The Kuiper Belt and the Oort Cloud are two regions in space that encircle our solar system. The Kuiper Belt contains thousands of asteroids that orbit the Sun outside Neptune's orbit hence their name as Trans-Neptunian Objects. Although asteroids and rocks are more associated with the Kuiper Belt, some short-distance comets are thought to exist come from there. The most famous comet of them all, Halley's Comet Aphelion is past Neptune at which point it then turns back and heads towards the Sun.
The Oort Cloud on the other hand has not been proven to definitely exist as yet unlike the Belt. The Oort Cloud is mainly believed to contain comets rather than asteroids. To give some idea of where everything is, have a look at the picture below.
The Kuiper Belt is similar to the Asteroid Belt that mainly straddles the area between the planets of Mars and Jupiter. The Kuiper Belt spreads out much further than the Asteroid belt. The objects in the Kuiper Belt are normally referred to as Trans-Neptunian Objects because they orbit outside the orbit of Neptune. The composition of the objects in the asteroid belt and the kuiper belt are different. The asteroid belt, the asteroids are made of rock and metal where as the objects in the Kuiper Belt are frozen material such as methane, ammonia and water. Ref: Wiki
The image is courtesy of Nova Celestia which has free use image policy.
The above picture illustrates the location of the Kuiper Belt in the Solar System.
In an area just beyond Neptune lies the Kuiper Belt, an area that contains thousands of asteroids. It is named after Gerard Peter Kuiper, a Dutch Born American Astronomer ( Dec 7, 1905 - Dec 23, 1973) who suggested the existence of the Belt. His theory was not confirmed until August 30, 1992 with the discovery of 1992 QB1 object.
It has never been given any other name apart from its original designation. The discoverers wanted to call it Smiley but as there was already an object out there with that name, they declined to give it another name. The object was discovered by David Jewitt and Jane Luu who had been searching space since 1987 on and off and finally with the help of the University of Hawaii's 2.2m telescope they found what they were looking for. The object was further out than Pluto.Ref: N.A.S.A.
Kuiper Belt Objects are also known as Trans-Neptunian Object as they orbit the orbit further out than Neptune. Its existence had first been put forward by Irish Astronomer Kenneth Edgeworth but he's received little or no recognition of this. ref:Britannica
The most important difference between the top is that the Kuiper Belt is known to exist. The Oort Cloud is a theory that has not yet been proved or disproved. The Kuiper Belt consists of asteroids and dwarf planets whilst the Oort Cloud will also include comets before they are sent on their way towards the inner reaches of the Solar System.
There is no clear distinction between where the Kuiper Belt ends and where the Oort Cloud begins. The current locations of both are, the Kuiper Belt is just outside Neptune, between 30 A.U. and 50 A.U. the distance between the Earth and the Sun and the Oort Cloud is about a light year away. One A.U. is the distance between the Sun and the Earth. The distance is not an arbitrary figure as some orbit inside that amount, other orbit outside that amount but its where the vast bulk of the asteroids are. The objects of the Oort Cloud are small, our telescopes are far too small for us to see any. Amazing Space
Pluto and Sedna aren't the only interesting objects in the Kuiper Belt. Haumea, a fast spinning egg-shaped object. It is believed that it was sent spinning as the result of a collision in the early days. It spins end over end every four hours. The object has two moons Hi'iaka and Namaka. Ref: N.A.S.A.
Sedna was at one time referred to as The Solar Systems tenth planet. However since then, its claim to that stature has diminished. It is three times the distance from the Sun as Pluto and people are questioning as to whether it is part of the Kuiper Belt or not.
There has been a debate as to what constitutes a planet, some saying Sedna is a planet and some saying that Pluto should no longer have that stature. The International Astronomer Union, the internationally recognised authority on all things with space tried to create a set of rules to determine what a planet is. The description proved controversial and it resulted in Pluto being downgrading as a planet to a dwarf planet in 2006. Ref: I.A.U.
Given Sedna's location being so far from the Sun but not nearly as far as where the Oort Cloud is supposed to be, astronomers are wondering if there is another belt, an 'Inner Oort Cloud'. Sedna is about 8 billion miles away from the Sun. Ref: Caltech. To put Sedna in to prospective, Pluto is about 3.67 billion miles away. Ref: Caltech
Pluto was the first Kuiper Belt Object discovered but was classed as a planet because other Kuiper Belt Objects had not yet been discovered. Pluto was downgraded when the KBO Eris was discovered and that it was believed that Eris was bigger than Pluto. Eris was originally called Xena and its moon called Gabrielle but was changed so that it was in line with naming other planetoids, that is being named after ancient gods. Eris has now been calculated to be 2,326 kilometers in diameter and Pluto is 2,300 kilometers Ref: Planetary . In terms of size, the two objects are not much different but it was the fact that Sedna was believed to be bigger that helped downgrade Pluto.
If you have a powerful telescope and want to know where to look, the following picture will give you an idea where to point the lense. The time given is in Pacific Standard Time, you will need to adjust depending on where in the world you are.
The hunt for the new ninth planet after Pluto was downgraded is in full swing. It has been noted that some kuiper belt asteroids are travelling differently to how they are supposed to be. The fact that they are is possibly down to a large planet on the outskirts of our solar system. Its orbit take it out to the far depths of outer space which is why its not been seen. The diagram released by artists at Caltech and NASA show the likely path that the planet takes around the Sun.
N.A.S.A. has taken to using the might of the internet and is calling on amateur astronomers to help through the Backyard Worlds project. The task involves going through thousands of photos and looking for any changes that might indicate a planet or something. It is exactly how Clyde Tombaugh discovered Pluto.
In 2006, it was revealed that two stars HD 53143 and HD 139664 were discovered to have their own versions of the Kuiper Belt. Both stars are relatively close to us, a mere 59.77 and 57.87 light years away from us respectively. Ref: universe Today
In addition to having an extrasolar planet (exoplanet), the star that we know as Fomalhaut in the southern hemisphere is reckoned to have a its own kuiper belt. Fomalhaut's Kuiper Belt is a little further out from its star than ours.
Our Kuiper belt is 50 A.U. from the Sun, in plain English, that means it is fifty times the distance between Earth and the Sun. Fomalhaut's kuiper belt is 133-158 times the distance from its Sun. It is well know that Fomalhaut has one planet but this discovery increases the chances that the star has multiple planets in orbit. ref:Sky and Telescope
Now that New Horizons space probe primary mission was to Pluto has been achieved, the space probe's life isn't over yet. New Horizons has been given a new target to head towards, the new target is 2014 MU69 which it is expected to fly by on 1st Jan 2019 so no celebrating the night before for the ground crew. Ref: N.A.S.A
In recognition of the visit, MU69 was renamed Ultima Thule by the I.A.U. It had been speculated that the object might actually be two objects but when photographs arrived of the object(s), it was only one. The object resembled a snowman, two objects merged into one probably as a result of a collision where they then became joined.
There are a number of different types of objects in the Kuiper Belt, a Plutino is an asteroid that for every two orbits that Neptune makes, the Plutino makes three. It doesn't specify any physical features on the object, just its path round the Sun however distant. Ref: Plutino
Whilst the Asteroid Belt and the Kuiper Belt both contain asteroids, the difference is the location. Both contain large rock objects. The Asteroid Belt is mainly between Mars and Jupiter where all the Kuiper Belt Asteroids are outside the orbit of Neptune. They asteroids are similar, probably the same composition, its just the location that determines whether it is an Astroid or a Trans-Neptunian Object.
|2002 AW197||Palomar||10th January 2002|
|2002 TC203||Palomar||9th October 2002|
|Albion||D. C. Jewitt, J. X. Luu||1992-08-30|
|Altjira||Deep Ecliptic Survey||2001-10-20|
|Arawn||M. J. Irwin, A. Zytkow||1994-05-12|
|Borasisi||C. A. Trujillo, J. X. Luu, D. C. Jewitt||1999-09-08|
|Chaos||Deep Ecliptic Survey||1998-11-19||Kuiper Belt|
|Deucalion||Deep Ecliptic Survey||18 April 1999||Trans-Neptunian|
|Eris||M. E. Brown, C. A. Trujillo and D. Rabinowitz||21st October 2003||Trans-Neptunian|
|Huya||I. R. Ferrin||2000-03-10||Trans-Neptunian|
|Ixion||Deep Ecliptic Survey||2001-05-22||Plutino|
|Lempo||E. P. Rubenstein, L.-G. Strolger||1999-10-01|
|MakeMake||M. E. Brown, C. A. Trujillo, D. L. Rabinowitz||2005-03-31||Trans-Neptunian|
|Manwe||M. W. Buie||2003-08-25|
|Mors-Somnus||S. S. Sheppard, C. Trujillo||2007-10-14|
|Orcus||M.Brown, C. Trujillo, D. Rabonowitz||17 February 2004||Plutino|
|Pluto||C. W. Tombaugh||1930-01-23|
|Praamzius||K. Cernis, R. P. Boyle||2012-01-23|
|Quaoar||C. A. Trujillo, M. E. Brown||2002-06-04||Kuiper Belt|
|Rhadamanthus||Deep Ecliptic Survey||1999-04-17||Trans-Neptunian|
|Salacia||H. G. Roe, M. E. Brown, K. M. Barkume||2004-09-22|
|Sedna||M.Brown, C. Trujillo, D. Rabonowitz||14 November 2003||Trans-Neptunian|
|Sila-Nunam||J. X. Luu, D. C. Jewitt, C. A. Trujillo, J. Chen||1997-02-03|
|Teharonhiawako||Deep Ecliptic Survey||2001-08-20|
|Ultima Thule||Hubble Space Telescope|
|Varda||J. A. Larsen||2003-06-21|
|Varuna||R. McMilan||28 November 2000||Kuiper Belt|
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