Earth:

The planet which we know the most about, due to our ability to explore its interior as well as exterior, is the Earth Most of this course will compare values and processes on other planets to those on the Earth, i.e. it is our yardstick for understanding other worlds. Therefore, knowing about our home world is crucial to appreciate the Universe, besides being necessary for our own survival.

In many ways, Earth is unique in the solar system. Its most obvious feature is the vast amounts of liquid water on its surface, as well as the ability to sustain intelligent life.

Earth rotating

The above color image of the Earth was obtained by the Galileo spacecraft when it was about 1.3 million miles from the planet, displays our world as would be seen by a space probe from another solar system. Galileo was making the first of two Earth flybys on its way to Jupiter. South America is near the center of the picture, and the white, sunlit continent of Antarctica is below. Picturesque weather fronts are visible in the South Atlantic, lower right.

The above is an infrared image of the Earth was taken by the GOES 6 satellite on September 21, 1986. A temperature threshold was used to isolate the clouds. The land and sea were separated and then the clouds, land and sea were separately colored and combined back together to produce this image.

Earth/Moon Viewer

Surface Features:

The above image is a map of North and South America using radar altimetry to reflect the underlying topography of the oceans and continents.

The above image is part of the Rocky Mountain Range in the Yukon Territory of Canada is an excellent example of young mountains on Earth. This space shuttle image was taken when the sun was low on the horizon; the sharp shadows on the snow-covered peaks show how rough and uneven the area is.

The above picture is a space shuttle image of the Colorado River in Arizona captures the Grand Canyon. The canyon is 30 km (18 miles) across at its widest point and 1.6 km (1 mile) deep at rock bottom. It is 446 km (277 miles) long and covers an area that is over 5000 square km (about 2000 square miles). The Grand Canyon was created by the erosional action of the Colorado River on the surface as this region has continued to rise high above sea level over the last several million years.

Observations of the Earth's weather and ocean changes require permanent space platforms such as the Mir space station.

Where do people live? i.e. where are the population centers? The fastest way to check this is to observe the USA at night

Observations:

The are a number of hard facts about the Earth that have been determined over the years of geological surveys:

  1. average density = mass of Earth/volume = 5.5 gm/cc (note that cc is shorthand notation for cm to the 3rd power). Granite has a mean density of 3.0, which is mostly what our crust is made of. Therefore, since the mean density of the whole Earth is larger than granite, the core of the Earth must be made of something much denser than granite -> Iron (Fe) and Nickel (Ni).

  2. Seismology uses the propagation of seismic waves from earthquakes to study the Earth's interior (similar to refracted light). Two types of seismic waves 1) pressure or P waves and 2) shear or S waves. Shear waves cannot propagate in liquids or gases, since there are no lateral restoring forces. P waves can travel through liquid or solids.

    Seismic waves travel at about 10 km/sec and, from mapping of the timing and type of wave around the globe, we are able to map the interior of the Earth. Changes in refraction of seismic waves are due to sharp changes in the density = discontinuities due to chemical composition.

    The result is that we know that the interior of the Earth has 4 components:

    1. a thin crust of density 3.3 gm/cc composed of metals, silicates (a substance called basalt)
    2. a semi-solid mantle of density 3.5 to 5.5 gm/cc composed of olivine Fe oxides
    3. a liquid outer core of density 9 to 11 gm/cc composed of molten Fe
    4. a solid inner core of density 17 gm/cc composed of Fe and Ni.

    The temperature of the inner core is 6200 K. The layers of lower density float on top of the the higher density ones, like cork on water. The rocky crust is therefore on the outside.

  3. Crustal dating -> radioactive dating (note this is not carbon dating, that's different) - radioactive elements have known half-life's = the time for the material to decay to a lighter atom.

    For example: uranium 238 decays to lead 206 with a half-life of 4.5x109 years. So, if a rock is 1/2 U 238 and 1/2 Pb 206 then its age is 4.5x109 years.

    Oldest rocks on the Earth are 3.8x109 years by radioactive dating. The oldest rocks in meteors are 4.7x109 years. Thus, the crust is not original Solar System material. It has been reprocessed by some method (hint: the age of the ocean floor is only 0.2x109 years).

Earth's Crust:

The surface of the Earth is 71% water and 29% land (we should have named our planet Ocean).

Note that the crust is thin under the oceans, thick under mountains. The convective motion of the mantle under the thin spots causes sea floor spreading/continental drift. How do we know the continents are moving? Look at the fossil record.

The dry land is composed primarily of:

  1. Igneous rock - formed from molten material, such as basalt and granite
  2. Sedimentary rock - minerals cemented by pressure, such as sandstone and limestone
  3. Metamorphic rock - igneous or sedimentary rock that has been subjected to high temperatures and pressures, such as marble

The lifecycle of these rocks is given in the following diagram:

The crust shaped by:

1. impact cratering in the early solar system

2. erosion - wind, water, slumping (gravity) - most early cratering erased by erosion on planets with thick atmospheres

3. thermal-tectonic activity (plate tectonics) - outflow of heat from core transfered to convective motion in mantle.

The motion is converted in linear motion of the crustal plates. There are 12 plates all floating on the mantle with speeds of a few cm per 100 years.

There are four (4) types of boundaries between the plates which give rise to particular surface features. For example, colliding plates form mountains.

Young mountain system are sharp and irregular (e.g. Himalayas), old mountain systems are low and rounded (e.g. Appalachians)

An example of tectonic activity in the form of volanic activity on the Earth = Mt. St. Helens:

before

after

don't be me

As early as the 1920s, scientists noted that earthquakes are concentrated in very specific narrow zones, now known to be plate edges . In 1954, French seismologist J.P. Roth published this map showing the concentration of earthquakes along the zones indicated by dots and cross-hatched areas.

Earth's Atmosphere:

The Earths atmosphere has undergone some extreme changes since the time of its formation. The process has 7 stages:

  1. proto-atmosphere phase: the original atmosphere of the Earth, the proto-atmosphere, was accreted from the early Solar System material and was very similar to the composition of Jupiter, thick and rich in light elements (hydrogen,helium,neon/H,He,Ne)

  2. early atmosphere phase: The original proto-atmosphere was lost into outer space because a) the earth is close to the Sun and the atoms are heated plus b) the gravity of the Earth is weak (compared to Jupiter for example). Thus, as atoms were heated by the Sun's radiation, their kinetic motion increased (see microscopic understanding of heat). For the lightest elements, the heating was sufficient to increase their average velocity to greater than the escape velocity, and they left the Earth.

  3. secondary atmosphere phase: Most of the original atmosphere was light elements (H and He are more abundant than any of other elements). A secondary atmosphere that was rich in water (H2O), carbon dioxide (CO2), nitrogen (N2) and sulfur (SO2) was built up by outgassing from volcanos. These materials were trapped in the mantle during the Earth's formation and also added to by later bombardment from icy comets.

  4. cooling phase: As the atmosphere cooled, H2O rains out to become the oceans

  5. photodisintegration: extra water vapor is converted into H2 and CO2 by photodisintegration

  6. carbonate rock formation: H2O and CO2 react in the oceans to become carbonate rocks and O2

  7. life: development of living organisms turns more CO2 into O2. In fact, since O2 is highly reactive, biological activity is the main source for the O2 content of today's atmosphere.

The endresult is a reducing atmosphere with a final composition of 78% N2, 21% O2, 1% Ar and trace amounts of H2O, CO2 (0.03%), Ne and Xe

Although the CO2 content is very small, this trace gas plays an important role in terrestrial climate, in that it is responsible for the greenhouse effect. Atmospheric CO2 traps IR radiation (heat), thereby increasing the surface temperature to levels compatible with the sustainability of life.

The atmosphere also plays an important role in protecting the surface from UV and cosmic rays, and space debris (meteoroids).

Earth's magnetic field:

A field is one of those mathematical conceptual tools to help us understand the behavior of objects with energy. A field assigns to every point in space a strength or force plus direction. A field is used to calculate resulting motion of object within the field and acted on by the field.

The concept of a field conveys the information about location and strength of its sources (in this example, magnetic poles).

The Earth is surrounded by a magnetic field, generated in the core of our planet, in the shape shown below. The field lines (red in diagram below) show different strengths where the lines closest to the Earth are stronger than the lines farther away.

Earth's magnetic field is distorted, compressed on the side facing the Sun, greatly extended on the opposite side. The reason for this is the solar wind, a particle flux from the sun, consisting mostly of protons and electrons.

Note that the Van Allen belts act as a magnetic mirror to trap high energy particles and direct them to the pole regions. When they interact with the upper atmosphere you get aurora. The mapping of the magnetic field around Earth, and the discovery of the Van Allen belts were the first important landmarks of scientific space exploration through spacecraft in the 1950s.

The origin of the Earth's magnetic field is its Iron/Nickel (Fe/Ni) inner core. The inner core is hot and its rotation produces friction which ionizes the Fe/Ni atoms. Ionization means many free electrons in the core. Free flowing electrons = electric current. By the dynamo effect, a changing electric field produces a magnetic field.