Asteroid Belt:
The “Night Spirits”
INNER BELT ASTEROID CLASSES:
A-type asteroids
In the Dremish system, these fairly uncommon asteroids
show within the spectra a strong showing of olivine. Olivine is a very common
material found in the established mantle of a planet. The Olivine will be
strong in either iron of magnesium (FeSiO4, MgSiO4). Iron
rich olivine is found in igneous rocks, yet magnesium rocks aren’t usually
sound with other silica minerals. One other oddity is that it is the magnesium
olivine that is found in asteroids and meteorites. How this material found it’s way to the asteroid belt is most likely a planet with a
fully developed mantle, usually from a small planet that was destroyed.
E-type of asteroids
In the Dremish system, these
asteroids are fairly rare as the formation of these asteroids is still up to
debate. The primary item for these floating space rocks is the unusual
substance called Troilite. Troilite is also known as Iron Sulfide, but Troilite
is non magnetic compared to pyrrhotite, which is magnetic. Troilite being an
iron sulfide is found in igneous rocks and some metamorphic rocks. So the
presence of an asteroid or meteorite being made of this material must dwell on
the idea of a destroyed planet large enough to establish volcanism. One theory
might be a mars sized planet crashed into a larger planet or orbited too close
to Drem and was therefore destroyed.
M-type asteroids
On Drem, these asteroids are fairly common. Most people
know that metallic asteroids have to a certain degree small amounts of stone,
and that the asteroids are usually the remnants of the cores of asteroids that
have been destroyed in the past. These asteroids are fairly bright, as some are
made of nickel-iron, just like planet cores are made of. These asteroids are
thought to be the source of all iron meteorites that impact the planets of the
Dremish system. One thing to note is that the M type asteroids are one of three
basic types, as the S and C types are the other two. On Drem, some of the large
asteroids can actually be considered an amalgamation of other metallic
asteroids combining, as the shapes are sometimes very unusual and weird to see.
Q-type asteroids
These fairly uncommon asteroids are found to be similar
to A type asteroids, with 2 significant differences.
The first is the strong presence of pyroxene, which is another mantle silicate.
Pyroxenes are unusual in that they can contain calcium, sodium, iron,
magnesium, titanium and other minerals, including its standard silica and
aluminum mixture. Pyroxenes are found in igneous and metamorphic rock within
the mantle so that just like a type-A asteroid, this
asteroid must be from a larger impact of some magnitude. Unusually for this
type of asteroid is a small presence of metals, usually seen as iron or
magnesium.
R-type asteroids
These asteroids are somewhat bright and fairly uncommon
asteroid fairly similar to type-Q asteroids. The difference with Q-type
asteroids is instead of the presence of metal; these asteroids show a presence
of plagioclase. Plagioclase shows up as either calcium aluminum or a sodium
aluminum style silicate. Either way, the mineral is commonly called Feldspar.
The plagioclase is found in igneous rocks with pyroxenes, and so the connection
is easy to make. The type of feldspar found currently is similar to earth
feldspars called Labradorite, which shows a bluish
iridescence when light is passed thru the crystal structure.
OUTER BELT ASTEROID CLASSES:
D-type
asteroids
In the Dremish system, these asteroids present an odd set
of questions. Most of the debate presents these asteroids forming from the very
beginning of the system and show an unusual chemistry. Being like a type-C
asteroid, these asteroids have a very low albedo. The
strange qualities of the asteroids show up in the organic rich silicates,
carbon and anhydrous silicates that are commonly found in these asteroids.
These asteroids have a lot of similarities with comets with the anhydrous
silicates, and so the asteroids are always found far out in the solar system.
Debate rages on, but common thought is that these asteroids have an icy core.
What the icy core is made of, is still up for debate.
Due to the rich organics, these asteroids show a reddish color due to the tholins on the surface.
P-type
asteroids
These asteroids are very similar to D-types as the
chemical similarities are all there, except for 1 main thing. The main
difference is that there is water mixed in with the organic rich silicates,
carbon and anhydrous silicates. Like the D-type, these asteroids contain a
reddish hue due to the tholins on the surface. These
asteroids also come from a very early time period of the systems formation, and
also are only found far out in the solar systems.
V-type
asteroids
The V-type asteroids are fairly rare in the far asteroid
belt of Drem, since this far out, icy carbonaceous asteroids are more likely.
Yet, these asteroids do show up. They have more pyroxene than a standard S-type
asteroid. Another feature of these asteroids is the spectra of basalt, yet not
any type of basalt, but of achondritic basalt. Where
one finds this type, since on earth, achondrite
meteorites are usually from the Mare (basalt) seas of the Moon. The debate will
continue as one need a place of large impact craters and lave seas to be
impacted for these to even exist. One theory is that a moon or planet was
destroyed providing this very rare type of stony-silicate asteroid.
Closer than life belt (destroyed
small proto-planet core, remains of asteroid impacts)
Type Inner
Belt: metallic, some silicates
Asteroid Belt mass .000006
of earth (almost 1000 times less than Sol’s belt)
Belt size ½
distances between orbits
Inner edge of belt: .0112
AU
Year
length .00237 (.8635 days)
Middle part of belt .0188
AU
Year
length .0051555 (1.878 days)
Outer edge of belt: .0264
AU
Year
length .008579 (3.125 days)
Notable
Asteroids:
Warriors Heart is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Warriors Heart
Class M
Distance: .0188 AU
Material: Nickel/Iron
Orbit
period: .0051555 (1.878 days)
Inclination: 10.584 degrees
Eccentricity: .0793
Size: 9.1 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .113
Surf Grav: G’s
Shadow Beast is a close-in, hot silicate asteroid that is
almost totally silicates mixed with some darker stone. The asteroid is covered
in a fine stony dust which dulls the surface somewhat. The colors overall are
darker due to the larger amount of green olivine, black pyroxene, and brown to
black plagioclase. Therefore, the asteroid is darker than normal asteroids, yet
is so large as to still be easily seen.
Name: Shadow Beast
Class R
Distance: .0179 AU
Material: Silicates – spectra show olivine,
pyroxene & plagioclase
Orbit
period: .0047897 (1.7446 days)
Inclination: 38.846 degrees
Eccentricity: .23
Size: 467 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 2 degrees
Albedo: .159
Surf Grav: G’s
Guardian is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Guardian
Class: M
Distance: .0195
Material: Nickel/Iron
Orbit
period: .005446 (1.98373 days)
Inclination: 12.972 degrees
Eccentricity: .2589
Size: 4.23 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 4 degrees
Albedo: .238
Surf Grav: G’s
Shining Claw is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Shining Claw
Class: M
Distance: .0192
Material: Nickel-Iron
Orbit
period: .005321 (1.9381 days)
Inclination: 7.1346 degrees
Eccentricity: .089753
Size: 28.9 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .423
Surf Grav: G’s
Eye of Night is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Eye of Night
Class: M
Distance: .0186
Material: Nickel/Iron
Orbit
period: .0050734 (1.84799 days)
Inclination: 4.097 degrees
Eccentricity: .1738752
Size: .7 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .1
Surf Grav: G’s
Night Stalker is a close-in, hot silicate asteroid that is
almost totally silicates from deeper in a mantle. The asteroid is covered in a
fine stony dust which dulls the surface somewhat. The color runs from stony
grey to creamy tans, but mixed in are obvious greens from olivine and black
from the pyroxene. There are chunks of nickel-iron also found within, yet
harder to see.
Name: Night Stalker
Class: Q
Distance: .0196
Material: Silicates – Spectra shows
Olivine, Pyroxene and a bit of metal (nickel/iron)
Orbit
period: .005488 (1.999004 days)
Inclination: 1.1371 degrees
Eccentricity: .043109
Size: 263 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .24
Surf Grav: G’s
Blood Oath is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Blood Oath
Class: M
Distance: .0199
Material: Nickel/Iron
Orbit
period: .0056145 (2.047045 days)
Inclination: 8 degrees
Eccentricity: .13
Size: 16.3 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .2
Surf Grav: G’s
Spirit of the Hunt is a close-in, hot silicate asteroid
that is almost totally silicates from a volcanic mantle. The asteroid is
covered in a fine stony dust which dulls the surface somewhat. The color is
more of a yellow due to the large presence of sulfur in the asteroid. Due to
the color, the asteroid is also brighter than normal silicate asteroids.
Name: Spirit of the Hunt
Class: E
Distance: .019
Material: Silicates – strong presence of Triolite (
Orbit
period: .005238 (1.90792 days)
Inclination: 10.83 degrees
Eccentricity: .222885
Size: 28.54 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 6 degrees
Albedo: .16
Surf Grav: G’s
Fertility Spirit is a close-in, hot metallic asteroid that
is almost totally metal, specifically nickel-iron mix. The asteroid is covered
in a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: Fertility Spirit
Class: M
Distance: .0127
Material: Nickel/Iron
Orbit
period: .002862 (1.042642 days)
Inclination: 6.7089 degrees
Eccentricity: .266182
Size: 2.53 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 14 degrees
Albedo: .44
Surf Grav: G’s
Warriors Speed is a close-in, hot silicate asteroid that is
almost silicate from within a mantle. The asteroid is covered in a fine stony
dust which dulls the surface somewhat. The color is a fine creamy tan, making
it appear a bit brighter than normal silicate asteroids. It also has a greenish
tint due to the olivine within it.
Name: Warriors Speed
Class: A
Distance: .0182
Material: Silicates – spectra strongly
shows olivine
Orbit
period: .004911 (1.788696 days)
Inclination: .46959 degrees
Eccentricity: .6342274
Size: 2.3 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .16
Surf Grav: G’s
Spirit of Plenty is a close-in, hot metallic asteroid that
is almost totally metal, specifically nickel-iron mix. The asteroid is covered
in a fine stony dust which dulls the surface somewhat, yet the Albedo stays
high, and the asteroid is easily seen when orbiting away from Drem.
Name: Spirit of Plenty
Class: M
Distance: .019
Material: Nickel/Iron
Orbit
period: .005238 (1.90792 days)
Inclination: 13.34 degrees
Eccentricity: .3354
Size: .55 km
Density: 1.1 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .326
Surf Grav: G’s
Good Hunt is a close-in, hot silicate asteroid that is almost
totally silicates from a mantle. The asteroid is covered in a fine stony dust
which dulls the surface somewhat. Just like other silicate asteroids, the color
is a fine tan color mixed with green from the olivine.
Name: Good Hunt
Class: A
Distance: .0183
Material: Silicates – spectra strongly
shows olivine
Orbit
period: .0049512 (1.8034586
days)
Inclination: 13.138 degrees
Eccentricity: .2531
Size: 130 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial tilt: 16 degrees
Albedo: .16 of earth
Surf Grav: G’s
The Spear is a close-in, hot metallic asteroid that is
almost totally metal, specifically nickel-iron mix. The asteroid is covered in
a fine stony dust which dulls the surface somewhat, yet the Albedo stays high,
and the asteroid is easily seen when orbiting away from Drem.
Name: The Spear
Class: M
Distance: .0181
Material: Nickel/Iron
Orbit
period: .0048702 (1.77397 days)
Inclination: 1.48127 degrees
Eccentricity: .201514
Size: .34 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 4 degrees
Albedo: .15
Surf Grav: G’s
Safe Hunt is a close-in, hot silicate asteroid that is
almost totally silicate material from a mantle. The asteroid is covered in a
fine stony dust which dulls the surface somewhat, The
color within is a tan stony color mixed with the greenish color of olivine.
Name: Safe Hunt
Class: A
Distance: .0178
Material: Silicates – Spectra strongly
shows olivine
Orbit
period: .0047496 (1.730054 days)
Inclination: 9.4316 degrees
Eccentricity: .3495
Size: 110 km
Density: .9 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .15
Surf Grav: G’s
Spirit of Loyalty is a close-in, hot metallic asteroid that
is almost totally metal, specifically nickel-iron mix. The asteroid is covered
in a fine stony dust which dulls the surface somewhat, yet the Albedo stays
high, and the asteroid is easily seen when orbiting away from Drem.
Name: Spirit of Loyalty
Class: M
Distance: .0192
Material: Nickel/Iron
Orbit
period: .005321 (1.9381 days)
Inclination: 2.28701 degrees
Eccentricity: .6011738
Size: .81 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 14 degrees
Albedo: .15
Surf Grav: G’s
Spirit of Truth is a close-in, hot metallic asteroid that
is almost totally metal, specifically nickel-iron mix. The asteroid is covered
in a fine stony dust which dulls the surface somewhat, yet the Albedo stays
high, and the asteroid is easily seen when orbiting away from Drem.
Name: Spirit of Truth
Class: M
Distance: .019
Material: Nickel/Iron
Orbit
period: .005238 (1.90792 days)
Inclination: 8.88806 degrees
Eccentricity: .48324394
Size: 2.5 km
Density: 1.2 of earth
Mass: of earth
Rotational
period: tidally locked
Axial
tilt: 1 degree
Albedo: .15
Surf Grav: G’s
Copyright 2006 by Kevin Urbanczyk
All Rights Reserved
Used with Celestia
1.4.1
Chris Laurel
<claurel@www.shatters.net>
Clint Weisbrod
<cweisbrod@cogeco.ca>
Fridger Schrempp
<t00fri@mail.desy.de>
Bob Ippolito
<bob@redivi.com>
Christophe Teyssier <chris@teyssier.org>
Hank Ramsey
<hramsey@users.sourceforge.net>
Grant Hutchison
<granthutchison@blueyonder.co.uk>
Resource sites:
Wikipedia: http://en.wikipedia.org/wiki/Main_Page
Solstation: http://www.solstation.com/