Featured Research

from universities, journals, and other organizations

Cosmic Paintbursh Revealed: Force That Shapes Nebulae Uncovered By Astronomers

Date:
January 25, 2001
Source:
University Of Rochester
Summary:
The cosmic “paintbrush” that creates some of the most dazzling images in the night sky may have been found by researchers at the University of Rochester, a paper in the January 25 issue of Nature suggests. A magnetic dynamo similar to the kind that produces storms on our sun appears to shape planetary nebulae, the wispy clouds of light that radiate from some dying stars.

The cosmic “paintbrush” that creates some of the most dazzling images in the night sky may have been found by researchers at the University of Rochester, a paper in the January 25 issue of Nature suggests. A magnetic dynamo similar to the kind that produces storms on our sun appears to shape planetary nebulae, the wispy clouds of light that radiate from some dying stars. The scientists have shown that as some stars die and expel their outer layers, they generate massive magnetic fields that twist the radiating material into beautiful and distinctive shapes.

Related Articles


“Astronomers have been puzzling over these objects for centuries,” says Adam Frank, associate professor of physics and astronomy. “They’re these vast cosmic sculptures and we’ve never known how they’re made.”

The group of scientists designed a model based on a typical star as it approached the last years of its life. Using data that suggests that the core of such a star decouples from the outer shell of the star like a yolk spinning inside an egg, the researchers found that magnetic fields power up and twist as the two spin at different rates. As matter is blown off the dying star, it roughly follows these bent magnetic lines, creating the majestic curves and contours of a planetary nebula.

The idea that magnetic fields play a role in shaping the material thrown off by dying stars has been addressed before, but the researchers had only looked at the activity of the outer shell, concluding that it could not generate fields of the necessary strength. It took a combination of University astronomers working in two different areas to define the new model and show that such strength is possible.

Astrophysicists John H. Thomas, Andrew Markiel and Hugh Van Horn, specialists in understanding the magnetic characteristics of stars, teamed up with astrophysicists Adam Frank and Eric Blackman, experts in planetary nebulae formation. “This paper probably couldn’t have been written by any one of us,” says Thomas, professor of mechanical and aerospace sciences and of astronomy. “We had a hunch that our two areas were related to this problem, and it took both to figure it out.”

The new model is reinforced by another well-known phenomenon. The leftover core of such stars, called a white dwarf, is known to spin more slowly than scientists have thought it should. The Nature paper suggests that the core is slowed by “magnetic braking”—a sort of drag produced by the magnetic fields twisting up like a wrung towel that gets harder and harder to twist. As this is happening, the surface of the white dwarf is thrown out into space along those magnetic lines, slowing its rotation further much as a skater’s spin slows when she extends her arms.

“The dynamo-generated magnetic field that we’ve proposed may explain many other phenomena of planetary nebulae, such as the launching of the stellar wind,” says Thomas. “This is potentially the kind of unifying concept that one seeks in science.” The implications of the research reach beyond nebulae. The same processes that generate the magnetic fields in dying stars are also at work in our own sun.

“This shows us a new way for our sun to die,” says Frank. Sunspots, solar storms and coronal mass ejections that endanger power grids and satellites are all directly caused by magnetic fields generated in the sun. When our sun runs out of fuel in a scant four or five billion years, we may be treated to front-row seats as its insides knot up and it sheds its skin in graceful arcs wider than our solar system.


Story Source:

The above story is based on materials provided by University Of Rochester. Note: Materials may be edited for content and length.


Cite This Page:

University Of Rochester. "Cosmic Paintbursh Revealed: Force That Shapes Nebulae Uncovered By Astronomers." ScienceDaily. ScienceDaily, 25 January 2001. <www.sciencedaily.com/releases/2001/01/010125082804.htm>.
University Of Rochester. (2001, January 25). Cosmic Paintbursh Revealed: Force That Shapes Nebulae Uncovered By Astronomers. ScienceDaily. Retrieved October 24, 2014 from www.sciencedaily.com/releases/2001/01/010125082804.htm
University Of Rochester. "Cosmic Paintbursh Revealed: Force That Shapes Nebulae Uncovered By Astronomers." ScienceDaily. www.sciencedaily.com/releases/2001/01/010125082804.htm (accessed October 24, 2014).

Share This



More Space & Time News

Friday, October 24, 2014

Featured Research

from universities, journals, and other organizations


Featured Videos

from AP, Reuters, AFP, and other news services

Raw: China Launches Moon Orbiter

Raw: China Launches Moon Orbiter

AP (Oct. 24, 2014) — China launched an experimental spacecraft Friday to fly around the moon and back to Earth in preparation for the country's first unmanned return trip to the lunar surface. (Oct. 24) Video provided by AP
Powered by NewsLook.com
China Prepares Unmanned Mission To Lunar Orbit

China Prepares Unmanned Mission To Lunar Orbit

Newsy (Oct. 23, 2014) — The mission is China's next step toward automated sample-return missions and eventual manned missions to the moon. Video provided by Newsy
Powered by NewsLook.com
Russian Cosmonauts Kick Off Final Spacewalk of 2014

Russian Cosmonauts Kick Off Final Spacewalk of 2014

Reuters - US Online Video (Oct. 22, 2014) — Russian cosmonauts Maxim Suraev and Alexander Samokutyaev step outside the International Space Station to perform work on the exterior of the station's Russian module. Rough Cut (no reporter narration) Video provided by Reuters
Powered by NewsLook.com
Comet Siding Spring Grazes Mars' Atmosphere

Comet Siding Spring Grazes Mars' Atmosphere

Newsy (Oct. 19, 2014) — A comet from the farthest reaches of the solar system passed extremely close to Mars this weekend, giving astronomers a rare opportunity to study it. Video provided by Newsy
Powered by NewsLook.com

Search ScienceDaily

Number of stories in archives: 140,361

Find with keyword(s):
 
Enter a keyword or phrase to search ScienceDaily for related topics and research stories.

Save/Print:
Share:  

Breaking News:

Strange & Offbeat Stories

 

Space & Time

Matter & Energy

Computers & Math

In Other News

... from NewsDaily.com

Science News

Health News

Environment News

Technology News



Save/Print:
Share:  

Free Subscriptions


Get the latest science news with ScienceDaily's free email newsletters, updated daily and weekly. Or view hourly updated newsfeeds in your RSS reader:

Get Social & Mobile


Keep up to date with the latest news from ScienceDaily via social networks and mobile apps:

Have Feedback?


Tell us what you think of ScienceDaily -- we welcome both positive and negative comments. Have any problems using the site? Questions?
Mobile iPhone Android Web
Follow Facebook Twitter Google+
Subscribe RSS Feeds Email Newsletters
Latest Headlines Health & Medicine Mind & Brain Space & Time Matter & Energy Computers & Math Plants & Animals Earth & Climate Fossils & Ruins