our sun 16 october 2003. today: basic facts about the sun solar details: granulation, sunspots,...

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Our Sun 16 October 2003

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Page 1: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Our Sun

16 October 2003

Page 2: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Today:

• Basic facts about the sun

• Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

• What is the sun made of?

Page 3: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Basic facts about the Sun

• Distance from earth: 150 million km (400 x as far as moon)

• Angular diameter: 1/2 degree (same as moon)• True diameter: 110 x earth’s diameter• Mass: 330,000 times earth’s mass• Average density: 1.4 times that of water• Intensity of sunlight at earth’s location: 1400 watts per

square meter• Total power output: 3.9 x 1026 watts• Surface temperature: 5800 K• Made of ionized gases

Page 4: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Basic facts about the Sun

• Distance from earth: 150 million km (400 x as far as moon) measured using radar

• Angular diameter: 1/2 degree (same as moon)• True diameter: 110 x earth’s diameter (400 x moon’s)• Mass: 330,000 times earth’s mass gravity!• Average density: 1.4 times that of water mass/volume• Intensity of sunlight at earth’s location: 1400 watts per

square meter measure directly• Total power output: 3.9 x 1026 watts calculate• Surface temperature: 5800 K from power or spectrum• Made of ionized gases too hot for anything else!

Page 5: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Sunspots, Granulation

Page 6: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Electromagnetism

• The sun is made of ionized atoms and electrons -- electrically charged particles

• Charged particles in motion create magnetic fields

• Magnetic fields can “trap” electrically charged particles (which can move parallel to the field but can’t go far in perpendicular directions)

Page 7: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Magnetic activity around sunspots

Page 8: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Magnetic activity around sunspots

Page 9: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Solar Prominences

Page 10: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

Solar Prominences

Page 11: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

The Solar Corona

Page 12: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

The Solar Corona and Solar Wind

Page 13: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

What is the sun made out of?• 74% hydrogen• 25% helium• 1% all other elements (oxygen, carbon,

nitrogen, neon, aluminum, silicon, iron, . . . )

Page 14: Our Sun 16 October 2003. Today: Basic facts about the sun Solar details: Granulation, sunspots, magnetic fields, flares, prominences, corona, solar wind

The Periodic Table

Masses and rarities increase (mostly) toward the bottom of the table.