Students using NASA and NSF data make stellar discovery; win science team competition

December 10, 2000

Three high school students, using data from NASA's Chandra X-ray Observatory and the National Science Foundation's Very Large Array (VLA), today won first place in the Siemens-Westinghouse Science and Technology Competition in Washington, DC. The team award was based on their discovery of the first evidence of a neutron star in the nearby supernova remnant IC443.

Charles Olbert, 18, Christopher Clearfield, 18, and Nikolas Williams, 16, all of the North Carolina School for Science and Mathematics (NCSSM) in Durham, N.C., found a point-like source of X-rays embedded in the remains of the stellar explosion, or supernova. Based on both the X-ray and radio data, the students determined that the central object in IC443 is most likely a young and rapidly rotating neutron star - an object known as a pulsar.

"This is a really solid scientific finding," said Dr. Bryan Gaensler of the Massachusetts Institute of Technology, Cambridge, a pulsar expert who reviewed the paper for the team. "Everyone involved should be really proud of this accomplishment."

Taking advantage of Chandra's superior angular resolution, the students found the source embedded in a region known to be emitting particularly high-energy X-rays. They had access to Chandra data because their science teacher, Dr. Jonathan Keohane, had applied for observation time while associated with NASA's Goddard Space Flight Center, Greenbelt, M.D.

"The students really went through the whole analysis process themselves," Keohane said. "They even lived together all summer near the school to complete the research."

In order to confirm the evidence from Chandra, the students turned to Dale Frail of the National Radio Astronomy Observatory in Socorro, N.M., who gave the team VLA data on IC443. The information strengthened the team's case that a pulsar powers the supernova remnant by confirming the existence of the point-like source and discovering a cloud, or nebula, of high-energy electrons around the central object. Such nebulas are a common characteristic of pulsars.

"The experience of doing new and relevant science has been one of the most rewarding experiences I have ever had," said Olbert, lead author on the paper submitted to the Astrophysical Journal. "I never expected to publish a scientific paper while I was still in high school."

The remnant of the IC443 supernova is a well-studied object. Astronomers have searched this region (approximately 5,000 light-years from Earth) for the neutron star, created in the explosion, that they thought should be there, judging from the size and dynamics of the supernova remnant.
-end-
The Siemens-Westinghouse Science and Technology Competition is open to individuals and teams of high school students who develop independent research projects in the physical or biological sciences or mathematics. The NCSSM is a free statewide residential high school for students with a strong aptitude and interest in math and science. About 550 high school juniors and seniors reside on the school's campus.

The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program. The Smithsonian's Chandra X-ray Center, Cambridge, Mass., controls science and flight operations.

For more information on NASA's Chandra X-ray Observatory, visit the Chandra site at: http://chandra.harvard.edu and http://chandra.nasa.gov

NASA/Marshall Space Flight Center News Center

Related Supernova Articles from Brightsurf:

Scientists discover supernova that outshines all others
A supernova at least twice as bright and energetic, and likely much more massive than any yet recorded has been identified by an international team of astronomers, led by the University of Birmingham.

Supernova observation first of its kind using NASA satellite
Their research, detailed in the Monthly Notices of the Royal Astronomical Society, represents the first published findings about a supernova observed using TESS, and add new insights to long-held theories about the elements left behind after a white dwarf star explodes into a supernova.

Astronomers find possible elusive star behind supernova
Astronomers may have finally found a doomed star that seemed to have avoided detection before its explosive death.

Stellar thief is the surviving companion to a supernova
Hubble found the most compelling evidence that some supernovas originate in double-star systems.

Supernova may have 'burped' before exploding
Only by increasing the rate at which telescopes monitor the sky has it been possible to catch more Fast-Evolving Luminous Transients (FELTs) and begin to understand them.

An unusual white dwarf may be a supernova leftover
Astronomers have identified a white dwarf star in our galaxy that may be the leftover remains of a recently discovered type of supernova.

Researchers show how to make your own supernova
Researchers from the University of Oxford are using the largest, most intense lasers on the planet, to for the first time, show the general public how to recreate the effects of supernovae, in a laboratory.

The big star that couldn't become a supernova
For the first time in history, astronomers have been able to watch as a dying star was reborn as a black hole.

Seeing quadruple: Four images of the same supernova, a rare find
Galaxies bend light through an effect called gravitational lensing that helps astronomers peer deeper into the cosmos.

Explosive material: The making of a supernova
Pre-supernova stars may show signs of instability for months before the big explosion

Read More: Supernova News and Supernova Current Events
Brightsurf.com is a participant in the Amazon Services LLC Associates Program, an affiliate advertising program designed to provide a means for sites to earn advertising fees by advertising and linking to Amazon.com.