Sun: Difference between revisions
imported>Ro Thorpe mNo edit summary |
imported>Mark Widmer (Added diameter relative to that of Earth. Added number of revolutions about milky way. Initial-caps on "Earth" in several places for consistency. Added colons after quantity names, for consistency.) |
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{{Image|391872main Filament Aheadzm.jpg|right|450px|Sun's eruption.<ref>Sun's eruption[http://www.nasa.gov/mission_pages/stereo/multimedia/filament_eruption.html]</ref>}} | {{Image|391872main Filament Aheadzm.jpg|right|450px|Sun's eruption.<ref>Sun's eruption[http://www.nasa.gov/mission_pages/stereo/multimedia/filament_eruption.html]</ref>}} | ||
As a star, there is nothing unusual about it. But the sun is more important to people than any other star. Without the heat and light of the sun, there would be no life on | As a star, there is nothing unusual about it. But the sun is more important to people than any other star. Without the heat and light of the sun, there would be no life on Earth. It is the only star of which we can clearly observe the surface. For this reason, scientists study it to learn about stars much farther away. The visible surface of the sun consists of hot gases that give off light and heat. Only about one two-billionth of sun's light and heat reaches Earth. The rest of the sun's light and heat is lost in space. | ||
'''Distance from | '''Distance from Earth:''' | ||
''Shortest'' about 147,100,000 kilometers; ''Greatest'' about 152,100,000 kilometers; ''Mean'' about 150 million kilometers. Sunlight takes about 8 minutes and 20 seconds to reach | ''Shortest'' about 147,100,000 kilometers; ''Greatest'' about 152,100,000 kilometers; ''Mean'' about 150 million kilometers. Sunlight takes about 8 minutes and 20 seconds to reach Earth, traveling at 299,792 km/s. | ||
'''Diameter:''' | '''Diameter:''' | ||
1,392,000 km | 1,392,000 km, or about 109 times that of Earth. | ||
'''Volume''' | '''Volume:''' | ||
1,300,000 times that of | 1,300,000 times that of Earth. | ||
'''Mass''' | '''Mass:''' | ||
99.8% mass of solar system; about 333,000 times that of | 99.8% of the mass of the solar system; about 333,000 times that of Earth | ||
'''Temperature''' | '''Temperature:''' | ||
''Center''- about 15,000,000° C; ''Surface'' about 5500° C. That represents cooling by a factor of more than 2,000 at the surface, to a temperature almost twice the temperature at which iron boils (iron boiling point: 3,000° C (5,432° F))<ref>[http://www.britannica.com/EBchecked/topic/294242/iron iron] Free full-text article from Encyclopedia Britannica Online</ref> | ''Center''- about 15,000,000° C; ''Surface'' about 5500° C. That represents cooling by a factor of more than 2,000 at the surface, to a temperature almost twice the temperature at which iron boils (iron boiling point: 3,000° C (5,432° F))<ref>[http://www.britannica.com/EBchecked/topic/294242/iron iron] Free full-text article from Encyclopedia Britannica Online</ref> | ||
'''Rotation period''' | '''Rotation period:''' | ||
About 1 month | About 1 month | ||
'''Revolution period in the Milky Way:''' | '''Revolution period in the Milky Way:''' | ||
About 225 million years | About 225 million years. The sun has made roughly 20 revolutions in its 4.6 billion year lifetime. | ||
'''Chemical makeup:''' | '''Chemical makeup:''' | ||
Hydrogen, about 75%; helium, about 25%; at least 70 other elements make up the remaining 1 to 2 percent | Hydrogen, about 75%; helium, about 25%; at least 70 other elements make up the remaining 1 to 2 percent | ||
'''Density''' | '''Density:''' | ||
Convection zone - about 1/10 that of water | Convection zone - about 1/10 that of water | ||
Revision as of 19:54, 21 July 2020
The sun is a middle-sized main sequence star, more specifically a yellow dwarf, which has eight recognized planets, three dwarf planets and myriad asteroids revolving around it. It mainly consists of hydrogen, which it converts to helium through a process of nuclear fusion, providing the heat and light that allowed life to form here on our planet, Earth. The sun is about 93 million miles, or about eight light minutes, away from Earth.
As a star, there is nothing unusual about it. But the sun is more important to people than any other star. Without the heat and light of the sun, there would be no life on Earth. It is the only star of which we can clearly observe the surface. For this reason, scientists study it to learn about stars much farther away. The visible surface of the sun consists of hot gases that give off light and heat. Only about one two-billionth of sun's light and heat reaches Earth. The rest of the sun's light and heat is lost in space.
Distance from Earth: Shortest about 147,100,000 kilometers; Greatest about 152,100,000 kilometers; Mean about 150 million kilometers. Sunlight takes about 8 minutes and 20 seconds to reach Earth, traveling at 299,792 km/s.
Diameter: 1,392,000 km, or about 109 times that of Earth.
Volume: 1,300,000 times that of Earth.
Mass: 99.8% of the mass of the solar system; about 333,000 times that of Earth
Temperature: Center- about 15,000,000° C; Surface about 5500° C. That represents cooling by a factor of more than 2,000 at the surface, to a temperature almost twice the temperature at which iron boils (iron boiling point: 3,000° C (5,432° F))[2]
Rotation period: About 1 month
Revolution period in the Milky Way: About 225 million years. The sun has made roughly 20 revolutions in its 4.6 billion year lifetime.
Chemical makeup: Hydrogen, about 75%; helium, about 25%; at least 70 other elements make up the remaining 1 to 2 percent
Density: Convection zone - about 1/10 that of water
Radiative zone - about equal to that of water
Core - about 100 times that of water