|
Creating an Earth System II:
The Electromagnetic Spectrum
|
A quick review:
The Sun is a star - a furnace in which hydrogen nuclei undergo
fusion to produce helium (and much rarer and heavier elements),
and during which, about 0.3% of their mass is converted to energy.
|
The Sun emits energy in two major forms:
-
The solid material is called plasma (which is actually the
composition of the sun), a mixture of ions, electrons, and neutral
atoms, which is emitted along perturbations in the Sun's magnetic
field, and causes solar flares and coronal mass ejections (CMEs).
- Radiation (heat energy) has no mass and travels at the speed
of light. Radiation is one of three ways in which heat is
transferred:
|
-
Conduction: Heat (energy is transferred
from warmer to cooler materials by direct molecular contact
(e.g. hand burned by a pot handle).
-
Convection: Heat moves with a substance
from one place to another.
- Radiation: Heat moves from source through
a material or vacuum.
|
|
|
Radiation is emitted throughout the electromagnetic
spectrum at the speed of light, whether or not we
can see it. The shorter the wavelength, the higher the energy.
In the image on the left, The electromagnetic spectrum illustrates
the wavelengths and names of various types of radiation.
image courtesy www.nasa.gov
Solar radiation is composed of:
|
|
Resources:
Infrared: More Than Your Eyes Can See
This NASA video discusses infrared light and the measurement of
temperature differences. It is appropriate for grades 5-8, 7 minutes
in length, closed-captioned, and sells for $10.00. It is available
from NASA CORE: Visit NASA CORE
or e-mail: nasaco@leeca.org.
Some important points from the video:
- Infrared is actually a measurement of temperature. Thus all
living organisms emit infrared, as do machines, etc.
- Infrared can pass through things, but at the same time it is
blocked by others (such as glass and water vapor).
- Planets do not give off visible light, but they do give off
infrared. Therefore infrared may be helpful in searching for planets
and in providing a more complete view of the universe.
|
Return to: Creating
an Earth System II | Dynamic Earth Homepage
| UCMP Homepege |
|