Trans-Neptunian Objects

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Trans-Neptunian Objects

NASA diagram shows the presumed distance of the Oort Cloud compared to the Solar System planets, the Kuiper Belt, and the orbit of Sedna.

Trans-Neptunian Objects are objects having semi-major axes larger than that of the planet Neptune.^[1]

1 Naming conventions
2 Primary theoretical considerations
- 2.1 As sources of comets
- 2.2 Origins
3 Classes of trans-Neptunian objects
4 Discovery and observation
5 References
6 Related Links

Naming conventions[edit]

A significant number of astronomers today insist that all trans-Neptunian objects, regardless of whether Neptune has any gravitational influence upon them, should be called Kuiper belt objects.^[2]^[3] But today, an increasing number of astronomers distinguish the Kuiper belt from other trans-Neptunian regions, primarily using orbital characteristics as the criterion for this distinction.^[4]

Primary theoretical considerations[edit]

As sources of comets[edit]

Since 1951, when Gerard P. Kuiper published his original hypothesis concerning non-accreted icy remnants of the solar nebula, trans-Neptunian objects, by whatever name, have been held to be the source of comets, of periods long or short.

Origins[edit]

Conventional theory supposes all these objects (except for the hypothetical Nemesis) to be remnants of the formation of the solar system that could not accrete into planets. Most of these objects, except for the most distant objects in the scattered disk, moved into their present orbits under the gravitational influence of Neptune. So says conventional theory.

False-color image of Pluto showing frozen lake of carbon monoxide (green) in the western lobe of Tombaugh Regio (the "heart shape").

The Hydroplate Theory suggests these objects are the heaviest component of a vast quantity of water, rock and mud – amounting to as much as four percent of the original mass of the Earth – that escaped from Earth during the Great Flood. These objects formed near the Earth. Then, under the influence of the Sun, they out-gassed vast amounts of water vapor (and perhaps of thermolyzed hydrogen and/or oxygen also) and thus propelled themselves into ever-higher orbits. Most of these objects likely passed close to Jupiter (largest of the gas giants) and got a slingshot-like gravity boost to the orbits they now travel in.

Pluto, the "king of the Kuiper Belt," typifies the lot. Its greatly eccentric and significantly inclined orbit carries it inside the orbit of Neptune at its closest approach to the Sun (perihelion). In 2015, the rocket probe New Horizons passed through the Plutonian system and photographed Pluto and its moons extensively. Among other findings: a lake of frozen carbon monoxide in the western "lobe" of "Tombaugh's Heart," a great heart-shaped contiguous plain. How did this carbon monoxide form? It could only have formed from the burning of wood in a confined space. Walter T. Brown, Jr., originator of the Hydroplate Theory, suggests much of the mass of Pluto originally consisted of uprooted trees and shrubs. The heat of accretion, and the presence of hydrolyzed hydrogen and oxygen, started a fire beneath the surface. The confined space produced carbon monoxide, not carbon dioxide. Eventually this carbon monoxide broke through to the surface, condensed, fell as rain onto Tombaugh's Heart, then froze.

NASA has the photograph of Pluto showing the frozen carbon monoxide lake. But to date they have never even tried to explain it.

In addition to this latest finding, the arguments of perihelion of the twelve largest trans-Neptunian objects, including Pluto, are nearly identical. Megan Schwamb, the astronomer who noticed this remarkable confluence of findings, flatly rejected mere coincidence in a conversation she had with Brown. She said any theory of the origin of trans-Neptunian objects must explain this tight grouping of arguments of perihelion.

Classes of trans-Neptunian objects[edit]

Trans-Neptunian objects today belong to four major classes (not counting the Centaurs, an entirely different class of object):

The Kuiper belt, containing those objects that remain between 30 and 50 AU distant from the Sun^[4]
The scattered disk, containing objects having perihelia of 30 AU or greater and semi-major axes of 50 AU or greater.^[4]
The Oort Cloud, the hypothetical and probably factitious sphere of icy objects held to be the source of long-period comets^[4]
Nemesis, the hypothetical and probably factitious red or brown dwarf star that is supposed to enter the Oort cloud and perturb it once every 26 million years.

Discovery and observation[edit]

The first-ever trans-Neptunian object to be discovered was the dwarf planet Pluto in 1930. The next was Pluto's largest satellite Charon in 1978.^[5] After the discovery of object 1992 QB1, astronomers have discovered more than 800 of these objects, but not nearly as many as some astronomers have predicted. Other notable TNO's that have been discovered include:

(15874) 1996 TL66, the first scattered disk object to be recognized
(48639) 1995 TL8, the earliest discovered scattered disc object, and a binary
1993 RO, the next plutino discovered after Pluto^[6]

The New Horizons rocket probe, passed through the Plutonian system in June 2015. It thus became the first rocket probe to study a Trans-Neptunian object. Mission planners hope to steer the probe to study at least two other Kuiper belt objects in addition to Pluto.

References[edit]

↑ "Space Topics: Trans-Neptunian Objects." The Planetary Society, n.d. Accessed June 24, 2008.
↑ Jewitt, David. "Kuiper Belt." University of Hawaii, n.d. Accessed June 20, 2008.
↑ Johnston, William Robert. "Trans-Neptunian Objects." October 1, 2007. Accessed June 24, 2008.
↑ ^4.0 ^4.1 ^4.2 ^4.3 "Types of Trans-Neptunian Objects." The Planetary Society, n.d. Accessed June 24, 2008.
↑ Whitman, Justine. "Pluto and the Kuiper Belt." <Aerospaceweb.org>, Apriil 16, 2006. Accessed June 24, 2008.
↑ http://www.answers.com/topic/trans-neptunian-object