1 00:00:02,040 --> 00:00:07,080 Speaker 1: Welcome to brain Stuff from how Stuff Works. Hi, brain Stuff, 2 00:00:07,160 --> 00:00:09,760 Speaker 1: Lauren Vogel bomb here. It's something we kind of take 3 00:00:09,800 --> 00:00:12,799 Speaker 1: for granted. Roses are red and planets are spherical. That's 4 00:00:12,840 --> 00:00:15,480 Speaker 1: just the way things are, right after all. Building model 5 00:00:15,520 --> 00:00:17,840 Speaker 1: solar systems would be way more challenging if instead of 6 00:00:17,920 --> 00:00:19,640 Speaker 1: using little phone balls we had to make a bunch 7 00:00:19,640 --> 00:00:22,840 Speaker 1: of dough decahedron shaped planet models. But have you ever 8 00:00:22,880 --> 00:00:25,959 Speaker 1: wondered why planets look like this? Why are they basically 9 00:00:26,000 --> 00:00:29,840 Speaker 1: spherical and not say cylindrical or cube shaped. We should 10 00:00:29,880 --> 00:00:32,320 Speaker 1: kick off this discussion by calling a spade a spade. 11 00:00:32,760 --> 00:00:36,199 Speaker 1: None of the planets in our solar system are perfect spheres, nor, 12 00:00:36,360 --> 00:00:38,959 Speaker 1: for that matter, is our Sun. All those bodies could 13 00:00:39,000 --> 00:00:42,720 Speaker 1: be more accurately described as oblate spheroids objects with the 14 00:00:42,760 --> 00:00:46,040 Speaker 1: shape bulge slightly around the middle. To borrow an analogy 15 00:00:46,080 --> 00:00:48,760 Speaker 1: from the astronomer philled plate, they look like a basketball 16 00:00:48,800 --> 00:00:51,320 Speaker 1: that someone is sitting on. But more technically, in a 17 00:00:51,360 --> 00:00:54,880 Speaker 1: celestial body with an oblate spheroid shape, the polar circumference 18 00:00:54,880 --> 00:00:58,320 Speaker 1: will be smaller than the equatorial one. So here on Earth, 19 00:00:58,360 --> 00:01:00,040 Speaker 1: if you were to travel from the north pole to 20 00:01:00,080 --> 00:01:02,440 Speaker 1: the South pole and back, you'd have walked a grand 21 00:01:02,520 --> 00:01:05,680 Speaker 1: total of twenty four thousand, eight hundred and twelve miles 22 00:01:05,680 --> 00:01:09,319 Speaker 1: that's thirty nine thousand, nine hundred and thirty one kilometers. 23 00:01:09,360 --> 00:01:11,720 Speaker 1: On the other hand, a complete trip around the equator 24 00:01:11,920 --> 00:01:14,679 Speaker 1: would be a bit longer. That's because the circumference of 25 00:01:14,720 --> 00:01:18,080 Speaker 1: Earth's equator is twenty four thousand, nine hundred miles or 26 00:01:18,200 --> 00:01:21,959 Speaker 1: forty thousand and seventy kilometers. As such, when you stand 27 00:01:21,959 --> 00:01:24,720 Speaker 1: at sea level on the equator, you're further away from 28 00:01:24,760 --> 00:01:26,760 Speaker 1: the center of our planet than you would be at 29 00:01:26,760 --> 00:01:29,720 Speaker 1: either the north or south pole on some other planets. 30 00:01:29,720 --> 00:01:32,360 Speaker 1: This bulge is even more pronounced. Just look at Jupiter. 31 00:01:32,680 --> 00:01:35,440 Speaker 1: Earth is only zero point three percent wider at the 32 00:01:35,480 --> 00:01:38,360 Speaker 1: equator than it is from poll to poll, but Jupiter's 33 00:01:38,360 --> 00:01:41,920 Speaker 1: measurements showcase a much bigger disparity. Astronomers have found that 34 00:01:41,920 --> 00:01:44,800 Speaker 1: this plus sized planet is a full seven percent wider 35 00:01:44,840 --> 00:01:47,680 Speaker 1: at its equator than it is between the polls. The 36 00:01:47,760 --> 00:01:50,760 Speaker 1: oblate spheroid shape is the result of two main factors, 37 00:01:50,880 --> 00:01:56,080 Speaker 1: gravity and rotation. Troy Carpenter, director of Washington State's Goldendale Observatory, 38 00:01:56,280 --> 00:01:59,000 Speaker 1: recently discussed the matter with us in an email exchange 39 00:01:59,280 --> 00:02:03,640 Speaker 1: they explain, everything which has mass experiences gravity, and gravity 40 00:02:03,640 --> 00:02:07,360 Speaker 1: attempts to crush an object inward in all directions. That's 41 00:02:07,400 --> 00:02:11,000 Speaker 1: because all objects experience self gravity, a force which pulls 42 00:02:11,040 --> 00:02:14,160 Speaker 1: their atoms toward a common center. As the massive an 43 00:02:14,160 --> 00:02:18,440 Speaker 1: object increases, so too does its self gravitational pull. After 44 00:02:18,480 --> 00:02:21,160 Speaker 1: it exceeds a certain mass, the pull gets overpowering to 45 00:02:21,200 --> 00:02:24,960 Speaker 1: the point where the object collapses into itself and becomes spherical. 46 00:02:25,480 --> 00:02:28,120 Speaker 1: Little items, like say a banana or a lug wrench, 47 00:02:28,320 --> 00:02:31,440 Speaker 1: can resist this fate because their self gravity is relatively weak, 48 00:02:31,680 --> 00:02:36,560 Speaker 1: allowing them to retain non spheroid shapes. However, in planets, suns, 49 00:02:36,639 --> 00:02:39,560 Speaker 1: and other truly massive bodies, the force is so strong 50 00:02:39,600 --> 00:02:43,959 Speaker 1: that they can't avoid being distorted into spheroids. But Carpenter 51 00:02:44,000 --> 00:02:47,480 Speaker 1: said gravity is not the whole story. While gravity conspires 52 00:02:47,520 --> 00:02:50,560 Speaker 1: to render the planet's spherical, the speed of their rotation 53 00:02:50,680 --> 00:02:55,160 Speaker 1: is simultaneously trying to flatten them. The faster celestial body spins, 54 00:02:55,320 --> 00:02:59,600 Speaker 1: the more disproportionate its equatorial bulge gets. Carpenter tells us 55 00:03:00,000 --> 00:03:02,120 Speaker 1: this is why there are no perfect spheres in our 56 00:03:02,120 --> 00:03:05,560 Speaker 1: Solar system, only oblate spheroids. The Sun is almost a 57 00:03:05,560 --> 00:03:08,480 Speaker 1: perfect sphere. Due to its immense gravity and relatively slow 58 00:03:08,560 --> 00:03:11,520 Speaker 1: rotation rate of twenty five days, A significant percentage of 59 00:03:11,520 --> 00:03:14,720 Speaker 1: stars in the sky rotate much faster and bulge noticeably 60 00:03:14,760 --> 00:03:18,560 Speaker 1: at their equators. One such star is all Tear, located 61 00:03:18,639 --> 00:03:21,320 Speaker 1: just sixteen point eight light years away from our home planet. 62 00:03:21,520 --> 00:03:24,120 Speaker 1: It's among the brightest objects in the night sky. All 63 00:03:24,200 --> 00:03:27,280 Speaker 1: Tear is also notable for spinning very very fast. It 64 00:03:27,320 --> 00:03:30,120 Speaker 1: completes a full rotation on its axis every ten point 65 00:03:30,160 --> 00:03:34,240 Speaker 1: four Earth hours. Accordingly, astronomers estimate that all Tears at 66 00:03:34,360 --> 00:03:37,280 Speaker 1: least fourteen percent wider at the equator than it is 67 00:03:37,320 --> 00:03:41,160 Speaker 1: from pole to pole. Rotational speed also explains Jupiter's bulge. 68 00:03:41,440 --> 00:03:43,400 Speaker 1: After all, a day on this gas giant is a 69 00:03:43,440 --> 00:03:46,800 Speaker 1: brisk nine point nine Earth hours long. Other forces act 70 00:03:46,880 --> 00:03:49,480 Speaker 1: upon the stars and planets as well, altering their shapes. 71 00:03:49,800 --> 00:03:52,520 Speaker 1: Although Earth is an oblate spheroid, it certainly isn't a 72 00:03:52,520 --> 00:03:55,320 Speaker 1: perfect one. The gravitational pull of the Sun and Moon 73 00:03:55,480 --> 00:03:58,560 Speaker 1: both influence the planet's shape to a degree. For that matter, 74 00:03:58,640 --> 00:04:01,720 Speaker 1: so do Earth's own plate to topics. Consequently, the mass 75 00:04:01,760 --> 00:04:04,800 Speaker 1: of our homeworld isn't evenly distributed. In fact, it's sort 76 00:04:04,840 --> 00:04:07,760 Speaker 1: of lumpy. Still, it looks a good deal rounder than 77 00:04:07,840 --> 00:04:10,880 Speaker 1: Jupiter and Saturn. In turn, the planets in our universe 78 00:04:10,920 --> 00:04:14,000 Speaker 1: appear way more spherical than some of their moons do. Mars, 79 00:04:14,040 --> 00:04:16,720 Speaker 1: for instance, has two small satellites, neither of which has 80 00:04:16,720 --> 00:04:19,800 Speaker 1: a self gravity to be pulled into an oblate spheroid. Instead, 81 00:04:19,880 --> 00:04:23,680 Speaker 1: their appearance is often described as potato shaped. In conclusion, 82 00:04:23,760 --> 00:04:26,360 Speaker 1: will say this much for our home planet. It may 83 00:04:26,360 --> 00:04:28,720 Speaker 1: not be flawless, but at least the place is fairly 84 00:04:28,720 --> 00:04:36,760 Speaker 1: well rounded. Today's episode was written by Mark Mancini and 85 00:04:36,800 --> 00:04:39,440 Speaker 1: produced by Tristan McNeil. For more on this and lots 86 00:04:39,480 --> 00:04:42,760 Speaker 1: of other interplanetary topics, visit our home planet how stuff 87 00:04:42,760 --> 00:04:54,880 Speaker 1: works dot com