Transcript The Sun * El Sol * Die Sonne

The Sun – El Sol – Die Sonne
ESPS- Palmer High School
Interesting Facts about the sun
 http://www.bing.com/videos/search?q=Sun&FORM=HDR
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http://www.bing.com/videos/search?
q=youtube+10+facts+about+the+su
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How big is the sun?
 About 110 times wider than Earth
 1.3 million times bigger than Earth
 Sun is 865 thousand miles wide
Properties of the sun
(what is it made of?)
 Contains 99.8% of the entire mass of Solar System
 Is our primary source of energy
 Made of Gases (what 2 types of gases?) 70%-28%
 Is a star
How does our Sun compare to
other Stars?
 Active stars range in size from supergiants to dwarfsOur sun is a dwarf with medium mass
 Stars range from very bright (supergiants) to very dim
(dwarfs)-Our Sun is a medium-bright dwarf
 Stars range from very hot blue on the outside (O class)
to cool red on the outside (M class)-Our Sun is inbetween--yellow
So is our Sun an average star?
 No—most stars are smaller and cooler than our Sun BUT
 Most of the bright stars we see are bigger and hotter
http://www.treehugger.com/slideshows/natural-sciences/12-mostamazing-time-lapse-videos-stars-landscapes-and-urbanscenes/page/3/#slide-top
Inside of the sun
 Core
 Radiative Zone
 Convection zone
The Sun’s Atmosphere
 Photosphere- the photosphere may be thought of as the
imaginary surface from which the solar light that we see
appears to be emitted.
 Chromosphere- The chromosphere is an irregular layer
above the photosphere where the temperature rises from
6000°C to about 20,000°C. At these higher temperatures
hydrogen emits light that gives off a reddish color
 Corona- This extended outer atmosphere of the Sun has a
temperature of millions of degrees, but it is 10 billion times
less dense than the atmosphere of the Earth at sea level.
How does the sun produce
energy?
 The Sun produces energy by the nuclear fusion of
hydrogen into helium in its core. Since there is a huge
amount of hydrogen in the core, these atoms stick
together and fuse into a helium atom. This energy is
then radiated out from the core and moves across the
solar system. This is radiation (gamma rays)
http://www.youtube.com/watch?v=4i
yS2WmT9NM
Features of the sun
 Sun Spots-
These are dark, cool areas that appear
on the photosphere. Sunspots always appear in pairs
and are intense magnetic fields (about 5,000 times
greater than the Earth's magnetic field) that break
through the surface. Caused by movement of gases.
Features of the sun continued…..
 Prominences- Clouds of gases from the
chromosphere will rise and orient themselves along the
magnetic lines from sunspot pairs and form arches.
Prominences can last two to three months and can
extend 30,000 miles (50,000 kilometers) or more above
the sun's surface. Upon reaching this height, they can
erupt for a few minutes to hours and send large
amounts of material racing through the corona and
outward into space at 600 miles per second (1,000
kilometers per second); these eruptions are called
coronal mass ejections.
Features of the sun continued…
 Solar Flares
occur at times in complex sunspot
groups, they are abrupt, violent explosions from the sun.
Solar flares are thought to be caused by sudden
magnetic field changes in areas where the sun's
magnetic field is concentrated. They're accompanied by
the release of gas, electrons, visible light, ultraviolet
light and X-rays. When this radiation and these particles
reach the Earth's magnetic field, they interact with it at
the poles to produce the auroras (borealis and australis).
Solar flares can also disrupt communications, satellites,
navigation systems and even power grids
Features of the sun continued…
Solar Wind
 Blows charged particles and magnetic fields away from
the Sun
 Charged particles captured by Earth’s magnetic field
 Create Auroras or Northern and Southern Lights
http://www.bin
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• Electrons from solar wind are
Auroras captured by the Earth’s magnetic
field
• Interact with atoms in our
atmosphere: oxygen and nitrogen
make red and green; nitrogen can
also make violet
• Northern lights are Aurora Borealis,
while southern are Aurora Australis
http://sohowww.nascom.nasa.gov/bestofsoho/Movies/animation/Solar
wind.mpg
Coronal Mass Ejection (CME’s)
 CME is a massive burst of solar wind and magnetic fields
rising above the solar corona or being released into
space
Effects of CME
• Can damage satellites
• Very dangerous to astronauts
• Power problems
This series of images of coronal mass ejections taken with LASCO C3
(May 1-31, 1997) at
http://sohowww.nascom.nasa.gov/bestofsoho/Movies/C3May97/C3M
ay97sm.mpg
How does the sun affect the
Earth?
 Gravity- Orbits- The Sun’s powerful gravity keeps the planets in
orbit
 Radiation- Our Sun (and all active stars) emits radiationRadio,
infrared, visible, ultraviolet, x-ray and even some gamma rays. Most
of the sunlight is yellow-green visible light or close to it
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
 Sunlight is absorbed by Earth
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