English subtitles for clip: File:ESOcast 24.webm
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1 00:00:02,000 --> 00:00:07,000 An exoplanet orbiting a star that entered our Milky Way from another galaxy 2 00:00:07,000 --> 00:00:11,000 has been detected by a European team of astronomers. 3 00:00:11,000 --> 00:00:14,000 The Jupiter-like planet is particularly unusual, 4 00:00:14,000 --> 00:00:18,000 as it is orbiting a star nearing the end of its life 5 00:00:18,000 --> 00:00:20,000 and could be about to be engulfed by it, 6 00:00:20,000 --> 00:00:24,000 giving tantalising clues about the fate of our own planetary system 7 00:00:24,000 --> 00:00:26,000 in the distant future. 8 00:00:31,000 --> 00:00:33,000 This is the ESOcast! 9 00:00:33,000 --> 00:00:36,000 Cutting-edge science and life behind the scenes at ESO 10 00:00:36,000 --> 00:00:38,000 the European Southern Observatory. 11 00:00:38,000 --> 00:00:44,000 Exploring the ultimate frontier with our host Dr J, a.k.a. Dr Joe Liske. 12 00:00:49,000 --> 00:00:51,000 Hello and welcome to the ESOcast. 13 00:00:51,000 --> 00:00:56,000 In this episode we are going to find out how an act of galactic cannibalism 14 00:00:56,000 --> 00:01:01,000 has brought a planet from another galaxy within astronomers’ reach. 15 00:01:01,000 --> 00:01:05,000 Astronomers have detected nearly 500 planets 16 00:01:05,000 --> 00:01:07,000 orbiting stars in our cosmic neighbourhood, 17 00:01:07,000 --> 00:01:11,000 but none outside our Milky Way has been confirmed. 18 00:01:11,000 --> 00:01:17,000 Now, however, a planet weighing at least 1.25 times as much as Jupiter 19 00:01:17,000 --> 00:01:21,000 has been discovered orbiting a star of extragalactic origin, 20 00:01:21,000 --> 00:01:26,000 even though the star now finds itself within our own galaxy. 21 00:01:26,000 --> 00:01:31,000 The star, which is known as HIP13044 22 00:01:31,000 --> 00:01:36,000 lies about 2000 light-years from Earth and is part of the so-called Helmi stream. 23 00:01:36,000 --> 00:01:40,000 This stream of stars originally belonged to a dwarf galaxy, 24 00:01:40,000 --> 00:01:42,000 which was devoured by our Milky Way 25 00:01:42,000 --> 00:01:47,000 in an act of galactic cannibalism six to nine billion years ago. 26 00:01:47,000 --> 00:01:52,000 Astronomers detected the planet by looking for tiny telltale wobbles of the star 27 00:01:52,000 --> 00:01:56,000 caused by the gravitational tug of an orbiting companion. 28 00:01:56,000 --> 00:01:58,000 For these precise observations, 29 00:01:58,000 --> 00:02:02,000 the team used a high resolution spectrograph called FEROS, 30 00:02:02,000 --> 00:02:08,000 attached to the 2.2-metre telescope at ESO’s La Silla Observatory in Chile. 31 00:02:11,000 --> 00:02:17,000 The planet, HIP 13044 b, is also one of the few exoplanets known 32 00:02:17,000 --> 00:02:21,000 to have survived its host star massively growing in size 33 00:02:21,000 --> 00:02:24,000 after exhausting the hydrogen fuel supply in its core 34 00:02:24,000 --> 00:02:28,000 i.e. the Red Giant phase of stellar evolution. 35 00:02:28,000 --> 00:02:33,000 HIP 13044 b is near to its host star. 36 00:02:33,000 --> 00:02:35,000 At the closest point in its elliptical orbit, 37 00:02:35,000 --> 00:02:39,000 it is less than one stellar diameter from the surface of the star 38 00:02:39,000 --> 00:02:44,000 (or only about 0.055 times the Sun-Earth distance), 39 00:02:44,000 --> 00:02:48,000 and it completes an orbit in only about 16 days. 40 00:02:48,000 --> 00:02:50,000 The astronomers hypothesise 41 00:02:50,000 --> 00:02:54,000 that the planet's orbit might initially have been much larger, 42 00:02:54,000 --> 00:02:58,000 but that it moved inwards during the Red Giant phase. 43 00:02:58,000 --> 00:03:02,000 Any closer-in planets may not have been so lucky. 44 00:03:02,000 --> 00:03:04,000 Astronomers suggest that some inner planets 45 00:03:04,000 --> 00:03:09,000 may have been swallowed by the star during its Red Giant phase. 46 00:03:09,000 --> 00:03:11,000 Although the Jupiter-like exoplanet 47 00:03:11,000 --> 00:03:14,000 has escaped the fate of these inner planets so far, 48 00:03:14,000 --> 00:03:18,000 the star will expand again in the next stage of its evolution. 49 00:03:18,000 --> 00:03:21,000 When this happens, the star may engulf the planet, 50 00:03:21,000 --> 00:03:25,000 meaning it may be doomed after all. 51 00:03:26,000 --> 00:03:29,000 The astronomers are now searching for more planets 52 00:03:29,000 --> 00:03:31,000 around stars near the end of their lives. 53 00:03:31,000 --> 00:03:36,000 Their work may tell us about the distant fate of the planets in our own Solar System, 54 00:03:36,000 --> 00:03:39,000 as the Sun is also expected to become a Red Giant 55 00:03:39,000 --> 00:03:41,000 in about five billion years. 56 00:03:42,000 --> 00:03:45,000 This is Dr J signing off for the ESOcast. 57 00:03:45,000 --> 00:03:49,000 Join me again next time for another cosmic adventure. 58 00:03:50,000 --> 00:03:54,000 ESOcast is produced by ESO, the European Southern Observatory. 59 00:03:54,000 --> 00:03:58,000 ESO, the European Southern Observatory, is the pre-eminent intergovernmental science and technology organisation in astronomy, 60 00:03:58,000 --> 00:04:01,000 designing, constructing and operating the world’s most advanced ground-based telescopes. 61 00:04:03,000 --> 00:04:08,000 Transcription by ESO ; translation by — 62 00:04:15,000 --> 00:04:18,000 Now that you've caught up with ESO, 63 00:04:19,000 --> 00:04:23,000 head 'out of this world' with Hubble. 64 00:04:24,000 --> 00:04:33,000 The Hubblecast highlights the latest discoveries of the world´s most recognized and prized space observatory, 65 00:04:34,000 --> 00:04:38,000 the NASA/ESA Hubble Space Telescope