The eruption of a huge bubble of hot gas from the Sun
This series of images of coronal mass ejections taken with LASCO C3 (May 1-31, 1997) at
Slide 19
Can damage satellites
Very dangerous to astronauts
Power problems
Animation of a CME leaving the Sun, slamming into our magnetosphere.
Slide 20
Let’s go observe the Sun
Sunspot graphing
Slide 21
Gravity
Light (Radiation)
Solar Wind (already discussed)
Slide 22
Gravity
Orbits
The Sun’s powerful gravity keeps the planets in orbit
Slide 23
Radiation
Our Sun (and all active stars) emits radiation
Radio, infrared, visible, ultraviolet, x-ray and even some gamma rays
Most of the sunlight is yellow-green visible light or close to it
The Sun at X-ray wavelengths
Image and info at http://imagine.gsfc.nasa.gov/docs/teachers/gammaraybursts/imagine/page18.html and
http://starchild.gsfc.nasa.gov/docs/StarChild/solar_system_level2/sun.html
.
Slide 24
Activities on Sunlight
UV Man (or woman, or dog, bug, etc.)
Observations of infrared light using filters and cell phones
Slide 25
The Earth’s atmosphere filters out some frequencies
Ozone layer protects us from some ultra-violet, and most x-rays and gamma rays
Water and oxygen absorb some radio waves
Water vapor, carbon dioxide, and ozone absorbs some infrared
Electromagnetic spectrum
.
Slide 26
Sunlight is absorbed by Earth
Let’s test what happens to the light.
Activity Time!!
Slide 27
The Sun does NOT send “heat rays” into space. Some of its light is infrared, but that is not the same thing as heat.
The Sun’s light is absorbed by Earth (clouds, plants, oceans, rock…)
By absorbing the light, we are transforming it into heat energy
Slide 28
Light from the Sun is absorbed by the Earth, unevenly to: