1 00:00:00,000 --> 00:00:05,338 For decades, astronomers believed that one thing was as certain as death 2 00:00:05,338 --> 00:00:07,640 and taxes: the Milky Way 3 00:00:07,640 --> 00:00:11,177 and our neighboring Andromeda galaxy were on a crash course… 4 00:00:11,177 --> 00:00:15,448 destined to collide in less than 5 billion years. 5 00:00:15,448 --> 00:00:18,785 That galactic smash-up would spark massive star 6 00:00:18,785 --> 00:00:22,722 formation, scatter stars like cosmic billiard balls, 7 00:00:22,722 --> 00:00:26,226 and possibly throw our Sun into a whole new orbit. 8 00:00:26,226 --> 00:00:29,662 But now… that future may not be so certain. 9 00:00:29,662 --> 00:00:35,168 Thanks to fresh data from NASA’s Hubble Space Telescope and ESA’s Gaia mission, 10 00:00:35,168 --> 00:00:39,939 researchers have re-run the numbers, and they’re telling a different story. 11 00:00:39,939 --> 00:00:43,777 Astronomers ran 100,000 computer simulations 12 00:00:43,777 --> 00:00:47,680 using the most precise data available today. 13 00:00:47,680 --> 00:00:48,882 The results? 14 00:00:48,882 --> 00:00:51,951 There’s only about a 50-50 chance of a collision 15 00:00:51,951 --> 00:00:55,221 happening within the next 10 billion years. 16 00:00:55,221 --> 00:00:58,525 That’s right, there’s now a decent chance the Milky Way 17 00:00:58,525 --> 00:01:02,362 and Andromeda will simply… pass by each other. 18 00:01:02,362 --> 00:01:03,797 No cosmic fireworks. 19 00:01:03,797 --> 00:01:05,398 No galactic pile-up. 20 00:01:05,398 --> 00:01:08,368 Just a long, swirling orbital dance. 21 00:01:08,368 --> 00:01:09,836 Why the change? 22 00:01:09,836 --> 00:01:11,371 This new study factors in 23 00:01:11,371 --> 00:01:14,974 not just the main galaxies, but also their massive satellite 24 00:01:14,974 --> 00:01:19,212 companions, like the Large Magellanic Cloud and M33. 25 00:01:19,212 --> 00:01:22,715 These smaller galaxies tug and twist the larger ones, 26 00:01:22,715 --> 00:01:26,953 disrupting the neat two-body collision model we once relied on. 27 00:01:26,953 --> 00:01:30,990 In fact, the Large Magellanic Cloud’s gravitational pull 28 00:01:30,990 --> 00:01:33,693 might even guide us away from Andromeda. 29 00:01:33,693 --> 00:01:34,627 So… 30 00:01:34,627 --> 00:01:37,397 The universe may be saving us from a collision 31 00:01:37,397 --> 00:01:39,799 we were never going to witness anyway. 32 00:01:39,799 --> 00:01:43,436 After all, Earth becomes uninhabitable in about a billion years 33 00:01:43,436 --> 00:01:47,340 due to the Sun’s heat, and the Sun itself burns out in five. 34 00:01:47,340 --> 00:01:50,477 But hey, you never know, someone might still be around! 35 00:01:50,477 --> 00:01:54,414 Andromeda and the Milky Way may eventually collide (or not) 36 00:01:54,414 --> 00:01:58,718 at the end of their orbital dance, but the uncertainties in the simulations 37 00:01:58,718 --> 00:02:01,788 means we just can't say one way or the other. 38 00:02:01,788 --> 00:02:06,126 While the fate of our galaxy remains uncertain, one thing is clear: 39 00:02:06,126 --> 00:02:11,397 the universe is more complex, and more surprising, than we ever imagined. 40 00:02:11,397 --> 00:02:27,614 Follow us on social media @NASAHubble and NASA.GOV/HUBBLE 41 00:02:27,614 --> 00:02:32,919 NASA Meatball