The
Neptune is eighth planet from our sun. The Neptune is farthest known planet.
Neptune is fourth largest planet in our solar system. Neptune is denser than
the Uranus. But Neptune is smaller in physical size. The mass of the Neptune is
more than its nearest planet Uranus. The Neptune requires 165 Earth years to
complete one orbit around the sun. The planet Neptune is discovered by
mathematical prediction. We cannot see Neptune by unaided eye. According to
Roman mythology, Neptune is the god of the ocean and in Greek mythology, the
planet Neptune is identified by the Greek god Poseidon.
The Neptune Planet |
The colour of the planet Neptune is
bluish. The colour of Neptune is influenced by the presence of the methane in
its atmosphere. The distance between our sun and the Neptune is about 2.8
billion miles or 4.5 billion km. The diameter of Neptune is of about 49,530 km
or 30,775 miles approximately. As like the Uranus, the Neptune is also an ice
giant. As the Neptune is farthest known planet, the temperature of the Neptune
is of -214 degree Celsius. But the Neptune is not as cold as the Uranus. The
Uranus is coldest planet in our solar system.
The Farthest planet Neptune |
The Neptune required 16 hours to
complete on rotation about its axis of rotation. That means the day on the
Neptune is just 16 hours. The rotation of the Neptune about its axis is
different from all other planets in our solar system. The polar region of
Neptune rotates 4 hours faster than the equator region. As like the Saturn,
Jupiter and Uranus, the Neptune also has a ring around it. Neptune has five
rings, Galle, Leverrier, Lassell, Arago and Adams. The planet Neptune has 14
known moons orbiting around it. The Triton moon is the largest moon of Neptune.
Inner
Composition of Neptune
The
Neptune has 4 layers, firstly the outermost atmosphere. This layer is the part
of the atmosphere. This consists of the clouds of gases. The second layer is
the atmosphere. This atmosphere consists of hydrogen, helium and methane in
gaseous form. The hydrogen is 80%, helium is 19% and rest percentage is of methane.
Both atmospheric layers are the 10% of the planet’s mass. Beneath the
atmosphere the mantle starts. The mantle of Neptune is 15 Earth masses. The
mantle is dense fluid. The mantle is rich is water, ammonia and methane. This
mixture is referred to as icy but it is hot dense fluid. So, this is also known
as “Water-ammonia ocean”. Now the last is the core of Neptune, the scientists
theoretically assumed that the core may be made up of rock and metal. The core
is assumed to be made up of silicate, iron and other metals. The temperature of
core is of about 70000C approximately. The huge difference between
the core temperature and the temperature of surface cause the huge wind storms.
The speed of storm reaches up to 2100 km per hours. This speed is the fastest
storm speed in our solar system. Due to pressure methane condensed at the upper
level. The Neptune has fastest moving wind storm in solar system 1500 miles per
hour approximately. The storm may remain for long period of time. As like
Jupiter, the Neptune has its grate dark spot. The temperature of Neptune is 200
degree Celsius. But its south pole region Temperature is 10 degree Celsius. So,
this causes the strongest and fastest wind storm in our entire solar system.
The Inner Composition of the Neptune |
When south pole exposed to sun approximately 40 Earth years. The temperature reaches to 10 degree Celsius. So, the methane which is frozen at the rest of the planet. But at south pole, methane escape into stratosphere. And when north pole exposed to sun approximately 40 Earth years. The temperature reaches to 10 degree Celsius. So, the methane which is frozen at the rest of the planet. But at north pole, methane escape into stratosphere.
Magnetic
field of the Neptune
The
Magnetic field of the Neptune is tilted 470 from the rotational
axis. Distance between magnetic pole and the geographical pole is approximately
13,500 km. The magnetic field of Neptune is represented approximately by the
dipole similar to the bar magnet. But the polarity is essentially reverse as
compared with the Earth’s magnetic field. The magnetic field of the Neptune is
not generated from the core. The Neptune’s magnetic field having offset of 56%
of the radius. The magnetic field is actually closer to the cloud top. The
magnetic field may be generated in the processes occurring in the upper layers
of the planetary interiors. The magnetosphere is nothing but the region of
space dominated by the magnetic field of the Neptune. The charged particles
electrons and protons trapped in the magnetosphere are repeatedly swept past
the orbits of the moons and rings. The most of the particles are absorbed by
the moons and the rings of the Neptune. The moons and the ring material almost
emptying the magnetosphere. So that, there are very few percentages of charged
particles in magnetosphere. As the magnetic field of the Neptune is generated
outward to the central core. The magnetic field lines can travel along into the
atmosphere. So, they collide with gases there, results to those gases to fluoresce.
This appears as the auroras.
Orbit of the
Neptune around the sun
The
Neptune requires 16 hours to complete one rotation around its axis. The axis of
rotation of the Neptune is tilted 280 with respect to plane of its
orbit around sun. This tilt is similar to the Earth’s tilt. So, this means the
Neptune also experiences the seasons. But its orbit is long each of 4 seasons
last for over 40 years. The Neptune requires 165 Earth years to complete one
orbit around the sun. the aphelion is 4.54 billion kilometers approximately and
perihelion is 4.46 billion kilometers approximately. The planet Neptune’s
rotation around its axis is very different than that of other planets. The
equatorial zone requires about 18 hours to complete one rotation and the polar
region requires about 12 hours to complete one rotation around its axis. The
one interesting thing about the Neptune planet is, after every 250 years
approximately pluto comes closer to the sun that means pluto moves inside the
orbit of the Neptune and it is for 20 years.
Orbit of the Neptune. |
Rings of the
Neptune
The
all outer planets in our solar system has a ring around them. The ice giant and
the last planet in our solar system has a ring. The Neptune has five rings. The
rings are Galle, Le Verrier, Lassell, Arago and Adams. The names of the rings
are given after the scientists who made important discovery related with the
planet Neptune.
The
rings are composed with dust and small rocks. The rings are consisting of at
least 20% to maximum 70% dust. And the rest material is small rocks. The rings
of the Neptune are very difficult to see. The rings are dark and the density of
it varies and size also. The study suggested that the Neptune’s rings are young
ass compared with the planet. The rings may be formed when one of the moons of
the Neptune was destroyed.
The rings of the Neptune. |
The
ring Galle named after the scientist Johann Gottfried Galle. The Johann Galle
is the first person who see planet Neptune using telescope. The Galle ring
starts from 41,000 km and ends at 43,000 km from the Neptune. The next ring is
La Verrier ring. The La Verrier ring is named after the scientist who predicted
the position of the planet Neptune. The La Verrier ring is very narrow. The
width of this ring is approximately 110 km. The next ring is Lassell ring. The
Lassell ring is the widest ring among all other rings of the Neptune. The name
of the ring is given after the scientist William Lassell. The Lassell ring
starts from 53,210 km and ended at 57,210 km from the Neptune. The width of
Lassell ring is approximately 4000 km, widest ring of the Neptune. The next
ring is Arago ring. The name of the ring is given after the Francois Arago
scientist. The ring Arago starts from approximately 57,199 km and ended at
57,300 km from the Neptune. The width of Arago ring is nearly 100 km. The
outermost ring is Adams ring. The name of the ring is given after the scientist
John couch Adams. The width of the ring is nearly 35 km. The Adams ring is
slightly inclined. The most interesting thing about the Adams ring are arc.
There are five arcs exists on the ring. The Arcs are the brightest parts of the
rings. The names are Fraternite, Egalite 1, Egalite 2, Liberte and Courage. The
Fraternite arc is the brightest among all the arcs of the Neptune. And the arc
Courage is the faintest arc of the Neptune. The scientist can not find out that
how these arcs are formed because according to law of motion, the ring material
must be distributed uniformly around the Neptune.
The Moons of
the Neptune
The
outer planets of our solar system have numerous moons orbiting around them. The
Neptune has 14 known moons orbiting around it. The ice giants Uranus and
Neptune both are quite similar in terms of composition and structure. But their
systems of moons are very different from each other. The scientists think that
the most of the moons of the Neptune are not their original moons. The original
moons mean, the moons are formed with the Neptune. The largest moon of the
Neptune is Triton. The Triton is one of the moons which is captured by the
Neptune’s gravity.
The Triton
moon of the Neptune
The Triton moon is largest moon of
the Neptune. The Triton is seventh largest moon in our solar system. The Triton
is larger than the dwarf planets Pluto and Eris. The unusual thing about the
Triton is the only large moon that orbits in opposite direction of its planet’s
rotation. The Triton is tidally locked with the Neptune. Tidally locked means
the one side of the moon always faces towards the planet. The Triton requires
5.88 Earth days to complete one orbit around the Neptune. The average orbital
speed of Triton is nearly 4.40 kilometer per second.
The Triton, largest moon of the Neptune. |
The
surface of Triton has nitrogen. But the nitrogen is in frozen state. The crust
of the Triton is mostly made up of the water-ice. The mantle is made up of
frozen ice. The core of the Triton is made up of the rocky material and some
metals. The atmosphere of the Triton consists of tenuous nitrogen, trace amount
of carbon monoxide. And very small amount of methane which is near the surface
of the Triton. The nitrogen is evaporating from the surface of the Triton.
The Proteus
moon of the Neptune
The moon Proteus is one of the largest moons of the Neptune. But Proteus is not as big as the Triton. The Proteus is second largest moon of the Neptune and it is one of the inner moon of the Neptune. The moon Proteus is not a perfect sphere. It has an odd box like shape. The moon is named after the Greek god who changing the shapes.
The second largest moon Proteus of the Neptune. |
The Proteus requires 27 hours to complete one orbit around the Neptune. The average orbital speed of the Proteus is approximately 7.6 km/s. The distance between the Proteus and the Neptune is nearly 117,650 km or 73,102 miles. The Proteus is tidally locked with the Neptune. This mean that the one face of the moon always faces towards the Neptune. The Proteus is irregularly shaped and surface is heavily cratered. The Proteus is one of the darkest objects in our solar system. Because Proteus reflects only six percent of the sunlight.
The Nereid
moon of the Neptune
The
Nereid moon is one of the largest moons of the Neptune. The Nereid is third
largest moon of all known moons. The Nereid moon requires approximately 360
Earth days to complete one orbit around the Neptune. The surface of the Nereid
consists of various types of ices and silicates. As like the Triton, the Nereid
moon is also a captured object of the Neptune. That means the Nereid moon is
not the original moon of the Neptune. The Nereid moon is one of the outermost
known moons of the Neptune. The moon Nereid detected the water ice on the
surface.
The Nereid moon of the Neptune. |
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