4/15/2024 0 Comments Ocean water density![]() Travel deeper and you will find the abyssopelagic zone-the abyss. Animals create their own bioluminescent light and, if they haven’t lost them, have highly light-sensitive eyes to see the light produced by other animals. You can’t dive to the deep ocean on your own, of course, but scientists have a variety of sophisticated technologies to explore this vast frontier.īeginning with the bathypelagic zone, the ocean is completely void of light from the sun, moon and stars. Despite these harsh conditions, there is life-an astounding variety of creatures that will boggle your mind. ![]() The further we dive down from the surface, the less new food is available, making the fight to survive that much more challenging. At this depth, we’ve reached the average depth of the deep-sea floor, a place that may start to get a little muddy. By 13,000 feet (4,000 meters), the temperature hovers just below the temperature of your refridgerator. Any light still filtering down has diminished to appear completely black, leaving only animals and bacteria to produce the light found here. Dive deeper and the weight of the water above continues to accumulate to a massive crushing force. By 650 feet (200 m) all the light is gone to our eyes and the temperature has dropped dramatically. As you dive down through this vast living space you notice that light starts fading rapidly. But the deep sea remains largely unexplored. The lack of a pycnocline (or a thermocline) allows cold, nutrient-rich deep water to more easily mix with the surface water, leading to higher primary production in polar regions.Below the ocean’s surface is a mysterious world that accounts for over 95 percent of Earth’s living space-it could hide 20 Washington Monuments stacked on top of each other. In the high latitudes the water is uniformly cold at all depths, so there is little density stratification. As stated above, this stratification prevents nutrient-rich water from reaching the surface and as a result tropical regions often have low productivity. In the tropics the surface water is warm and low density, and there is a pronounced thermocline separating it from the colder, denser deep water. In this way, nutrient-rich deep water may be prevented from coming to the surface to support primary production.Īs with temperature, there are also latitudinal differences in density. By creating a stratified water column, the thermocline and pycnocline together create a barrier that prevents mixing between the warmer, less dense surface water and the colder, denser bottom water. This vertical movement of water masses based on density (as determined by temperature and salinity) is referred to as thermohaline circulation, which is the topic of section 9.8. ![]() If denser water happened to form at the surface, the water masses would be unstable, and the denser water would sink to the bottom, to be replaced by less dense water at the surface. The profile above represents a stable state, or a high degree of stratification, where the warm, low density layer sits atop the colder, denser layer. The warm surface water causes a decrease in surface density (PW). Figure 6.3.2 Representative density profile for the open ocean at mid-latitudes. Below the pycnocline, density may be fairly constant (as is temperature), or it may continue to increase slightly towards the bottom. The pycnocline coincides with the thermocline, as it is the sudden decrease in temperature that leads to the increase in density. As depth increases, there is a region of rapidly increasing density with increasing depth, which is called the pycnocline. Density is lowest at the surface, where the water is the warmest. Since temperature has the greatest effect on density, density profiles are usually mirror images of temperature profiles (Figure 6.3.2). Colder polar regions display higher densities than warmer tropical zones (By Plumbago (Own work), via Wikimedia Commons). However, if not for the slight compression of water due to pressure, sea level would be approximately 50 m higher than it is today! That leaves temperature and salinity as the primary factors determining density, and of these, temperature has the greatest impact (Figure 6.3.1).įigure 6.3.1 Global sea surface density. Pressure has the least impact on density as water is fairly incompressible, so pressure effects are not very significant except at extreme depths. The density of seawater can be increased by reducing its temperature, increasing its salinity, or increasing the pressure. The density of fresh water is 1 g/cm 3 at 4 o C (see section 5.1), but the addition of salts and other dissolved substances increases surface seawater density to between 1.02 and 1.03 g/cm 3. Density refers to the amount of mass per unit volume, such as grams per cubic centimeter (g/cm 3).
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