WEBVTT FILE 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 ]