- Date: September 2016
- Location: France, Alpes, Haute-Savoie
- Camera: Moravian G4 CCD (Kaf 16803)
- Optics: Takahashi FSQ-106
- Mount: EQ6 Pro Evolution
- Filters: Astrodon LRGB Astrodon
- Exposure: L 84 x 600s, RGB 10 x 600s each. Total 19 hours.
Many people imagine outer space to be a complete vacuum, devoid of any material. Although the interstellar regions are more devoid of matter than any vacuum artificially created on earth, there is matter in space, which is clearly seen in this wonderful wide-field image of the Iris nebula made by Idir Saci from France. We refer to this material as the Interstellar Medium and it consists mainly of gas (99%) and dust.
75% of the mass of the interstellar gas is in the form of hydrogen (either molecular or atomic), with the remaining 25% as helium. The interstellar gas consists partly of neutral atoms and molecules, as well as charged particles, such as ions and electrons. This gas is extremely dilute, with an average density of about 1 atom per cubic centimeter. (For comparison, the air we breathe has a density of approximately 25,000,000,000,000,000,000 molecules per cubic centimeter). Even though the interstellar gas is very dilute, the amount of matter adds up over the vast distances between the stars. The interstellar gas is typically found in two forms: cold clouds of neutral atomic or molecular hydrogen and hot ionized hydrogen near hot young stars.
The cold clouds of neutral or molecular hydrogen are the birthplace of new stars if they become gravitationally unstable and collapse. The neutral and molecular forms emit radiation in the radio band of the electromagnetic spectrum.
The ionized hydrogen is produced when large amounts of ultraviolet radiation are released by hot newly-formed stars. This radiation ionizes the surrounding clouds of gas. Visible light is emitted when electrons recombine with the ionized hydrogen, which is seen as beautiful red colors of emission nebulae.
Interstellar dust is not like the dust that you might find under your bed; it is made of very different substances. These dust particles are extremely small, just a fraction of a micron across, which happens to be approximately the wavelength of blue light waves. The particles are irregularly shaped, and are composed of silicates, carbon, ice and/or iron compounds.
When light from other stars passes through the dust, a few things can happen. If the dust is thick enough, the light will be completely blocked, leading to dark areas. These dark clouds are known as dark nebulae.
Light passing through a dust cloud may not be completely blocked, although all wavelengths of light passing through will be dimmed somewhat. This phenomenon is known as extinction. The extinction is caused by the light being scattered off of the dust particles out of our line of sight, preventing the light from reaching us. The amount that the light is dimmed depends upon a few factors, including the thickness and density of the dust cloud, as well as the wavelength (color) of the light.
Because of the size of the dust particles, scattering of blue light is favored. Therefore, less of the blue light reaches us, which means that the light that reaches us is more red than it would have been without the interstellar dust. This effect is known as interstellar reddening (this is not the same thing as redshift, which is due to the effects of relative movement between a light source and its receiver). This process is similar to those that make the sun red at sunset. In turn, a dust cloud that is illuminated by star light, when viewed from the side, appears blue. This is similar to the blue sky we see, which is produced by sunlight scattered by the Earth’s atmosphere.
Aside from passing through, or being blocked from passing through, interstellar dust, light may also be reflected from the clouds of dust. This is seen as a reflection nebula, like the iris nebula in the Idir’s picture above.
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