Transcript Sun ppt

THE SUN
The Sun is a star = hot ball of plasma fuelled
by nuclear fusion at its core
Age: 4.6 billion years
4.60
billion
years
old
Solar Dynamic Observatory (SDO)
Different features of the Sun can be revealed by
viewing it under different wavelengths
https://youtu.be/kS57VH3QN1g
Layers of the Sun
Corona
2 millionoC; 2100 km above photosphere
Chromosphere Sits above photosphere
Photosphere
“Sphere of light”
Layer of Sun’s atmosphere; 6000oC
Sunspot
Areas of strong magnetic field located on the
photosphere; cooler than surrounding; 4500oC
Core
Nuclear fusion reaction occurs (H atoms fused
into He atoms); 15 mil. oC
The churning motion of the Sun's
convection zone creates magnetic
fields that
• float to the surface
(photosphere) and
• appear as darker (cooler)
sunspots
Monitor the Sun live:http://www.helioviewer.org
Sun’s rotation
The Sun rotates faster at its equator
Inferences?
the Sun is not a solid body; it doesn’t have
uniform rotation
Sun’s Corona mass ejection
(cme)
• Huge emission of energy
and charged particles
• So powerful that it shuts
down communications,
power grids, satellites on
Earth
Solar wind
Solar flare/storm
= an intense burst of a stream of fastradiation coming from moving charged
the release of
particles ejected by
magnetic energy
the Sun – creates
associated with
Auroras
sunspots.
Solar flares/ corona mass ejection
Pros
- Can disrupt
- Gives beautiful auroratelecommunications
fantastic light show
- Damage electronic
equipment
- Cause overload of power
network resulting in blackout
Practice Label the layers of the
Sun
• Watch Secret of the Sun
Secret of the Sun
https://www.youtube.com/watch?v=ncphh8FWUUE