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SPACE GEOSCIENCE ARTICLE
New definition of planet adopted by IAU
by MIKE BALDWIN
09.02.2006: The IAU has adopted a new definition of
"planet" and Pluto no longer qualifies. We now
officially only have eight planets in our solar system. This
change in terminology does not change what's actually out
there. Ultimately, it's not as important to know how we
classify the various objects in our solar system as it is to
learn about their physical nature and their histories.
On 24 August 2006 members of the International Astronomical
Union (IAU) agreed that a "planet" is defined as 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 hydrostatic equilibrium (nearly
round) shape, and (c) has cleared the neighbourhood around its
orbit. A "dwarf planet" 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 hydrostatic equilibrium (nearly round) shape, (c) has not
cleared the neighbourhood around its orbit, and (d) is not a
satellite.
All other objects, except satellites, orbiting the Sun shall
be referred to collectively as "Small Solar-System Bodies". An
IAU process will be established to assign borderline objects
into either dwarf planet and other categories. These currently
include most of the Solar System asteroids, most
Trans-Neptunian Objects (TNOs), comets, and other small
bodies.
This means that the Solar System consists of eight "planets"
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and
Neptune. A new distinct class of objects called "dwarf
planets" was also decided. It was agreed that "planets" and
"dwarf planets" are two distinct classes of objects. The first
members of the "dwarf planet" category are Ceres, Pluto and
2003 UB 313 (temporary name). More "dwarf planets" are
expected to be announced by the IAU in the coming months and
years. Currently a dozen candidate "dwarf planets" are listed
on IAU's "dwarf planet" watchlist, which keeps changing as new
objects are found and the physics of the existing candidates
becomes better known.
The "dwarf planet" Pluto is recognised as an important
proto-type of a new class of trans-Neptunian objects. The IAU
will set up a process to name these objects.
Five planets (Mercury, Venus, Mars, Jupiter, and Saturn) were known to the ancients. To the unaided eye, these
planets appear starlike. However, the planets moved relative
to the stars. For this reason they were called wandering
stars. Our word "planet" comes from the Greek word
planetes, meaning "wanderer".
The planet Uranus was
discovered by the noted British astronomer, Sir William
Herschel, on March 13, 1781. Uranus had been observed numerous
times by other astronomers as early as 1690, but it was
thought to be another star.
In the course of preparing a star catalog in 1801, the
Sicilian astronomer Guiseppi Piazzi accidentally discovered a
small planet between the orbits of Mars and Jupiter. He named
the planet Ceres after the
Sicilian god of the harvest. Ceres is now known to be the
largest of thousands of asteroids, most of which have orbits
in the region of the Solar System between Mars and Jupiter.
Ceres is one of the newly classified "dwarf
planets".
Unlike Uranus and Ceres,
Neptune was not discovered by
accident. It was proposed that a planet beyond Uranus could
account for irregularities in Uranus' orbit. Independently,
two astronomers, John Couch Adams in England and
Urbain-Jean-Joseph Le Verrier in France, calculated the
position of this yet unknown planet. The search began. The
British astronomer James Challis, using Adams' predictions,
observed the planet on the night of August 4, 1846, but failed
to compare his observations with those of the previous night
and did not recognize the planet. On September 23, 1846, the
planet was finally found on the first try by the German
astronomer Johann Galle using Le Verrier's predictions.
Several astronomers interpreted irregularities in the orbits
of Uranus and Neptune as being caused by a more distant
planet. Among these astronomers was the American Percival
Lowell who is credited with the successful prediction of the
planet's orbit. Lowell also started the search for the planet
which was ultimately found in 1930 by his successors at the
Lowell Observatory in Arizona.
Pluto was discovered by Clyde
Tombaugh of the Lowell Observatory by comparing a photographic
plate taken on the night of January 23, 1930 with two others
taken in the same month. Pluto has been reclassified from
"planet" to "dwarf planet".
2003 UB313, discovered on
October 21, 2003, is the largest known dwarf planet in the
solar system. A trans-Neptunian object (TNO), it orbits the
Sun in a region of space known as the scattered disc
accompanied by at least one moon; the pair are currently the
most distant known objects in the solar system. Mike Brown,
who led the Mount Palomar-based discovery team, announced in
April 2006 that the Hubble Telescope has measured 2003 UB313's
diameter to be 2400 km, or slightly larger than Pluto. Its
size, and the prospect of discovering other similarly-sized
objects in the future stimulated the International
Astronomical Union (IAU) to define the term 'planet' more
precisely. Under a new definition approved on August 24, 2006,
2003 UB313 was designated a "dwarf planet". Before
this clarification, it had been described as our solar
system's "tenth planet" by its discoverers and NASA.
This article was written by MAGS member, Mike Baldwin
©2006. Information in this article used for educational
purposes under the provisions of the Fair Use Act of 1976.
References:
01 Bill Arnett; The 8 Planets; http://www.nineplanets.org/.
Updated 25 August 2006; Accessed 02 September 2006.
02 IAU 2006 General Assembly: Result of the IAU Resolution
votes;
http://www.iau2006.org/mirror/www.iau.org/iau0603/index.html;
Accessed 02 September 2006.
03 Ancient Times; Discovering the Planets;National Air and
Space Museum;
http://www.nasm.si.edu/research/ceps/etp/discovery/etpdiscovery.html;
Accessed 02 September 2006.
03 Discovering New Planets; Discovering the Planets;National
Air and Space Museum;
http://www.nasm.si.edu/research/ceps/etp/discovery/etpdiscovery.html;
Accessed 02 September 2006.
04 2003 UB313; Wikipedia;
http://en.wikipedia.org/wiki/2003_UB313; Accessed 02 September
2006.
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