The Daily Insight
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Where are HII regions found?

H II regions are found only in spiral galaxies like the Milky Way and irregular galaxies. They are not seen in elliptical galaxies. In irregular galaxies, they may be dispersed throughout the galaxy, but in spirals they are most abundant within the spiral arms.

What is h2 in astronomy?

H II region, also called diffuse nebula or emission nebula, interstellar matter consisting of ionized hydrogen atoms. The energy that is responsible for ionizing and heating the hydrogen in an emission nebula comes from a central star that has a surface temperature in excess of 20,000 K.

What is an HII region in the Milky Way?

HII regions are emission nebulae created when young, massive stars ionise nearby gas clouds with high-energy UV radiation. They are composed primarily of hydrogen, hence the name (astronomers use the term HII to refer to ionised hydrogen, HI for neutral hydrogen), and have temperatures of around 10,000 Kelvin.

Where are emission nebulae HII regions found?

interstellar medium
Some of the most beautiful extended objects that we can see are HII regions, or diffuse or emission nebulae. So-named because they contain mostly ionized hydrogen (H+ or HII), HII regions are found throughout the interstellar medium in the Galaxy and in other galaxies.

How much hydrogen is in interstellar space?

The actual density of hydrogen as it exist in interstellar space is on the average of about 1 atom per cubic centimeter. In the extremes, as low as 0.1 atom per cubic centimeter has been found in the space between the spiral arms and as high as 1000 atoms per cubic centimeter are known to exist near the galactic core.

Why do H II regions glow?

The Rosette is a prominent star formation region, glowing due to ultraviolet light from the young, hot, blue stars whose winds also cleared the central hole. Image Credit. In this case, the HII clouds (blue) are surrounding hot, young stars (yellow).

How molecular hydrogen is formed?

Molecular Hydrogen, commonly written H2, is a molecule formed by two hydrogen atoms that share their electrons. H2 is a molecule formed by two hydrogen atoms that share their electrons. In astronomy, molecular hydrogen is notoriously difficult to detect.

What is the space between stars called?

In astronomy, the interstellar medium (ISM) is the matter and radiation that exist in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space.

Is there any medium in space?

The common explanation for this is that space is a vacuum and so there’s no medium for sound to travel through. Space is never completely empty – there are a few particles and sound waves floating around.

Is there any oxygen in space?

In space, there is very little breathable oxygen. A ground—based experiment by an experimental astrophysicist at Syracuse University found that oxygen atoms cling tightly to stardust. Their spacesuits are outfitted with a backpack called the Primary Life Support Subsystem that provides breathable oxygen.

How hot is interstellar gas?

8000 Kelvin
The hottest interstellar gas has a temperature of 8000 Kelvin (or more). (The Solar System, by the way, seems to be located within a large, low-density bubble within the interstellar medium.)

Why is H2 not h?

Molecular hydrogen gas, or H2, is the primary form in which hydrogen is found. Because there are two hydrogen atoms, we call this diatomic hydrogen, di meaning two. Because the hydrogen atoms are covalently bonded together they form a molecule; so H2 is also referred to as molecular hydrogen.

What is an H II region?

Areas in space which are luminous with the emission spectrum of ionized hydrogen are called H II regions. They are associated with the presence of massive O-type and B-type stars.

What is another name for the HII region?

Alternative Titles: HII region, diffuse nebula, ionized hydrogen cloud. H II region, also called diffuse nebula or emission nebula, interstellar matter consisting of ionized hydrogen atoms.

What is the temperature of H2 region?

When an H II region is produced from cold molecular gas by the formation of a hot star, the temperature is raised from roughly 25 to 8,000 K, and the number of particles per cubic centimetre is almost quadrupled because each H 2 molecule is split into two ions and two electrons.

What is the largest H II region in our galaxy?

The largest H II regions (none of which occur in the Milky Way Galaxy) are 500 light-years across and contain at least 100,000 solar masses of ionized gas. These enormous H II regions are powered by clusters of massive hot stars rather than by any single stellar body.