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Ced 110

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description Ced 110 Overview

Ced 110, also known as Cederblad 110, is a reflection nebula located within the Chamaeleon I molecular cloud complex. Illuminated by embedded young stars, the cloud of interstellar dust scatters blue light, making it visible to astronomers. The region is notable for its active star formation and the presence of young stellar objects, such as the dense core Cha-MMS1. It is primarily studied by astrophysicists and deep-sky observers interested in the early stages of stellar evolution.

help Ced 110 FAQ

What is Ced 110?

Ced 110, also called Cederblad 110, is a reflection nebula in the Chamaeleon I molecular cloud complex. It is made of interstellar dust that scatters light from nearby young stars.

Why does Ced 110 look blue?

The dust in Ced 110 scatters blue light from embedded or nearby young stars. This scattering effect is why reflection nebulae often appear blue in astronomical images.

Is Ced 110 a site of star formation?

Yes. Ced 110 lies in the active Chamaeleon I star-forming region, where dense clouds of gas and dust are associated with young stellar objects.

What is the difference between Ced 110 and a planetary nebula such as Abell 36?

Ced 110 is a reflection nebula associated with young stars and scattered starlight. Abell 36 is a planetary nebula made from material expelled by an evolved dying star.

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