 It was known as the three body problem, as it looked at 15 00:01:19,430 --> 00:01:22,510 the Sun, a planet, and a third object traveling in space, 16 00:01:22,510 --> 00:01:25,020 and how gravity from the two objects 17 00:01:25,020 --> 00:01:27,123 affected the trajectory of the third. 18 00:01:29,040 --> 00:01:30,380 Minovitch was eager to take advantage 19 00:01:30,380 --> 00:01:33,640 of IBM's latest computer, the 7090. 20 00:01:33,640 --> 00:01:35,510 This computer was a second generation 21 00:01:35,510 --> 00:01:39,000 transistorized version of the IBM 709. 22 00:01:39,000 --> 00:01:41,930 A vacuum tube mainframe which had a processing speed 23 00:01:41,930 --> 00:01:44,330 of around 100 kiloflops per second. 24 00:01:44,330 --> 00:01:47,023 Unthinkably slow by today's standards. 25 00:01:50,250 --> 00:01:52,710 The laws of physics and the conservation of momentum 26 00:01:52,710 --> 00:01:54,330 demand that the probe approaching 27 00:01:54,330 --> 00:01:56,460 the gravitational influence of the planet 28 00:01:56,460 --> 00:01:59,920 and accelerating will then decelerate upon leaving 29 00:01:59,920 --> 00:02:04,240 that gravitational field with a net speed increase of zero. 30 00:02:04,240 --> 00:02:06,583 However, the probe's speed and direction 31 00:02:06,583 --> 00:02:08,853 will change in reference to the Sun. 32 00:02:09,870 --> 00:02:11,290 His solution has become known 33 00:02:11,290 --> 00:02:13,813 as gravity assist or sling shot. 34 00:02:18,710 --> 00:02:21,680 While undertaking an internship at NASA's JPL, 35 00:02:21,680 --> 00:02:24,523 he convinced them to test his model using their data. 36 00:02:25,480 --> 00:02:28,210 The results confirmed his predictions that if it flew 37 00:02:28,210 --> 00:02:31,240 close enough to a planet, a spacecraft could utilize 38 00:02:31,240 --> 00:02:34,993 that planet's motion to accelerate itself away from the Sun. 39 00:02:38,960 --> 00:02:41,920 When Cal Tech graduate Gary Flandro was tasked to see 40 00:02:41,920 --> 00:02:44,440 if gravity assist could aid deep space missions 41 00:02:44,440 --> 00:02:47,090 to the outer planets, he discovered there was to be 42 00:02:47,090 --> 00:02:50,890 an alliance of Jupiter, Saturn, Uranus, and Neptune, 43 00:02:50,890 --> 00:02:54,770 an even that occurred only once over 176 years. 44 00:02:54,770 --> 00:02:56,913 An opportunity not to be missed. 45 00:02:59,280 --> 00:03:03,190 So it was decided to launch a mission in 1977. 46 00:03:03,190 --> 00:03:04,750 Two spacecraft would be launched 47 00:03:04,750 --> 00:03:07,400 which would sling shot past all four of them. 48 00:03:07,400 --> 00:03:09,350 A grand tour of the solar system's 49 00:03:09,350 --> 00:03:12,550 outer planets in a 12 year time frame. 50 00:03:12,550 --> 00:03:14,861 This was to become known as the Voyager missions, 51 00:03:14,861 --> 00:03:16,513 and the rest is history. 52 00:03:21,380 --> 00:03:23,930 - Ultimately we're able to put together a picture 53 00:03:23,930 --> 00:03:27,360 of where we are in the galaxy and how that environment 54 00:03:27,360 --> 00:03:30,522 then influences our environment right here at home. 55 00:03:30,522 --> 00:03:33,070 In particular, the radiation environment 56 00:03:33,070 --> 00:03:35,760 which has implications for all sorts of things, 57 00:03:35,760 --> 00:03:38,723 including human exploration of space. 58 00:03:42,010 --> 00:03:44,340 - [Narrator] Today, those two spacecraft have continued on 59 00:03:44,340 --> 00:03:48,020 beyond the influence of our Sun into interstellar space. 60 00:03:48,020 --> 00:03:50,233 The farthest traveled by a manmade object. 61 00:03:59,440 --> 00:04:01,180 This field of influence found the basis 62 00:04:01,180 --> 00:04:03,840 for all future missions, allowing man to set 63 00:04:03,840 --> 00:04:06,693 his sights on getting into deep space economically. 64 00:04:07,840 --> 00:04:10,240 The Rosetta mission had different challenges 65 00:04:10,240 --> 00:04:12,510 to catch up with and orbit a comet, 66 00:04:12,510 --> 00:04:15,700 67P Churyumov-Gerasimenko. 67 00:04:15,700 --> 00:04:18,970 It had a large elliptical orbit around the Sun stretching 68 00:04:18,970 --> 00:04:22,173 from the orbit of Jupiter to within the orbit of Mars. 69 00:04:28,030 --> 00:04:31,140 Launched in 2004, a year later the probe 70 00:04:31,140 --> 00:04:33,700 passed by Earth for the first gravity assist 71 00:04:33,700 --> 00:04:35,903 that flung it towards the orbit of Mars. 72 00:04:41,210 --> 00:04:44,890 Two years later, Rosetta grazed Mars building up momentum, 73 00:04:44,890 --> 00:04:46,887 then swung by Earth for a second time, 74 00:04:46,887 --> 00:04:49,393 launching it deeper into space. 75 00:04:54,270 --> 00:04:56,547 The following year, Rosetta passed by asteroid Steins 76 00:04:56,547 --> 00:05:01,547 before swinging back for a third gravity assist from Earth. 77 00:05:01,570 --> 00:05:05,313 And in 2010, Rosetta passed by asteroid Lutetia. 78 00:05:06,630 --> 00:05:09,670 Going into hibernation, Rosetta continued its parabolic 79 00:05:09,670 --> 00:05:12,163 trajectory towards its final destination. 80 00:05:15,440 --> 00:05:17,810 Four years later, Rosetta emerged from 81 00:05:17,810 --> 00:05:21,092 its cold sleep as it crossed paths with the comet. 82 00:05:21,092 --> 00:05:22,743 A fortuitous flight indeed. 83 00:05:36,069 --> 00:05:38,090 The spacecraft then embarked on a series of maneuvers 84 00:05:38,090 --> 00:05:41,510 that took it on two successive triangular paths. 85 00:05:41,510 --> 00:05:44,970 It's trajectory was fine tuned with thruster burns until 86 00:05:44,970 --> 00:05:48,070 it closed in to within about 30 kilometers of the comet, 87 00:05:48,070 --> 00:05:50,783 where the spacecraft entered actual orbit around it. 88 00:05:51,690 --> 00:05:54,860 Rosetta remained with the comet, delivering it cargo, 89 00:05:54,860 --> 00:05:57,460 then conducting science observations as it swung 90 00:05:57,460 --> 00:06:00,740 about the Sun, then concluded with a gentle impact 91 00:06:00,740 --> 00:06:03,273 on the comet's surface in 2015. 92 00:06:06,240 --> 00:06:09,360 - We're gonna refine our ideas of what the comet is, 93 00:06:09,360 --> 00:06:11,720 where the comet came from, and encapsulate that 94 00:06:11,720 --> 00:06:14,899 within our ideas of how the solar system formed. 95 00:06:14,899 --> 00:06:17,900 And the complexity of the data set that we have also 96 00:06:17,900 --> 00:06:21,960 allows us to be more complex in our ideas and our theories. 97 00:06:21,960 --> 00:06:23,860 And that is the beauty of Rosetta, 98 00:06:23,860 --> 00:06:26,060 and we're starting to see that happening now. 99 00:06:26,060 --> 00:06:29,080 We're really able to hone down our ideas 100 00:06:29,080 --> 00:06:32,580 of how the comet formed, how that fits in the evolution 101 00:06:32,580 --> 00:06:35,080 of the solar system, and that's going to continue. 102 00:06:38,761 --> 00:06:41,090 The Ulysseys spacecraft had to leave the ecliptic plane 103 00:06:41,090 --> 00:06:44,950 of the solar system to study the polar regions of the Sun. 104 00:06:44,950 --> 00:06:48,650 Accordingly, it needed to change its orbital inclination. 105 00:06:48,650 --> 00:06:52,100 This required a large change in heliocentric velocity. 106 00:06:52,100 --> 00:06:56,230 So a gravity assist maneuver around Jupiter was chosen. 107 00:06:56,230 --> 00:06:59,080 The giant planet's gravity bent the spacecraft's 108 00:06:59,080 --> 00:07:01,620 flight path southward, putting it into a an orbit 109 00:07:01,620 --> 00:07:04,803 over and under the Sun's north and south poles. 110 00:07:06,920 --> 00:07:08,960 The ion powered Dawn spacecraft 111 00:07:08,960 --> 00:07:10,813 took maneuvering a step further. 112 00:07:12,320 --> 00:07:13,930 - [Marc] Dawn's the only spacecraft ever 113 00:07:13,930 --> 00:07:16,640 in more than 58 years of space exploration 114 00:07:16,640 --> 00:07:19,660 to orbit two extraterrestrial destinations. 115 00:07:19,660 --> 00:07:24,020 The last uncharted worlds in the inner solar system. 116 00:07:24,020 --> 00:07:27,530 And it not only allows us to get to these distant bodies, 117 00:07:27,530 --> 00:07:29,750 but once we're in orbit, we can maneuver 118 00:07:29,750 --> 00:07:32,490 extensively in order to get the best possible 119 00:07:32,490 --> 00:07:34,789 science that we can from them. 120 00:07:34,789 --> 00:07:37,539 (dramatic music) 121 00:07:46,380 --> 00:07:48,270 - [Narrator] NASA's latest mission is under way. 122 00:07:48,270 --> 00:07:51,100 Osirus Rex is the agency's first attempt 123 00:07:51,100 --> 00:07:54,520 at intercepting and touching down on an asteroid. 124 00:07:54,520 --> 00:07:56,580 No ordinary asteroid, either. 125 00:07:56,580 --> 00:07:58,280 Bennu is its name. 126 00:07:58,280 --> 00:08:00,870 Orbiting the Sun very close to Earth's orbit, 127 00:08:00,870 --> 00:08:02,140 it has been deemed a possible 128 00:08:02,140 --> 00:08:04,313 impact threat in the coming centuries. 129 00:08:06,540 --> 00:08:08,930 NASA intends to take a sample of the asteroid 130 00:08:08,930 --> 00:08:11,330 and return it to Earth for further study, 131 00:08:11,330 --> 00:08:14,373 and possibly help form plans to redirect Bennu. 132 00:08:17,650 --> 00:08:20,160 To match the orbit, Osiris Rex made a very close 133 00:08:20,160 --> 00:08:22,110 swing by the Earth a year after launch. 134 00:08:23,498 --> 00:08:26,998 (serene electronic music) 135 00:08:40,060 --> 00:08:42,540 It passed by the south pole to change its orbital 136 00:08:42,540 --> 00:08:46,156 inclinations several degrees to match that of Bennu. 137 00:08:46,156 --> 00:08:49,410 Once matching orbits, Osiris Rex must perform 138 00:08:49,410 --> 00:08:52,360 a series of braking maneuvers to match the velocity 139 00:08:52,360 --> 00:08:54,833 and enter an orbit around the asteroid. 140 00:09:01,910 --> 00:09:04,040 After mapping and studying the body, 141 00:09:04,040 --> 00:09:06,143 Osiris Rex will drop down to the surface 142 00:09:06,143 --> 00:09:08,513 and collect a sample of material. 143 00:09:09,580 --> 00:09:11,380 With some clever robotics, 144 00:09:11,380 --> 00:09:14,633 the sample return capsule will be delivered back to Earth. 145 00:09:19,870 --> 00:09:21,290 - Well the thing that is so intriguing to me 146 00:09:21,290 --> 00:09:24,240 about asteroids is that they really are time capsules. 147 00:09:24,240 --> 00:09:26,450 They actually are samples of what the solar system 148 00:09:26,450 --> 00:09:28,200 was like billions of years ago. 149 00:09:28,200 --> 00:09:30,330 Asteroids are small bodies that never 150 00:09:30,330 --> 00:09:32,640 got made into something big like a planet. 151 00:09:32,640 --> 00:09:35,440 So anything that got made into a planet got melted down, 152 00:09:35,440 --> 00:09:37,451 got changed, there were lots of things that went on. 153 00:09:37,451 --> 00:09:39,630 Asteroids are pristine. 154 00:09:39,630 --> 00:09:42,520 Nothing really altered them for billions of years. 155 00:09:42,520 --> 00:09:45,030 So when you go out and you take a sample of an asteroid, 156 00:09:45,030 --> 00:09:47,820 you have in your hands a real sample of 157 00:09:47,820 --> 00:09:49,910 what the solar system was like billions of years ago. 158 00:09:49,910 --> 00:09:52,420 What were the conditions, what was the chemistry like? 159 00:09:52,420 --> 00:09:54,680 What can you learn about the formation of our own planet 160 00:09:54,680 --> 00:09:57,070 and ourselves by looking at what the solar system 161 00:09:57,070 --> 00:09:59,060 was like billions of years ago? 162 00:09:59,060 --> 00:10:01,670 And this sample is incredibly scientifically important. 163 00:10:01,670 --> 00:10:02,820 I think that people will be studying it 164 00:10:02,820 --> 00:10:04,020 for generations to come. 165 00:10:15,040 --> 00:10:16,370 - [Narrator] The Juno space vehicle 166 00:10:16,370 --> 00:10:18,605 was launched in August 2011. 167 00:10:18,605 --> 00:10:21,950 In 2012 at Perihelion, the craft performed 168 00:10:21,950 --> 00:10:25,135 some maneuvers out beyond Mars orbit and arched back 169 00:10:25,135 --> 00:10:28,303 towards Earth for a kick in speed and direction. 170 00:10:35,630 --> 00:10:37,327 In October 2013, it flew by Earth 171 00:10:37,327 --> 00:10:40,770 a mere 500 kilometers from the surface. 172 00:10:40,770 --> 00:10:43,111 This sling shot sent it on a three year journey 173 00:10:43,111 --> 00:10:46,223 directly towards an intersection with Jupiter. 174 00:10:53,752 --> 00:10:56,170 - Jupiter orbit insertion is probably one 175 00:10:56,170 --> 00:10:58,510 of the most important things in the entire mission, 176 00:10:58,510 --> 00:11:01,840 and it's because that changes us from being in orbit 177 00:11:01,840 --> 00:11:05,488 around the Sun to being captured in orbit around Jupiter. 178 00:11:05,488 --> 00:11:07,612 And if you're not in orbit around Jupiter, 179 00:11:07,612 --> 00:11:10,933 you can't do the science we want to do. 180 00:11:10,933 --> 00:11:14,433 (serene electronic music) 181 00:11:25,290 --> 00:11:29,220 And what we're learning now is, even in other solar systems, 182 00:11:29,220 --> 00:11:32,460 they don't always all have a monster like Jupiter. 183 00:11:32,460 --> 00:11:34,060 And many people think, 184 00:11:34,060 --> 00:11:37,119 boy you almost need a Jupiter to have an Earth maybe. 185 00:11:37,119 --> 00:11:40,230 Jupiter played a big important role. 186 00:11:40,230 --> 00:11:44,410 But its environment, everything about it is extreme. 187 00:11:44,410 --> 00:11:47,130 It's the planet on steroids, right? 188 00:11:47,130 --> 00:11:51,707 It is the most extreme in every way it can be. 189 00:11:51,707 --> 00:11:54,300 So it has the strongest magnetic field, 190 00:11:54,300 --> 00:11:57,380 the strongest gravity field, it has the most 191 00:11:57,380 --> 00:12:00,960 harsh radiation, it's spinning super fast. 192 00:12:00,960 --> 00:12:04,893 I mean it's, everything about it is extreme environment. 193 00:12:10,910 --> 00:12:13,814 - The Juno mission is unique because it's the first time 194 00:12:13,814 --> 00:12:16,720 that we've ever gone in a polo of it, 195 00:12:16,720 --> 00:12:18,320 which goes from pole to pole. 196 00:12:18,320 --> 00:12:21,340 Over the north pole, through periapsis, 197 00:12:21,340 --> 00:12:23,322 and under the south pole. 198 00:12:23,322 --> 00:12:27,040 All the other missions we've done and all the observations 199 00:12:27,040 --> 00:12:30,080 we've made from Earth were made from the equator. 200 00:12:30,080 --> 00:12:32,720 And you don't see the poles very well 201 00:12:32,720 --> 00:12:33,730 if you're sitting on the equator. 202 00:12:33,730 --> 00:12:37,320 So this is the first time we got the first clear, 203 00:12:37,320 --> 00:12:40,030 unobstructed view of what the aurora looks like 204 00:12:40,030 --> 00:12:42,170 and what the polar phenomenon looks like. 205 00:12:42,170 --> 00:12:45,410 And at the same time we're flying through the magnetosphere 206 00:12:45,410 --> 00:12:47,824 right above the aurora so we can sample 207 00:12:47,824 --> 00:12:52,580 the charged particles that are precipitating down 208 00:12:52,580 --> 00:12:55,580 magnetic field lines, the guys that are exciting 209 00:12:55,580 --> 00:12:57,120 the emissions that we see. 210 00:12:57,120 --> 00:12:59,870 This is the first time we've ever been able to do that. 211 00:13:00,904 --> 00:13:03,654 (dramatic music) 212 00:13:16,276 --> 00:13:18,500 - [Narrator] The 6.7 year, five billion kilometer 213 00:13:18,500 --> 00:13:20,800 transit journey of the Cassini probe 214 00:13:20,800 --> 00:13:23,743 was slightly longer than the direct home and transfer. 215 00:13:28,240 --> 00:13:30,370 The mass of the Cassini spacecraft was such 216 00:13:30,370 --> 00:13:33,150 that even with a Titan Four launch vehicle, 217 00:13:33,150 --> 00:13:36,542 Cassini needed added help to reach Saturn. 218 00:13:36,542 --> 00:13:40,330 So to gain momentum, the Cassini mission 219 00:13:40,330 --> 00:13:43,221 included several gravitational sling shot maneuvers. 220 00:13:43,221 --> 00:13:46,378 Two flyby passes of Venus, one of the Earth, 221 00:13:46,378 --> 00:13:49,283 and then one from the mighty planet Jupiter. 222 00:13:53,240 --> 00:13:56,040 The Cassini orbiter then spent several years orbiting 223 00:13:56,040 --> 00:13:58,440 and maneuvering around the planet and its moons. 224 00:14:00,970 --> 00:14:03,620 Finally diving through the inner rings of the planet. 225 00:14:04,630 --> 00:14:07,572 - When we go into the proximal orbits between the rings 226 00:14:07,572 --> 00:14:10,350 and the planet, we've never been there before 227 00:14:10,350 --> 00:14:12,160 and we'll be a little bit more concerned. 228 00:14:12,160 --> 00:14:14,640 Here we've actually been closer to these rings, 229 00:14:14,640 --> 00:14:16,350 the Janus/Epimetheus Ring and the F Ring, 230 00:14:16,350 --> 00:14:18,320 when we went into orbit around Saturn. 231 00:14:18,320 --> 00:14:22,200 So this is not unexplored territory at this point. 232 00:14:22,200 --> 00:14:24,070 The nice thing about this though is that 233 00:14:24,070 --> 00:14:26,530 we've got a much better viewing angle of the rings 234 00:14:26,530 --> 00:14:29,040 because of the Sun this time around. 235 00:14:29,040 --> 00:14:31,633 - [Narrator] And eventually, into its atmosphere. 236 00:14:31,633 --> 00:14:34,383 (dramatic music) 237 00:14:52,724 --> 00:14:55,260 The New Horizons spacecraft had further to go than Cassini, 238 00:14:55,260 --> 00:14:57,870 but being far less massive a probe it was able 239 00:14:57,870 --> 00:15:00,153 to be launched directly towards Jupiter. 240 00:15:01,300 --> 00:15:03,550 The spacecraft was launched in 2006 241 00:15:03,550 --> 00:15:05,750 and made its way to Jupiter. 242 00:15:05,750 --> 00:15:08,050 Its closest approach happened only a year after 243 00:15:08,050 --> 00:15:11,833 its departure at a distance of 2.5 million kilometers. 244 00:15:17,570 --> 00:15:19,580 The flyby provided a gravity assist 245 00:15:19,580 --> 00:15:21,690 that increased the probes speed. 246 00:15:21,690 --> 00:15:24,310 It also allowed for a general test of New Horizon's 247 00:15:24,310 --> 00:15:27,107 scientific capabilities, returning data about 248 00:15:27,107 --> 00:15:30,860 the planet's atmosphere, moons, and magnetosphere. 249 00:15:36,640 --> 00:15:38,730 Most of the post Jupiter voyage was spent 250 00:15:38,730 --> 00:15:41,603 in hibernation mode to preserve onboard systems. 251 00:15:42,740 --> 00:15:45,070 In 2014, New Horizons was brought back 252 00:15:45,070 --> 00:15:47,470 online for the Pluto encounter. 253 00:15:47,470 --> 00:15:51,480 It flew 12,500 kilometers above the surface of Pluto, 254 00:15:51,480 --> 00:15:55,020 making it the first spacecraft to explore the dwarf planet. 255 00:15:55,020 --> 00:15:58,350 And the on into the Kuiper belt towards its next target, 256 00:15:58,350 --> 00:16:00,553 A Kuiper belt object most likely composed of frozen 257 00:16:00,553 --> 00:16:04,923 volatiles or ice, such as methane, ammonia, and water. 258 00:16:16,440 --> 00:16:18,640 A future probe to return to Jupiter's moons 259 00:16:18,640 --> 00:16:21,590 is destined for another multi-year journey. 260 00:16:21,590 --> 00:16:25,640 Juice, to be launched in 2022, will embark upon a seven year 261 00:16:25,640 --> 00:16:29,150 odyssey taking the spacecraft via an Earth swing by, 262 00:16:29,150 --> 00:16:32,880 then to Venus, back to Earth with a sling shot to Mars, 263 00:16:32,880 --> 00:16:37,363 then back to Earth for a final kick direct to Jupiter. 264 00:16:37,363 --> 00:16:40,863 (serene electronic music) 265 00:17:00,350 --> 00:17:03,540 Heading outward bound is one thing, but launching payloads 266 00:17:03,540 --> 00:17:07,230 inward towards the Sun is another set of problems. 267 00:17:07,230 --> 00:17:10,240 For example, the BepiColombo mission from Mercury launching 268 00:17:10,240 --> 00:17:14,073 this year will require nine gravity assist maneuvers. 269 00:17:18,760 --> 00:17:21,690 After launch, a two year journey using ion propulsion 270 00:17:21,690 --> 00:17:24,353 will bring it back to Earth for a kick towards Venus. 271 00:17:27,140 --> 00:17:29,690 Followed a year later by another flyby of Venus 272 00:17:29,690 --> 00:17:32,193 sending it closer towards the orbit of Mercury. 273 00:17:33,050 --> 00:17:35,720 In the following four years the spacecraft will pass by 274 00:17:35,720 --> 00:17:39,080 Mercury, tightening its heliocentric orbit, until it can 275 00:17:39,080 --> 00:17:42,560 match Mercury's speed, and with the aid of chemical rocket 276 00:17:42,560 --> 00:17:47,233 motors, insert itself into that planet's orbit in 2025. 277 00:17:51,690 --> 00:17:54,780 - So studying Mercury is crucial to better understand 278 00:17:54,780 --> 00:17:57,030 the formation of our solar system. 279 00:17:57,030 --> 00:17:59,250 Our Earth was formed, it evolved, 280 00:17:59,250 --> 00:18:01,140 and where we are coming from. 281 00:18:01,140 --> 00:18:04,520 So Mercury is in a way, the missing piece in the big puzzle 282 00:18:04,520 --> 00:18:07,610 of the formation of the solar system, and a crucial end 283 00:18:07,610 --> 00:18:11,788 member because it's close to the Sun and if you're going to 284 00:18:11,788 --> 00:18:15,610 get the full picture you have to look at the planet 285 00:18:15,610 --> 00:18:20,057 close to the Sun, as we also did in past missions that 286 00:18:20,057 --> 00:18:23,850 we were looking at the comets and planets further out. 287 00:18:23,850 --> 00:18:27,638 - Our main target is the environment around Mercury, 288 00:18:27,638 --> 00:18:30,000 especially the interaction between 289 00:18:30,000 --> 00:18:32,410 the solar wind and magnetosphere. 290 00:18:32,410 --> 00:18:35,490 - Mercury is three times closer to the Sun, 291 00:18:35,490 --> 00:18:39,470 and therefore the radiation or the heat 292 00:18:39,470 --> 00:18:42,090 which we are getting from Mercury is 10 times higher. 293 00:18:42,090 --> 00:18:44,489 So everything which we had to develop had to 294 00:18:44,489 --> 00:18:47,590 withstand the higher temperatures, but also the higher 295 00:18:47,590 --> 00:18:50,890 radiation doses, which we got from the solar wind. 296 00:18:50,890 --> 00:18:54,370 And for that we need special insulation of our space craft, 297 00:18:54,370 --> 00:18:57,130 special materials to be developed for the antenna, 298 00:18:57,130 --> 00:19:02,130 for the solar panels, and that was a very big 299 00:19:02,440 --> 00:19:04,627 challenge for the mission in itself. 300 00:19:06,321 --> 00:19:09,071 (dramatic music) 301 00:19:14,563 --> 00:19:18,063 (upbeat electronic music) 302 00:19:33,580 --> 00:19:35,410 - [Narrator] There are two more missions in the next year 303 00:19:35,410 --> 00:19:38,560 or two that will travel further inward than Mercury. 304 00:19:38,560 --> 00:19:42,283 ESA's solar orbiter, and NASA's Parker solar probe. 305 00:19:52,490 --> 00:19:57,020 Planned for a 2018/19 launch, ESA's solar orbiter will take 306 00:19:57,020 --> 00:20:00,710 several gravity assists from Earth and Venus to enter 307 00:20:00,710 --> 00:20:04,260 an elliptical orbit resonant with Venus so that subsequent 308 00:20:04,260 --> 00:20:07,370 gravity assists will raise the orbital inclination, 309 00:20:07,370 --> 00:20:10,260 resulting in an operational orbit of 25 degrees 310 00:20:10,260 --> 00:20:12,140 and climb to the ecliptic plane, 311 00:20:12,140 --> 00:20:14,390 and increasing to 34 degrees, 312 00:20:14,390 --> 00:20:17,823 making direct viewing of the Sun's polar regions possible. 313 00:20:21,610 --> 00:20:24,950 During the nominal seven year mission, the main scientific 314 00:20:24,950 --> 00:20:28,170 activity will take place during the near Sun encounter 315 00:20:28,170 --> 00:20:30,510 and high latitude parts of each orbit, 316 00:20:30,510 --> 00:20:33,433 with different science goals planned for each orbit. 317 00:20:52,681 --> 00:20:55,060 Together with NASA's Parker solar probe mission, 318 00:20:55,060 --> 00:20:57,450 it's hoped it will revolutionize our understanding 319 00:20:57,450 --> 00:21:00,880 of the Sun, where changing conditions can percolate out 320 00:21:00,880 --> 00:21:04,653 into the solar system affecting Earth and other worlds. 321 00:21:05,488 --> 00:21:08,988 (serene electronic music) 322 00:21:34,250 --> 00:21:36,886 Launch window is late 2018. 323 00:21:36,886 --> 00:21:38,900 It will use Venus gravity assists during 324 00:21:38,900 --> 00:21:41,730 seven flybys over nearly seven years 325 00:21:41,730 --> 00:21:44,080 to gradually bring its orbit closer to the Sun. 326 00:21:45,233 --> 00:21:48,733 (serene electronic music) 327 00:22:05,276 --> 00:22:08,120 At closest approach, the Parker solar probe will travel 328 00:22:08,120 --> 00:22:12,405 around the Sun at approximately 700,000 kilometers an hour. 329 00:22:12,405 --> 00:22:15,810 At closest approach to the Sun, some 10 times closer 330 00:22:15,810 --> 00:22:19,599 than Mercury, the front of Parker solar probe's solar shield 331 00:22:19,599 --> 00:22:24,543 faces temperatures approaching 1,377 degrees Celsius. 332 00:22:29,720 --> 00:22:32,040 It will travel through the Sun's atmosphere, 333 00:22:32,040 --> 00:22:35,014 closer to the surface than any space craft before it, 334 00:22:35,014 --> 00:22:38,005 facing brutal heat and radiation conditions, 335 00:22:38,005 --> 00:22:40,540 and ultimately providing humanity 336 00:22:40,540 --> 00:22:43,513 with the closest ever observations of a star. 337 00:22:51,550 --> 00:22:54,410 Flying into the outer most part of the Sun's atmosphere, 338 00:22:54,410 --> 00:22:58,000 known as the corona for the first time, Parker solar probe 339 00:22:58,000 --> 00:23:01,220 will employ a combination of instrumental measurements and 340 00:23:01,220 --> 00:23:05,240 imaging to revolutionize our understanding of the corona, 341 00:23:05,240 --> 00:23:07,960 expand our knowledge of the origin and evolution 342 00:23:07,960 --> 00:23:11,144 of the solar wind, and explore what accelerates 343 00:23:11,144 --> 00:23:14,623 the solar wind as well as solar energetic particles. 344 00:23:23,690 --> 00:23:26,588 It will also make critical contributions to our ability 345 00:23:26,588 --> 00:23:30,100 to forecast changes in our space environment 346 00:23:30,100 --> 00:23:33,473 that effect life and technology on Earth. 347 00:23:40,733 --> 00:23:43,483 (dramatic music) 29585

Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.