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HH 211, Metal Print

HH 211, Metal Print

Regular price $75.99 USD
Regular price Sale price $75.99 USD
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Bring the Universe Home: High-Quality Metal Prints

Transform your space with stunning cosmic wonders. These high-quality metal prints showcase the universe's vibrant colors and intricate details in a way that has never been seen before.

Lasting Visions of the Cosmos:

Scratch- and Fade-Resistant: Crafted with a durable aluminum surface, these prints withstand everyday wear and tear.

Exceptional Vibrancy: The meticulous printing process utilizes the metal's reflective properties to create stunningly vivid colors that bring the cosmos to life.

Easy to Care For: Simply wipe clean with a damp cloth, making them ideal for high-traffic areas.

Multiple Sizes Available: Find the perfect fit for your space, whether you're seeking a captivating focal point or a mesmerizing gallery wall.

Modern Elegance:

These metal prints have a sleek, contemporary look that adds a touch of sophistication. The artwork appears almost luminescent against the wall, adding a unique dimension to your décor.

About this image

NASA's James Webb Space Telescope's high-resolution, near-infrared view of Herbig-Haro 211 reveals exquisite detail of the outflow from a young star, an infantile analogue of our Sun. Herbig-Haro objects are formed when stellar winds or jets of gas spewing from newborn stars collide with nearby gas and dust at high speeds, creating shock waves.

The image showcases a series of bow shocks to the southeast (lower left) and northwest (upper right), as well as the narrow bipolar jet that powers them in unprecedented detail. Molecules excited by the turbulent conditions, including molecular hydrogen, carbon monoxide, and silicon monoxide, emit infrared light, which is collected by Webb, mapping out the structure of the outflows.

Constellation             Perseus

Distance                    1,000 light-years

Exposure Dates        28 Aug 2022

Size and materials

Format: Metal Print

Size: 8″×10″, 16″×20″, 24″×36″

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Image credit

                       ESA/Webb, NASA, CSA, Tom Ray (Dublin)

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