Hydrosphere
Hydrosphere (Greek hydro means "water") in physical geography, describes the collective mass of water found on, under, and over the surface of a planet.
The abundance of water on Earth is a unique feature that distinguishes our "Blue Planet" from others in the solar system. Approximately 70.8 per cent of the Earth is covered by water and only 29.2 per cent is terra firma.
The water cycle (or hydrologic cycle) describes the methods of transport for water in the hydrosphere. This cycle includes water beneath the Earth's surface and in rocks (lithosphere), the water in plants and animals (biosphere), the water covering the surface of the planet in liquid and solid forms, and the water in the atmosphere in the form of water vapor, clouds, and precipitation. Movement of water witin the hydrosphere is described by the hydrologic cycle. It is easy to see this motion in rivers and streams, but it is harder to tell that there is this motion in lakes and ponds.
The characteristics of the ocean that affects its motion are its temperature and salinity. Warm water is lighter or less dense than cold water which is more dense or heavier and salty water is also more dense than fresh water. The combination of the water's temperature and salinity determines whether it rises to the surface, sinks to the bottom, or stays at some intermediate depth.
The hydrosphere consists chiefly of the oceans, but technically includes all water surfaces in the world, including inland seas, lakes, rivers, and underground waters. The average depth of the oceans is 3,794 m (12,447 ft), more than five times the average height of the continents. The mass of the oceans is approximately 1.35 × 1018 tonnes, or about 1/4400 of the total mass of the Earth.
History
Formation
There are several theories regarding the formation of the hydrosphere on the Earth. The planet contains proportionately more surface water than comparable bodies in the inner solar system. Outgassing of water from the interior of the Earth is not sufficient to explain the quantity of water.
A hypothesis that has gained popularity among scientists is that the early Earth was subjected to a period of bombardment by Comets and water-rich Asteroids. Much of the water on the surface today is thought to have originated from the outer parts of the solar system, such as from trans-Neptunian objects.
Ice ages
During the history of the Earth there have been a series of periods in which a significant portion of the hydrosphere was locked up in the form of glacial ice. It has even been hypothesized that during the Cryogenian period this sea ice extended all the way to the equator. (See Snowball Earth).
In all there are currently believed to have been four major ice ages during the Earth's history. The current ice age began about 4 × 107 years ago, and gained in intensity during the Pleistocene. The most recent withdrawal of the ice sheets occurred only 10,000 years ago.
Life
All currently recognized forms of life rely on an active hydrosphere. All organic chemistry indicative of life occurs with water as its solvent. The water cycle in the Earth's hydrosphere allows for the purification of salt water into fresh water. The action of both evaporation and wetland swamps serves to remove a large portion of atmospheric pollutants from the atmosphere (ie. acid rain). Through this process the water cycle purifies the gaseous atmosphere. Although most life on the planet exists in the salt water oceans, humans are particularly interested in the hydrosphere because it provides the fresh water we depend upon.
The search for life in other celestial bodies in our solar system is focused on first locating water. The hydrosphere's of other planetary bodies is also the focus of research to find places that humans can inhabit without having to transport all their water with them.
Extinction
Scientists estimate that in approximately 4 × 109 years the Sun will have exhausted the supply of Hydrogen in its core and will evolve into a supergiant. The outer atmosphere will expand significantly and the planet Earth will lie within the photosphere. During this process the surface temperature will rise far above the boiling point of water, and all water on the Earth's surface will evaporate.
Other hydrospheres
A thick hydrosphere is thought to exist around the Jovian moon Europa. The outer layer of this hydrosphere is almost entirely frozen, but current models predict that there is an ocean up to 100 km in depth underneath the ice. This ocean remains in a liquid form due to tidal flexing of the moon in its orbit around Jupiter.
It has been suggested that the moon Ganymede may also possess a sub-surface ocean. However the ice covering is expected to be thicker on Ganymede than on Europa.
See also
- Atmosphere
- Biosphere
- Cryosphere
- Lithosphere
- Pedosphere
- Water Cycle
External links
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