WEBVTT FILE 1 00:00:00.000 --> 00:00:01.334 (music throughout) 2 00:00:01.334 --> 00:00:09.342 On January 9, 2020, NASA’s Lucy Mission Team revealed that it would be visiting not seven asteroids as planned, but eight. 3 00:00:09.342 --> 00:00:13.646 As it turns out, Eurybates, one of the Trojan asteroids along Lucy’s path, 4 00:00:13.646 --> 00:00:16.816 has a small satellite or moonlet orbiting it. 5 00:00:16.816 --> 00:00:22.088 Finding these tiny, new worlds before Lucy is launched in 2021 means that 6 00:00:22.088 --> 00:00:27.327 the team can investigate their orbits and plan for more detailed follow-up observations during fly-bys. 7 00:00:27.327 --> 00:00:30.263 Dr. Keith Noll and other Lucy science team members 8 00:00:30.263 --> 00:00:35.402 have been using the Hubble Space Telescope to search for satellites and rings around Lucy’s targets. 9 00:00:35.402 --> 00:00:36.669 This can be challenging 10 00:00:36.669 --> 00:00:40.807 since the raw images are often filled with bumps, blobs and diffraction spikes. 11 00:00:40.807 --> 00:00:45.412 The Lucy team didn’t see any evidence of a new satellite until November 2019. 12 00:00:45.412 --> 00:00:49.416 After experimenting with the brightness and contrast on the Hubble images, 13 00:00:49.416 --> 00:00:53.386 Dr. Noll saw a peculiar, faint spot near the much brighter Eurybates. 14 00:00:53.386 --> 00:00:55.855 Dr. Mike Brown, another team member, 15 00:00:55.855 --> 00:00:59.159 noticed the spot showed up in a slightly different position 16 00:00:59.159 --> 00:01:01.327 on another set of Hubble images taken two days later 17 00:01:01.327 --> 00:01:05.165 This change suggested that the spot was an orbiting satellite. 18 00:01:05.165 --> 00:01:09.636 The team went back to Hubble and got 3 more chances to make observations of the possible new satellite. 19 00:01:09.636 --> 00:01:13.673 On the first two tries, the little moonlet was nowhere to be found. 20 00:01:13.673 --> 00:01:19.212 But on the third observation on January 3rd, 2020 they found the possible new satellite again 21 00:01:19.212 --> 00:01:24.250 It was clearly visible next to Eurybates, which is over 6000 times brighter. 22 00:01:24.250 --> 00:01:29.122 This huge difference in brightness suggests that the satellite is less than 1 kilometer in diameter, 23 00:01:29.122 --> 00:01:32.859 very small compared to Eurybates at 64 kilometers. 24 00:01:32.859 --> 00:01:34.294 With a few more Hubble observations 25 00:01:34.294 --> 00:01:36.663 the team pinned down the new satellite's orbit 26 00:01:36.663 --> 00:01:37.630 And they proposed a name 27 00:01:37.630 --> 00:01:39.532 The International Astronomical Union approved 28 00:01:39.532 --> 00:01:44.003 and from now on the little satellite will be known as "Queta" after Enriqueta Basilio 29 00:01:44.003 --> 00:01:46.072 the first woman to light the Olympic cauldron 30 00:01:46.072 --> 00:01:48.608 Evidence indicates that the Trojan Asteroid Eurybates 31 00:01:48.608 --> 00:01:53.313 is the largest fragment from a massive asteroid collision that happened billions of years ago 32 00:01:53.313 --> 00:01:57.183 It is possible that the new satellite, Queta, is a remnant of that catastrophic event. 33 00:01:57.183 --> 00:02:00.620 Whether with Hubble or with the Lucy spacecraft’s flyby, 34 00:02:00.620 --> 00:02:04.090 each observation enriches our understanding about the Trojan asteroids’ formation 35 00:02:04.090 --> 00:02:07.293 and Eurybates’ relationship with its newly discovered companion. 36 00:02:07.293 --> 00:02:09.696 The discovery of this new moonlet around the Trojan asteroid Eurybates 37 00:02:09.696 --> 00:02:13.333 is just a preview of the incredible scientific knowledge 38 00:02:13.333 --> 00:02:18.371 that will be captured by the Lucy mission as it explores this area of our Solar System.