University of Hawaii Institute for Astronomy
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Embargoed until
Thursday, January 10, 2008
10:30 a.m. CST (6:30 a.m. HST)

Contacts:


Dr. Evgenya Shkolnik
NASA Astrobiology Institute/ Institute for Astronomy
University of Hawaii at Manoa shkolnik@ifa.hawaii.edu
www.ifa.hawaii.edu/~shkolnik/

Dr. Michael C. Liu
Institute for Astronomy
University of Hawaii at Manoa mliu@ifa.hawaii.edu
1-808-956-6666

Mrs. Karen Rehbock
Assistant to the Director
Institute for Astronomy
University of Hawaii at Manoa
1-808-956-6829
rehbock@ifa.hawaii.edu

Dr. I. Neill Reid
Space Telescope Science Institute
inr@stsci.edu
1-410-338-4971

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Institute for Astronomy
Director's office
2680 Woodlawn Drive Honolulu, Hawaii 96822
Telephone: 1-808-956-8566
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A Rare Quartet of Stars May Unlock Secrets of Stellar Evolution

quadruple system
Figure 1. Artistís view of the gaseous disk that may have once engulfed and maneuvered the quadruple stellar system into its unusually small orbit. (Credit: K. Teramura, UH IfA)

Astronomers using telescopes on Mauna Kea have found an extremely rare quartet of stars that orbit each other within a region smaller than Jupiter's orbit round the Sun.  The quartet appears as a speck of light even when viewed with the world's most powerful telescopes but its spectrum reveals not one, but four distinct stars arranged in two pairs.  Astronomers are now struggling to work out whether they could have been born that way, or were forced together by a dense disk of gas in their youth.

This discovery that the star called "BD -22º5866" is really a very rare system of four closely orbiting stars was announced by Dr. Evgenya Shkolnik of the University of Hawaii's Institute for Astronomy and the NASA Astrobiology Institute on January 8, 2008, at the annual meeting of the American Astronomical Society in Austin, TX. She and collaborators Dr. Michael C. Liu, also of the University of Hawaii, and Dr. I. Neill Reid of the Space Telescope Science Institute in Baltimore were monitoring several hundred nearby low-mass stars when one observation caught their attention because it was unlike anything they had seen before.

At the time of the observations, two of the stars were orbiting each other at 133 km/s (300,000 mph, a speed that would get you from Honolulu to New York in less than a minute), while the second pair moved at a more modest speed of 52 km/s (120,000 mph). Using these speeds and the stars' masses, astronomers were able to determine the maximum sizes of their oddly tight orbits. Less than 1 in 2,000 stars observed might be such tightly bound systems, making this quadruple stellar system extremely rare.

The first pair orbits each other in less than 5 days with the orbit’s radius of at most 0.06 AU (where 1 AU is the distance from Earth to the sun). The second pair orbits with a period of less than 55 days and a maximum radius of 0.26 AU.  The two pairs are orbiting each other with a maximum radius of only 5.8 AU (= orbital period of less than 9 years), about the same as Jupiter's distance from the sun.

"The extraordinarily tight configuration of this stellar system tells us that there may have been a single gaseous disk that forced them into such small orbits within the first 100,000 years of their evolution, as the stars could not have formed so close to one another. This is the first evidence of a disk completely encompassing four stars," says Dr. Shkolnik. "It is remarkable how much a single stellar spectrum can tell us about both the present and the past of these stars."

The data were acquired at the Keck I 10-m (33-foot) telescope and on the Canada-France-Hawaii 3.6-m (12-foot) telescope, both located on the summit of Mauna Kea, a 14,000-foot-high dormant volcano on the Big Island of Hawaii. Each telescope is equipped with a high-resolution spectrograph, an instrument capable of breaking up the star's light into different colors (or wavelengths), known as a spectrum.

The stellar system is 51 pc (or 166 light-years) away from the Sun and lies just south of the constellation Aquarius (The Water Bearer).  Though BD -22º5866 cannot be seen without a telescope, it is relatively bright and will be carefully monitored to map the orbits in more detail. Since most stars form as part of a binary- or multiple-star system, the enormous potential of this quadruple system to give us previously unavailable physical information makes it a key to unlocking a few mysteries of stellar evolution.

This work has been submitted to the Astrophysical Journal Letters and was funded by the NASA Astrobiology Institute and the University of Hawaii.


quadruple stellar system compared with solar system

Figure 2. A to-scale schematic of the quadruple stellar system overlaid for comparison with a diagram of the solar system’s planetary orbits. (Credit: Evgenya Shkolnik)


Founded in 1967, the Institute for Astronomy at the University of Hawaii at Manoa conducts research into galaxies, cosmology, stars, planets, and the sun. Its faculty and staff are also involved in astronomy education, deep space missions, and in the development and management of the observatories on Haleakala and Mauna Kea.

Established in 1907 and fully accredited by the Western Association of Schools and Colleges, the University of Hawaii is the state's sole public system of higher education. The UH System provides an array of undergraduate, graduate, and professional degrees and community programs on 10 campuses and through educational, training, and research centers across the state. UH enrolls more than 50,000 students from Hawaii, the U.S. mainland, and around the world.

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