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.