Even before the discovery of Eris, an icy body of the outer solar
system larger than Pluto, a heated debate was raging over how we should
define a planet. Something had to be done. Either Eris was a planet, or
Pluto wasn’t.
So the International Astronomical Union set up a committee to consider the issue, to report back to the IAU conference.
The committee came back with the new definition that a planet had to
be orbiting a star, big enough to have collapsed into a spherical shape
under its own gravity, and not be the satellite of a planet.
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I had to think about it for a while, but in the end it was clear
that this was a good definition, not because it saved Pluto, but
because it was a robust, physical definition. It could be applied to
new discoveries without the need for further arguments and conferences.
This definition included the nine existing planets and added Eris,
Ceres and Charon making a total of 12 planets.
Alas, the IAU didn’t ratify the recommendation. Instead of thinking
about what a planet really is, physically, it decided instead to draw
an arbitrary line in order to preserve an arbitrary and by no means
broadly-held perception of what a planet should be.
The change to the committee’s recommendation was to invent a new
category called “Dwarf Planets” to apply to Pluto, Eris and other
similar bodies.
Even the name doesn’t make sense. Dwarf planets, the ruling goes,
are not determined by size. In fact, they’re the same as normal
planets, except that they have not “cleared out the neighbourhood
around their orbit” of other bodies.
The orbital neighbourhoods of all planets are cluttered with other
bodies. What exactly is an orbital neighbourhood? Here again we have an
arbitrary decision and description, not a physical one.
Even Jupiter has a whole retinue of asteroids which share its orbit,
the Trojans. We now need to insert a special “secondary” set of
definitions - again arbitrary - to exclude the Trojans, just so that
Jupiter can still be called a planet.
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Space in the outer solar system is huge. If we finally find out, in
years to come, that there is nothing else sharing Pluto’s orbit, will
we then call it a planet after all? How close to it does another body
have to be before it is deemed to have not been “cleared out”?
And what about ellipticity? Just because the orbits of the planets
out to Neptune have low ellipticities and obliquities, what logic is
there in deciding that all planets have to have this? How small an
orbital ellipticity and obliquity does a body need to have before it is
a planet? Here is yet another arbitrary, non-physical, line which has
been drawn.
What if we find a body the size of Earth out in the Kuiper Belt? Is
this still a “dwarf planet”? What if we find a body the size of Neptune
out there? Will we suddenly insert some post hoc reason to call it a
planet after all? Maybe its ellipticity will be low, so we could just
“tweak” the definition to include it that way, without including all
that other icy riff-raff out past Neptune.
If a chance gravitational encounter threw a large KBO (Kuiper Belt
Object) into an orbit between Uranus and Neptune, would it become a
planet? Why is Neptune regarded as a planet anyway, when there are
whole families of asteroids and KBO’s - including Pluto - whose orbits
cross its own?
And if we exclude Trojans and resonant orbiting bodies from the
“cleared out orbit” rule, isn’t Pluto then a planet after all, along
with Eris and others?
The IAU has rejected a clean, simple system based on purely physical
elements, where you could look at a body and say, yes, that’s a planet.
In its stead it has set up an artificial and unworkable one requiring
ongoing arbitrary adjustments purely so that what they’ve already
decided to call planets, can still be called planets.
What earthly purpose is there in the IAU taking to itself a process
of “accreditation” for planets? If it was just a matter of awarding
planet status to those bodies they already wanted to be planets,
couldn’t they have just published a list, saying, “These are planets
and nothing else is, unless we say so”.
It would have been a lot easier, and a lot less dumb. Planets are
now no longer a physical class of bodies, but merely a label conferred
by committee, subject to ongoing argument.
Worst of all though, is that the word will no longer have any
scientific value. It has already been noted by the IAU itself that we
can no longer say that the bodies we have found orbiting other stars
can be called planets, because they’re too far away, and we can’t test
the new criteria for planethood. So now only our own solar system has
planets.
In a few years when we start to find significant numbers of
terrestrial bodies around other stars, does this mean they too will
have to be called something else - not because they’re strange or small
or don’t look like planets, but simply because we can’t “accredit” them
without first finding out if they’ve “cleared out their orbits of other
bodies - except (presumably) Trojans?”
Nobody is going to go for this. The general public already see it as
a joke. Certainly the scientific community will cease to use the word
“planet” for any constructive purpose, and the “definition” will break
down within a few years as we find bodies that don’t fit the
description, or whose orbital or physical elements test the limits and
the vagueness of the terms used by the IAU in its definition.
They will be obviously “planets” in any sensible sense - but we
won’t be able to call them that, because a bunch of scientists didn’t
like the idea of accepting the fact that, out past Neptune, planets
simply look like that. They have elliptical orbits, and they’re small
and icy. So what?
Ceres is a planet. Again, what’s the problem? It’s a little planet
because Jupiter stole most of the stuff that would have made a
decent-sized body out of it. That’s fine. At least we can look at it
and say, “It’s big enough to be spheroidal, so it’s a planet”. We don’t
have to investigate its “orbital neighbourhood” (however defined) to
decide if it should have planethood “conferred” on it by the IAU.
Losing one planet might be regarded as a mistake, but losing four really does look like carelessness.
The author will be among the astronomers and enthusiasts
converging on Bendigo from March 23-25, 2007, for VASTROC the Victorian
Astronomy Conference. To find out more about the conference vist the website.