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Science Journal
Summer 2000 -- Vol. 17, No. 1

 

International Team of Astronomers Finds Most Distant Object

In April 2000 an international team of astronomers, including Penn State professor of astronomy and
astrophysics
Donald Schneider, announced it had discovered the most distant known object in the universe. 
The object was first spotted in March while the scientists were examining data from the Sloan Digital Sky
Survey
(SDSS), a project designed to map a large portion of the sky in unprecedented detail.

Xioahui Fan, a Princeton graduate student, was examining some of the SDSS data base and noted the presence of a faint, red object that had a very unusual color.  A spectrum of the source was obtained on 29 March with the Keck telescope in Hawaii and within minutes the astronomers knew the radiation they had just recorded had originated in a distant quasar when the universe was less than a billion years old.  Quasars are thought to be massive (up to a billion times the mass of the Sun) black holes that are accreting matter at the rate of more than one solar mass per year.

 

Donald Schneider's Record of Discovering the Most Distant Quasar

Date
Redshift*
Schneider's Collaborators
Most Distant Object?
1987
1989
1991
1998
1999
2000
4.04
4.73
4.90
5.00
5.02
5.82
Maarten Schmidt+James Gunn
Maarten Schmidt+James Gunn
Maarten Schmidt+James Gunn
Sloan Digital Sky Survey Team
Sloan Digital Sky Survey Team
Sloan Digital Sky Survey Team
Yes
Yes
Yes
No
No
Yes
*The distance to a quasar is typically expressed in terms of the object¹s redshift, which is a measure of how far the wavelength of its light is lengthened, or shifted to the red end of the spectrum. The larger the redshift, the more distant the source (see box, page 16). The quasar Schneider and his collaborators discovered in March 2000 has a redshift of 5.82, breaking the distance record previously held by a galaxy with redshift 5.7 discovered last year by Esther Hu and colleagues at the University of Hawaii and the Institute of Astronomy in Cambridge, England.

Distances to quasars are usually expressed in terms of the object's redshift, which is a measure of how far the
wavelength of its light is lengthened, or shifted, to the red end of the spectrum; the larger the redshift, the more
distant the source.  The newly discovered quasar has a redshift of 5.82, breaking the distance record previously held by a galaxy with redshift of 5.7, discovered last year by Esther Hu and colleagues at the University of Hawaii and the Institute of Astronomy in Cambridge, England.  Moreover--and ultimately perhaps much more significant --this isn't the first far-off quasar the SDSS sky survey has found.

"Finding the most distant object is, of course, an event worth noting, but what particularly excites me is the un-precedented rate at which the SDSS is finding high-redshift quasars," said Schneider.  "When the SDSS obtained its first observations in May 1998, only one quasar was known with a redshift larger than 4.74, and that was a redshift 4.90 quasar discovered back in 1991. As of the middle of April 2000, the SDSS has found a total of 12 such objects; five with redshifts above five."

This theme was echoed by the SDSS Project Scientist, James Gunn of Princeton University.

"The real significance of the Sloan quasars," said Gunn,"is not their record-breaking distances but the size and quality of the sample.  The scale and the homogeneity of the data will allow SDSS and other scientists to use quasars to chart the birth and formation of galaxies, explore structure on the largest scales, and better understand black holes.  Past quasar surveys have included a smaller and less uniform selection of objects."

Schneider is the chairman of the SDSS Quasar Science Working Group, and is using the Hobby-Eberly Telescope at McDonald Observatory to observe SDSS high-redshift quasar candidates. Penn State is the originator and one of the principal operating partners of the Hobby-Eberly Telescope, the largest optical telescope on the North American continent and one of the largest in the world.  To date, the Hobby-Eberly Telescope has discovered more than two dozen high-redshift quasars, and Schneider believes that the best is yet to come.  "The SDSS has only covered a few percent of the planned survey area, and the Hobby-Eberly Telescope has only recently completed its commissioning phase.  I will be quite disappointed if in five years we have not discovered more than 100 quasars above redshift five."

Penn State


Math--and Several Other Factors--Matter
When Associating Redshifts with Distances





(Editor's note: In many instances, astronomers and scientists make reference to the redshifts of the objects they view and the distance of those objects from Earth.  Making the connection between those factors is not easy.  Professor Donald Schneider, who helped discover the most distant quasar described in the previous article, provides some insights into the process.)

Redshift is related to the amount that the radition (light) from the quasar is shifted to the red--the larger the redshift, the more the light is shifted.  Redshift is usually represented by the symbol "z."
The formal definition is:

z  =   wavelength observed    -1
 wavelength emitted

Thus an object that is not moving with respect to the observation point has a redshift of 0 (no shift as the observed wavelength equals the emitted wavelength).

For an object of redshift 5, the observed wavelengths are larger by a factor of six than the emitted wavelength.

For example, if a quasar at redshift 5.0 emitted light at a wavelength of 1,000Å (far in the ultraviolet spectrum), we would observe this radiation at a wavelength of 6,000Å (red).

That's exactly what we do to determine redshift.

We measure the observed wavelength of a "feature" in the spectrum and deduce what the emitted wavelength is from atomic physics, then calculate the redshift.

That, however, is the easy part.

To determine a distance, one must adopt a theory of the universe that relates redshift to distance.  The only serious model at this time is Einstein's General Theory of Relativity.

The values of two particularly important parameters are required to calculate a distance: Hubble's Constant (how fast the universe is expanding) and the amount of mass in the universe.

While Hubble's Constant is known to  a factor of 50 percent, the amount of mass is uncertain by at least a factor of two.

The distance to an object (and the age of the universe) is inversely related to the value of Hubble's Constant.

If you double Hubble's Constant, the distance scale (and the age) decreases by a factor of two.

The amount of mass in the universe also has important, but nonlinear, effects on these quantities.

With these caveats (as the most important among several), if you assume our best current estimates for Hubble's Constant and the amount of mass, the distance to an object is:

           d =         10 billion       x     [1-(1+z)-1.5]
light years 

For example, if the redshift is 0, then the distance is zero.

If the redshift is infinity, the distance is 10 billion light years, which is the age of the universe (light emitted at the instant of the Big Bang has a redshift of infinity).

At a redshift of 4.0, the last factor in the equation above becomes:

1 - 5-1.5 = 0.91

The distance to the object is 9.1 billion light years--and the radiation was emitted when the universe was 900 million years old, 9 percent of its current age.

At a redshift of 6.0, the factor becomes:

1 - 7-1.5 = 0.95

The distance to the object is 9.5 billion light years--and the radiation was emitted when the universe was 500 million years old, 5 percent of its current age.

If our best estimate of Hubble's Constant suddenly doubles, all distances and ages would be cut in half, but the percentages of those ages/distances in terms of the universe's age would remain unchanged.
 

 

Back to Science Journal Summer 2000 Index

 


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