New method of estimated dwarf novae distances
Posted: May 30, 2003

Astronomers using the Fine Guidance Sensors of the Hubble Space Telescope to study dwarf novae unexpectedly discovered a new method of estimating the distances to these strange double-star systems, using their orbital periods and outburst brightness. In the process they learned that dwarf novae tend to be farther away and much brighter than previously thought.

"This sends everybody back to the drawing board," said New Mexico State University astronomer Joni Johnson. "The models for dwarf novae have to be adjusted."

The findings of Johnson and her collaborators from NMSU, the University of California at Riverside, the University of Washington and the University of Texas at Austin were reported May 26 to the American Astronomical Society meeting in Nashville.

The researchers used the orbiting Hubble Space Telescope to directly calculate the distances to six dwarf novae and determine the star systems' brightness. Their original intention was to check the accuracy of commonly used methods of estimating distances to dwarf novae, but "along the way serendipity intervened," Johnson said.

The researchers not only found that dwarf novae estimates have been off the mark. They also discovered a remarkably tight correlation between the orbital period of a dwarf nova system and the system's brightness during its occasional outbursts -- the longer it takes the pair of stars to orbit each other, the brighter the outburst, Johnson said.

"What this means is that we now have a better method of estimating the distances to these systems," she said. "If we know the orbital period of the binary system, we can predict its true luminosity at outburst and calculate the distance to the system."

Dwarf nova systems are a type of cataclysmic variable -- stars that sometimes increase in brightness dramatically. They are binary systems in which the primary, more massive star is a white dwarf -- a star about the size of Earth but with the mass of the sun -- and the secondary star is often a cool red dwarf.

The two stars are locked in a tight orbit, so close to each other that the powerful gravity of the white dwarf strips material away from the red dwarf. This material swirls around the white dwarf in what is known as an accretion disk.

"At times the system becomes unstable and the accretion disk dumps a lot of material onto the surface of the white dwarf," Johnson said. "During these outbursts, the system gets anywhere from a few times brighter to 250 times brighter."

The two stars in a dwarf nova are so close they orbit each other in a matter of hours, compared with the month it takes the moon to orbit Earth or the year it takes Earth to orbit the sun. Known orbital periods range from 78 minutes to 48 hours, Johnson said.

A key to learning more about these systems is knowing how far away they are, she said. Previous distance estimates have been based primarily on comparing the light spectrum of the secondary star in a dwarf nova to that of a standard star of the same type a known distance away.

For more accurate measurements, the astronomers used the Fine Guidance Sensors on the HST to obtain high-precision parallaxes for six dwarf novae, including RU Pegasi, WZ Sagittae and YZ Cancri. They also examined existing data on four other similar objects. Parallaxes provide a way to accurately calculate distances by observing an object from two vantage points and measuring its shift against its background -- the greater the shift, or parallax angle, the closer the object is to the observer.

With these measurements in hand, the researchers could calculate the brightness of the dwarf novae without having to make any assumptions.

"It immediately became obvious that the secondary stars were not normal by any means," Johnson said. "They didn't have the normal luminosity for a star of the measured temperature and in fact were brighter than expected. So the distance measurements to dwarf nova systems were often wrong."

The serendipity came in the unexpected discovery of a tight correlation between the orbital period of the binary stars and their true luminosity when the system is in outburst, she said. This correlation gives astronomers a new tool for measuring the distances to dwarf novae that are too far away to measure by parallaxes.

Johnson's collaborators on the project are Tom Harrison of NMSU, Steve Howell of UC-Riverside, Paula Szkody of the University of Washington, and Barbara McArthur and Fritz Benedict of UT-Austin. The project was funded by NASA's HST Guest Observer Program.

Clearance sale

Price cuts on spectacular calendars featuring the Hubble Space Telescope, Space Station and Earth from space.

Gemini 7
Gemini 7: The NASA Mission Reports covers this 14-day mission by Borman and Lovell as they demonstrated some of the more essential facts of space flight. Includes CD-ROM.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Apollo patches
The Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Mars Rover mission patch
A mission patch featuring NASA's Mars Exploration Rover is available from our online.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Apollo 9 DVD
On the road to the moon, the mission of Apollo 9 stands as an important gateway in experience and procedures. This 2-DVD collection presents the crucial mission on the voyage to the moon.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Get e-mail updates
Sign up for our NewsAlert service and have the latest news in astronomy and space e-mailed direct to your desktop (privacy note: your e-mail address will not be used for any other purpose).
Enter your e-mail address:

ERROR: Random File Unopenable

ERROR: Random File Unopenable

The random file, as specified in the $random_file perl variable was unopenable.

The file was not found on your file system. This means that it has either not been created or the path you have specified in $trrandom_file is incorrect.
An insider's view of how Apollo flight controllers operated and just what they faced when events were crucial.
 Choose your store:

Columbia Report
A reproduction of the official accident investigation report into the loss of the space shuttle Columbia and its crew of seven.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Mars Panorama

DISCOUNTED! This 360 degree image was taken by the Mars Pathfinder, which landed on the Red Planet in July 1997. The Sojourner Rover is visible in the image.
 Choose your store:

Apollo 11 Mission Report
Apollo 11 - The NASA Mission Reports Vol. 3 is the first comprehensive study of man's first mission to another world is revealed in all of its startling complexity. Includes DVD!
 Choose your store:
U.S. - U.K. - E.U. - Worldwide

Rocket DVD
If you've ever watched a launch from Kennedy Space Center, Cape Canaveral, Vandenberg Air Force Base or even Kodiak Island Alaska, there's no better way to describe what you witnessed than with this DVD.
 Choose your store:
U.S. - U.K. - E.U. - Worldwide



© 2014 Spaceflight Now Inc.