NASA's WISE Catches Aging Star Erupting With Dust

[Date Prev] [Date Next] [Thread Prev] [Thread Next] [Date Index] [Thread Index]

 



April 26, 2012

J.D. Harrington 
Headquarters, Washington 
202-358-5241 
j.d.harrington@xxxxxxxx 

Whitney Clavin 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-4673 
whitney.clavin@xxxxxxxxxxxx 

RELEASE: 12-131

NASA'S WISE CATCHES AGING STAR ERUPTING WITH DUST

WASHINGTON -- Images from NASA's Wide-field Infrared Survey Explorer 
(WISE) reveal an old star in the throes of a fiery outburst and 
spraying the cosmos with dust. The findings offer a rare, real-time 
look at the process by which stars like our sun seed the universe 
with building blocks for other stars, planets and even life. 

The star, catalogued as WISE J180956.27-330500.2, was discovered in 
images taken during the WISE survey in 2010, the most detailed 
infrared survey to date of the entire celestial sky. It stood out 
from other objects because it glowed brightly with infrared light. 
When compared to images taken more than 20 years ago, astronomers 
found the star was 100 times brighter. 

"We were not searching specifically for this phenomenon, but because 
WISE scanned the whole sky, we can find such unique objects," said 
Poshak Gandhi of the Japan Aerospace Exploration Agency (JAXA), lead 
author of a new paper to be published in the Astrophysical Journal 
Letters. 

Results indicate the star recently exploded with copious amounts of 
fresh dust, equivalent in mass to our planet Earth. The star is 
heating the dust and causing it to glow with infrared light. 

"Observing this period of explosive change while it is actually 
ongoing is very rare," said co-author Issei Yamamura of JAXA. "These 
dust eruptions probably occur only once every 10,000 years in the 
lives of old stars, and they are thought to last less than a few 
hundred years each time. It's the blink of an eye in cosmological 
terms." 

The aging star is in the "red giant" phase of its life. Our own sun 
will expand into a red giant in about 5 billion years. When a star 
begins to run out of fuel, it cools and expands. As the star puffs 
up, it sheds layers of gas that cool and congeal into tiny dust 
particles. This is one of the main ways dust is recycled in our 
universe, making its way from older stars to newborn solar systems. 
The other way, in which the heaviest of elements are made, is through 
the deathly explosions, or supernovae, of the most massive stars. 

"It's an intriguing glimpse into the cosmic recycling program," said 
Bill Danchi, WISE program scientist at NASA Headquarters in 
Washington. "Evolved stars, which this one appears to be, contribute 
about 50 percent of the particles that make up humans." 

Astronomers know of one other star currently pumping out massive 
amounts of dust. Called Sakurai's Object, this star is farther along 
in the aging process than the one discovered recently by WISE. 

After Poshak and his team discovered the unusual, dusty star with 
WISE, they went back to look for it in previous infrared all-sky 
surveys. The object was not seen at all by the Infrared Astronomical 
Satellite (IRAS), which flew in 1983, but shows up brightly in images 
taken as part of the Two Micron All-Sky Survey (2MASS) in 1998. 

Poshak and his colleagues calculated the star appears to have 
brightened dramatically since 1983. The WISE data show the dust has 
continued to evolve over time, with the star now hidden behind a very 
thick veil. The team plans to follow up with space and ground-based 
telescopes to confirm its nature and to better understand how older 
stars recycle dust back into the cosmos. 

NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif., manages and 
operates WISE for NASA's Science Mission Directorate in Washington. 
The spacecraft was put into hibernation mode after it scanned the 
entire sky twice, completing its main objectives. The principal 
investigator for WISE, Edward Wright, is at the University of 
California, Los Angeles. The mission was selected competitively under 
NASA's Explorers Program managed by the agency's Goddard Space Flight 
Center in Greenbelt, Md. The science instrument was built by the 
Space Dynamics Laboratory in Logan, Utah. The spacecraft was built by 
Ball Aerospace & Technologies Corp. in Boulder, Colo. Science 
operations and data processing take place at the Infrared Processing 
and Analysis Center at the California Institute of Technology 
(Caltech) in Pasadena. Caltech manages JPL for NASA. 

The IRAS mission was a collaborative effort between NASA (JPL), the 
Netherlands and the United Kingdom. The 2MASS mission was a joint 
effort between Caltech, the University of Massachusetts and NASA 
(JPL). Data are archived at the Infrared Processing and Analysis 
Center at Caltech. 

For more information about WISE, visit: 

http://www.nasa.gov/wise 

	
-end-



To subscribe to the list, send a message to: 
hqnews-subscribe@xxxxxxxxxxxxxxxxxxxxxx
To remove your address from the list, send a message to:
hqnews-unsubscribe@xxxxxxxxxxxxxxxxxxxxxx

[Index of Archives]     [JPL News]     [Cassini News From Saturn]     [NASA Marshall Space Flight Center News]     [NASA Science News]     [James Web Space Telescope News]     [JPL Home]     [NASA KSC]     [NTSB]     [Deep Creek Hot Springs]     [Yosemite Discussion]     [NSF]     [Telescopes]

  Powered by Linux