| Official Name |
Sol, The Sun
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| Class |
G2V |
| Mass |
1,047 Jupiter masses or
333,054 Earth Masses |
| Diameter |
1,390,000 km |
| Planets |
13 (and counting) |
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| Mercury |
| Sol b |
| D, Iron Dwarf Planet |
| 0.055 Earth Mass |
| 4,880 km |
| 0.38 AU |
|
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Mercury is a very desolate and strange
world. It's extremely dense, and thought to be composed of almost 75%
Iron. Like Venus it has no moon of it's own.
There is some speculation that Mercury,
because of it's iron content, might be the iron core remnant of a
failed Neptune or Uranus like planet. It formed to close to the Sun,
and when the sun ignited, it striped the planet of all its atmosphere.
It could also be the core remnant of
the planet that might have been responsible for the Asteroid belt (See
Below) and fell into a close orbit with the Sun.
Image used with NASA's public release
rights, Ref: NASA/JPL/Mariner
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| Venus |
| Sol c |
| S, Hot Stock Planet |
| 0.81 Earth Mass |
| 12,103 km |
| 0.72 AU |
|
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Venus is the
closest neighbor and similar in size and mass to The Earth. There the
similarity ends, its super dense atmosphere mostly CO2 with Sulfuric
Acid clouds, make this world even hotter then Mercury even though it's
further from the sun. Its temperatures in places reach over
450°C(842°F) which is hot enough to melt lead.
It's also an odd planet in that it is
the only sizable planet in our solar system, without any moon. It also
rotates in the opposite direction then all the other planets. On Venus,
The sun rises in the West and sets in the East! There is only
speculation on it's odd rotation, and nothing really proven as to why
it is that way. Thankfully it orbits the sun in the same direction as
the other planets.
Thumbnail of image used by courtesy
rights granted by © Calvin J. Hamilton, please visit his website website
http://www.solarviews.com/ for full sized images. It's also a great
resource on our Solar System!
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| Earth |
| Sol d |
| S, Habitable Stock Planet |
| 1 Earth Mass |
| 12,756 km |
| 1 AU |
|
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It's our home World. See our Earth page for more
details. Earths moon is a bit unique, as it was formed by a collision
early on in The Earths history by a object with roughly the mass of
mars. So moon rocks, and earth rocks have roughly the same trace gas
elements inside them.
But the moon has almost no iron in it's
core, the iron from the impactor planet, (nick named Osiris by some)
merged with the earths core.
Image used with NASA's public release
rights, Ref: NASA/USGS/MODIS
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| Mars |
| Sol e |
| D, Cold Dwarf Planet |
| 0.11 Earth Mass |
| 6,794 km |
| 1.52 AU |
|
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The Red Planet as seen by the Hubble
Telescope. It's another strange world in that it does have water (as
the clouds prove) but is so cold and dry it's a desert planet. For a
short time in it's life, it had oceans, and a substantial atmosphere.
But even though it's half the diameter (size) of Earth, it only had a
tenth of the mass so it atmosphere bled off into space. It's once
molten iron core eventually cooled, and both the volcanoes, and the
core itself shut down. When this happened its volcanic out-gassing, now
done, no longer replaced the air it lost.
It 'may' have had one period of renewed
warmth and water due to a large impact from a meteor.
But again, the oceans slowly froze into
the ground, leaving a dead rust colored world. If it had only held
maybe a half of earth mass, it would be a habitable, if a bit chilly of
a world.
Although there has been some talk about
'Terraforming' Mars (making it more earth like) it really isn't
practical. It just doesn't have the mass to hold onto an Atmosphere.
Image used with NASA's public release
rights, Ref: NASA/StScI/Hubble
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| Asteroid Belt |
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| Asteroid Belt Planetoids |
| Of all the cataloged asteroids,
1/3 moon mass. Of all estimated, 2 earth masses |
| Various |
| 1.9 AU - 4.5 AU |
|
 |
The asteroid belt is nestled between the
orbits of Mars and Jupiter. It's considered either a failed planet
(Jupiter's proximity prevented it from forming) or a destroyed planet.
The variety of their composition seems indicate the first theory is the
more likely, as does the lack of mass.
However, we've discovered the even
single planets have a variety of different compositions, a destroyed
world might leave behind around 5 different types of asteroids, 2
planets colliding might lead to even more, around 10 or so.
The leading theory for the destroyed
scenario, has a 1.5 mass earth sized world, named Titanica, with Mars
as a Habitable Moon, being impacted by a .8 Earth mass planet,
asteroid, or super comet. It might have survived that, if it hadn't
been for Jupiter's gravity, which finished pulling the planet apart,
and dispersed it's remains into the now Asteroid belt. The lack of mass
now can be explained by scattering of the remains into and out of the
solar system. Mars moved into a lower orbit, after suffering a huge
impact from the remains, (Hellas Impact Crater). Without it's parent
planet, Mars lost it's tectonics, leading to the loss of its air.
Asteroid Vesta also appears to be the core like remains of something,
lending some credence to this.
Both theories have equal validity, its
one of the mysteries yet to be solved.
The picture is of Asteroid Ida and it's
very tiny moon Dactyl, used with NASA's public release rights, Ref:
NASA/JPL/Galileo
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| Ceres |
| Sol f |
| B (D), Cold Belt (Dwarf) Planet |
| .0014 Earth Masses |
| 975 km |
| 2.766 AU |
|
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Discovered in 1801 this planet has
changed status from planet to asteriod, to planet, then back, and now
finally to Dwarf Planet.
Not much is known about it other then is
appears to have a thin atmosphere and is warm enough for water frost to
form.
Although a Dwarf Planet it is also a
member of the asteriod belt objects, and the largest containing a full
third of the estimated total mass in the asteroid belt.
Image used with NASA's public release
rights, Ref: NASA/StScI/Hubble
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| Jupiter |
| Sol g |
| G, Gas Giant Planet |
| 318 Earth Masses |
| 142,984 km |
| 5.2 AU |
|
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The largest planet in our Solar system.
Jupiter with it whooping 63 Moons!, is a prime example of a failed
solar system within a solar system. If Jupiter had only 13 times more
mass, it would of been a Red or Brown Dwarf star, and it's moons would
of been called Planets.
Use the link below to see a highly
detailed, and one of the best photo's of our gigantic neighbor. It's
one of my favorites, the amount of detail is just breathtaking. It was
taken by the Cassini Space Craft as it flew by Jupiter on it's way to
Saturn.
Image used with NASA's public release
rights, Ref: NASA/Cassini/APOD
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| Saturn |
| Sol h |
| G, Ringed Giant Planet |
| 95 Earth Masses (0.29 Mj) |
| 120,536 km |
| 9.54 AU |
|
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The second largest planet in our solar
system, Saturn and its is 31 moons are currently being studied by the
Cassini Space Craft.
Although it's not as as picturesque as
Jupiter, its rings more then make up for that. Actually the truth is
once you penetrate Saturn's hazy atmosphere, it looks a lot like the
stormier Jupiter
Image used with NASA's public release
rights, Ref: NASA/JPL/Cassini
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| Uranus |
| Sol i |
| G, Ice Giant Planet |
| 14 Earth Masses |
| 51,118 km |
| 19.218 AU |
|
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The third largest planet in our solar
system (bet less massive then Neptune) Uranus is a complete odd ball.
Most planets equator's are lined up with the sun, however Uranus is
tilted 90 degrees, such that it's poles face the sun. Which pole faces
the sun depends on where it's at in it's orbit. It also has quite a few
moons, 21 named and 6 still unnamed.
Also a ringed planet, it's rings are
tilted along with the planet. There is only speculation as how Uranus
got tilted or formed this way, as it doesn't fit with planetary models
well. One speculation is that a long time ago our solar system passed
through another, and Uranus got to close to that systems sun or one of
it's Jupiter like worlds, which as they passed through, pulled Uranus'
axis off center to it's current position.
Image used with NASA's public release
rights, Ref: NASA/StScI/Hubble
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| Neptune |
| Sol j |
| G, Ice Giant Planet |
| 17.1 Earth Masses |
| 49,532 km |
| 30.06 AU |
|
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The forth largest planet in our solar
system (but more massive then Uranus) it probably has rocky/iron core
about the size and mass of Earth and also has some very faint rings.
Because of Pluto's eccentric orbit, sometimes Neptune is actually
further away then Pluto.
It sports 13 moons, only one of which is
sizable called Triton, a full third the size and mass of Mars.
Image used with NASA's public release
rights, Ref: NASA/StScI/Hubble
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| Pluto and Charon |
| Sol k1 & Sol k2 |
| B(D), Icey Belt (Dwarf) Double
Planet System |
| 0.0021 Earth Masses |
| 2274 km |
| 30 AU inner to 50 AU outer |
|
 |
The smallest planet in our system
(excluding planetiods) Pluto and is companion Charon have a eccentric
orbit that carries it in side the orbit of Neptune at its closest, and
out into the Kruiper Belt at it's farthest. Compared to other systems,
it's moon Charon is proportionately the largest for it's planets mass.
Charon is fully 1/2 the diameter of Pluto, and 1/6th of it's mass.
Pluto and Charon have two small moons,
Nix and Hydra which orbit around the bary center (The gravitational
Center between Pluto and Charon) of the double planets.
The Pluto-Charon system will soon be
visited (around 2015) by the New Horizons Space Craft.
Image used with NASA's public release
rights, Ref: NASA/StScI/Hubble
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Eris (formerly UB313 code named
Xena)
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| Sol l |
| B(D), Icey Belt (Dwarf) Planet |
| 0.0037 Earth Masses (estimated) |
| 3000 km (estimated) |
| 38 AU inner to 97 AU outer |
|
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The most recent addition to our Solar
system, Planet Eris and it's moon Dysnomia!
First discovered in 2003, then determined a solar system object in mid
2005, prematurely announced in late 2005. It is currently the object of
most interest right now. It's Larger then Pluto, and possibly even
colder.
The name Eris is after the Roamn goddes
of Stife and Discord, and was given this name for the issues it's
discovery caused in the IAU about planet classifications. It's
moon Dysnomia, is after the roma Goddess of
Lawlessness. And intrestingchoice is as its code name Xena, the
actress of Xena was Lucy Lawless.
Like Pluto, it's a member of the Kuiper
Belt objects.
Artists rendering image used with NASA's
public release rights, Ref: NASA/JPL/Caltech
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| Sedna |
| Sol m |
| B(D), Icey Belt (Dwarf) Planet |
| 0.0019 Earth Masses (estimated) |
| 1200 km (estimated) |
| 90 AU inner to 250 AU outer |
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This may be the first dwarf planet of
it's class, as it's orbit exists outside of the Kuiper Belt objects,
making it a
an Inner Oort Cloud object.
Artists rendering image used with NASA's
public release rights, Ref: NASA/JPL/Caltech
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