WEBVTT FILE 1 00:00:00.000 --> 00:00:03.837 [music throughout] It appears some pieces of asteroid Vesta 2 00:00:03.837 --> 00:00:09.876 ended up on asteroid Bennu, according to observations from NASA’s OSIRIS-REx spacecraft. 3 00:00:09.876 --> 00:00:14.280 The new result sheds light on the intricate orbital dance of asteroids 4 00:00:14.280 --> 00:00:15.982 and on the violent origin of Bennu, 5 00:00:15.982 --> 00:00:20.387 which is a “rubble pile” asteroid that coalesced from the fragments of a massive collision. 6 00:00:20.387 --> 00:00:24.324 Six boulders, ranging in size from 5 to 14 feet, 7 00:00:24.324 --> 00:00:27.927 were discovered scattered across Bennu’s southern hemisphere near the equator. 8 00:00:27.927 --> 00:00:30.597 These boulders are much brighter than the rest of Bennu, 9 00:00:30.597 --> 00:00:33.733 with some appearing as much as 10x brighter than their surroundings. 10 00:00:33.733 --> 00:00:37.170 The unusual boulders on Bennu first caught the team’s eye in images 11 00:00:37.170 --> 00:00:39.406 from the OSIRIS-REx Camera Suite instrument. 12 00:00:39.406 --> 00:00:42.742 The team analyzed the boulders using an onboard spectrometer, 13 00:00:42.742 --> 00:00:45.111 which separates light into its component colors. 14 00:00:45.111 --> 00:00:49.249 Since elements and compounds have distinct, signature patterns of bright and dark 15 00:00:49.249 --> 00:00:52.685 across a range of colors, they can be identified using a spectrometer. 16 00:00:52.685 --> 00:00:55.555 The signature from the boulders was characteristic of the mineral 17 00:00:55.555 --> 00:00:57.757 pyroxene from Vesta and the vestoids, 18 00:00:57.757 --> 00:01:00.894 smaller asteroids that are fragments blasted from Vesta 19 00:01:00.894 --> 00:01:03.630 when it sustained significant asteroid impacts. 20 00:01:03.630 --> 00:01:07.233 The team tested a few different theories to determine the origin of these boulders: 21 00:01:07.233 --> 00:01:10.670 First, it’s possible that the boulders were originally part of Bennu 22 00:01:10.670 --> 00:01:15.275 or its parent body; however, this is unlikely based on how pyroxene is created. 23 00:01:15.275 --> 00:01:19.112 This mineral typically forms when rocky material melts at high-temperature. 24 00:01:19.112 --> 00:01:21.514 Bennu is composed of water-bearing minerals, 25 00:01:21.514 --> 00:01:24.350 so it wouldn’t have experienced very high temperatures in its history. 26 00:01:24.350 --> 00:01:27.020 Next, the team considered localized heating, 27 00:01:27.020 --> 00:01:28.455 perhaps from an impact. 28 00:01:28.455 --> 00:01:31.191 The scale of an impact needed to create large pyroxene boulders 29 00:01:31.191 --> 00:01:35.128 is much more significant than what is expected to take place in the main asteroid belt. 30 00:01:35.128 --> 00:01:37.197 So, the team ruled out these scenarios, 31 00:01:37.197 --> 00:01:39.899 and instead considered other pyroxene-rich asteroids 32 00:01:39.899 --> 00:01:42.869 that might have implanted this material to Bennu or its parent. 33 00:01:42.869 --> 00:01:46.139 This is possible because as asteroids move through the solar system, 34 00:01:46.139 --> 00:01:48.208 their orbits can be altered in many ways 35 00:01:48.208 --> 00:01:51.177 including by the pull of gravity from planets and other objects, 36 00:01:51.177 --> 00:01:54.380 meteoroid impacts, and even the slight pressure from sunlight. 37 00:01:54.380 --> 00:01:57.350 The new result helps pin down the complex journey Bennu 38 00:01:57.350 --> 00:02:00.086 and other asteroids have traced through the solar system.