Tuesday, July 5, 2011

Solar System


Neptune's <a href="/neptune/lower_atmosphere.html">atmosphere</a> shows

a striped pattern of

<a href="/neptune/atmosphere/N_clouds_overview.html">clouds</a>.

This cloud pattern is very similar to that of

<a href="/jupiter/jupiter.html">Jupiter</a> and

<a href="/saturn/saturn.html">Saturn</a>.

Neptune even has a <a href="/neptune/atmosphere/N_clouds_GDS.html">Great Dark

Spot</a> similar

to Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great

Red Spot</a>.

The Great Dark Spot of Neptune is thought to be a hole, similar to the hole

in the <a href="/earth/Atmosphere/ozone_layer.html">ozone layer on

Earth</a>,

in the <a href="/physical_science/chemistry/methane.html">methane</a> cloud

deck of Neptune.<p><small><em>Image courtesy of NASA</em></small></p>This dramatic view of Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great Red Spot</a> and its surroundings was obtained by <a href="/space_missions/voyager.html">Voyager 1</a> on Feb. 25, 1979, when the spacecraft was 5.7 million miles (9.2 million kilometers) from Jupiter. Cloud details as small as 100 miles (160 kilometers) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex end variable wave motion.<p><small><em>Image courtesy of NASA</em></small></p>This historic image is the first ever taken from a spacecraft in orbit about <a href="/mercury/mercury.html">Mercury</a>, the innermost planet of the solar system.  Taken on 3/29/2011 by <a href="/space_missions/robotic/messenger/messenger.html">MESSENGER</a>, it shows numerous craters across the <a href="/mercury/Interior_Surface/Surface/surface_overview.html">surface</a> of the planet.  Temperatures there can reach over 800°F because Mercury is so close to the Sun and rotates so slowly.  MESSENGER entered orbit around Mercury earlier in March 2011.<p><small><em>NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em></small></p>Comets are <a href="/comets/comet_nucleus.html">lumps</a> of ice

and dust that periodically come into the center of the solar system from

its <a href="/comets/Oort_cloud.html">outer

reaches</a>.

Some comets make <a href="/comets/perihelion_pass.html">repeated

trips</a> to the inner

solar system. When comets get close enough to the Sun, heat

makes them start to <a href="/comets/sublimation.html">evaporate</a>.

Jets of gas and dust form long

<a href="/comets/tail.html">tails</a> that we can see from

Earth. 

This photograph shows <a href="/comets/comets_table.html">Comet

Kohoutek</a>,

which visited the inner solar system in 1973.  It has an

<a href="/physical_science/physics/mechanics/orbit/orbit_shape_interactive.html">orbit</a> of

about 75,000 years!<p><small><em>Image courtesy of NASA</em></small></p>
<a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>


Our Solar System

Our solar system is filled with a wide assortment of celestial bodies - the Sun itself, our eight planets, dwarf planets, and asteroids - and on Earth, life itself! The inner solar system is occasionally visited by comets that loop in from the outer reaches of the solar system on highly elliptical orbits. In the outer reaches of the solar system, we find the Kuiper Belt and the Oort cloud. Still farther out, we eventually reach the limits of the heliosphere, where the outer reaches of the solar system interact with interstellar space. Solar system formation began billions of years ago, when gases and dust began to come together to form the Sun, planets, and other bodies of the solar system.

 

Neptune's <a href="/neptune/lower_atmosphere.html">atmosphere</a> shows

a striped pattern of

<a href="/neptune/atmosphere/N_clouds_overview.html">clouds</a>.

This cloud pattern is very similar to that of

<a href="/jupiter/jupiter.html">Jupiter</a> and

<a href="/saturn/saturn.html">Saturn</a>.

Neptune even has a <a href="/neptune/atmosphere/N_clouds_GDS.html">Great Dark

Spot</a> similar

to Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great

Red Spot</a>.

The Great Dark Spot of Neptune is thought to be a hole, similar to the hole

in the <a href="/earth/Atmosphere/ozone_layer.html">ozone layer on

Earth</a>,

in the <a href="/physical_science/chemistry/methane.html">methane</a> cloud

deck of Neptune.<p><small><em>Image courtesy of NASA</em></small></p>This dramatic view of Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great Red Spot</a> and its surroundings was obtained by <a href="/space_missions/voyager.html">Voyager 1</a> on Feb. 25, 1979, when the spacecraft was 5.7 million miles (9.2 million kilometers) from Jupiter. Cloud details as small as 100 miles (160 kilometers) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex end variable wave motion.<p><small><em>Image courtesy of NASA</em></small></p>This historic image is the first ever taken from a spacecraft in orbit about <a href="/mercury/mercury.html">Mercury</a>, the innermost planet of the solar system.  Taken on 3/29/2011 by <a href="/space_missions/robotic/messenger/messenger.html">MESSENGER</a>, it shows numerous craters across the <a href="/mercury/Interior_Surface/Surface/surface_overview.html">surface</a> of the planet.  Temperatures there can reach over 800°F because Mercury is so close to the Sun and rotates so slowly.  MESSENGER entered orbit around Mercury earlier in March 2011.<p><small><em>NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em></small></p>Comets are <a href="/comets/comet_nucleus.html">lumps</a> of ice

and dust that periodically come into the center of the solar system from

its <a href="/comets/Oort_cloud.html">outer

reaches</a>.

Some comets make <a href="/comets/perihelion_pass.html">repeated

trips</a> to the inner

solar system. When comets get close enough to the Sun, heat

makes them start to <a href="/comets/sublimation.html">evaporate</a>.

Jets of gas and dust form long

<a href="/comets/tail.html">tails</a> that we can see from

Earth. 

This photograph shows <a href="/comets/comets_table.html">Comet

Kohoutek</a>,

which visited the inner solar system in 1973.  It has an

<a href="/physical_science/physics/mechanics/orbit/orbit_shape_interactive.html">orbit</a> of

about 75,000 years!<p><small><em>Image courtesy of NASA</em></small></p><a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>Lunar eclipses are special events that only occur when certain conditions are met. First of all, the Moon must be in <a href="/the_universe/uts/moon3.html">full phase</a>. Secondly, the <a href="/sun/sun.html">Sun</a>, <a href="/earth/earth.html">Earth</a> and <a href="/earth/moons_and_rings.html">Moon</a> must be in a perfectly straight line. If both of these are met, then the Earth's shadow can block the Sun's light from hitting the Moon.  The reddish glow of the Moon is caused by light from the Earth's limb scattering toward the Moon, which is reflected back to us from the Moon's surface.<p><small><em>Image credit - Doug Murray, Palm Beach Gardens, Florida</em></small></p>
Neptune's atmosphere shows a striped pattern of clouds. This cloud pattern is very similar to that of Jupiter and Saturn. Neptune even has a Great Dark Spot similar to Jupiter's Great Red Spot. The Great Dark Spot of Neptune is thought to be a hole, similar to the hole in the ozone layer on Earth, in the methane cloud deck of Neptune.

Neptune's <a href="/neptune/lower_atmosphere.html">atmosphere</a> shows

a striped pattern of

<a href="/neptune/atmosphere/N_clouds_overview.html">clouds</a>.

This cloud pattern is very similar to that of

<a href="/jupiter/jupiter.html">Jupiter</a> and

<a href="/saturn/saturn.html">Saturn</a>.

Neptune even has a <a href="/neptune/atmosphere/N_clouds_GDS.html">Great Dark

Spot</a> similar

to Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great

Red Spot</a>.

The Great Dark Spot of Neptune is thought to be a hole, similar to the hole

in the <a href="/earth/Atmosphere/ozone_layer.html">ozone layer on

Earth</a>,

in the <a href="/physical_science/chemistry/methane.html">methane</a> cloud

deck of Neptune.<p><small><em>Image courtesy of NASA</em></small></p>This dramatic view of Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great Red Spot</a> and its surroundings was obtained by <a href="/space_missions/voyager.html">Voyager 1</a> on Feb. 25, 1979, when the spacecraft was 5.7 million miles (9.2 million kilometers) from Jupiter. Cloud details as small as 100 miles (160 kilometers) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex end variable wave motion.<p><small><em>Image courtesy of NASA</em></small></p>This historic image is the first ever taken from a spacecraft in orbit about <a href="/mercury/mercury.html">Mercury</a>, the innermost planet of the solar system.  Taken on 3/29/2011 by <a href="/space_missions/robotic/messenger/messenger.html">MESSENGER</a>, it shows numerous craters across the <a href="/mercury/Interior_Surface/Surface/surface_overview.html">surface</a> of the planet.  Temperatures there can reach over 800°F because Mercury is so close to the Sun and rotates so slowly.  MESSENGER entered orbit around Mercury earlier in March 2011.<p><small><em>NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em></small></p>Comets are <a href="/comets/comet_nucleus.html">lumps</a> of ice

and dust that periodically come into the center of the solar system from

its <a href="/comets/Oort_cloud.html">outer

reaches</a>.

Some comets make <a href="/comets/perihelion_pass.html">repeated

trips</a> to the inner

solar system. When comets get close enough to the Sun, heat

makes them start to <a href="/comets/sublimation.html">evaporate</a>.

Jets of gas and dust form long

<a href="/comets/tail.html">tails</a> that we can see from

Earth. 

This photograph shows <a href="/comets/comets_table.html">Comet

Kohoutek</a>,

which visited the inner solar system in 1973.  It has an

<a href="/physical_science/physics/mechanics/orbit/orbit_shape_interactive.html">orbit</a> of

about 75,000 years!<p><small><em>Image courtesy of NASA</em></small></p><a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>Lunar eclipses are special events that only occur when certain conditions are met. First of all, the Moon must be in <a href="/the_universe/uts/moon3.html">full phase</a>. Secondly, the <a href="/sun/sun.html">Sun</a>, <a href="/earth/earth.html">Earth</a> and <a href="/earth/moons_and_rings.html">Moon</a> must be in a perfectly straight line. If both of these are met, then the Earth's shadow can block the Sun's light from hitting the Moon.  The reddish glow of the Moon is caused by light from the Earth's limb scattering toward the Moon, which is reflected back to us from the Moon's surface.<p><small><em>Image credit - Doug Murray, Palm Beach Gardens, Florida</em></small></p>
This dramatic view of Jupiter's Great Red Spot and its surroundings was obtained by Voyager 1 on Feb. 25, 1979, when the spacecraft was 5.7 million miles (9.2 million kilometers) from Jupiter. Cloud details as small as 100 miles (160 kilometers) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex end variable wave motion.



Comets are <a href="/comets/comet_nucleus.html">lumps</a> of ice

and dust that periodically come into the center of the solar system from

its <a href="/comets/Oort_cloud.html">outer

reaches</a>.

Some comets make <a href="/comets/perihelion_pass.html">repeated

trips</a> to the inner

solar system. When comets get close enough to the Sun, heat

makes them start to <a href="/comets/sublimation.html">evaporate</a>.

Jets of gas and dust form long

<a href="/comets/tail.html">tails</a> that we can see from

Earth. 

This photograph shows <a href="/comets/comets_table.html">Comet

Kohoutek</a>,

which visited the inner solar system in 1973.  It has an

<a href="/physical_science/physics/mechanics/orbit/orbit_shape_interactive.html">orbit</a> of

about 75,000 years!<p><small><em>Image courtesy of NASA</em></small></p><a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>Lunar eclipses are special events that only occur when certain conditions are met. First of all, the Moon must be in <a href="/the_universe/uts/moon3.html">full phase</a>. Secondly, the <a href="/sun/sun.html">Sun</a>, <a href="/earth/earth.html">Earth</a> and <a href="/earth/moons_and_rings.html">Moon</a> must be in a perfectly straight line. If both of these are met, then the Earth's shadow can block the Sun's light from hitting the Moon.  The reddish glow of the Moon is caused by light from the Earth's limb scattering toward the Moon, which is reflected back to us from the Moon's surface.<p><small><em>Image credit - Doug Murray, Palm Beach Gardens, Florida</em></small></p>
This historic image is the first ever taken from a spacecraft in orbit about Mercury, the innermost planet of the solar system. Taken on 3/29/2011 by MESSENGER, it shows numerous craters across the surface of the planet. Temperatures there can reach over 800°F because Mercury is so close to the Sun and rotates so slowly. MESSENGER entered orbit around Mercury earlier in March 2011.NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington


Neptune's <a href="/neptune/lower_atmosphere.html">atmosphere</a> shows

a striped pattern of

<a href="/neptune/atmosphere/N_clouds_overview.html">clouds</a>.

This cloud pattern is very similar to that of

<a href="/jupiter/jupiter.html">Jupiter</a> and

<a href="/saturn/saturn.html">Saturn</a>.

Neptune even has a <a href="/neptune/atmosphere/N_clouds_GDS.html">Great Dark

Spot</a> similar

to Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great

Red Spot</a>.

The Great Dark Spot of Neptune is thought to be a hole, similar to the hole

in the <a href="/earth/Atmosphere/ozone_layer.html">ozone layer on

Earth</a>,

in the <a href="/physical_science/chemistry/methane.html">methane</a> cloud

deck of Neptune.<p><small><em>Image courtesy of NASA</em></small></p>This dramatic view of Jupiter's <a href="/jupiter/atmosphere/J_clouds_GRS.html">Great Red Spot</a> and its surroundings was obtained by <a href="/space_missions/voyager.html">Voyager 1</a> on Feb. 25, 1979, when the spacecraft was 5.7 million miles (9.2 million kilometers) from Jupiter. Cloud details as small as 100 miles (160 kilometers) across can be seen here. The colorful, wavy cloud pattern to the left of the Red Spot is a region of extraordinarily complex end variable wave motion.<p><small><em>Image courtesy of NASA</em></small></p>This historic image is the first ever taken from a spacecraft in orbit about <a href="/mercury/mercury.html">Mercury</a>, the innermost planet of the solar system.  Taken on 3/29/2011 by <a href="/space_missions/robotic/messenger/messenger.html">MESSENGER</a>, it shows numerous craters across the <a href="/mercury/Interior_Surface/Surface/surface_overview.html">surface</a> of the planet.  Temperatures there can reach over 800°F because Mercury is so close to the Sun and rotates so slowly.  MESSENGER entered orbit around Mercury earlier in March 2011.<p><small><em>NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington</em></small></p>Comets are <a href="/comets/comet_nucleus.html">lumps</a> of ice

and dust that periodically come into the center of the solar system from

its <a href="/comets/Oort_cloud.html">outer

reaches</a>.

Some comets make <a href="/comets/perihelion_pass.html">repeated

trips</a> to the inner

solar system. When comets get close enough to the Sun, heat

makes them start to <a href="/comets/sublimation.html">evaporate</a>.

Jets of gas and dust form long

<a href="/comets/tail.html">tails</a> that we can see from

Earth. 

This photograph shows <a href="/comets/comets_table.html">Comet

Kohoutek</a>,

which visited the inner solar system in 1973.  It has an

<a href="/physical_science/physics/mechanics/orbit/orbit_shape_interactive.html">orbit</a> of

about 75,000 years!<p><small><em>Image courtesy of NASA</em></small></p><a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>Lunar eclipses are special events that only occur when certain conditions are met. First of all, the Moon must be in <a href="/the_universe/uts/moon3.html">full phase</a>. Secondly, the <a href="/sun/sun.html">Sun</a>, <a href="/earth/earth.html">Earth</a> and <a href="/earth/moons_and_rings.html">Moon</a> must be in a perfectly straight line. If both of these are met, then the Earth's shadow can block the Sun's light from hitting the Moon.  The reddish glow of the Moon is caused by light from the Earth's limb scattering toward the Moon, which is reflected back to us from the Moon's surface.<p><small><em>Image credit - Doug Murray, Palm Beach Gardens, Florida</em></small></p>
Comets are lumps of ice and dust that periodically come into the center of the solar system from its outer reaches. Some comets make repeated trips to the inner solar system. When comets get close enough to the Sun, heat makes them start to evaporate. Jets of gas and dust form long tails that we can see from Earth. This photograph shows Comet Kohoutek, which visited the inner solar system in 1973. 



Lunar eclipses are special events that only occur when certain conditions are met. First of all, the Moon must be in <a href="/the_universe/uts/moon3.html">full phase</a>. Secondly, the <a href="/sun/sun.html">Sun</a>, <a href="/earth/earth.html">Earth</a> and <a href="/earth/moons_and_rings.html">Moon</a> must be in a perfectly straight line. If both of these are met, then the Earth's shadow can block the Sun's light from hitting the Moon.  The reddish glow of the Moon is caused by light from the Earth's limb scattering toward the Moon, which is reflected back to us from the Moon's surface.<p><small><em>Image credit - Doug Murray, Palm Beach Gardens, Florida</em></small></p> Lutetia is a medium-sized asteroid. It orbits the Sun in the main asteroid belt between the planets Mars and Jupiter. This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe Rosetta flew past Lutetia in July 2010, and gave us our first good look at the asteroid.
 <a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>

<a href="/asteroids/asteroid_lutetia.html">Lutetia</a> is a medium-sized <a href="/our_solar_system/asteroids.html">asteroid</a>. It orbits the <a href="/sun/sun.html">Sun</a> in the main asteroid belt between the planets <a href="/mars/mars.html">Mars</a> and <a href="/jupiter/jupiter.html">Jupiter</a>.  This lumpy object is about 96 km (60 miles) in diameter. It isn't a perfect sphere, though. Lutetia is 132 km (82 miles) across one way, but only about 76 km (47 miles) long in another direction. The European space probe <a href="/space_missions/robotic/rosetta_flyby_asteroid_lutetia_july_2010.html">Rosetta flew past Lutetia</a> in July 2010, and gave us our first good look at the asteroid.<p><small><em>Image courtesy of ESA 2010 MPS for OSIRIS Team MPS/UPD/LAM/IAA/RSSD/INTA/UPM/DASP/IDA.</em></small></p>

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