Press Release

Hubble and Einstein Weight Nearest White Dwarf Star

By SpaceRef Editor
December 13, 2005
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Hubble and Einstein Weight Nearest White Dwarf Star

Astronomers have used NASA’s Hubble Space Telescope to get the most precise measurement ever made of a tiny shift in the light from Earth’s nearest white dwarf star and, using Einstein’s theory of general relativity, accurately determined the incredibly dense star’s mass.

The white dwarf star, Sirius B, is a companion to Sirius A, the brightest star in the night sky. The binary star system is only 8.6 light years from Earth. (A light year is the distance light travels in one year, roughly six trillion miles.) But ground-based astronomers have found it impossible to precisely measure light from Sirius B because it is swamped by the glare of the ten-thousand times brighter Sirius A.

Jay B. Holberg and Ivan Hubeny of The University of Arizona are members of the team led by Martin Barstow of the University of Leicester, U.K., who used the Hubble to get sharp views of just the white dwarf star, unpolluted by light from Sirius A. White dwarf stars are the dying remnant cores of stars similar to the sun. Our sun will eventually become a white dwarf.

Applying Einstein’s general relativity theory, the team determined that Sirius B packs 98 percent of the mass of our sun within its 7,500-mile diameter (12,000 kilometers), or within a volume slightly smaller than Earth.

Albert Einstein proposed the general relativity theory in 1915. It says that the gravity of any mass, such as a planet or star, has the effect of warping the space and time around it.

Einstein predicted that astronomers would observe light losing a fraction of its energy because of a massive star’s intense gravitational field. They would see light shifted to longer, redder wavelengths. The phenomenon is called “gravitational redshift” effect.

Sirius B has an intense gravitational field that warps space and slows time far more dramatically than we experience on Earth. If we humans were to stand on Sirius B, we’d be crushed by space warped by gravity. A 150-pound person would weigh 50 million pounds. (But on the upside, if we Earthlings could survive, we wouldn’t age as quickly.)

“The nature of the ashes of these dead stars give us important clues about the lives and deaths of stars like our own sun,” Barstow said. “The nuclear waste of carbon and oxygen produced in the process are essential elements for life and are eventually recycled into interstellar space to form new stars, planets and, possibly, living beings.”

“Sirius’ strange companion (Sirius B) has played a key role in the development of physics and astrophysics since 1915, when it first alerted astronomers to the existence of enormously dense states of matter,” Holberg added.

Astronomers first measured the gravitational redshift in light from Sirius B in 1925, helping confirm Einstein’s general relativity theory. As a young graduate student at Cambridge University in the early 1930s, Subramanyan Chandrasekhar used Einstein’s theory of special relativity and quantum mechanics to show how white dwarf stars could exist. He also deduced that no white dwarf could ever have more mass than 1.4 solar masses. Chandrasekhar’s work was dismissed until the 1960s, then recognized with the Nobel Prize in physics in 1983.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. The Space Telescope Science Institute in Baltimore conducts Hubble science operations. The institute is operated for NASA by the Association of Universities for Research in Astronomy, Inc., Washington.

SpaceRef staff editor.