Ring Nebula: Synchrotron Radiation & Magnetic Fields

In summary, the Ring Nebula is due to synchrotron radiation of particles (electrons) with higher energy (spin) being blueshifted the closer they are to the white dwarf at the center. The magnetic field that spins the electrons intensly and the futher away the electrons are from the field, the less spin, and are redshifted with distance.
  • #1
DB
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Is the beauty and color to the Ring Nebula due to synchrotron radiation of particles (electrons) with higher energy (spin) being blueshifted the closer they are to the white dwarf at the center? If so is it the magnetic field that spins the electrons intensly and the futher away the electrons are from the field, the less spin, and are redshifted with distance?

Pic:
http://www.tivas.org.uk/archive/images/ring-nebula_m57.jpg

Thnx
 
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  • #2
http://antwrp.gsfc.nasa.gov/apod/ap030322.html

Astronomers of the Hubble Heritage Project produced this strikingly sharp image from Hubble Space Telescope observations using natural appearing colors to indicate the temperature of the stellar gas shroud. Hot blue gas near the energizing central star gives way to progressively cooler green and yellow gas at greater distances with the coolest red gas along the outer boundary
 
  • #3
Thnx Phobos, after looking through the link, (http://heritage.stsci.edu/1999/01/fast_facts.html) it's seems that this a false colour image with Red being assigned to Nitrogen II, Green to Oxygen III and Blue to Helium II. So this isn't what it actually looks like in space?
 
  • #4
DB said:
So this isn't what it actually looks like in space?

Unfortunately not.

Human eyes aren't so good at seeing color from faint objects. You need long-time exposures onto film (or digital) to capture colors. Plus, astronomers usually mess with the colors in the photos in order to bring out certain details they're studying.

If you were present within a nebula, it would be too thin to notice right around you (space would still look empty around you). From further away, it would probably look like a gray cloud (which is how it looks through a telescope).

Maybe we could see some faint colors if we had bigger, more sensitive eyes. :bugeye:
 
  • #6
Side note...it may be possible to see some color in a nebula (not sure how much) if it were bright enough/if you were at the right distance/etc...but certainly nothing like the photos.
 

1. What is the Ring Nebula?

The Ring Nebula, also known as Messier 57 or NGC 6720, is a planetary nebula located in the constellation of Lyra. It is a cloud of glowing gas and dust that was formed when a dying star shed its outer layers.

2. What is synchrotron radiation in relation to the Ring Nebula?

Synchrotron radiation is a type of electromagnetic radiation emitted by charged particles moving at high speeds in a magnetic field. In the case of the Ring Nebula, this radiation is produced by electrons spiraling around the magnetic field lines in the nebula.

3. How does synchrotron radiation affect the appearance of the Ring Nebula?

Synchrotron radiation contributes to the bright, extended ring-like structure of the Ring Nebula. The emission of this type of radiation is strongest in regions where the magnetic field is most intense, which creates the distinct shape of the nebula.

4. What role do magnetic fields play in the Ring Nebula?

Magnetic fields play a crucial role in shaping and maintaining the structure of the Ring Nebula. They help to confine and channel the gas and dust ejected by the dying star, and also contribute to the emission of synchrotron radiation.

5. What can studying the Ring Nebula's magnetic fields and synchrotron radiation tell us about the universe?

Studying the Ring Nebula's magnetic fields and synchrotron radiation can provide insight into the physical processes that occur in the final stages of a star's life. It can also help us better understand the role of magnetic fields in shaping and influencing the evolution of objects in the universe, such as galaxies and clusters of galaxies.

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