1 00:00:00,000 --> 00:00:03,136 NASA’s James Webb Space Telescope has captured 2 00:00:03,136 --> 00:00:06,306 the sharpest infrared view of the Horsehead Nebula,   3 00:00:06,306 --> 00:00:08,875 located within the constellation Orion, 4 00:00:08,875 --> 00:00:11,945 nearly 1,300 light-years away. 5 00:00:11,945 --> 00:00:15,215 Webb’s Mid-Infrared Instrument and Near-Infrared Camera 6 00:00:15,215 --> 00:00:17,117 were pointed towards the illuminated edge 7 00:00:17,117 --> 00:00:20,620 of this iconic nebula, capturing the  region’s complexity 8 00:00:20,620 --> 00:00:23,356 with unprecedented spatial resolution. 9 00:00:23,356 --> 00:00:24,991 As with many Webb images, 10 00:00:24,991 --> 00:00:28,194 distant galaxies are sprinkled in the background. 11 00:00:28,194 --> 00:00:30,330 The ethereal clouds that appear blue at the bottom 12 00:00:30,330 --> 00:00:34,034 of the image are dominated by cold, molecular hydrogen. 13 00:00:34,034 --> 00:00:36,870 Red-colored wisps extending above the main nebula 14 00:00:36,870 --> 00:00:39,572 represent mainly atomic hydrogen gas. 15 00:00:39,572 --> 00:00:43,376 This nebula formed from a collapsing  interstellar cloud of material,   16 00:00:43,376 --> 00:00:47,247 and it glows because it’s illuminated by a nearby hot star. 17 00:00:47,247 --> 00:00:50,784 The gas clouds surrounding the Horsehead have already dissipated, 18 00:00:50,784 --> 00:00:53,753 and astronomers estimate that the Horsehead itself has about 19 00:00:53,753 --> 00:00:57,023 five million years before it also disintegrates. 20 00:00:57,023 --> 00:00:59,826 As ultraviolet light evaporates the dust cloud, 21 00:00:59,826 --> 00:01:02,562 dust particles are swept out away from the cloud, 22 00:01:02,562 --> 00:01:04,364 carried with the heated gas. 23 00:01:04,364 --> 00:01:08,601 Webb has detected a network of thin features tracing this movement. 24 00:01:08,601 --> 00:01:11,704 Using Webb to observe the small-scale structures 25 00:01:11,704 --> 00:01:13,339 at the nebula’s edge that have 26 00:01:13,339 --> 00:01:15,909 never been observed before allows astronomers 27 00:01:15,909 --> 00:01:19,079 to investigate how the dust blocks and emits light, 28 00:01:19,079 --> 00:01:24,250 and to better understand the  multidimensional shape of the nebula.