Staetements from
- The
American
Museum of Natural History
- Phil Plait,
the Bad Astronomer
- Nine
Planets and Counting
A
Geologist
Surveys the Solar System
I received the following letter in the wake of the
IAU’s
ill-fated
redefinition
of the word “planet”.
The north wall of Troster now has little signs
explaining which orbit belongs to which planet or dwarf object.
Pollux
has a planet.
August 17, 2006.
Rather than counting how many planets are dancing
on the head of this particular stellar pin,
let’s start here.
There are several families of objects in the
Solar System.
- Sun.
Category of one.
A
star,
and the lynchpin of the whole kit and kaboodle.
Without the gravity of the
Sun, there is no
Solar System.
- Terrestrial
planets.
Four of these.
Two are nearly identical in size.
These larger two have been able to retain
heat
from their formation
and produce some
heat
due to
radioactive decay
in their cores,
thus exhibiting active
volcanism.
The other two are smaller;
the
slightly bigger one
with very little geological activity,
the
smallest
with no geological activity that we know of.
- basic geology of
Earth
and
Venus
- terrestrial planetary atmospheres
- what are
clouds?
- Earth’s
atmosphere—a
sign of life
- Earth’s
oceans
and the
Water Cycle
- Why dynamism is important
(the motion of the crust, mantle, and core,
made possible by the internal source of heat)
- Asteroids.
Amalgams of rock, dust, and ices.
The ices are stable.
A few of these are round,
but most are small enough that thay take on all kinds of bizarre
shapes—dog bones, peanuts, shoes, half-eaten wedges of cheesecake.
These are divided into several families.
One type of family describes their present orbit/position;
like the
Trojan asteroids,
two “camps” of which which follow and preceed
Jupiter
around the
Sun.
(Earth
merely has “Trojan dust.”)
Saturn,
and probably
Uranus
and
Neptune,
also seen to have these asteroidal hangers-on.
Another type of family is connected by their purported origin;
by analyzing the composition and orbital parameters of many asteroids,
it seems that there may have originally been several larger bodies
which were shattered in collisions.
- How many asteroids are there?
- Are they all in the
“asteroid
belt?”
- How far apart are they from each other?
- Where do they come from?
- How are they held together? (some just barely)
- Giant
planets.
Serious-a** planets, yo.
Four of these.
Two are similar in composition to the
Sun,
and considerably larger than anything else in the
Solar System,
both ruling over complex systems of
moons
and
rings,
with powerful
magnetic fields.
Slightly smaller are the “Ice Giants,”
with substantial amounts of
methane,
water,
and
ammonia,
cores which are proportionally much larger,
and weird, off-center
magnetic fields.
- internal
heat
sources
- deep, energetic atmospheres
- fantastic
pressures
within
- may have formed close in and spiraled out
- crucial to the evolution of the
Solar System
- Kuiper Belt.
Many of these objects are larger than most
asteroids,
and contain more ices,
but otherwise may be similar in origin and structure to asteroids.
The “Kuiper Belt” is the area
which starts a little ways inside
Neptune’s
orbit
and extends out to about 50 times the
distance
of the
Earth
from the
Sun.
In this formulation,
Sedna
is a KBO, I guess.
- how are they discovered?
- how did they get there?
- Comets.
Comets
are similar in structure and size to
asteroids
and in composition to
Kuiper belt
objects,
but they have orbits which bring them close enough to the
Sun
that their ices “boil off” and form a tenuous cloud.
If they get close enough to the
sun,
they can even form tails,
as so much material boils off that it is swept away into space in a long stream.
Most
comets
are thought to come from the
Oort cloud,
a swarm of comets residing as much as half a
light-year
from the
Sun.
- how did they get there?
- what about those crazy orbits?
- what can we learn from
comets?