Celestial hemisphere:  Southern  ·  Constellation: Sagittarius (Sgr)  ·  Contains:  NGC 6559
A Reflection Nebula Embedded to an Emission Nebula in NGC 6559, Fernando
A Reflection Nebula Embedded to an Emission Nebula in NGC 6559
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A Reflection Nebula Embedded to an Emission Nebula in NGC 6559

A Reflection Nebula Embedded to an Emission Nebula in NGC 6559, Fernando
A Reflection Nebula Embedded to an Emission Nebula in NGC 6559
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A Reflection Nebula Embedded to an Emission Nebula in NGC 6559

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Description

NGC 6559 is a cloud of gas and dust located at a distance of about 5000 light-years from Earth, in the constellation of Sagittarius (The Archer).

The glowing region is a relatively small object, just a few light-years across, in contrast to the one

hundred light-years and more spanned by its famous neighbour, the Lagoon Nebula. Although it is usually overlooked in favor of its distinguished companion, I thought it is worthy capturing this image.

The gas in the clouds of NGC 6559, mainly hydrogen, is the raw material for star formation. When a region inside this nebula gathers enough matter, it starts to collapse under its own gravity. The centre of the cloud grows ever denser and hotter, until thermonuclear fusion begins and a star is born. The hydrogen atoms combine to form helium atoms, releasing energy that makes the star shine.

These brilliant hot young stars born out of the cloud energise the hydrogen gas still present around them in the nebula. The gas then re-emits this energy, producing the glowing threadlike red cloud seen near the centre of the image, as an emission nebula.

But NGC 6559 is not just made out of hydrogen gas. It also contains solid particles of dust, made of heavier elements, such as carbon, iron or silicon. The bluish patch next to the red emission nebula shows the light from the recently formed stars being scattered — reflected in many different directions — by the microscopic particles in the nebula. Then the reflection nebula,

usually appears blue because the scattering is more efficient for these shorter wavelengths of light.

In regions where it is very dense, the dust completely blocks the light behind it, as is the case for the dark isolated patches and sinuous lanes to the bottom left-hand side and right-hand side of the image. To look through the clouds at what lies behind,

The Milky Way fills the background of the image with countless older stars. Some of them appear fainter and redder because of the dust in NGC 6559.

Source: quantumday.com

Stack:

5 frames Ha 20 min

15 frames LRGB 15 min.

Telescope: LX200 f/10 with focal reducer f/6.3

Camera: Atik 314L

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A Reflection Nebula Embedded to an Emission Nebula in NGC 6559, Fernando