Our Solar System

 

 

U N D E R C O N S T R U C T I O N ! ! ! ! !

The Center of Our Solar System.

Interior of the Sun

Regions of the sun include the core, radiation zone, convection zone, and photosphere. Gases in the core are about 150 times as dense as water and reach temperatures as high as 16 million degrees C (29 million degrees F). The sun’s energy is produced in the core through nuclear fusion of hydrogen atoms into helium. In the radiation zone, heat flows outward through gases that are about as dense as water. The radiation zone is cooler than the core, about 2.5 million degrees C (4.5 million degrees F). In the convection zone, churning motions of the gases carry the sun’s energy further outward. The convection zone is slightly cooler, about 2 million degrees C (1.1 million degrees F), and less dense, about one-tenth as dense as water. The photosphere is much cooler, about 5500° C (10,000° F) and much less dense, about one-millionth that of water. The turbulence of this region is visible from earth in the form of sunspots, solar flares, and small patches of gas called granules.

 

Microsoft Illustration

 

 


 

 

 

 

Mercury

Mercury orbits closer to the sun than any other planet, making it dry, hot, and virtually airless. Although the planet’s cratered surface resembles that of the moon, it is believed that the interior is actually similar to the earth’s, consisting primarily of iron and other heavy elements. This photograph was taken in 1974 by Mariner 10, the first probe to study Mercury in detail.

 

NASA/Science Source/Photo Researchers, Inc.

 


Venus: our sister planet

 

Venus

Venus is the brightest object in our sky, after the sun and moon. Swirling clouds of sulfur and sulfuric acid and a deep atmosphere obscure the planet’s surface, inhibiting study of it from earth, but space vehicles, outfitted with probes, have successfully returned data. Probes determined that Venus is the hottest of the planets, with a surface temperature of about 462° C (864° F). Scientists believe a greenhouse effect causes the extreme temperature; the planet’s thick clouds and dense atmosphere allow the sun’s radiant energy to reach the planet, but inhibit the escape of the heat.

 

NASA/Science Source/Photo Researchers, Inc.

 


Earth

An oxygen-rich and protective atmosphere, moderate temperatures, abundant water, and a varied chemical composition allow earth to support life, the only planet to do so. The slightly pear-shaped planet is composed of rock and metal, which are present in molten form beneath its surface. This photograph, taken by the Apollo 17 spacecraft in 1972, shows Arabia, the African continent, and Antarctica (most of the white area near the bottom).

 

NASA/Science Source/Photo Researchers, Inc.

 


Mars: the home of the pathfinder mission

Mars

Unpiloted spacecraft from the United States, launched between 1964 and 1976, have supplied the most detailed information on Mars. From this data, scientists determined that the planet’s atmosphere predominantly consists of carbon dioxide (CO2), with small amounts of nitrogen, oxygen, and water vapor also present. Due to the thinness of the atmosphere, daily temperatures often vary as much as 100° C (180° F). In general, surface temperatures are too cold and surface pressures too low for water to exist in a liquid state on Mars, so the planet resembles a cold, high-altitude desert.

 

Chris Bjornberg/Photo Researchers, Inc.

Jupiter: the gas giant

Jupiter and its Moons

Jupiter is the largest of the planets, with a volume 1400 times greater than that of the earth. Jupiter’s colorful bands are caused by strong atmospheric currents and accentuated by a dense cloud cover. The massive planet, upper right, is shown here with the four largest of its sixteen satellites: Europa, center, nearest Jupiter, Io upper left, Callisto lower left, and Ganymede lower right.

 

NASA/Science Source/Photo Researchers, Inc.

Saturn: home of the rings

Saturn

Saturn, distinguished by its rings, ranks as the second largest planet—Jupiter is the largest—in the solar system. In 1610 the Italian physicist and astronomer Galileo discovered the ring system using one of the first telescopes ever made. Although the planet formed more than 4 billion years ago, it continues to settle and contract, generating three times as much heat as it receives from the sun. The Hubble Space Telescope obtained this image of Saturn on August 26, 1990.

 

Liaison International

Uranus: one of the most beautiful planets

Uranus

Uranus’s blue-green color comes from the methane gas present in its cold, clear atmosphere. The dark shadings at the right edge of the sphere correspond to the day-night boundary on the planet. Beyond this boundary, Uranus’ northern hemisphere remains in perpetual darkness because of the way the planet rotates. Scientists compiled this view of Uranus from images returned from Voyager 2 in 1986, when the probe was 9.1 million km (5.7 million mi) away from the planet.

 

NASA

Neptune: very beautiful

Neptune

The 1989 Voyager 2 mission produced this false-color image of Neptune showing the different components of Neptune’s atmosphere. The red layer shows scattered sunlight from a haze around the planet, the blue/green indicates methane, and the white areas are high-level clouds that reflect sunlight above the atmosphere.

 

NASA/Science Source/Photo Researchers, Inc.

Pluto: the most distant planet

Pluto

Pluto is farther from the sun than the other planets in the solar system, although it occasionally moves in closer than Neptune due to an irregular orbit. The small, rocky, and cold planet takes 247.7 years to revolve around the sun. This artist's rendition depicts Pluto, foreground; its moon, Charon, background; and the distant sun, upper right.

 

NASA/Science Source/Photo Researchers, Inc.

 

 

 

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