- Normally ships in 7-10 business days, if we have to manufacture it.
- We do custom work at times. Have something in mind?
Solid Wood Frame
We use only real wood for our frames with that comes all the imperfections that come with using real wood.
The occasional knot and other character markings.
While we try to miss the knots in cutting out of the shapes some do make it into our finished frames.
This is what gives each one of our pieces an uniqueness.
Each frame is stained with a distressed pecan stain to help with the aged look we are going for and then topcoated with a polyurethane for long lasting life.
We use commercial grade professional waterbourne finishes that are better for the environment then solvent based finishes.
Wood is carved, sanded and stained, also the aluminum is cut and printed in-house.
Wood and aluminum are cut on specialized machinery and the aluminum is printed using a specialized printer.
Free Shipping on orders $500+
Everything is cut and printed in my Texas shop.
100% USA Made
This celestial object looks like a delicate butterfly. But it is far from serene.
What resemble dainty butterfly wings are actually roiling cauldrons of gas heated to more than 36,000 degrees Fahrenheit. The gas is tearing across space at more than 600,000 miles an hour—fast enough to travel from Earth to the Moon in 24 minutes!
A dying star that was once about five times the mass of the Sun is at the center of this fury. It has ejected its envelope of gases and is now unleashing a stream of ultraviolet radiation that is making the cast-off material glow. This object is an example of a planetary nebula, so-named because many of them have a round appearance resembling that of a planet when viewed through a small telescope.
Cataloged as NGC 6302, but more popularly called the Butterfly Nebula. NGC 6302 lies within our Milky Way galaxy, roughly 3,800 light-years away in the constellation Scorpius. The glowing gas is the star's outer layers, expelled over about 2,200 years. The "butterfly" stretches for more than two light-years, which is about half the distance from the Sun to the nearest star, Alpha Centauri.
The central star itself cannot be seen, because it is hidden within a doughnut-shaped ring of dust, which appears as a dark band pinching the nebula in the center. The thick dust belt constricts the star's outflow, creating the classic "bipolar" or hourglass shape displayed by some planetary nebulae.
The star's surface temperature is estimated to be about 400,000 degrees Fahrenheit, making it one of the hottest known stars in our galaxy. Spectroscopic observations made with ground-based telescopes show that the gas is roughly 36,000 degrees Fahrenheit, which is unusually hot compared to a typical planetary nebula.
The nebula's reddish outer edges are largely due to light emitted by nitrogen, which marks the coolest gas visible in the picture. WFC3 is equipped with a wide variety of filters that isolate light emitted by various chemical elements, allowing astronomers to infer properties of the nebular gas, such as its temperature, density, and composition.
The white-colored regions are areas where light is emitted by sulfur. These are regions where fast-moving gas overtakes and collides with slow-moving gas that left the star at an earlier time, producing shock waves in the gas (the bright white edges on the sides facing the central star). The white blob with the crisp edge at upper right is an example of one of those shock waves.
September 9, 2009
Credit: NASA, ESA, and the Hubble SM4 ERO Team
Wall Decor Specs:
Solid Pine Wood Frame with Printed Aluminum Insert