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Martin Kornmesser, IAU -- Larger illustration
The newly defined class of "dwarf planets" includes Ceres in the Main Asteroid Belt (between the orbits of Mars
and Jupiter) and Pluto and Eris (2003 UB 313) in the Edgeworth-Kuiper Belt (beyond the orbit of Neptune).
On September 17, 2008, the International Astronomical Union (IAU) announced that the trans-Neptunian object 2003 El61 had been designated a "dwarf planet and accepted the Polynesian names submitted by its discoverers for the primary body (Haumea) and its two moons, Hi'aka and Namaka, (press release).
On July 14, 2008, the IAU declared the outer Solar System object 2005 FY9 to be a dwarf planet and accepted the Polynesian name Make-make submitted by its discoverers.
On August 24, 2006, the International Astronomical Union voted at the end of its 26th General Assembly to establish definitions for three classes of substellar objects in the Solar System: planets, dwarf planets, and smaller Solar System bodies. These classes were defined as follows:
Planet - This is a celestial body that: (a) is in orbit around the Sun; (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a nearly round shape (due to a hydrostatic equilibrium); and (c) has cleared the neighborhood around its orbit. As now defined, the Solar System has eight planets: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.
Dwarf Planet - This is a celestial body that: (a) is in orbit around the Sun; and (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a nearly round shape (due to a hydrostatic equilibrium); but (c) has not cleared the neighborhood around its orbit; and (d) is not a satellite of another planet. As defined, the Solar System has probably has at least one dwarf planet in the Main Asteroid Belt (Ceres), Edgeworth-Kuiper Belt (Pluto and Eris); and Oort Cloud (possibly Sedna). In addition, the "dwarf planet" Pluto is recognized as a prototype of a new class of trans-Neptunian objects.
Smaller Solar System Bodies - This category collectively refers to all other celestial bodies orbiting our Sun, Sol (including asteroids, comets, and satellites).
Some astronomers believe that these controversial definitions will be revisited before the next IAU assembly in 2009. (More discussion is available from IAU 2006, Astronomy Picture of the Day; and from "Planetesimals to Brown Dwarfs: What is a Planet?," Basri and Brown, 2006.) For example, on November 6, 2000, astronomers associated with exoplanets.org (Geoffrey W. Marcy and R. Paul Butler) began using a generalized definition of "planet" that they also apply to objects found outside the Solar System.
Like the eight larger planets, the class of Solar System objects newly defined as "dwarf planets" are massive enough to be roughly round in shape. They also orbit the Sun, Sol, rather than other planets like Earth's Moon or Pluto's satellite Charon. However, they are still small enough that they have not cleared their orbital region around Sol of objects of roughly similar size. (A list of over 40 current dwarf planetary candidates -- that does not include unannounced objects recently discovered -- and a comparison of their average orbital distances from the Sun and estimated diameters with the eight larger planets is available from Astronomer Michael Brown's web page on "How many planets are there?")
By the IAU's definition, dwarf planets can be found anywhere in the Solar system. Ceres, the largest Main-Belt asteroid, has been acknowledged by many astronomers as a dwarf planet. In addition, the next three largest asteroids in the Main Belt (Vesta, Pallas, and Hygeia) may also be "round enough" to be eventually classified as dwarf planets.
Ann Feild, STScI,
("Xena" or 2003
UB313), the largest
orbit the Sun
beyond the orbit
of Neptune (more).
Based on tentative size estimates, most candidates for dwarf planethood, however, reside beyond the orbit of Neptune in the Edgeworth-Kuiper Belt. Many astronomers have already recognized Eris (2003 UB313), Pluto, Haumea, and Make-make as dwarf planets and so anticipate that many more icy Edgeworth-Kuiper objects (EKOs) already discovered will eventually be classified as dwarf planets as well. Moreover, some astronomers are monitoring over a dozen more unannounced but recently discovered EKOs that also may eventually be found to be large and round enough to be designated as dwarf planets.
The huge and loosely defined region of the Solar System's Oort Cloud also holds candidates for dwarf planethood. Sedna, designated by some astronomers as a member of the "inner" Oort Cloud, may also become classified as a dwarf planet. More Oort-Cloud candidates may eventually be detected, but visual confirmation of their spherical shape would likely be difficult.
Information and images about proposals to mine asteroids (and comets) as economical sources of raw materials for last space construction projects can be found at Sol Station.
More information and images of Pluto, Charon, and the Edgeworth-Kuiper Belt are available at NASA's Pluto-Kuiper Belt Mission and Planetary Photojournal. Fact sheets on Pluto and the Centaur object Chiron are also available from NASA's National Space Science Data Center.
David Seal (a mission planner and engineer at NASA's Jet Propulsion Laboratory at CalTech) has a web site that generates simulated images of the Sun, planets, and major moons from different perspectives and at different times of the year. Try his Solar System Simulator.
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