WEBVTT 00:00:01.222 --> 00:00:04.643 Chad Kiel: Hey guys, it's Chad Kiel with Learning Geology and Nature Reconnection, 00:00:04.643 --> 00:00:07.213 and today we're learning about Alluvial Fans. 00:00:07.213 --> 00:00:08.897 What is an alluvial fan? 00:00:08.897 --> 00:00:12.500 And I'm going to tell you about some interesting data about this alluvial fan, 00:00:12.500 --> 00:00:15.135 and the processes that created it, because it happens to be in 00:00:15.135 --> 00:00:16.321 my backyard. 00:00:16.321 --> 00:00:19.499 Let's go check it out. 00:00:19.499 --> 00:00:23.520 So before we dive down the rabbit hole of alluvial fans, let's first take a 00:00:23.520 --> 00:00:28.058 second to talk about weathering and erosion, because those are two factors 00:00:28.058 --> 00:00:30.895 that are gonna come into play again and again when we're talking about this 00:00:30.895 --> 00:00:32.395 alluvial fan. 00:00:32.395 --> 00:00:36.300 Right here around 6,500 feet into the mountains, temperatures can vary from 00:00:36.300 --> 00:00:42.471 20 degrees each day, causing the rocks to kind of expand and contract, and this 00:00:42.471 --> 00:00:45.993 expanding and contracting's gonna cause fracturing. 00:00:45.993 --> 00:00:51.641 Now these fractures are susceptible for water to percolate down into the rock, and 00:00:51.641 --> 00:00:55.745 when the water freezes in the rock, we all know that ice has a larger volume than 00:00:55.745 --> 00:00:58.914 water, it again fractures out that rock, and these fractured blocks are deposited 00:00:58.914 --> 00:01:05.037 here in this active channel, and then we have the erosion factor that comes and 00:01:05.037 --> 00:01:07.073 transports it down mountain. 00:01:07.073 --> 00:01:11.844 So that's the beginning process of this whole alluvial fan story. 00:01:11.844 --> 00:01:15.414 Alluvial fans are triangular-shaped deposits of water transported material 00:01:15.414 --> 00:01:17.422 often referred to as alluvium. 00:01:17.422 --> 00:01:21.227 There are examples of an unconsolidated sedimentary deposit, and tend to be 00:01:21.227 --> 00:01:25.766 larger and more prominent in arid to semi-arid regions, like we are today. 00:01:25.766 --> 00:01:29.569 These alluvial fans typically from in elevated or even mountainous regions 00:01:29.569 --> 00:01:33.689 where there's a rapid change in the slope from a high to a low gradient. 00:01:33.689 --> 00:01:36.876 The river or the stream carrying the sediment flows at a relatively high 00:01:36.876 --> 00:01:41.031 velocity due to the high slope angle, which is why coarse material is able 00:01:41.031 --> 00:01:43.182 to remain in the flow. 00:01:43.182 --> 00:01:48.236 When the slope decreases rapidly into a relatively plane area or plateau, the 00:01:48.236 --> 00:01:51.466 stream loses the energy it needs to move its sediment. 00:01:51.466 --> 00:01:56.373 Deposition subsequently occurs, and the sediment ultimately spreads out, creating 00:01:56.373 --> 00:01:58.875 the alluvial fan. 00:01:58.875 --> 00:02:03.330 As the streams gradient decreases, it drops the coarse grain material. 00:02:03.330 --> 00:02:07.099 It makes swagger of the channel, and forces it to change direction, and 00:02:07.099 --> 00:02:11.688 gradually build up a slightly mounded or shallow conical fan shape. 00:02:11.688 --> 00:02:15.893 The sediment that results from the erosion in this elevated mountainous region right 00:02:15.893 --> 00:02:21.353 here, ultimately flows into the primary streams and the regions, where the streams 00:02:21.353 --> 00:02:25.257 act as a drainage system, and carry the sediment to the alluvial plane, which is 00:02:25.257 --> 00:02:26.540 down below us. 00:02:26.540 --> 00:02:30.646 Once the sediment exits the feeder stream, the sediment is no longer confined to the 00:02:30.646 --> 00:02:31.848 channel walls. 00:02:31.848 --> 00:02:36.636 With this unconfinement, the sediment begins to fan out, the alluvial fan 00:02:36.636 --> 00:02:40.757 becomes wider with increasing distance from the mouth of the canyon. 00:02:40.757 --> 00:02:44.610 The biggest natural hazard on alluvial fans are floods, and debris flows. 00:02:44.610 --> 00:02:47.997 Floods on alluvial fans are commonly flash floods, they occur with little to 00:02:47.997 --> 00:02:53.263 no warning, usually have high velocities in sediment transporting capabilities, and 00:02:53.263 --> 00:02:54.949 are relatively short. 00:02:54.949 --> 00:02:58.736 Modern flood control infrastructure is essential to stop flooding, property 00:02:58.736 --> 00:03:01.771 damage, and the loss of life from happening. 00:03:01.771 --> 00:03:06.609 Successful development can and does occur on alluvial fans, even in rural 00:03:06.609 --> 00:03:11.466 areas like ours, mitigation measures are utilized; building pads are elevated, 00:03:11.466 --> 00:03:15.537 obvious drainage paths are left unobstructed, and in some cases, 00:03:15.537 --> 00:03:17.291 flood walls are built. 00:03:17.291 --> 00:03:21.246 Floodplain management principles of alluvial fans are part of everyone's 00:03:21.246 --> 00:03:24.266 life that chooses to live in this special place. 00:03:24.266 --> 00:03:28.235 I hope this helps you understand more about alluvial fans, and the processes 00:03:28.235 --> 00:03:29.439 that create them. 00:03:29.439 --> 99:59:59.999 Until next time, I'm Chad Kiel.