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]