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Sharpless 2-106 - Nebula
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Sharpless 2-106

description Sharpless 2-106 Overview

Sharpless 2-106 is a bipolar H II nebula in Cygnus, shaped by the massive young star S106 IR and imaged in detail by Gemini North in 2010.

help Sharpless 2-106 FAQ

What kind of astronomical object is Sharpless 2-106?

Sharpless 2-106 is an emission nebula characterized by its distinct bipolar shape, making it look like an hourglass or a cosmic snow angel. It is classified as an H II region located in the northern constellation of Cygnus.

What creates the unique bipolar shape of Sharpless 2-106?

The nebula's dramatic shape is created by a massive, young stellar object designated as S106 IR. The central star's high-speed particles and radiation squeeze the surrounding gas into two opposing lobes of glowing plasma.

What telescope famously captured detailed images of Sharpless 2-106?

The Gemini North telescope, located atop Mauna Kea in Hawaii, captured incredibly detailed images of the nebula in 2010. These high-resolution images allowed astronomers to clearly see the complex gas and dust structures surrounding the central star.

Where is the Sharpless 2-106 catalog name derived from?

The "Sharpless" catalog was compiled by the American astronomer Stewart Sharpless in the 1950s. He cataloged over 300 H II regions across the Milky Way galaxy, giving this object its official designation.

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