Title: THE SUN: AWESOME AND ACTIVE
1THE SUN AWESOME AND ACTIVE
- Boston University PHOTON
- Outreach Presentation
2The Sun
- An average-size yellow star, just like billions
of others in the universe - Center of the solar system, Earth orbits around
it - Formed about 4.6 billion years ago
- The sun has a mass of 2x1030 kg or 330,000
Earths, thats 99.8 of the mass in the solar
system.
3The Suns Energy Earth
- The Sun is the source of all of the energy on
Earth. - The amount of energy that reaches Earth from the
Sun in one second is enough energy to meet
Massachusetts current energy needs for
32,655,294 years!!! - About half the energy that hits the Earth is
absorbed and used to heat the planet. - You can feel this energy in the form of heat on
your skin on a sunny day.
figure based on data from California Energy
Commision http//www.energy.ca.gov/electricity/us
_percapita_electricity_2003.html
4Where does the Suns Energy Come From?
- Energy is produced in the Suns core through a
process known as nuclear fusion. - Nuclear fusion is when nuclei of one kind of
element combine to make a new nucleus in that
requires less energy to hold it together. This
difference in energy is spit out as a result of
the reaction. - The Suns nuclear fusion occurs when four
hydrogen nuclei combine to make helium and
release energy. - This type of reaction cant happen just
anywhere, it can only happen at incredibly high
temperatures and pressures like those found in
stars, somewhere around 23 million degrees!!
Energy
1 Helium nucleus
4 Hydrogen nuclei
5How much energy does the Sun make?
- We know how much energy the Sun emits by
measuring the amount of energy that reaches
Earth. - The Sun consumes 660 million tons of hydrogen
releasing 100 billion megatons of energy per
second! Thats the same energy as 20 billion
Hydrogen bombs every second! - Based on the amount of hydrogen the Sun consumes
per second and the mass of the Sun, we estimate
its lifetime to be 50 billion years.
Nuclear Fusion Hydrogen Bomb50 megatons
6Whats inside the sun?
Layers of the Sun 1. Core the core of the sun
alone is the size of 13 Earths! 2. Radiative
Zone energy from the core radiates through this
part of the Sun 3. Convective Layer convection
cells move energy through this part of the
Sun 4. Photosphere This is the part of the sun we
see 5. Chromosphere a part of the Suns
atmosphere 6. Corona This is a bright halo
around the Sun
Diameter of the Sun Diameter of 56 Earths!
7Energy Escapes the Sun
- Fusion occurs in the Suns core, the hottest
part. - The energy released by the fusion in the Suns
core is in the form of light. - It only takes 8 minutes for light from the
surface of the Sun to reach Earth - But it takes 170,000 for the light energy from
the core to reach the Suns surface because it
doesnt go in a straight line
8The Changing Sun
- The surface of the Sun is constantly changing
- The Sun is shooting particles off it all the time
called the Solar Wind - There is an 11-year Solar Cycle when the Sun
goes from being very active (solar maximum) to
not not very active (solar minimum
9How is the Sun active?
- The solar cycle is characterized by the rising
and falling of solar activity - The solar maximum is the period of greatest solar
activity - During solar maximum the Sun is more active
meaning there are more sunspots and solar flares
10Sunspots
- What?
- Dark spots on the Sun's surface that are cooler
than the surrounding areas - Temperature of
- Sunspot 3800 K
- Surrounding area 5800 K
- Why?
- The strong magnetic field in that area stops the
area from being able to transfer energy so the
temperature isnt as high
11More about Sunspots
- Sunspots can be about the size of Earth or even
bigger!!! - They come in pairs
- They are still really hot, just not as hot as the
rest of the Suns surface - Sunspots move across Suns surface as it rotates
12Magnetic Activity on the Sun
- Sunspots are caused by strong magnetic fields
- Magnetic ropes break through the Suns surface
- At each end of the rope is a sunspot
- It is the Suns magnetic activity that causes
solar storms and solar flares
13How do we know all of this about the Sun?
- Telescopes
- You can look at the Sun through a telescope with
special filters. - You can also use a solar telescope that projects
the image of the Sun onto a piece of paper
instead of into your eye. - Satellites
- There are also several spacecraft that
- are observing the Sun SOHO, TRACE, STEREO
- These satellites look at the Sun in all
- different kinds of light (ultraviolet, visible,
- infrared, X-ray) to see everything that is
- going on
- Many cameras on telescopes need to use
- a caronagraph, where a disk is used to block
- out the Suns surface so we can see all the dim
- stuff that the Suns brightness would drown out