WEBVTT FILE 1 00:00:00.020 --> 00:00:04.070 The solar system is a dangerous place. 2 00:00:04.090 --> 00:00:08.110 One hazard is impacts from rocky debris 3 00:00:08.130 --> 00:00:12.130 traveling tens of thousands of miles an hour. 4 00:00:12.150 --> 00:00:16.190 Large fragments can tear a spacecraft apart, but even the smallest 5 00:00:16.210 --> 00:00:20.270 pieces gradually take their toll, eroding spacecraft surfaces 6 00:00:20.290 --> 00:00:24.320 and components. Dust-sized particles shed 7 00:00:24.340 --> 00:00:28.340 from comets and asteroids and smaller than a single grain of sand, 8 00:00:28.360 --> 00:00:32.450 traverse the solar system at speeds reaching 40,000 miles an hour. 9 00:00:32.470 --> 00:00:36.590 Our best knowledge of these tiniest meteoroids 10 00:00:36.610 --> 00:00:40.720 comes from measurements made near Earth. 11 00:00:40.740 --> 00:00:44.910 Now, a clever new technique using the LISA Pathfinder spacecraft is measuring 12 00:00:44.930 --> 00:00:49.100 this population of particles at nearly a million miles away. 13 00:00:49.120 --> 00:00:53.170 Launched in 2015, LISA Pathfinder is a 14 00:00:53.190 --> 00:00:57.210 technology demonstrator for the space-based detection of gravitational waves 15 00:00:57.230 --> 00:01:01.270 led by the European Space Agency and with participation 16 00:01:01.290 --> 00:01:05.360 by NASA. The full observatory would work by tracking 17 00:01:05.380 --> 00:01:09.440 reference objects called proof masses that move under the 18 00:01:09.460 --> 00:01:13.460 influence of gravity, which means the spacecraft must reduce all 19 00:01:13.480 --> 00:01:17.590 other forces to an astonishing degree. Tests show 20 00:01:17.610 --> 00:01:21.730 LISA Pathfinder is the most precise tool for measuring accelerations 21 00:01:21.750 --> 00:01:25.930 ever flown, reducing non-gravitational forces to levels 22 00:01:25.950 --> 00:01:30.120 required to detect passing gravitational waves. 23 00:01:30.140 --> 00:01:34.310 Because LISA Pathfinder is extremely sensitive to its environment, 24 00:01:34.330 --> 00:01:38.420 it's also sensitive to those tiny nudges from micrometeoroids. 25 00:01:38.440 --> 00:01:42.460 These impacts would be reflected in motions of the proof masses, 26 00:01:42.480 --> 00:01:46.500 how the spacecraft thrusters fired to counteract the impact, and other data. 27 00:01:46.520 --> 00:01:50.570 Using software originally written to sift out the the faint signatures of 28 00:01:50.590 --> 00:01:54.620 gravitational waves in ground-based detectors, the science team found 29 00:01:54.640 --> 00:01:58.670 several impacts. When it is struck, the impact 30 00:01:58.690 --> 00:02:02.750 both pushes and twists the spacecraft. Onboard sensors 31 00:02:02.770 --> 00:02:06.820 detect this change and fire the Pathfinder's ultra-precise thrusters to 32 00:02:06.840 --> 00:02:10.890 compensate. At full power, each of these only generates about as much 33 00:02:10.910 --> 00:02:14.950 force as the weight of a mosquito. Knowing what it took to restore 34 00:02:14.970 --> 00:02:19.010 the spacecraft's orientation gives scientists information 35 00:02:19.030 --> 00:02:23.070 on the original direction of the particle, its momentum, and where it struck the 36 00:02:23.090 --> 00:02:27.250 spacecraft. LISA Pathfinder is located at Earth-sun L1, 37 00:02:27.270 --> 00:02:31.430 a gravitational balance point about million miles from Earth's 38 00:02:31.450 --> 00:02:35.540 sunward side. This is essentially unexplored territory for 39 00:02:35.560 --> 00:02:39.590 understanding the solar system's dust distribution. By comparing 40 00:02:39.610 --> 00:02:43.640 how often Pathfinder is hit, and the particles' origins, 41 00:02:43.660 --> 00:02:47.690 scientists can refine their models of solar system composition and formation. 42 00:02:47.710 --> 00:02:51.790 By improving our understanding of the solar system's 43 00:02:51.810 --> 00:02:55.840 dust environment, LISA Pathfinder will also help pave the way 44 00:02:55.860 --> 00:02:59.900 for future giant telescopes whose large optics could be degraded 45 00:02:59.920 --> 00:03:03.990 by these impacts. It's an intriguing side benefit from testing spacecraft 46 00:03:04.010 --> 00:03:08.110 technology that will one day be used to observe merging black holes 47 00:03:08.130 --> 00:03:12.240 billions of light years away. 48 00:03:12.260 --> 00:03:16.280 [Music] 49 00:03:16.300 --> 00:03:20.460 50 00:03:20.480 --> 00:03:24.650 [Beeping] 51 00:03:24.670 --> 00:03:28.830 [Beeping] 52 00:03:28.850 --> 00:03:33.127 [Beeping]