Chapter 16: The Sun - Summary Notes
Physical Properties of the Sun
Radius: km, Mass: kg, Density: kg/m.
Differential rotation with a period of about a month.
Surface temperature: K, Core temperature: K.
Apparent surface is the photosphere.
Escape velocity: Km/s.
The sun is a fusion reactor held together by gravity.
Chemical composition: 70.5% Hydrogen, 27.5% Helium, 2% other elements.
Luminosity: Watts.
Solar Interior
Core: Nuclear fusion occurs.
Mathematical models help understand the interior by comparing model outcomes with experiments like solar oscillation and neutrino experiments.
In equilibrium, inward gravity balances outward pressure.
Complex vibration patterns are observed via Doppler shifts of solar spectral lines.
Hydrogen content increases from the center to the surface.
Energy transport occurs via radiation in the radiation zone and convection in the convection zone.
Photons take ~10 million years to escape the sun's surface, while neutrinos take only 2 seconds.
The Sun’s Atmosphere
Spectral analysis identifies elements in the chromosphere and photosphere.
Spectral lines form when light is absorbed before escaping the Sun.
The chromosphere is above the photosphere and is cooler.
The corona is hotter than lower layers, likely due to electromagnetic interactions.
Solar Magnetism
Sunspots are cooler areas due to intense magnetism.
Sunspots are linked by magnetic field lines and originate from the Sun's differential rotation.
The sunspot cycle is 11 years, with polarity switching every 11 years (22-year cycle).
The Active Sun
Areas around sunspots are active, leading to solar prominences (large gas sheets) and solar flares (large explosions).
Coronal mass ejections involve large bubbles detaching from the Sun.
Solar wind escapes through coronal holes.
The corona varies with the sunspot cycle.
The Heart of the Sun
Nuclear fusion (proton-proton chain) is the energy source: .
Energy is released as gamma rays.
Mass-energy conversion follows .
The sun converts about 600 million tons of hydrogen per second.
Solar Neutrinos
Neutrinos provide a direct view of the core.
Detectors use large volumes to observe single interaction events.
Neutrino observations confirm standard solar model predictions after accounting for neutrino type changes.