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Monday, September 24, 2007

NASA Restarts Telescope Mission to Detect Black Holes

NASA Restarts Telescope Mission to Detect Black Holes

NASA has made a decision to restart an astronomy mission that will have greater capability than any existing instrument for detecting black holes in the local universe.

The Nuclear Spectroscopic Telescope Array, or NuSTAR, will expand our understanding of the origins and destinies of stars and galaxies. NASA had stopped the study effort on the NuSTAR mission in 2006 due to funding pressures within the Science Mission Directorate.

"We are very excited to be able restart the NuSTAR mission, which we expect to be launched in 2011," said Alan Stern, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. "NuSTAR has more than 500 times the sensitivity of previous instruments that detect black holes. It's a great opportunity for us to explore an important astronomical frontier. We are getting more and more from the science budget we have, and the restart of the highly-valued NuSTAR mission is an example of that."

NuSTAR will bridge a gap between the 2009 launch of the Wide-field Infrared Survey Explorer and the 2013 launch of the James Webb Space Telescope. The spacecraft will map areas of the sky in the light of high-energy X-rays and complement astrophysics missions that explore the cosmos in other regions of the electromagnetic spectrum.

"NuSTAR will perform deep observations in hard X-rays to detect black holes of all sizes and other exotic phenomena," said Jon Morse, director of the Astrophysics Division at NASA Headquarters. "It will perform cutting-edge science using advanced technologies and help to provide a balance between small and large missions in the NASA astrophysics portfolio."

NuSTAR is a part of NASA's Explorer Program. The program provides frequent, low-cost access to space for missions with small- to mid-sized spacecraft. NuSTAR originally was selected from proposals submitted in response to an announcement of opportunity in 2003. Fiona Harrison of the California Institute of Technology, Pasadena, is the NuSTAR principal investigator.

NASA expects to select three additional Small Explorer missions for flight in the first half of the next decade through a competitive selection within the astrophysics and heliophysics scientific communities.

NASA's Jet Propulsion Laboratory, Pasadena, Calif. manages the NuSTAR mission. The Goddard Space Flight Center, Greenbelt, Md., manages the Explorer Program for the Science Mission Directorate. Orbital Sciences Corp., Dulles, Va., is the industry partner for the mission..


How We Detect Them

Black holes and neutron stars don't give off light, so we can't just look for them. However, astronomers can find black holes and neutron stars by observing the gravitational effects on other objects nearby.


Astronomers can discover some black holes and neutron stars because they are sources of x-rays. The intense gravity from a black hole or a neutron star will pull in dust particles from a surrounding cloud of dust or a nearby star. As the particles speed up and heat up, they emit x-rays. So the x-rays don't come directly from the black hole or neutron star, but from its effect on the dust around it. Although x-rays don't penetrate our atmosphere, astronomers use satellites to observe x-ray sources in the sky.

Rotating stars

Many stars rotate around each other, much as the planets orbit our Sun. When astronomers see a star circling around something, but they cannot see what that something is, they suspect a black hole or a neutron star.

Gravity lenses
Astronomers use a technique called gravity lensing to search for black holes and neutron stars. When a very massive object passes between a star and the earth, the object acts like a lens and focuses light rays from the star on the Earth. This causes the star to brighten.

How can a black hole or a neutron star act like a lens? The answer comes from Albert Einstein, who proved in 1919 that light follows in the path of the bent time and space which is warped due to the gravitational force of a massive object. Einstein predicted that a star positioned behind the sun would be visible during a total eclipse. The Sun bent the light rays coming from the star and made it appear next to the sun..

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