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The Sun. Solar Facts. Our Sun is a star, just like all the other stars in the night sky The name of our star is “The Sun”, but also “Sol” Latin for sun is “solis”, Greek for sun is “helios” Holds the entire Solar System together by its immense gravity. Solar Facts. - PowerPoint PPT Presentation
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The SunThe Sun
Solar FactsSolar Facts
• Our Sun is a star, just like all the other stars in the night sky
• The name of our star is “The Sun”, but also “Sol”
• Latin for sun is “solis”, Greek for sun is “helios”
• Holds the entire Solar System together by its immense gravity
Solar FactsSolar Facts• Size: 1.4 million km. 110x Earth’s diameter. 1 million
Earths could fit inside the Sun.
• Temperature: Surface = 5,000° C (9,932° F), Inside = 15,000,000° C (27,000,000° F)
• Mass: 99.8% of entire Solar System’s mass, gravity = 28x Earth’s.
• Rotation (spinning): 25 days for equator to rotate, 27 days for poles to rotate
• Revolution: Sun revolves around center of our Milky Way galaxy.
Sun’s InteriorSun’s Interior1. Photosphere
2. Chromosphere
3. Core
4. Corona
5. Sunspots
6. Prominences & Solar FlaresWhere is the . . .
Convective Zone?
Radiation Zone?
Sun’s AtmosphereSun’s Atmosphere
• Corona (“Crown”)– Outer atmosphere, normally not visible (except during full solar
eclipse)– extends into space for millions of kilometers
• Photosphere (photo = “light”)– Middle atmosphere, is visible– Considered the surface layer of the sun
• Chromosphere (chromo = “color”)– Inner atmosphere, has a reddish color– Sometimes partially visible during a solar eclipse
Sun’s InteriorSun’s Interior• Convection Zone
– Outermost layer of interior– Gases move thru zone by convection currents (transfer of heat
by fluid movement)
• Radiation Zone– Middle layer of interior– Energy produced in core moves outward thru zone by radiation
(transfer of heat by energy waves)
• Core– Produces enormous amount of energy by nuclear fusion, fusing
hydrogen atoms (H) into helium atoms (He) under intense pressure and heat
Solar FeaturesSolar Features• Sunspots
– Dark spots on the sun’s surface– Areas of gas that are cooler than surrounding gases
• Prominences– Huge loops of gases linking sunspot regions
• Solar Flares– Prominences sometimes connect, causing the sun’s surface
gases to erupt far into space
• Solar Wind– Charged particles streaming from the sun, increased during
solar flares– Causes the planetary auroras, can interfere and damage
electronic equipment