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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:01,100 --> 00:00:05,700 Somewhere, far away in the boundless reaches of the universe, there is a 2 00:00:05,700 --> 00:00:10,760 of space so large and empty that defies imagination, a cosmic void. 3 00:00:11,260 --> 00:00:16,660 This vast expanse stretches across a billion light years with scarcely a 4 00:00:16,660 --> 00:00:17,660 of matter. 5 00:00:18,140 --> 00:00:22,420 Mounting evidence suggests that we are likely floating within a cosmic void of 6 00:00:22,420 --> 00:00:23,420 about the same size. 7 00:00:23,600 --> 00:00:27,520 This region is incredibly vast, enormous beyond words. 8 00:00:28,080 --> 00:00:32,060 Although, in truth, language falls short of capturing the magnitude of this 9 00:00:32,060 --> 00:00:36,340 nothingness. It is within these voids that the true nature of the universe's 10 00:00:36,340 --> 00:00:38,660 structure and evolution can be discerned. 11 00:00:39,060 --> 00:00:44,540 Moreover, Earth, our home planet, is quite insignificant in the grand scheme 12 00:00:44,540 --> 00:00:49,620 things. Once believed to occupy the hallowed center of the universe, our 13 00:00:49,620 --> 00:00:52,540 is now known to be just one among billions upon billions. 14 00:00:53,520 --> 00:00:57,620 In the depths of the night, as we gaze at the stars, we see galaxies, 15 00:00:57,920 --> 00:01:00,360 constellations, and celestial beauty. 16 00:01:01,160 --> 00:01:05,300 However, we seldom consider the immense voids that lie between them. 17 00:01:06,780 --> 00:01:11,900 Cosmic voids, vast regions of seemingly empty space, are some of the most 18 00:01:11,900 --> 00:01:14,640 enigmatic and fascinating structures in the universe. 19 00:01:15,080 --> 00:01:19,440 Though they may appear barren, these voids hold crucial information about the 20 00:01:19,440 --> 00:01:21,780 large -scale structure and evolution of the cosmos. 21 00:01:22,640 --> 00:01:27,060 By sheer volume, most of our universe is simply nothing. 22 00:01:27,600 --> 00:01:32,020 And when it comes to understanding the universe, this nothing holds immense 23 00:01:32,020 --> 00:01:37,060 power. This emptiness possesses a secret influence that subtly shapes the 24 00:01:37,060 --> 00:01:40,420 distribution of galaxies and the movement of cosmic matter. 25 00:01:40,960 --> 00:01:44,240 Therefore, one should not ask, is there any void? 26 00:01:44,620 --> 00:01:47,920 But rather, is there anything apart from the void? 27 00:01:55,150 --> 00:01:59,590 Our home galaxy, the Milky Way, is just one of billions in our universe. 28 00:01:59,850 --> 00:02:04,710 It resides within a complex environment shaped by various cosmic structures, 29 00:02:04,930 --> 00:02:06,590 including nearby voids. 30 00:02:07,150 --> 00:02:11,130 Understanding our place in the universe requires an appreciation of the 31 00:02:11,130 --> 00:02:13,130 intricate interplay between these structures. 32 00:02:14,290 --> 00:02:19,930 Evidence suggests that our galaxy is inside a cosmic void, a vast expanse of 33 00:02:19,930 --> 00:02:21,210 relatively empty space. 34 00:02:21,980 --> 00:02:27,240 The surprising aspect is that, according to the laws of cosmology, such a giant 35 00:02:27,240 --> 00:02:29,480 void shouldn't exist in the first place. 36 00:02:29,820 --> 00:02:35,420 The cosmological principle, a fundamental theory of cosmology, posits 37 00:02:35,420 --> 00:02:39,500 matter in the universe should be uniformly distributed on very large 38 00:02:40,080 --> 00:02:44,920 This principle underpins many of our cosmological models and the 39 00:02:44,920 --> 00:02:46,160 of the universe's structure. 40 00:02:46,960 --> 00:02:52,190 However, multiple observations over the past decade suggests that matter in the 41 00:02:52,190 --> 00:02:56,850 universe may clump into regions of high and low densities, meaning it may not be 42 00:02:56,850 --> 00:02:58,450 as uniform as previously thought. 43 00:02:59,010 --> 00:03:04,070 To understand voids, we need to zoom out far beyond the solar system, the Milky 44 00:03:04,070 --> 00:03:07,810 Way, and even beyond the groups and clusters of galaxies nearby. 45 00:03:08,350 --> 00:03:13,050 We need to zoom out so far that entire galaxies, each with hundreds of millions 46 00:03:13,050 --> 00:03:15,790 of stars, look like tiny dots of light. 47 00:03:16,250 --> 00:03:19,510 At this vast scale, an amazing structure emerges. 48 00:03:20,310 --> 00:03:22,130 Galaxies are not scattered randomly. 49 00:03:22,430 --> 00:03:25,210 Instead, they form the largest pattern in nature. 50 00:03:25,650 --> 00:03:29,890 We see dense clusters with thousands of galaxies and long, thin strands 51 00:03:29,890 --> 00:03:33,770 connecting these clusters, like highways with galaxies along them. 52 00:03:34,270 --> 00:03:39,150 These strands come together to form broad, immense walls, the regions that 53 00:03:39,150 --> 00:03:41,910 contain the typical cosmic mean density of matter. 54 00:03:42,470 --> 00:03:45,410 We call this vast structure the cosmic web. 55 00:03:45,730 --> 00:03:49,230 It's made of galaxies, much like your body is made of cells. 56 00:03:49,790 --> 00:03:51,730 but scaled to an unimaginable level. 57 00:03:52,410 --> 00:03:57,770 Voids now occupy over 80 % of the universe's volume, but hold less than a 58 00:03:57,770 --> 00:03:58,709 of its mass. 59 00:03:58,710 --> 00:04:03,030 The bright stars and galaxies of the cosmic web highlight the edges of these 60 00:04:03,030 --> 00:04:09,010 vast, empty regions. These cosmic voids dominate the universe, meaning most of 61 00:04:09,010 --> 00:04:10,010 it is nearly empty. 62 00:04:10,390 --> 00:04:15,610 Within these voids, you might find a few small, dim dwarf galaxies and a thin 63 00:04:15,610 --> 00:04:17,290 mix of radiation and particles. 64 00:04:18,060 --> 00:04:22,400 Yet they remain largely empty, devoid of significant structures or matter. 65 00:04:22,840 --> 00:04:27,500 The seeds of voids were planted in the earliest moments of the universe, even 66 00:04:27,500 --> 00:04:29,320 before the first stars and galaxies. 67 00:04:30,440 --> 00:04:34,260 Billions of years ago, the matter in the universe was almost perfectly uniform, 68 00:04:34,560 --> 00:04:36,600 with only tiny, random differences. 69 00:04:37,320 --> 00:04:40,700 Just a millionth more matter here, or a millionth less there. 70 00:04:41,260 --> 00:04:45,780 However, within this uniformity, there existed minute, random fluctuations. 71 00:04:46,890 --> 00:04:50,870 Tiny variations where there was a slightly higher concentration of matter 72 00:04:50,870 --> 00:04:52,810 place and slightly less in another. 73 00:04:53,570 --> 00:04:57,890 These minuscule differences played a pivotal role in the formation of 74 00:04:57,890 --> 00:04:58,950 we observe today. 75 00:04:59,530 --> 00:05:02,550 As the universe aged, these differences grew. 76 00:05:03,230 --> 00:05:06,590 Gravity, though weak, is persistent and patient. 77 00:05:07,650 --> 00:05:11,630 Regions with a bit more matter had a slightly stronger gravitational pull, 78 00:05:11,810 --> 00:05:14,490 attracting more matter and emptying their surroundings. 79 00:05:15,370 --> 00:05:19,670 As more matter gathered, the gravitational pull grew stronger, and 80 00:05:19,670 --> 00:05:21,250 surroundings emptied even more. 81 00:05:22,170 --> 00:05:27,710 Over hundreds of millions of years, the cosmic web began to form, first as small 82 00:05:27,710 --> 00:05:32,190 clumps that ignited the birth of earliest stars, then as small galaxies 83 00:05:32,190 --> 00:05:36,470 merged together, eventually forming the great clusters of galaxies, the 84 00:05:36,470 --> 00:05:38,070 filaments, and the walls. 85 00:05:38,780 --> 00:05:43,600 The cosmic web represents the grandest pattern discovered in nature, extending 86 00:05:43,600 --> 00:05:45,500 throughout the entirety of the universe. 87 00:05:45,900 --> 00:05:51,680 It forms an immense and expansive structure, almost overpowering in scale, 88 00:05:51,680 --> 00:05:55,420 its appearance is delicate and fragile, like fine strands of silk. 89 00:05:55,900 --> 00:06:01,740 As the cosmic web flourished, so too did the voids. They began as small, subtle 90 00:06:01,740 --> 00:06:04,460 dips in the otherwise uniform fabric of the universe. 91 00:06:05,280 --> 00:06:09,940 Over time, these voids expanded as their contents gravitated towards larger, 92 00:06:10,020 --> 00:06:11,020 luminous structures. 93 00:06:11,860 --> 00:06:16,780 Cosmic voids are akin to holes in the universe, resembling gaps in Swiss 94 00:06:16,780 --> 00:06:18,820 or the openings in a spider's web. 95 00:06:19,320 --> 00:06:23,760 It stretches hundreds of millions of light -years across. These voids are the 96 00:06:23,760 --> 00:06:28,480 true deserts of the cosmos, almost entirely devoid of matter. This 97 00:06:28,480 --> 00:06:30,100 holds a mysterious influence. 98 00:06:31,050 --> 00:06:35,570 In the late 1990s, when astronomers discovered that the universe's expansion 99 00:06:35,570 --> 00:06:39,790 accelerating, that instead of slowing down under gravitational pull, as 100 00:06:39,790 --> 00:06:41,730 expected, it's speeding up. 101 00:06:42,330 --> 00:06:47,350 This phenomenon, confirmed by multiple experiments, is attributed to dark 102 00:06:47,350 --> 00:06:50,330 energy. Dark energy remains an enigma. 103 00:06:50,770 --> 00:06:55,390 Scientists speculate it's a fundamental property of space -time itself, driving 104 00:06:55,390 --> 00:06:56,410 universal expansion. 105 00:06:57,380 --> 00:07:01,580 Locally, however, its effects are masked by the gravitational pull of stars, 106 00:07:01,940 --> 00:07:04,820 gas, dust, and other matter in our vicinity. 107 00:07:05,320 --> 00:07:09,260 But in the voids, there's nothing to counteract dark energy's influence. 108 00:07:09,660 --> 00:07:14,160 They expand relentlessly, pushing against the surrounding filaments and 109 00:07:14,380 --> 00:07:15,840 perpetuating their growth. 110 00:07:23,080 --> 00:07:27,860 On a grand scale, the universe resembles a sponge, with voids dominating its 111 00:07:27,860 --> 00:07:32,600 vast expanse. Some voids span hundreds of millions of light -years in diameter. 112 00:07:33,020 --> 00:07:38,360 To study these voids, astronomers rely on optical and radio telescopes to 113 00:07:38,360 --> 00:07:40,280 for any signs of matter within them. 114 00:07:41,100 --> 00:07:45,940 Superclusters of galaxies and voids are frequently studied in tandem, as they 115 00:07:45,940 --> 00:07:49,060 are thought to share a common evolutionary history and dynamics. 116 00:07:50,000 --> 00:07:56,200 Our own Milky Way galaxy lies in a void called the KBC Void, or Local Hole. 117 00:07:56,540 --> 00:08:00,460 Other notable cosmic voids that have been discovered and studied in detail, 118 00:08:00,680 --> 00:08:05,000 providing valuable insights into the nature of the universe, include the 119 00:08:05,000 --> 00:08:08,600 Southern Local Super Void and the Eridanus Super Void. 120 00:08:09,240 --> 00:08:14,960 However, none is as big as the BOTUS Super Void, sometimes called the Great 121 00:08:14,960 --> 00:08:20,010 Nothing. or the Great Void, the Boötes Void is a spherical region located 122 00:08:20,010 --> 00:08:24,470 approximately 700 million light years away from Earth in the constellation 123 00:08:24,470 --> 00:08:28,810 Boötes. Boötes is depicted as the herdsman in Greek mythology. 124 00:08:29,370 --> 00:08:35,130 The Boötes Void stretches across an immense area spanning 330 million light 125 00:08:35,130 --> 00:08:38,789 years, distinguishing it as the largest known void in the universe. 126 00:08:39,210 --> 00:08:45,930 Despite its vast size, it harbors very few galaxies, approximately 60, 127 00:08:45,930 --> 00:08:48,030 within a tube -shaped region at its center. 128 00:08:48,590 --> 00:08:52,830 Typically, a region of this size would host around 2 ,000 galaxies. 129 00:08:54,010 --> 00:08:57,770 Surrounding the boda's void are several superclusters including Ursa Major, 130 00:08:58,150 --> 00:09:01,150 Shapley, Hercules, and Corona Borealis. 131 00:09:01,950 --> 00:09:03,470 Why is it so empty? 132 00:09:04,110 --> 00:09:08,550 Apart from dark energy, which we discussed earlier, the regions where 133 00:09:08,550 --> 00:09:13,180 cluster together, such as in galaxy clusters or groups, are significantly 134 00:09:13,180 --> 00:09:17,740 influenced by the life cycles of stars and the presence of supermassive black 135 00:09:17,740 --> 00:09:19,400 holes at the centers of galaxies. 136 00:09:20,100 --> 00:09:26,760 These supermassive black holes, also known as active galactic nuclei, AGN, 137 00:09:26,760 --> 00:09:28,860 a crucial role in shaping their surroundings. 138 00:09:30,000 --> 00:09:34,400 Supernovae are explosive events that occur when massive stars reach the end 139 00:09:34,400 --> 00:09:35,239 their lives. 140 00:09:35,240 --> 00:09:39,900 These explosions release enormous amounts of energy, including shockwaves 141 00:09:39,900 --> 00:09:40,900 high -energy particles. 142 00:09:41,530 --> 00:09:43,250 into the surrounding interstellar medium. 143 00:09:43,930 --> 00:09:48,590 The energy and momentum from supernovae can heat up the surrounding gas and 144 00:09:48,590 --> 00:09:52,810 drive it outward, preventing it from collapsing under its own gravity to form 145 00:09:52,810 --> 00:09:54,050 new stars or galaxies. 146 00:09:54,510 --> 00:10:00,090 This process, known as supernova feedback, regulates the rate of star 147 00:10:00,090 --> 00:10:04,830 within galaxies and can extend its influence into the surrounding 148 00:10:04,830 --> 00:10:05,830 medium. 149 00:10:06,550 --> 00:10:11,910 AGNs. powered by supermassive black holes at the centers of galaxies, also 150 00:10:11,910 --> 00:10:15,150 a crucial role in regulating the growth and evolution of galaxies. 151 00:10:15,830 --> 00:10:19,610 These black holes can accrete large amounts of gas and dust from their 152 00:10:19,610 --> 00:10:23,530 surroundings, releasing tremendous amounts of energy in the form of 153 00:10:23,530 --> 00:10:25,690 and powerful jets of particles. 154 00:10:26,150 --> 00:10:31,130 This AGN activity can heat up and ionize the gas in their vicinity, affecting 155 00:10:31,130 --> 00:10:32,610 the formation of new stars. 156 00:10:33,200 --> 00:10:36,900 and influencing the dynamics of the interstellar and intergalactic medium. 157 00:10:37,360 --> 00:10:42,380 In the context of cosmic voids as a whole, where galaxies are sparse or 158 00:10:42,600 --> 00:10:47,120 the lack of such energetic feedback mechanisms can have profound 159 00:10:47,720 --> 00:10:52,640 Without the heating and disruption caused by supernova and AGNs, the gas in 160 00:10:52,640 --> 00:10:55,560 voids may remain relatively cool and undisturbed. 161 00:10:56,030 --> 00:11:00,190 As a result, there may be insufficient energy to prevent the gas from simply 162 00:11:00,190 --> 00:11:04,390 diffusing away or remaining in a state that does not promote the formation of 163 00:11:04,390 --> 00:11:05,390 new galaxies. 164 00:11:06,030 --> 00:11:11,410 Therefore, the absence of significant supernova and AGN feedback in cosmic 165 00:11:11,410 --> 00:11:16,350 can contribute to their observed emptiness and lack of dense galaxy 166 00:11:16,350 --> 00:11:17,350 structures. 167 00:11:18,270 --> 00:11:23,230 Within the vast expanse of a void like Botus, gravitational forces play a 168 00:11:23,230 --> 00:11:25,250 crucial role in the distribution of matter. 169 00:11:25,880 --> 00:11:30,080 In regions where the density of matter is lower, gravitational attraction is 170 00:11:30,080 --> 00:11:34,340 weaker. This can result in slower or less efficient formation of galaxies, 171 00:11:34,700 --> 00:11:38,440 clusters, and other cosmic structures compared to denser regions. 172 00:11:39,140 --> 00:11:44,900 As a result, voids may remain relatively empty over cosmic timescales because 173 00:11:44,900 --> 00:11:49,180 the gravitational pull needed to pull matter together into dense structures is 174 00:11:49,180 --> 00:11:53,660 insufficient. Moreover, the ongoing expansion of the universe further 175 00:11:53,660 --> 00:11:54,720 complicates matters. 176 00:11:55,440 --> 00:12:00,100 cosmic expansion stretches space itself, causing regions with lower initial 177 00:12:00,100 --> 00:12:04,580 densities, like voids, to expand more quickly than regions with higher 178 00:12:04,580 --> 00:12:06,480 densities, like galaxy clusters. 179 00:12:06,820 --> 00:12:11,420 This expansion can further hinder the gravitational collapse and clustering of 180 00:12:11,420 --> 00:12:15,820 matter within voids, perpetuating their emptiness over billions of years. 181 00:12:16,590 --> 00:12:21,550 Therefore, a combination of weaker gravitational forces and the expansive 182 00:12:21,550 --> 00:12:26,510 of the universe itself likely contributes to why cosmic voids such as 183 00:12:26,510 --> 00:12:30,630 Void remain so sparsely populated with galaxies and matter. 184 00:12:31,950 --> 00:12:36,850 The concept of the Boötes Void as an exceptionally large and empty region in 185 00:12:36,850 --> 00:12:38,350 space invites speculation. 186 00:12:39,400 --> 00:12:44,480 Does this perplexing structure align with Nikolai Kardashev's 1962 theory on 187 00:12:44,480 --> 00:12:47,020 advanced alien civilizations and their activities? 188 00:12:47,640 --> 00:12:52,540 Could it have potentially hosted a hyper -intelligent extraterrestrial species? 189 00:12:53,660 --> 00:12:58,680 In the context of the Buddha's void, we can draw parallels to urban development 190 00:12:58,680 --> 00:12:59,840 dynamics on Earth. 191 00:13:00,560 --> 00:13:05,420 Imagine the void as a neighborhood that, in the distant past, may have witnessed 192 00:13:05,420 --> 00:13:08,380 bustling activity and utilization of its resources. 193 00:13:09,550 --> 00:13:13,810 Just as civilizations on Earth have developed and consumed resources over 194 00:13:14,030 --> 00:13:18,170 so too might advanced civilizations have once flourished within the void. 195 00:13:18,630 --> 00:13:22,970 They could have tapped into its energy reservoirs and utilized its resources, 196 00:13:23,350 --> 00:13:27,350 analogous to how humans have utilized Earth's resources for millennia. 197 00:13:27,710 --> 00:13:32,330 As time passed and resources within the void were exhausted or rendered 198 00:13:32,330 --> 00:13:37,410 obsolete, any advanced civilizations that once thrived there may have moved 199 00:13:37,410 --> 00:13:38,410 or diminished. 200 00:13:38,520 --> 00:13:42,780 leaving behind a vast expanse that appears desolate and empty to us today. 201 00:13:43,660 --> 00:13:48,380 This perspective allows us to speculate on the potential history and life cycle 202 00:13:48,380 --> 00:13:53,260 of civilizations within cosmic voids, considering both their rise and eventual 203 00:13:53,260 --> 00:13:54,460 decline or departure. 204 00:13:55,060 --> 00:13:59,760 The existence of the Buddhist void challenges fundamental theories about 205 00:13:59,760 --> 00:14:03,560 large -scale structure and distribution of matter in the universe. 206 00:14:04,590 --> 00:14:09,570 It somehow contradicts the cosmological principle, which posits a smooth and 207 00:14:09,570 --> 00:14:13,890 homogeneous distribution of matter on the largest scales when viewed over 208 00:14:13,890 --> 00:14:14,890 sufficient distances. 209 00:14:15,350 --> 00:14:21,170 This enormous void spans hundreds of millions of light years, far exceeding 210 00:14:21,170 --> 00:14:22,970 current models can easily explain. 211 00:14:23,390 --> 00:14:28,370 Its existence suggests structural complexities that current theories 212 00:14:28,370 --> 00:14:29,370 accommodate. 213 00:14:29,770 --> 00:14:35,030 Some hypotheses propose that such remarkably empty regions may highlight 214 00:14:35,030 --> 00:14:39,090 our understanding of dark matter and its gravitational influence on cosmic 215 00:14:39,090 --> 00:14:43,410 scales. While not impossible to form from early universe density 216 00:14:43,870 --> 00:14:48,470 the extreme emptiness of the void makes it a statistically improbable anomaly 217 00:14:48,470 --> 00:14:50,230 that prompts numerous questions. 218 00:14:54,590 --> 00:14:58,530 Cosmic voids represent the most enduring time capsules in the cosmos. 219 00:14:59,260 --> 00:15:01,740 remaining largely unchanged over billions of years. 220 00:15:02,280 --> 00:15:06,780 Defined by their sparse matter content, these voids provide a pristine and 221 00:15:06,780 --> 00:15:09,420 unparalleled environment for studying dark energy. 222 00:15:09,740 --> 00:15:14,360 Within these vast expanses lie answers to numerous cosmological mysteries. 223 00:15:14,940 --> 00:15:19,780 As cosmological laboratories, they offer insights into the fundamental nature of 224 00:15:19,780 --> 00:15:24,760 dark matter and dark energy, reveal details about the ancient universe, and 225 00:15:24,760 --> 00:15:27,520 provide crucial information on the formation of galaxies. 226 00:15:28,400 --> 00:15:33,200 Thus, our greatest insights into the universe's mysteries may only be 227 00:15:33,200 --> 00:15:37,880 through careful exploration and study of these expansive regions of emptiness. 228 00:15:38,460 --> 00:15:44,040 In the distant future, the cosmic web, adorned with galaxies, filaments and 229 00:15:44,040 --> 00:15:45,960 walls, will gradually unravel. 230 00:15:46,740 --> 00:15:51,240 Filaments will thin out as voids expand, squeezing them into oblivion. 231 00:15:51,900 --> 00:15:53,160 Walls will fade away. 232 00:15:53,850 --> 00:15:57,830 Clusters will endure, but become isolated islands in a vast emptiness. 233 00:15:58,310 --> 00:16:02,410 But before this distant future arrives, there's urgent work to be done. 234 00:16:02,870 --> 00:16:07,370 Dark energy permeates all of space -time, but its effects are most 235 00:16:07,370 --> 00:16:08,370 within voids. 236 00:16:08,850 --> 00:16:12,810 Understanding this mysterious force, which dictates the universe's fate, 237 00:16:13,010 --> 00:16:15,990 requires focusing beyond galaxies and clusters. 238 00:16:16,450 --> 00:16:20,670 Their powerful gravitational pull masks dark energy's subtle influence. 239 00:16:21,390 --> 00:16:24,930 Instead, attention turns to the silent expanses of voids. 240 00:16:25,290 --> 00:16:28,610 Voids hold keys to unlocking dark energy secrets. 241 00:16:29,010 --> 00:16:34,250 Their growth, shapes, and distribution reveal insights into dark energy's 242 00:16:34,250 --> 00:16:35,250 strength and evolution. 243 00:16:35,730 --> 00:16:40,910 By meticulously mapping cosmic voids, scientists hope to unravel the elusive 244 00:16:40,910 --> 00:16:44,970 properties of dark energy and compare findings with theoretical models. 245 00:16:45,550 --> 00:16:49,230 Moreover, cosmic voids act as timeless archives. 246 00:16:50,090 --> 00:16:55,990 While galaxies evolve, stars are born, die, and matter shifts, voids remain 247 00:16:55,990 --> 00:17:00,930 serene, empty spaces, largely unchanged over billions of years. 248 00:17:01,490 --> 00:17:06,250 Although the void appears completely dark to our eyes, solving its mysteries 249 00:17:06,250 --> 00:17:10,329 could paradoxically shine a light on outstanding problems in our theories of 250 00:17:10,329 --> 00:17:15,310 universe's evolution, structure, and perhaps even the nature of the elusive 251 00:17:15,310 --> 00:17:16,310 matter itself. 252 00:17:16,839 --> 00:17:21,099 The vast nothingness may contain hidden insights into cosmic something we are 253 00:17:21,099 --> 00:17:22,099 yet to understand. 254 00:17:22,720 --> 00:17:24,160 And that's it for this video. 255 00:17:24,500 --> 00:17:26,980 Thanks for watching, and I'll see you in the next one. 24147

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