Neptune Voyager reached Neptune on 26 August 1989. Its final targets were Neptune and its collection of moons. The largest of them, Triton, had long been expected to be one of the most extraordinary places in the solar system. Members of NASA imaging team were delighted but baffled. Triton and Neptune turned out to be active and violent worlds.  Now they had to work out why.

SURFACE AND ATMOSPHERE OF NEPTUNE

Neptune is chiefly made of helium, hydrogen, water and silicates. The clouds of hydrogen, helium, and water cover Neptune's surface.Streaks of clouds on NeptuneThe interior of the planet begins with a region of heavily compressed gases. Deep in the interior, these gases blend into a liquid layer that surrounds the planet's central core of rock and ice. The tilt of Neptune's axis causes the sun to heat the planet's northern and southern hemispheres resulting in seasons and temperature changes. Neptune is surrounded by thick layers of clouds in rapid motion. Winds blow these clouds at speed up to 1,100 kilometres per hour. The clouds farthest from Neptune's surface consist mainly of methane. Neptune's dark clouds, which lie below the clouds of methane are composed of hydrogen sulphide.

THE DARK SPOT OF NEPTUNE

The Great Dark Spot of NeptuneThe Dark Spot of NeptuneA dark region about the size of the earth called the Great Dark Spot, consist of violently swirling masses of gas that resemble a hurricane. The high winds and the shape of the Great Dark Spot are similar to those of the Great Red Spot on Jupiter.

THE RINGS OF NEPTUNE

Voyager 2 discovered rings round Neptune. Rings of Neptune Observations from the earth had shown that Neptune, insteadParting look at Neptune from Voyager of having completed rings, has ring arcs - fragments of rings. But Neptune turned out to have complete rings after all. They are so faint that they would be invisible even to the person who was actually there. In addition to the rings, there is a faint layer of dust stretching from near the surface of Neptune to the two bright outer rings.The rings of Neptune are made of billions ofTwisted rings of Neptune independently orbiting moonlets varying from boulders to single atoms like a chain of endless train cars. For some reason the moonlets appear to have bunched together. That is why we see the arcs. All the moons of the giant planets confine the rings and prevent them from getting away into space. But no such relation was discovered between Neptune and its moons. By looking back towards the sun,  Voyager captured light being scattered by Neptune's tenuous charcoal-dark rings. Ring movements smeared another image of one of the arcs showing that they hold knots of accumulated particles.

Moons of NeptuneNeptune Statistics

Graphics, photographs and statistical data used by the courtesy of NASA and National Geographic Magazine
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