This is my personal diary of painting experiments and Warmachine, Hordes and other miniature adventures (and perhaps a splash of real life thrown in occasionally too). This blog is as much for my own motivation as to share my experiences with others. My self imposed rule for my army is that I only field painted models. If you're a fellow painter, I encourage you to challenge yourself, learn new skills, try new things, and most of all, paint like you have a pair!
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Friday, December 30, 2011
From the Desk: An alligator, a Sorceress, and a Gun Mage walk into a bar...
Thursday, December 29, 2011
From the Desk: Yay for Vacation!
- Legion - 99.0% painted
- Protectorate - 98.0% painted
- Mercenaries - 97.4% painted
- Cryx - 95.6% painted
- Cygnar - 87.5% painted
- Minions - 30.8% painted
Tuesday, December 27, 2011
From the Desk: Legion Metals
My buddy Lance suggested that I should do a blog post about how I painted the metals on Belphagore, so here it goes. This process is pretty straightforward, but somewhat lengthy. I'm not going to show any in-progress shots obviously since Belphagore is already done. First, let's look at the finished product...
I like to have a good pop to my metals overall, but I'm not a huge fan of non-metallic metals (NMM). So to accomplish a good amount of distinction between metal surfaces, I have to somewhat force and exaggerate the look of the metal plates. My end goal is to have metal that is shaded to represent a normal zenithal highlighting look, but still preserve enough metallic appearance so that it doesn't look overly forced. For this model I also wanted to introduce a little bluish tint to the recesses just to create a little more style. It gives the metal enough variation and interest to the eye.
Ok, so that's the end goal. Now to talk about the process. For the benefit of those who haven't read my older posts about philosophies on metallics, I'm going to go into some detail here on my reasoning. This reasoning has evolved over time and I am sure it will continue to evolve yet further. So here's the process I went through as I remember it for this model:
- Basecoat black - I always basecoat my metallic surfaces black first, especially if I primed white. I just find that it helps the metallics to reflect a little better.
- Basecoat GW Boltgun Metal - GW makes some of the best metallics out there for my personal style. I start with this darker metallic tone as the basecoat. This is a pretty sketchy basecoat too. A few missed or thin spots helps with the look of the armor I feel.
- Wash GW Badab Black - I'm so addicted to this stuff. I use it all the time for metallics. It just helps get those recesses dulled back down and create good separation. This wash doesn't need to be even. It just needs to hit recesses real good. Nothing blows the look of metallics like deep corners that are reflecting light.
- Heavy wash GW Asurmen Blue - This is just applied to the recessed sections. This technique works well for Circle armor as well, except using the green wash over bronzes. As I recall, I did at least 2 coats of this wash.
- Re-basecoat GW Boltgun Metal - Now I go back and use thinned Boltgun to "re-basecoat" the raised portions of the plates. I use a thinner version of this to keep it from getting too bright. Again, I'm attempting to force some shading here and reinforce the zenithal highlight effect by not lightening up the surfaces that are pointed more downwards.
- 2BB VMC Black - Now I do some very deep forced shading by two brush blending in some slightly thinned black into recesses and on lower plates that should be darker.
- Highlight GW Boltgun Metal - Now I start working highlights back up. Nothing revolutionary here, just hitting the higher angled plates that would get more light from above.
- Highlight GW Mithril Silver - Same as the previous step, just less area being highlighted.
- Highlight VMC Metallic Medium - Again, just like previous step. Note that the metallic medium is crazy bright and has no black pigment in it at all. I try to reserve this for specific points.
Monday, December 26, 2011
From the Desk: Albino Gators (part 2)
Saturday, December 24, 2011
From the Desk: Albino Gators
- Thin P3 Moldy Ochre wash
- Thin P3 Midlund Flesh wash
- Thin P3 Ordic Olive wash
- Medium MWH drybrush over scales
- Thin P3 Carnal Pink wash in limited places
- Thin P3 Battle Dress Green wash in limited places
- Slightly thinned RMS Jade Green stippled in key areas
- Thin P3 Thornwood green wash in limited places to shade
- Thin P3 CBB+Sanguine Base wash in limited places to shade
- Thinned MWH to highlight
Friday, December 23, 2011
Solar System: Neptune
- Neptune, like Uranus, has only been visited by one spacecraft: Voyager 2 in 1989.
- Neptune was discovered in 1846.
- Even though you couldn't stand on the surface of Neptune (since it's a gas giant), if you could you would experience nearly identical gravity as on Earth.
- Neptune's planet Triton was probably a captured satellite, inferred by it's retrograde orbit.
- The winds on Neptune can reach a ridiculous 2,100 km/hr.
The Nine Planets
Universe Today
Thursday, December 22, 2011
Solar System: Uranus
- Uranus wasn't discovered to be a planet until March 13, 1781.
- Uranus has only been visited by a single spacecraft: Voyager 2 in 1986.
- Uranus spins on an axis nearly perpendicular with its axis of rotation around the sun. When visited by Voyager 2, its south pole was pointed towards the Sun.
- There are rings around Uranus, but they, like its axis of rotation, are nearly perpendicular to its orbit around the Sun.
- Even though it isn't the farthest planet out, it is the coldest planet in our solar system (below -200 C).
The Nine Planets
Universe Today
Tuesday, December 20, 2011
Solar System: Saturn
- Saturn was first visited by Pioneer 11 in 1979.
- Saturn's specific gravity is 0.7, which means it would float in water (assuming you could find a big enough pond to put it in.
- Despite spanning a diameter of over a quarter million kilometers, the rings of Saturn are less than 1000 meters thick. Those rings are made primarily of water in ice form.
- Always overshadowed by Jupiter, Saturn has the second most satellites, currently counting at 62.
- Saturn's day is a mere 10.5 hours, and that rapid spin actually translates to forces that cause the planet to shape into a flattened ball (wider than it is tall).
- One of Saturn's moons (Enceladus) has ice geysers, which has the implication of potentially being the home of some form of life.
The Nine Planets
Universe Today
Tuesday, December 13, 2011
Solar System: Jupiter
- Jupiter was first visited by Pioneer 10 in 1973.
- Although the 4 larger moons are fairly well known (Io, Europa, Ganymede, and Callisto), there are at least 59 other smaller moons.
- Jupiter's Great Red Spot is a swirling storm 26,000 km across. To put that in perspective, that's more than twice the diameter of the Earth.
- Jupiter is approximately 90% hydrogen and 10% helium.
- Despite only having "trace" amounts of rock by mass and volume, Jupiter's core is probably rock consisting of 10 to 15 "Earths" worth of mass. Trace apparently means ~2% or less (by mass).
- Outside of the core is the main bulk of the planet, consisting of (get this) liquid metallic hydrogen.
- The different bands that surround the surface of Jupiter are clouds. Each band is actually blowing in opposite directions from its adjacent bands.
- As gas giants go, Jupiter is about as big as it gets. Adding more material wouldn't significantly increase its size due to the gravitational compression.
- Jupiter has dark rings, a huge magnetic field, emits more energy outward than it receives from the Sun, and generally just has a lot going on.
The Nine Planets
Sunday, December 11, 2011
Solar System: Mars
- The first spacecraft to visit Mars was Mariner 4 in 1965. Mars has been the destination for many spacecraft and landers for over 45 years now.
- Despite being half the diameter of Earth, Mars has twice as many moons (Phobos and Deimos) and a volcano (Olympus Mons) which is 4 times has tall as Everest, which also happens to be the largest mountain in the entire solar system.
- Mars has a very thin atmosphere with about 1% the atmospheric pressure of Earth. It is composed of mostly carbon dioxide.
- Despite the thin atmosphere, strong winds can cause dust storms that engulf the entire surface of the planet for up to a month at a time.
- Mars has polar ice caps at both poles, composed of both water and carbon dioxide (dry ice)
The Nine Planets
Wednesday, December 07, 2011
Solar System: Earth
- Due to erosion and tectonic activity, the Earth literally replaces its crust every half billion years, erasing any past geological history such as crater impacts.
- The Earth's composition (by mass) is approximately 1/3 iron and 1/3 oxygen.
- Earth is the only planet in the solar system where water can exist in liquid form on the surface.
- The Moon's gravitation is actually causing the Earth's rotation to slow very gradually (2 milliseconds per century). That means in another 180 million years, we'll get an extra hour in each day for painting and playing!
The Nine Planets
Sunday, December 04, 2011
Solar System: Venus
Venus! Talk about an unpleasant place to visit. It's probably the most inhospitable planet in our solar system. I actually really enjoyed painting this one. I used a combination of washes and streaking and stippling to create the look of the whirling clouds that cover the entire surface of the planet. Speaking of which, let's take a look at some fun Venus facts...
- Venus is the brightest object in Earth's sky after the Sun and Moon.
- The surface of Venus is not visible through the complete cloud cover. These clouds are droplets of sulfuric acid, and they are pushed around constantly by permanent hurricane force winds.
- Venus' atmosphere is crushing at 90 atmospheres of pressure. That's the equivalent of being half a mile underwater on earth.
- It takes Venus 243 Earth days for it to complete one of its own days. In addition, it rotates backwards from Earth and has no magnetic field.
- Venus is a mere 5% smaller than Earth, and has a similar composition as Earth.
- Venus was first visited in 1962 by the Mariner 2 spacecraft.
The Nine Planets
Saturday, December 03, 2011
Solar System: Mercury
- Mercury's day lasts for a Mercury year and a half. Alaska's got nothing on these long days.
- Mercury has no atmosphere because it all got boiled away from being so close to the Sun.
- One side of Mercury is 430 C, and the other is -180 C. The slow rotation keeps the hot side hot, and the cold side cold. This makes for the most extreme temperature variations of any planet in our solar system.
- If it wasn't for the gravitational compression that the Earth exerts on itself, Mercury would be the densest planet in our solar system.
- Mercury was first visited by the Mariner 10 spacecraft in 1974.
The Nine Planets
Universe Today
National Geographic
Solar System: The Sun
- The sun accounts for 99.8% of the mass in our solar system.
- It's approximately 4.5 billion years old, which is about middle aged for its expected lifespan.
- It's composed of about 70% hydrogren, 28% helium, and the rest is assorted metals. If you do the math, there's more than 10 times more metal in the Sun than in the entire rest of our solar system.
- The Sun's light comes from the fusion reactions taking place, where hydrogen is turned into helium.
- The Sun's output isn't constant. During a period of time in the 17th century, the Sun was less "active" and it caused a mini ice age on Earth.
The Nine Planets