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Research Paper Writing Planet

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Essay on Science Research Papers

Essay/Term paper: Neptune Essay, term paper, research paper: Science Research Papers

Free essays available online are good but they will not follow the guidelines of your particular writing assignment. If you need a custom term paper on Science Research Papers: Neptune. you can hire a professional writer here to write you a high quality authentic essay. While free essays can be traced by Turnitin (plagiarism detection program), our custom written essays will pass any plagiarism test. Our writing service will save you time and grade.

Neptune is the outermost planet of the gas giants. It has an equatorial
diameter of 49,500 kilometers (30,760 miles) and is the eighth planet from the
sun. If Neptune were hollow, it could contain nearly 60 Earth's. Neptune
orbits the Sun every 165 years. It has eight moons, six of which were found by
Voyager 2. A day on Neptune is 16 hours and 6.7 minutes. Neptune was
discovered on September 23, 1846 by Johann Gottfried Galle, of the Berlin
Observatory. Neptune got its named from the Roman God of the Sea. Much of what
is know today about Neptune was discovered in 1989 by the U.S Voyager 2
spacecraft during its 1989 flyby f Neptune. Neptune as compared to Earth is 3.9
times the diameter, 30 times the distance from the sun, 17 times as massive, and
0.3 times the density. Neptune travels around the Sun in an elliptical orbit at
an average distance of 4.504 billion km (2.799 billion miles). Neptune consists
largely of hydrogen and helium, and it has no apparent solid surface. The first
two thirds of Neptune is composed of a mixture of molten rock, water, liquid
ammonia and methane. The outer third is a mixture of heated gases comprised of
hydrogen, helium, water and methane. The atmospheric composition is 85%
Hydrogen, 13% Helium, and 2% methane. The planet's atmosphere, particularly
the outer layers, contains substantial amounts of methane gas. Absorption of
red light by the atmospheric methane is responsible for Neptune's deep blue
color. Neptune is a dynamic planet with several large, dark spots reminiscent of
Jupiter's hurricane-like storms. The largest spot, known as the Great Dark Spot,
is about the size of the earth and is similar to the Great Red Spot on Jupiter.
Neptune receives less than half as much sunlight as Uranus, but heat escaping
from its interior makes Neptune slightly warmer than Uranus. The heat liberated
may also be responsible for Neptune's stormier atmosphere, which exhibits the
fastest winds seen on any planet in the solar system. Most of the winds there
blow westward, opposite to the rotation of the planet. Near the Great Dark Spot,
winds blow up to 2,000 kilometers (1,200 miles) an hour. Voyager 2 found that
the winds averaged about 300 meters per second (700 miles/hour) in the planet's

Long bright clouds, similar to cirrus clouds on Earth, were seen high in
Neptune's atmosphere. At low northern latitudes, Voyager captured images of
cloud streaks casting their shadows on cloud decks below.

Feathery white clouds fill the boundary between the dark and light blue regions
on the Great Dark Spot. The pinwheel shape of both the dark boundary and the
white cirrus suggests that the storm system rotates counterclockwise. Periodic
small scale patterns in the white cloud, possibly waves, are short lived and do
not persist from one Neptunian rotation to the next. (Courtesy NASA/JPL)

Until the Voyager 2 encounter in 1989, the rings surrounding Neptune were
thought to be arcs. We now know that the rings completely circle the planet, but
the thickness of each ring varies along its length. Neptune has a set of four
rings which are narrow and very faint. The rings are made up of dust particles
thought to have been made by tiny meteorites smashing into Neptune's moons.
From ground based telescopes the rings appear to be arcs but from Voyager 2 the
arcs turned out to be bright spots or clumps in the ring system. The exact
cause of the bright clumps is unknown. The magnetic field of Neptune, like that
of Uranus, is highly tilted at 47 degrees from the rotation axis and offset at
least 13,500 kilometers or 8,500 miles from the physical center. Comparing the
magnetic fields of the two planets, scientists think the extreme orientation may
be characteristic of flows in the interior of the planet and not the result of
that planet's sideways orientation or of any possible field reversals within the
planet. Neptune also has eight known satellites. Only two of these, Triton and
Nereid, had been observed prior to the Voyager 2 flyby. Triton is the largest
of the eight satellites and is almost as big as the Earth's Moon. The other
Neptunian satellites range in diameter from 58 to 416 km (36 to 258 miles).
Apart from Triton, the moons of Neptune are irregularly shaped and have very
dark surfaces.

Triton is the largest moon of Neptune, with a diameter of 2,700 kilometers
(1,680 miles). It was discovered by William Lassell, a British astronomer, in
1846 scarcely a month after Neptune was discovered. Triton is colder than any
other measured object in the Solar System with a surface temperature of -235�° C
(-391�° F). It has an extremely thin atmosphere. Nitrogen ice particles might
form thin clouds a few kilometers above the surface. The atmospheric pressure at
Triton's surface is about 14 microbars, 1/70,000th the surface pressure on Earth.
Triton is the only large satellite in the solar system to circle a planet in a
retrograde direction -- in a direction opposite to the rotation of the planet.
It also has a density of about 2.066 grams per cubic centimeter (the density of
water is 1.0 gram per cubic centimeter). This means Triton contains more rock
in its interior than the icy satellites of Saturn and Uranus do. The relatively
high density and the retrograde orbit has led some scientists to suggest that
Triton may have been captured by Neptune as it traveled through space several
billion years ago. If that is the case, tidal heating could have melted Triton
in its originally eccentric orbit, and the satellite might even have been liquid
for as long as one billion years after its capture by Neptune. Triton is scarred
by enormous cracks. Voyager 2 images showed active geyser-like eruptions spewing
nitrogen gas and dark dust particles several kilometers into the atmosphere.

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Planet research paper outline - Writing Custom Research Papers Quickly and Hassle-Free

Planet research paper outline

Caspar 28/06/2015 19:11:09

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Solar System Research Paper

Solar System Research Paper

Solar system is defined as the gravitational system of the Sun. The solar system includes the sun, orbiting by planets and their natural satellites, the dwarf planets and other small bodies such as comets, asteroids, and meteoroids, and the total of all gas and dust particles attracted and held together by the sun gravitational field. The Solar System also includes the Earth.

Those who are about to write their research paper on Solar system it is important to know that the central star of the solar system is the sun.

It is followed by the terrestrial planets:

which make up the inner part of the planetary system. The outer part consist of the gas planets:

In addition to dwarf planets, there are millions of asteroids (also called planetoids or minor planets) and comets, which are primarily found in three small areas of the solar system: the asteroid belt between the inner and the outer planets, the Kuiper Belt beyond the outer planets, and the Oort Cloud on the very outside.

Within the area dominated by the individual planets, there often are smaller celestial body orbiting companions. After the well-known moon of the earth, they are also analogous as moons, as well as called a satellite or satellites. Down to the Earth’s Moon and Pluto moon Charon, they are much smaller than their main body at least for the planets and dwarf planets in general. Moonless exceptions among the planets are Mercury and Venus. A definitely lower limit size, from the one as with the constituents of the rings no longer speaks of a moon of the gas giant planets, has not yet been officially defined.

The sun makes up 99.86 percent of the total mass of the system. Even its diameter is about 1.39 million kilometers far greater than the diameter of all other objects in the system. The largest of these objects are the eight planets, the four moons of Jupiter, Ganymede, Callisto, Europa and Io (the Galilean moons), Saturn’s moon Titan and the Earth’s moon.

Two-thirds of the remaining mass of 0.14 percent is accounted for by Jupiter.

As a result of the formation of the solar system all the planets, dwarf planets, and the asteroid belt move in a retrograde orbit around the sun. Most of the larger moons also movie in this direction to their main body. Also, the rotation of most major bodies of the solar system is in retrograde motion. Of the planets, only Venus rotates opposite, and the rotation axis of Uranus lies nearly in its orbital plane.

The sun next individual star is the red dwarf Proxima Centauri. Its distance to the solar system is about 4.22 light-years or 268,000 AE. The closest planetary system is Alpha Centauri at 4.34 light years (1.33 pc) distance, probably gravitationally bound to the Proxima Centauri.

Main components of Alpha Centauri are two sun-like stars one of which is orbited by a planetary companion, discovered in 2012.

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Research paper writing planet

Astronomy/ Planet X term paper 19747

Disclaimer: Free essays on Astronomy posted on this site were donated by anonymous users and are provided for informational use only. The free Astronomy research paper (Planet X essay ) presented on this page should not be viewed as a sample of our on-line writing service. If you need fresh and competent research / writing on Astronomy, use the professional writing service offered by our company.

Is Pluto really a planet? Researchers have been trying to determine whether Pluto is really big enough to be a planet. Over the last few years, the gathered information on Pluto and the discovery of an increasing number of other objects in the outer solar system have been discussed within a group of astronomers (called minor-planets). The planet Pluto is not given the respect of other planets and some have designation to be changed to ‘minor planet’. Astronomer Brian Marsden of Harvard Smithsonian Center said if Pluto were discovered seventy years ago, it would be considered a minor planet number. A minor planet is a term used to describe asteroids and most astronomers agree that Pluto is no asteroid.

Marsden said it’s not a demotion for Pluto to be referred to as the 10,000th minor planet, it is an honor.

Some astronomers do not agree with the Brian Marsden theory. Pluto deserves to be considered more than just a minor planet. Most astronomers would probably consider stripping Pluto of is status akin to stripping [the U.S. state of] Connecticut or Vermont of statehood because Texas and Alaska later joined. It was estimated that Pluto contained mass of eleven Earth but dropped rapidly over time. This is what is giving the astronomers a second opinion about being a planet.

Pluto is about 1,500 miles in diameter, larger than the largest asteroid. It is known to have density of two grams per cubic centimeter, so is estimated to be sixty percent rock and forty percent ices of frozen nitrogen, carbon monoxide, methane, and water. Pluto is tilted 122.5 degrees on its axis. Because of the shape of Pluto’s orbit, it actually slips inside of Neptune’s orbit once every 248 Earth years for a period of twenty years. Pluto, the planet farthest from the sun, is smaller than Earth’s moon. And while other ‘major planets’ have roughly circular orbits, Pluto carves out a sweeping ellipse that frequently takes it closer than Neptune to the sun. Pluto has one natural satellite, Charon, which is half the size of Pluto. Because Pluto and Charon are comparable is size, many scientists consider them to be a double plant, but many scientists don’t consider Pluto a planet at all. Studies conducted using a spectroscope have detected methane frost on Pluto and water frost on Charon. Like Triton, Neptune’s satellite, Pluto has an atmosphere of nitrogen and methane. Pluto’s atmosphere appears to extend out to include Charon, which suggests that they may share an atmosphere. Through the Hubble Space Telescope, Charon appears to be bluer in color than Pluto. During the time in its orbit when Pluto is farthest from the Sun, its atmosphere condenses and falls to the surface as frost.

Nicholson calls the Pluto debate a “’Tempest in a teapot’ with little effect on the course of solar-system research”. Nicholson also states no matter what we call it, people are not going to stop thinking about Pluto as a member of the Kuiper Belt. All the current discussions about the origin of Pluto starts premise that Pluto is a very big Kuiper Belt object. Transition Neptunian Objects is a new class A’Hearn wants to create for ice balls that orbit beyond Neptune and Pluto would be Transition Neptunian Object number 1. Does this mean Pluto has been demoted? The answer is no. Pluto will have dual classification as a planet and a Transition Neptunian Object, at least for the time being.

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