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DEFINITIONS
The International Astronomical Union held a meeting in Prague on 24th August at which it passed three new definitions, of a planet, a dwarf planet and a Small Solar System Body. The IAU definitions are:
PLANET: a celestial body having all the following attributes as a "planet". It:
(1) is in orbit around a star or stellar remnants;
(2) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape;
(3) is above the minimum mass/size for a planet in our solar system*;
(4) if in our solar sytem it has cleared the neighbourhood around its orbit; and
(5) is below the limiting mass for thermonuclear fusion of deuterium.
(*What this mass/size is has not been specifically defined. However, it must be somewhere between the mass required in (2) above, and the mass of the planet Mercury.)
Our solar system is considered to have eight planets under this definition: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Three bodies in orbit around our Sun and which only fulfil conditions (1) and (2), but not (4), and are not natural satellites, are now classified as dwarf planets: Ceres, Pluto and Eris. To date, there have been more than two hundred planets discovered orbiting other stars.
The IAU further defines any celestial object having any of the following attributes as not being a planet:
(1) it is below the minimum mass/size for a planet in our solar system;
(2) it is above the limiting mass for thermonuclear fusion of deuterium; or
(3) it is a free-floating object in a young star cluster.
(MY INTERJECTION: the point about fusing deuterium is to distinguish planets from brown dwarf stars, which can be as small as about twelve Jupiter masses.)
DWARF PLANET: a dwarf planet as an object 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 hydrostatic equilibrium (nearly round) shape
c) Has not "cleared the neighbourhood" around its orbit
d) Is not a satellite of a planet, or other nonstellar body
SMALL SOLAR SYSTEM BODY: A small solar system body (SSSB) is a term defined in 2006 by the International Astronomical Union to describe solar system objects which are not planets or dwarf planets:
"All other objects orbiting the Sun shall be referred to collectively as "Small Solar System Bodies" ... These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies."
Therefore it refers to these objects that can be further classified based on their orbit or composition:
all known minor planets that are not dwarf planets, i.e.:
i) the classical asteroids (except the largest one, 1 Ceres);
ii) the Centaurs and Neptune Trojans;
iii) the smaller Trans-Neptunian Objects (except dwarf planets such as Pluto and Eris);
iv) all comets;
It is not yet clear whether there will be a lower bound on the group of small solar system bodies, or if it will encompass all material down to the level of meteoroids.
Some of the larger "small solar system bodies" may be reclassified in future as dwarf planets, pending further examination to determine whether or not they are in hydrostatic equilibrium.
MY COMMENT: All rather legalistically phrased and a little dry to read, but that is because these were formal motions put to a General Assembly for approval.
HISTORY
There have been as many as 27* solar system bodies that were greeted as planets on discovery (most recently first Sedna and then Eris were so hailed by newspapers when they were discovered) but were later removed from that status, so Pluto is merely the latest in a long line to have been reclassified, The number of planets has gone up and down like a yo-yo as a result.
First to get the chop, in the 16th Century, were the Sun and the Moon, regarded as planets from antiquity.
Then in the 17th Century, the 4 Galilean moons of Jupiter and Titan, Iapeter and Rhea, the first 3 moons of Saturn to be discovered. were defined by their discoverers as planets but came to generally be regarded as moons, as that new concept became accepted.
Since the acceptance of the heliocentric model over the geocentric model, the solar system has been seen as having various numbers of accepted planets over the years:
1543 - six (Mercury, Venus, Earth, Mars, Jupiter and Saturn) (among those who accepted the new view)
1781 - seven (with Uranus)
1807 - eleven (with 1 Ceres, 2 Pallas, 3 Juno and 4 Vesta)
1845 - twelve (with 5 Astraea)
1846 - thirteen (with Neptune)
1851 - twenty-three (with 6 Hebe, 7 Iris, 8 Flora, 9 Metis, 10 Hygiea, 11 Parthenope, 12 Victoria, 13 Egeria, 14 Irene and 15 Eunomia)
1852 - eight (without Ceres and the asteroids)
1930 - nine (with Pluto)
2006 - eight (without Pluto)
When the objects 1 Ceres, 2 Pallas, 3 Juno and 4 Vesta were found orbiting between Mars and Jupiter in the early 1800s, they were declared and accepted as planets (though Herschel, who had discovered Uranus 20 years beforehand, felt they were disappointingly small and did not really rank alongside his discovery; he therefore coined the term "asteroid" for them),
They remained classed as planets for many years. However, as more and more objects began to be found in the same region of the solar system, they became classified as asteroids, along with their orbital kin. Just as well as we now know of over 340,000 asteroids. To have 340,0008 planets would be getting silly.
A similar scenario has occurred with Pluto. It was first discovered beyond Neptune in 1930 and was accepted by the IAU as a planet after it was initially believed to be larger than the Earth. However, after further observation it was found that Pluto was actually much smaller, being less massive than the Moon.
After more than 1,000 similar new bodies were found beyond Neptune during the 1990s and the early 2000s, the IAU decided to reclassify Pluto as a dwarf planet in 2006.
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