astronomy picture of the day. the sun core temperature - 15 million k surface temperature - 6000 k...
Post on 21-Dec-2015
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Astronomy Picture of the Day
The Sun
• Core temperature - 15 million K
• Surface temperature - 6000 K
• 99.9% of all of the matter in the solar system
• Entirely gaseous
• Supplies the energy essential for life on Earth
• All normal matter was created inside a star similar to the sun!
The Sun
The Sun in X-rays over several years
The Sun is a star: a shining ball of gas powered by nuclear fusion.
Mass of Sun = 330,000 MEarth
Radius of Sun = 109 REarth
Luminosity of Sun = 4 x 1026 Watts(Equivalent to 100 billion 1-megaton explosions every second!)
Why doesn't the sun blow itself apart?
Hydrostatic Equilibrium
Internal heat and pressure directed outward Gravity pulling mass inward Two forces balance When all hydrogen transformed to helium, Sun will begin to collapse
Let's start with the core, where the Sun's energy is generated.
The Interior Structure of the Sun
• Core - nuclear fusion• Radiation zone - completely
ionized => no photon absorption
• Convection zone - less ionization => photon absorption
• Photosphere - radiation, the part of the sun that we see
• How do we get this info?
What Powers the Sun?
Nuclear Fusion: An event where the nuclei of two atoms join together.
Need high temperatures. Why? To overcome electric repulsion.
Energy is produced. (A small amount of mass = a lot of energy)
E = mc2. Sum of mass and energy always conserved in reactions. Mass is just “frozen” energy.
Why High Temperatures?
To overcome electric repulsion High temp => fast atomic motion (Molecular Motion Demo)
Nuclear forces - very short range (10-15m)
100 times EM force
1039 times gravity(“Fusion” Demo)
How does energy get from core to surface?
core
"radiation zone":
photons slowly drift outwards
"convection zone"
"surface" or photosphere: photons escape into space.
photon path
Sunspots (evidence for 11 year cycle)
Roughly Earth-sized
Last ~2 months
Usually in pairs
Follow motion of sunspots => can determine rotation rate(Sunspot Demo)
Magnetic Fields
Rotating Earth generates a magnetic field
- Like bar magnet aligned with Earth’s axis
Influences paths of electrically charged particles
AuroraeCharged particles from solar wind spiral towards polesCollide with and excite atmospheric moleculesEmission spectra!
The Sun's Rotation
The Sun exhibits Differential Rotation just like the Jovian planets. ~25-36 days
What is this? (animation)
What might this mean for the magnetic field of the Sun?
Sun’s Magnetic FieldRotating sun also generates a magnetic fieldDifferential rotation => magnetic field distortion
Loops extending beyond photosphere can form
SunspotsThey are darker because they are cooler (4500 K vs. 5800 K).
Related to loops in the Sun's magnetic field.
radiation from hot gas flowing along magnetic field loop of Sun.
Solar Flares
Violent ejection of large amount of particles from Sun surface.
(animation)
Above the photosphere, there is the chromosphere, transition zone, and...
The Corona
Best viewed during eclipses.
Solar wind => Evaporation
1 million tons/s lost. But Sun has lost only 0.1% of its mass from solar wind in its 4.6 billion year lifetime.
Apparent Brightness vs. Luminosity
Luminosity – Intrinsic power output
Apparent Brightness – Perceived intensity when viewed from some distance
Does an object emitting light appear brighter or dimmer as it moves away from you?
Apparent Brightness and Distance
• Calculate luminosity, measure apparent brightness => figure out distance!