1 00:00:01,167 --> 00:00:03,436 Joan Cartan-Hansen, Host: From up here, you can see all the 2 00:00:03,436 --> 00:00:06,239 planets in our solar system, but do you know exactly what a 3 00:00:06,239 --> 00:00:07,774 planet is? 4 00:00:07,774 --> 00:00:08,942 Find out. 5 00:00:09,609 --> 00:00:15,382 (MUSIC) 6 00:00:15,382 --> 00:00:18,585 Mercury, Venus, Mars, Jupiter and Saturn were the first 7 00:00:18,585 --> 00:00:20,553 space objects called planets. 8 00:00:20,553 --> 00:00:24,657 The word planet means wanderer because the ancient Greeks saw 9 00:00:24,657 --> 00:00:27,093 them as moving lights in the sky. 10 00:00:27,093 --> 00:00:29,829 But the ancient Greeks didn't think of Earth as a planet. 11 00:00:29,829 --> 00:00:32,532 They thought it was the center of the universe and all space 12 00:00:32,532 --> 00:00:34,200 bodies revolved around it. 13 00:00:34,200 --> 00:00:37,337 Over time, humans learned the Sun is the center of our solar 14 00:00:37,337 --> 00:00:38,605 system. 15 00:00:38,605 --> 00:00:41,474 And all the planets, including Earth, orbit around it. 16 00:00:41,474 --> 00:00:44,110 Still, defining a planet was back then was easy. 17 00:00:44,110 --> 00:00:46,980 Everything, the Sun, the Moon, the Earth, all space bodies 18 00:00:46,980 --> 00:00:48,448 were called planets. 19 00:00:48,448 --> 00:00:50,817 Until a new invention came along. 20 00:00:50,817 --> 00:00:54,120 In 1781, Uranus became the first planet discovered by 21 00:00:54,120 --> 00:00:55,321 telescope. 22 00:00:55,321 --> 00:00:57,757 And by then, scientists had realized that the Sun was a 23 00:00:57,757 --> 00:01:00,126 star and the Moon was a natural satellite of the 24 00:01:00,126 --> 00:01:01,127 Earth. 25 00:01:01,127 --> 00:01:04,030 But everything else was pretty much described as a planet. 26 00:01:04,030 --> 00:01:08,301 Neptune was discovered in 1846 and Pluto in 1930. 27 00:01:08,301 --> 00:01:11,237 But Pluto is different from terrestrial planets like 28 00:01:11,237 --> 00:01:14,974 Mercury, Venus, Earth and Mars or the gas giants like Jupiter 29 00:01:14,974 --> 00:01:19,112 and Saturn or the ice giants like Uranus or Neptune. 30 00:01:19,112 --> 00:01:20,380 Pluto is small. 31 00:01:20,380 --> 00:01:23,049 And its moon, Charon, is half the size of Pluto. 32 00:01:23,049 --> 00:01:25,785 It's so big that the two are sometimes called a double 33 00:01:25,785 --> 00:01:27,387 planet system. 34 00:01:27,387 --> 00:01:30,523 Pluto has an usual orbit that sometimes brings it closer to 35 00:01:30,523 --> 00:01:31,891 the Sun than Neptune. 36 00:01:31,891 --> 00:01:34,761 And its orbit isn't circular like the other planets. 37 00:01:34,761 --> 00:01:38,131 Pluto is different and that lead to confusion. 38 00:01:38,131 --> 00:01:41,601 By 1992, planetary scientists found a number of ice worlds 39 00:01:41,601 --> 00:01:43,436 in the Kuiper Belt. 40 00:01:43,436 --> 00:01:44,304 Brian Jackson, Assoc. 41 00:01:44,304 --> 00:01:46,673 Prof. of Physics, Boise State University: The Kuiper Belt is 42 00:01:46,673 --> 00:01:49,142 a donut shaped region in the outer solar system, beyond the 43 00:01:49,142 --> 00:01:50,443 orbit of Neptune. 44 00:01:50,443 --> 00:01:53,646 And it's filled with objects, made up mostly of ice, so 45 00:01:53,646 --> 00:01:56,483 water ice, but also methane and ammonia ice. 46 00:01:56,483 --> 00:01:58,818 And some of these objects are large enough that we would 47 00:01:58,818 --> 00:01:59,819 call them ice worlds. 48 00:01:59,819 --> 00:02:02,489 And some of these ice worlds in the Kuiper Belt, they 49 00:02:02,489 --> 00:02:03,790 look a lot like Pluto. 50 00:02:03,790 --> 00:02:05,992 And so, astronomers were faced with this question. 51 00:02:05,992 --> 00:02:08,194 If we were going to call Pluto a planet, what were we going 52 00:02:08,194 --> 00:02:11,197 to call all these hundreds of thousands of other objects, 53 00:02:11,197 --> 00:02:13,867 very similar to Pluto in the Kuiper Belt. 54 00:02:13,867 --> 00:02:16,636 Cartan-Hansen: So, astronomers, decided they needed to clarify 55 00:02:16,636 --> 00:02:19,539 what exactly is a planet. 56 00:02:19,539 --> 00:02:23,176 In 2006, the International Astronomical Union, a 57 00:02:23,176 --> 00:02:26,012 worldwide group of top astronomers, came up with a 58 00:02:26,012 --> 00:02:28,114 new definition... 59 00:02:28,114 --> 00:02:30,817 A planet is a celestial body that is in orbit around the 60 00:02:30,817 --> 00:02:32,051 Sun. 61 00:02:32,051 --> 00:02:35,421 It has enough mass so gravity helps make it round. 62 00:02:35,421 --> 00:02:38,358 And it has cleared the neighborhood around its orbit. 63 00:02:38,358 --> 00:02:41,528 Jackson: So that means that the object has enough mass and 64 00:02:41,528 --> 00:02:45,231 enough gravity that it consumes or sweeps up other 65 00:02:45,231 --> 00:02:48,701 small bodies in its orbital path and Pluto, since there's 66 00:02:48,701 --> 00:02:51,337 a lot of other objects out there, doesn't do that. 67 00:02:51,337 --> 00:02:53,273 It's just too small. 68 00:02:53,273 --> 00:02:55,208 Cartan-Hansen: So, what to do with Pluto? 69 00:02:55,208 --> 00:02:58,044 Astronomers came up with the idea of a dwarf planet. 70 00:02:58,044 --> 00:03:00,480 A dwarf planet orbits around the Sun. 71 00:03:00,480 --> 00:03:03,383 It has enough mass and gravity to form an almost round shape. 72 00:03:03,383 --> 00:03:05,785 But it isn't big enough to clear the neighborhood. 73 00:03:05,785 --> 00:03:08,254 It also can't be a moon. 74 00:03:08,254 --> 00:03:11,791 As of 2020, we have five dwarf planets in our solar system. 75 00:03:11,791 --> 00:03:15,295 In order closest to the sun out, they are Ceres, Pluto, 76 00:03:15,295 --> 00:03:18,565 Haumea, Makemake and Eris. 77 00:03:18,565 --> 00:03:21,200 Ceres is the closest dwarf planet to the Sun. 78 00:03:21,200 --> 00:03:23,636 It's located in the asteroid belt, between Mars and 79 00:03:23,636 --> 00:03:26,406 Jupiter, making it the only dwarf planet in the inner 80 00:03:26,406 --> 00:03:27,907 solar system. 81 00:03:27,907 --> 00:03:30,376 Next comes Pluto, then Haumea. 82 00:03:30,376 --> 00:03:33,346 Haumea has an elongated shape rather than being totally 83 00:03:33,346 --> 00:03:36,449 round, probably because of the speed of its rotation. 84 00:03:36,449 --> 00:03:37,884 Next is Makemake. 85 00:03:37,884 --> 00:03:41,220 Makemake has a moon and is a classic Kuiper Belt object. 86 00:03:41,220 --> 00:03:42,689 And finally, Eris... 87 00:03:42,689 --> 00:03:45,625 Eris is almost as large as Pluto and was once considered 88 00:03:45,625 --> 00:03:48,661 our solar system's tenth planet. 89 00:03:48,661 --> 00:03:51,064 Jackson: Planetary scientists are still looking for dwarf 90 00:03:51,064 --> 00:03:52,165 planets. 91 00:03:52,165 --> 00:03:54,167 This is an active area of research. 92 00:03:54,167 --> 00:03:56,636 There may be another hundred in our solar system and 93 00:03:56,636 --> 00:04:00,506 probably hundreds more just outside of the Kuiper Belt. 94 00:04:00,506 --> 00:04:02,775 Cartan-Hansen: Not everyone agrees with the new definition 95 00:04:02,775 --> 00:04:04,010 of a planet. 96 00:04:04,010 --> 00:04:07,280 Some still think Pluto deserves that title. 97 00:04:07,280 --> 00:04:10,116 Jackson: That's true, but the definition of a planet may 98 00:04:10,116 --> 00:04:12,952 still change as we learn more about our solar system and 99 00:04:12,952 --> 00:04:16,389 just because Pluto and Ceres and all those other objects 100 00:04:16,389 --> 00:04:18,691 are called dwarf planets it really doesn't make them any 101 00:04:18,691 --> 00:04:19,993 less interesting. 102 00:04:19,993 --> 00:04:22,996 What we call them is almost the least interesting aspect 103 00:04:22,996 --> 00:04:25,598 of these objects which have a fascinating variety of 104 00:04:25,598 --> 00:04:26,699 phenomena. 105 00:04:26,699 --> 00:04:29,802 It's just our current way of classifying one of the many 106 00:04:29,802 --> 00:04:31,537 wonders of space. 107 00:04:32,372 --> 00:04:34,741 Cartan-Hansen: If you want to learn more about planets and 108 00:04:34,741 --> 00:04:37,010 dwarf planets, check out the science trek website. 109 00:04:37,010 --> 00:04:39,545 You'll find it at science trek dot org. 110 00:04:40,580 --> 00:05:00,433 (MUSIC) 111 00:05:00,433 --> 00:05:02,802 Announcer: Presentation of Science Trek on Idaho Public 112 00:05:02,802 --> 00:05:06,305 Television is made possible through the generous support 113 00:05:06,305 --> 00:05:09,375 of the Laura Moore Cunningham Foundation, committed to 114 00:05:09,375 --> 00:05:12,145 fulfilling the Moore and Bettis family legacy of 115 00:05:12,145 --> 00:05:14,614 building the great state of Idaho. 116 00:05:14,614 --> 00:05:17,917 By the Idaho National Laboratory, mentoring talent 117 00:05:17,917 --> 00:05:20,887 and finding solutions for energy and security 118 00:05:20,887 --> 00:05:24,891 challenges, by the Friends of Idaho Public Television and 119 00:05:24,891 --> 00:05:27,226 the Corporation for Public Broadcasting.