Featured Research

from universities, journals, and other organizations

Far Ultraviolet Spectroscopic Explorer (FUSE) Spacecraft Sees Solar System Under Construction

Date:
August 22, 2001
Source:
NASA/Goddard Space Flight Center
Summary:
A nearby young star recently gave birth to millions of comets, according to new observations using NASA's Far Ultraviolet Spectroscopic Explorer (FUSE) spacecraft. The result provides clues to how our own solar system formed and evolved.

A nearby young star recently gave birth to millions of comets, according to new observations using NASA's Far Ultraviolet Spectroscopic Explorer (FUSE) spacecraft. The result provides clues to how our own solar system formed and evolved.

Related Articles


The star, Beta Pictoris, is estimated to be about 20 million years old, relatively young for a star whose life will span billions of years. It is about 60 light years from Earth, in the direction of the southern constellation Pictor (Painter's Easel). (One light year is almost 6 trillion miles, or about 9.6 trillion kilometers.) A 200 billion-mile diameter disk of dust and gas surrounds Beta Pictoris, and previous observations have given hints that planets may be forming (or recently formed) deep within.

The new research by an international team of astronomers shows how the chemistry of the disk implies that comets have formed around Beta Pictoris as well, and gives additional evidence that these comets are evaporating by the millions. The journal Nature will publish this research August 16.

"We are very excited about these observations because they are a rare glimpse at the chaotic birth of a solar system," said Dr. George Sonneborn, FUSE Project Scientist at NASA's Goddard Space Flight Center in Greenbelt, Md. "Young planetary systems are surprisingly active; we are witnessing the birth and evaporation of millions and millions of comets."

A team of scientists from the Institut d'Astrophysique de Paris-CNRS (IAP, France) led by Dr. Alain Lecavelier des Etangs, together with colleagues from the Johns Hopkins University (Baltimore, Md.), and the Laboratoire d'Astrophysique de Marseille (France), has found no evidence of molecular hydrogen (H2), the most abundant molecule in the universe, in the Beta Pictoris disk. This was unexpected because the same team, using the Hubble Space Telescope, had previously found carbon monoxide (CO) in the Beta Pictoris disk. What is seen in the Beta Pictoris system is thus contrary to what is commonly seen in the gaseous clouds of our galaxy, where CO is only seen when H2 is present. When these clouds collapse, they form new stars and planetary systems; thus, they are the raw material for new solar systems like Beta Pictoris.

"In interstellar gas clouds, carbon monoxide gets broken apart by starlight in about 1,000 years, a relatively short time compared to the estimated 20 million-year age of Beta Pictoris. Since we still see carbon monoxide, we think the amount originally present in the cloud that formed Beta Pictoris is now locked up in some kind of reservoir where it is shielded from starlight as it is slowly released back into the Beta Pictoris disk," said Dr. Alfred Vidal-Madjar of IAP.

"Add this to the fact that the amount of molecular hydrogen is too low to be seen by FUSE. This is strange because normally there are about 100,000 molecular hydrogen molecules for every carbon monoxide molecule in interstellar gas clouds. So we think the molecular hydrogen has been locked away in some kind of reservoir also," said Lecavelier.

According to the researchers, comets, which consist largely of frozen gasses, are a likely reservoir. "In our own solar system, there is a swarm of thousands, perhaps millions, of comets beyond the orbit of Pluto, called the Kuiper belt. If a similar comet swarm surrounds Beta Pictoris, the comets would still be warm enough to slowly release carbon monoxide, but far too cold to release molecular hydrogen, which would remain locked up as water ice (H2O)," said Dr. Paul Feldman of the Johns Hopkins University.

FUSE uncovered new mysteries in the Beta Pictoris disk as well. "It gets really exciting when we compare our result to others," said Feldman. "Previous observations of infrared emission from Beta Pictoris with the Infrared Space Observatory actually contradict our lack of detection of ultraviolet absorption by molecular hydrogen along a narrow line-of-sight to the star. They claim to have detected a large amount of molecular hydrogen in the disk. If both results are correct, the only way for this conflict to be resolved is if the molecular hydrogen is not evenly distributed throughout the disk."

Molecular hydrogen absorbs certain kinds of ultraviolet light; when it does so, FUSE can detect its presence, but molecular hydrogen has to be more or less evenly distributed in a cloud to block ultraviolet light from stars behind the cloud, or it won't reveal itself to FUSE. However, molecular hydrogen can also emit infrared light; celestial objects containing molecular hydrogen will glow in infrared if they are warm enough, and can be seen directly by the Infrared Space Observatory, depending on how close they are and how brightly they glow.

"The molecular hydrogen clumps could be left over gas from the formation of the star, or perhaps from failed protoplanets. The initial carbon monoxide would no longer be in gaseous form but rather condensed into cometesimals or comets. All we can say for certain is that carbon monoxide must be continuously generated in the disk," said Feldman.

FUSE is a NASA Origins mission developed and operated by The Johns Hopkins University in collaboration with NASA's Goddard Space Flight Center, the Centre National d'Etudes Spatiales (France), the Canadian Space Agency, the University of Colorado, and the University of California, Berkeley. FUSE was launched on June 24, 1999, from Cape Canaveral on a three-year mission to obtain high resolution spectra in the far ultraviolet wavelength region (905-1185 Angstroms) of faint objects within and beyond our galaxy.

For more information about FUSE, refer to:

http://fuse.pha.jhu.edu

For images of the Beta Pictoris disk, refer to:

http://www.iap.fr/betapic/images/images_index_e.html

http://oposite.stsci.edu/pubinfo/PR/96/02.html

Planet-forming disks around other stars:

http://oposite.stsci.edu/pubinfo/pr/1999/03/index.html

http://oposite.stsci.edu/pubinfo/PR/1999/05/index.html


Story Source:

The above story is based on materials provided by NASA/Goddard Space Flight Center. Note: Materials may be edited for content and length.


Cite This Page:

NASA/Goddard Space Flight Center. "Far Ultraviolet Spectroscopic Explorer (FUSE) Spacecraft Sees Solar System Under Construction." ScienceDaily. ScienceDaily, 22 August 2001. <www.sciencedaily.com/releases/2001/08/010821074522.htm>.
NASA/Goddard Space Flight Center. (2001, August 22). Far Ultraviolet Spectroscopic Explorer (FUSE) Spacecraft Sees Solar System Under Construction. ScienceDaily. Retrieved December 20, 2014 from www.sciencedaily.com/releases/2001/08/010821074522.htm
NASA/Goddard Space Flight Center. "Far Ultraviolet Spectroscopic Explorer (FUSE) Spacecraft Sees Solar System Under Construction." ScienceDaily. www.sciencedaily.com/releases/2001/08/010821074522.htm (accessed December 20, 2014).

Share This


More From ScienceDaily



More Space & Time News

Saturday, December 20, 2014

Featured Research

from universities, journals, and other organizations


Featured Videos

from AP, Reuters, AFP, and other news services

Spokesman: 'NORAD Ready to Track Santa'

Spokesman: 'NORAD Ready to Track Santa'

AP (Dec. 19, 2014) Pentagon spokesman Rear Adm. John Kirby said that NORAD is ready to track Santa Claus as he delivers gifts next week. Speaking tongue-in-cheek, he said if Santa drops anything off his sleigh, "we've got destroyers out there to pick them up." (Dec. 19) Video provided by AP
Powered by NewsLook.com
NASA's Planet-Finding Kepler Mission Isn't Over After All

NASA's Planet-Finding Kepler Mission Isn't Over After All

Newsy (Dec. 18, 2014) More than a year after NASA declared the Kepler spacecraft broken beyond repair, scientists have figured out how to continue getting useful data. Video provided by Newsy
Powered by NewsLook.com
Rover Finds More Clues About Possible Life On Mars

Rover Finds More Clues About Possible Life On Mars

Newsy (Dec. 17, 2014) NASA's Curiosity rover detected methane on Mars and organic compounds on the surface, but it doesn't quite prove there was life ... yet. Video provided by Newsy
Powered by NewsLook.com
Evidence of Life on Mars? NASA Rover Finds Methane, Organic Chemicals

Evidence of Life on Mars? NASA Rover Finds Methane, Organic Chemicals

Reuters - US Online Video (Dec. 16, 2014) NASA's Mars Curiosity rover finds methane in the Martian atmosphere and organic chemicals in the planet's soil, the latest hint that Mars was once suitable for microbial life. Linda So reports. Video provided by Reuters
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