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Similar Designs More Acrylic Prints from Leonhard Scheckkonstantinos Kifonidismax Planck Institute For Astrophysics

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Bring your artwork to life with the stylish lines and added depth of an acrylic print.   Your image gets printed directly onto the back of a 1/4" thick sheet of clear acrylic.

The image is the art - it doesn't get any cleaner than that!

All acrylic prints ship within 3 - 4 business days and arrive "ready to hang" with four aluminum mounting posts (Option #1) or hanging wire (Option #2).

The high gloss of the acrylic sheet complements the rich colors of any image to produce stunning results.

There are two different ways to mount your acrylic print.

Option #1 (Mounting Posts) - Attach your print to your wall with four aluminum mounting posts.   The cylindrical cap of each mounting post can be removed, allowing you to thread a small screw along the center axis of the of post and into the wall.   When you're finished, simply reattached each cap, and you're done.   The mounting posts act as stand-offs and keep your print separated from the wall by 1".   All of the required mounting hardware (i.e. posts, screws, and wall anchors) is included with your print.   Click here for mounting details.

Option #2 (Hanging Wire) - With this option, your acrylic print is attached to a 1/4" thick black board which has a wooden frame and hanging wire attached to the back.   There are no metal mounting posts at the corners.   Simply put a nail in your wall, hang your print from the hanging wire, and you're done.   Due to the thickness of the black board and mounting frame, your print is separated from the wall by 1.50"   Click here for mounting details.

Acrylic Print Reviews (1999)

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Supernova explosion. Image 1 of 4. Supercomputer simulation showing a supernova explosion of a 15- solar-mass star 0.05 seconds after core collapse. Supernovae occur when a massive star has run out of nuclear fuel and its core collapses to form a neutron star. The collapsed core triggers a shock wave that powers the supernova explosion. This simulation shows bubbles of hot, buoyant gas (light brown), 400 kilometres in diameter, that envelope the neutron star (unseen). In-falling cold gas bubbles are heated by neutrinos at the core. The heated gas rises and mixes with more in- falling cold gas resulting in turbulence. It is thought that neutrino-driven convection energy accompanies the shock wave to power the supernova explosion. Simulation created at the Max Planck Institute for Astrophysics, Germany. (For complete sequence, see images R730/094 - R730/097).

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Delivery

All acrylic prints ship from our production facility within 3 - 4 business days of your order.