Solar systems around dead Suns?

Apr 20, 2009
Emission from the White Dwarf System GD 16. Image: NASA / JPL-Caltech / University of Leicester

( -- Using NASA’s Spitzer Space Telescope, an international team of astronomers have found that at least 1 in 100 white dwarf stars show evidence of orbiting asteroids and rocky planets, suggesting these objects once hosted Solar Systems similar to our own.

Using the infrared detectors on NASA's , a team of researchers based in the U.K. and in the United States have placed new constraints on how often rocky planets like Earth may exist around stars other than our Sun.

The team of researchers, including Jay Farihi, from the University of Leicester; and Michael Jura and Ben Zuckerman, both from UCLA, looked at the environments surrounding a number of "dead" stars known as a "". Using Spitzer's sensitive infrared eyes, they found that at least 1-3% of all white dwarf stars of a certain age are surrounded by dust and rocky debris.

"The infrared glow from dust around these white dwarfs is a road sign that tells us there were — or are — unseen rocky planets in these systems," said Farihi.

The team believes that the dust was produced when asteroids - the building blocks of rocky planets - surrounding the star were pushed and pulled apart by the force of the star's gravity. The dust then formed a glowing disk of orbiting, rocky material that Spitzer detected.

Just how common are rocky bodies around white dwarfs? In a previous study by this team, a sample of eight white dwarfs were shown to have the dusty remnants of shredded asteroids. In this study Farihi and his team systematically searched around metal-rich white dwarfs and placed statistical constraints on the frequency of inferred rocky planets.

"We now know of 14 white dwarfs circled by dusty debris. This suggests that at least 1-3% of main-sequence A and F stars — stars slightly hotter and larger than the Sun — have rocky planets, like Earth," said Farihi.

For the rocky bodies to be destroyed by the gravitational effects of the white dwarf, they would have to be knocked out of their orbits, towards the star. Farihi and his team believe that, although in principle this kick could come from a terrestrial planet, a large gas giant planet like Jupiter would do the job much more efficiently. Therefore, the small percentage of white dwarfs that might possess probably have larger, gas-giant-like planets as well.

Asteroid 'Bites the Dust' Around Dead Star. Image: NASA/JPL-Caltech

White dwarfs are the remnants of relatively low-mass stars that have passed through their red giant stage. Stars are composed mostly of hydrogen, and, during their lives, they burn more and more of the hydrogen, converting hydrogen into helium, until very little hydrogen is left. Then, the star begins to burn helium to create even heavier elements. When the supply of helium runs out, the star burns heavier and heavier elements, until it produces iron, which cannot be burned.

At this point, the star's contraction — due to its gravity — and its expansion — due to the energy produced by its thermonuclear reactions — become unbalanced, and the outer layers of the star puff out. Over time, the layers blow out into space, leaving behind a small core, which, because of the extreme gravity, compresses until it is extraordinarily dense. This core is called a "white dwarf."

A white dwarf may be the size of the Earth, but contain the same mass as the Sun. This star remnant is so dense, in fact, that one teaspoon of white dwarf material would weigh several tons. Over 90% of all stars — including our Sun — will end their lives as white dwarfs.

According to Farihi and his team, studying white dwarf stars is a good way to study planetary systems outside of our own . First, a white dwarf star is relatively dim and small -so its heat won't outshine the heat emitted by giant planets or dust orbiting it. Second, white dwarf stars do not contain significant amounts of heavy elements, like metals, so if metals are detected in a white dwarf, one can assume that the white dwarf has been absorbing those elements from surrounding debris. This permits an indirect way of studying the composition of distant planets.

This research paper was written by Jay Farihi, at the University of Leicester, UK; and Michael Jura and Ben Zuckerman, both at UCLA.

Team member Professor Jay Farihi of the University of Leicester presents this discovery on Monday 20th April at the European Week of Astronomy and Space Science conference at the University of Hertfordshire.

Provided by JPL/NASA (news : web)

Explore further: Computers beat brainpower when it comes to counting stars

add to favorites email to friend print save as pdf

Related Stories

Dead Stars Tell Story of Planet Birth

Jan 05, 2009

( -- Astronomers have turned to an unexpected place to study the evolution of planets -- dead stars. Observations made with NASA's Spitzer Space Telescope reveal six dead "white dwarf" stars littered ...

Astronomers discover how white dwarf stars get their 'kicks'

Dec 04, 2007

University of British Columbia astronomer Harvey Richer and UBC graduate student Saul Davis have discovered that white dwarf stars are born with a natal kick, explaining why these smoldering embers of Sun-like stars are found ...

White dwarf and ultra-cool dwarf keep their distance

Apr 18, 2007

Scientists from the University of Hertfordshire have discovered a rare binary system consisting of a white dwarf, a Sun-like star that has reached the end of its life, and an ultra-cool dwarf, which is the smallest kind of ...

New type of pulsating white dwarf star discovered

May 01, 2008

University of Texas at Austin astronomers Michael H. Montgomery and Kurtis A. Williams, along with graduate student Steven DeGennaro, have predicted and confirmed the existence of a new type of variable star, ...

Recommended for you

ESO image: A study in scarlet

12 hours ago

This new image from ESO's La Silla Observatory in Chile reveals a cloud of hydrogen called Gum 41. In the middle of this little-known nebula, brilliant hot young stars are giving off energetic radiation that ...

Astronomers: 'Tilt-a-worlds' could harbor life

Apr 15, 2014

A fluctuating tilt in a planet's orbit does not preclude the possibility of life, according to new research by astronomers at the University of Washington, Utah's Weber State University and NASA. In fact, ...

Pushy neighbors force stellar twins to diverge

Apr 15, 2014

( —Much like an environment influences people, so too do cosmic communities affect even giant dazzling stars: Peering deep into the Milky Way galaxy's center from a high-flying observatory, Cornell ...

Image: Multiple protostars within IRAS 20324+4057

Apr 14, 2014

( —A bright blue tadpole appears to swim through the inky blackness of space. Known as IRAS 20324+4057 but dubbed "the Tadpole", this clump of gas and dust has given birth to a bright protostar, ...

User comments : 3

Adjust slider to filter visible comments by rank

Display comments: newest first

5 / 5 (1) Apr 21, 2009
It is misleading for you to entitle an apparent 'artist's rendition' as an 'Image' from JPL !!
An 'image' implies that an 'imaging device' was used, eg, a camera. Ascribing the 'image' to JPL further misleads the public, for JPL is a science-based organization, not a collective of artists.

5 / 5 (2) Apr 21, 2009
first they state that a white dwarf has preceeded through sucessive fusions arriving at iron..then state they have little heavy metal content????
not rated yet Apr 21, 2009
"white dwarf material is not composed of atoms bound by chemical bonds, but rather consists of a plasma of unbound nuclei and electrons"

More news stories

Meteorites yield clues to Martian early atmosphere

( —Geologists who analyzed 40 meteorites that fell to Earth from Mars unlocked secrets of the Martian atmosphere hidden in the chemical signatures of these ancient rocks. Their study, published ...

Red moon at night; stargazer's delight

Monday night's lunar eclipse proved just as delightful as expected to those able to view it. On the East Coast, cloudy skies may have gotten in the way, but at the National Science Foundation's National Optical ...

Down's chromosome cause genome-wide disruption

The extra copy of Chromosome 21 that causes Down's syndrome throws a spanner into the workings of all the other chromosomes as well, said a study published Wednesday that surprised its authors.

Researchers see hospitalization records as additional tool

Comparing hospitalization records with data reported to local boards of health presents a more accurate way to monitor how well communities track disease outbreaks, according to a paper published April 16 in the journal PLOS ON ...

Ebola virus in Africa outbreak is a new strain

The Ebola virus that has killed scores of people in Guinea this year is a new strain—evidence that the disease did not spread there from outbreaks in some other African nations, scientists report.