Emission nebulae tend to
be red in color because
of the abundance of hydrogen. Additional colors, such as blue and green, can be produced by the atoms of other elements, but hydrogen is almost always the most abundant. A fine example of an emission nebula is the Orion Nebula (M42).
What does the spectrum of an emission nebula look like?
Not all nebulae are galaxies; some have completely different spectra than do the galaxies. Instead of looking like stars, they show only
a few bright, narrow lines of pure red, blue, or green color from a continuous background
.
What are the characteristics of an emission nebula?
Emission nebulae are clouds of ionised gas that, as the name suggests,
emit their own light at optical wavelengths
. Their mass generally ranges from 100 to 10,000 solar masses and this material can be spread over a volume of less than light year to several hundred light years.
What does a nebula look like?
Most nebulae – clouds of interstellar gas and dust – are difficult if not impossible to see with the unaided eye or even binoculars. But the Orion Nebula is in a class nearly all by itself. It’s visible to the unaided eye on a dark, moonless night. To me, it looks like
a star encased in a globe of luminescent fog
.
What do emission nebulae do?
An emission nebula is a cloud
of interstellar gas and dust that emits light in different colours
. There are several different types of emission nebulae with diverse sources of energy that are responsible for the glowing of gas and dust.
What color do emission nebulae have in common?
Emission nebulae are usually
red
, because hydrogen, the most common gas in the universe, most commonly emits red light. Reflection nebulae are clouds of dust that simply reflect the light of a nearby star or stars. Reflection nebulae are usually blue, because blue light scatters more easily.
What is the difference between an emission and a reflection nebula?
Emission Nebula – An emission nebula is a cloud of high temperature gas. … Reflection Nebula – A reflection nebula differs from an emission nebula
in that it does not emit radiation of its own
. It is a cloud of dust and gas that reflects the light energy from a nearby star or group of stars.
Why doesn’t the sun create an emission nebula?
Our Sun would not produce much of an emission nebula
because it emits very little ultraviolet (UV) light
. What little UV light emitted by our Sun, would be quickly absorbed by the gas nearest the Sun and the inner emission nebula would be hidden by the glare of sunlight.
Which two ingredients are needed to make an emission nebula?
9. Which two ingredients are needed to make an emission nebula? A.
Interstellar gas and dust
.
What two things are needed to create an emission nebula?
| Term Interstellar gas is composed mainly of Definition 90% hydrogen, 9% helium by weight | Term What two things are needed to create an emission nebulae? Definition hot stars and interstellar gas, particularly hydrogen |
|---|
What if we were inside a nebula?
Simple. After gathering the data on our own Sun, we can calculate the expected brightness of the neighboring stars. If we did live inside a nebula, we’d
notice that our star was much brighter compared to others
. The nebula would be dimming the light coming in from outside of it.
How do you see a nebula?
To find the nebula, look
below the three stars of Orion’s Belt
(or above, if viewing from the southern hemisphere). You will see a faint line of stars, which make up Orion’s sword. The nebula is halfway down the sword and will appear as a fuzzy-looking star. Looking for stargazing tips?
What causes a nebula?
A nebula is a giant cloud of dust and gas in space. Some nebulae (more than one nebula) come from
the gas and dust thrown out by the explosion of a dying star, such as a supernova
. Other nebulae are regions where new stars are beginning to form. For this reason, some nebulae are called “star nurseries.”
What are the different types of emission nebula?
Among the several different types of emission nebulae are H II regions, in which star formation is taking place and young, massive stars are the source of the ionizing photons; and
planetary nebulae
, in which a dying star has thrown off its outer layers, with the exposed hot core then ionizing them.
How are emission nebula formed?
Essentially, an Emission Nebulae is either
when the star is being created or when it has died
. Emission nebulae located in regions of star formation are lit up by the young protostars that are currently being formed. Over time the gas and dust will either be consumed by the star or form the orbiting planets.
Can emission nebulae form stars?
Emission Nebula / Star-Forming Region
The density attracts matter and eventually becoming
dense
enough to create the formation of stars. The remaining material is then believed to form planets and other planetary system objects.
