1 00:00:00,000 --> 00:00:07,710 [ music ] 2 00:00:07,730 --> 00:00:12,180 The Milky Way - home to billions of stars, 3 00:00:12,200 --> 00:00:17,310 rising and setting over billions of worlds, including our own. 4 00:00:17,330 --> 00:00:25,440 In this vast expanse, how did our Sun, the Earth, and the planets come to be? 5 00:00:25,460 --> 00:00:31,190 In recent decades, our understanding of the solar system's evolution has greatly improved, 6 00:00:31,210 --> 00:00:34,400 but deep questions remain. 7 00:00:34,420 --> 00:00:41,060 To answer those questions, astronomers are preparing to visit someplace very small. 8 00:00:41,080 --> 00:00:46,130 Asteroid Bennu. A lump of rock and organic material, 9 00:00:46,150 --> 00:00:52,930 the early building blocks of the solar system, of Earth, of us. 10 00:00:52,950 --> 00:01:01,550 Bennu is a time capsule, and its journey takes us way, way back...four and a half billion years. 11 00:01:01,570 --> 00:01:08,200 The raw ingredients of Bennu, and our solar system, originated in a stellar nursery: 12 00:01:08,220 --> 00:01:13,810 a vast cloud of hydrogen, helium, and dust. 13 00:01:13,830 --> 00:01:16,680 Our own Sun doesn't yet exist. 14 00:01:16,700 --> 00:01:21,510 Nearby are hot stars like this one, quickly burning up its fuel... 15 00:01:21,530 --> 00:01:28,430 and destroying itself in a colossal explosion called a supernova. 16 00:01:28,450 --> 00:01:35,880 The explosion destabilizes our cloud, causing it to collapse. 17 00:01:35,900 --> 00:01:40,660 In the geologic blink of an eye, a hundred thousand years, 18 00:01:40,680 --> 00:01:46,240 gravity and angular momentum flatten the cloud into a swirling disc. 19 00:01:46,260 --> 00:01:50,590 In the center, where molecules crash together tightest, 20 00:01:50,610 --> 00:01:55,600 a proto-star revs up to incredible pressures and temperatures. 21 00:01:55,620 --> 00:02:01,080 Deep within the disc, clumps of dust not much larger than a grain of wheat 22 00:02:01,100 --> 00:02:07,080 are flash heated into droplets of molten rock, called chondrules. 23 00:02:07,100 --> 00:02:10,330 The source of this heat remains a mystery. 24 00:02:10,350 --> 00:02:15,250 Chondrules are destined to become the building blocks of the solar system. 25 00:02:15,270 --> 00:02:20,230 Coaxed by gravity and turbulence, the chondrules clump. 26 00:02:20,250 --> 00:02:28,480 They grow into the first asteroids, into mountains, into planets. 27 00:02:28,500 --> 00:02:35,800 The asteroids are rubble piles of rock, metal, ice and organics. 28 00:02:35,820 --> 00:02:44,540 This large asteroid is the parent body of Bennu, a proto-planet whose size we can only guess. 29 00:02:44,560 --> 00:02:49,130 Closer to the proto-star, a planet begins to form. 30 00:02:49,150 --> 00:02:54,890 And then...dawn in the solar system. 31 00:02:54,910 --> 00:03:00,490 The proto-star undergoes fusion and ignites, revealing our Sun. 32 00:03:00,510 --> 00:03:05,080 But the solar system is far from finished. 33 00:03:05,100 --> 00:03:08,830 Jupiter most likely forms near its outer edge, 34 00:03:08,850 --> 00:03:15,820 but just 500 million years after the Sun ignites, some believe that it slowly moves inward. 35 00:03:15,840 --> 00:03:22,180 Its massive gravity ripples the asteroid belt, disrupting countless asteroids and comets, 36 00:03:22,200 --> 00:03:26,980 flinging them toward the Sun. 37 00:03:27,000 --> 00:03:33,380 They rain down on the inner planets, hammering and re-melting large portions of their crust. 38 00:03:33,400 --> 00:03:40,410 Did these impacts also deliver organics and water, key ingredients for life? 39 00:03:40,430 --> 00:03:44,600 Back in the asteroid belt, Bennu's parent body is lucky, 40 00:03:44,620 --> 00:03:48,500 it survives this period of heavy bombardment. 41 00:03:48,520 --> 00:03:56,120 The solar system cools and calms. Jupiter and its many moons assume the orbits that we see today. 42 00:03:56,140 --> 00:04:02,600 Billions of years of quiet follow...[ impact ] more or less. 43 00:04:02,620 --> 00:04:09,450 Then a billion years ago, one theory suggests a collision shatters the proto-planet. 44 00:04:09,470 --> 00:04:13,780 [ loud explosion ] 45 00:04:13,800 --> 00:04:20,580 Some of the debris loosely coalesces into a new, smaller body: Bennu. 46 00:04:20,600 --> 00:04:28,630 But Bennu will not stay in place. Dull, non-reflective, it slowly migrates toward the Sun. 47 00:04:28,650 --> 00:04:34,080 Solar heating turns its warm side into a low-intensity thruster. 48 00:04:34,100 --> 00:04:38,660 Through millions of years, Bennu's orbit gradually tightens, 49 00:04:38,680 --> 00:04:48,700 until it interacts with Saturn's gravity, altering its trajectory and hurling it into the inner solar system. 50 00:04:48,720 --> 00:04:52,730 Close encounters with Earth and Venus follow. 51 00:04:52,750 --> 00:04:57,940 Their gravitational tugs may have repeatedly stretched and reformed Bennu... 52 00:04:57,960 --> 00:05:02,880 turning it inside out and pulling off loose material. 53 00:05:02,900 --> 00:05:10,950 As a result, it has no satellites of its own...until now. 54 00:05:10,970 --> 00:05:19,190 Today, NASA is sending a spacecraft called OSIRIS-REx to explore Bennu and retrieve a sample. 55 00:05:19,210 --> 00:05:22,510 Why? Bennu has survived its long journey 56 00:05:22,530 --> 00:05:27,950 and settled into a near-Earth orbit, bringing its secrets within our reach. 57 00:05:27,970 --> 00:05:32,880 Now it is ready to teach us more about the solar system's history, 58 00:05:32,900 --> 00:05:40,980 its formation, its evolution, and our own place among the stars. 59 00:05:41,000 --> 00:05:47,280 [ music fades ] 60 00:05:47,300 --> 00:06:00,340 [ satellite beeping ]