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UCLA, British Astronomers Discover The Wake Of A Planet Around A Nearby Star – Strong Evidence For Solar Systems Like Ours

Date:
October 11, 2002
Source:
University Of California - Los Angeles
Summary:
An international team of astronomers reports the first strong evidence for the existence of massive planets on wide orbits -- like those of Saturn, Uranus and Neptune -- around many stars. The new research provides some of the strongest evidence so far that solar systems similar to our own, or even larger, are likely to exist.

An international team of astronomers reports the first strong evidence for the existence of massive planets on wide orbits -- like those of Saturn, Uranus and Neptune -- around many stars. The new research provides some of the strongest evidence so far that solar systems similar to our own, or even larger, are likely to exist.

"Our evidence for large planets on wide orbits around many stars is iron-clad, while before there was some weasel room," said Benjamin Zuckerman, UCLA professor of astronomy and member of the research team who analyzed and interpreted the new data. "For life-bearing, Earth-like planets to exist in other solar systems, large planets on wide orbits are likely to be essential."

The research team reports the discovery of a huge distorted disk of cold dust surrounding Fomalhaut (pronounced Fo-mal-ought), one of the brightest stars in the sky. Fomalhaut is located about 25 light years away from our sun, is estimated to be 2.3 times as massive as the sun and about 1.7 times the diameter. The most likely cause of the distortion is the gravitational influence of a Saturn-like planet at a large distance from the star tugging on the disk. The new observations of Fomalhaut are reported in a paper to be published in the Astrophysical Journal -- the most widely read journal in astronomy.

One hundred planets are already known to exist outside our solar system, none of which has yet been seen directly by a telescope. These planets, nicknamed "hot-Jupiters," are roughly the size of the planet Jupiter, but have orbits much closer to their star than Jupiter's is to our sun.

"What is new and exciting about the observation of Fomalhaut is that it probes the space much more distant from the star -- on scales of the orbits of Uranus, Neptune and beyond," said Wayne Holland of the UK Astronomy Technology Centre (UK ATC) in Edinburgh, who led the research team. "We were amazed to find that the disk is actually bent around the star. This strongly suggests there is an orbiting giant planet shaping the dust we see."

Fomalhaut, which lies in the constellation of Piscis Austrinus (the Southern Fish), is only about 200 million years old -- an infant compared to our sun at 4.5 billion years. Fomalhaut, the 17th-brightest star in the sky, derives from the Arabic name for this star, Fum al Hut, meaning "The Fish's Mouth." The alternative Latin names for the star, Os Piscis Meridiani or Os Piscis Notii, mean "The Mouth of the Southern Fish."

The giant planets in the Milky Way, Jupiter and Saturn, are believed to have formed 10 million years after the sun, while the Earth formed in about 100 million years. For about 600 million years, our solar system was bombarded by comets and asteroids, until, as Zuckerman said, "the gravitation of Jupiter and Saturn, the 'garbagemen of the solar system,' cleaned out these massive objects that could have decimated life.

"We believe Fomalhaut's solar system looks quite similar to our own solar system when it was only 200 million years old," Zuckerman said. "At that age, a planetary system already would have formed. We would have trouble seeing it with optical telescopes because of the shroud of dust."

High-resolution image

The research team presented widely reported findings on Fomalhaut in 1998, and has an image now with twice the resolution of the 1998 image.

"Our previous image did not have the resolution to pinpoint the detail we are now seeing," said Jane Greaves, one of Holland's colleagues on the project. "We could see a hole in the disk near the star, and thought it was cleared out by the gravity of a planet like Jupiter, but we had no idea there was anything further from the star."

The dust disk surrounding Fomalhaut is so cold, and emits so little light, that it is completely invisible to optical telescopes such as the Hubble Space Telescope. Instead, the astronomers used a telescope and camera that operate in the so-called "submillimeter" region of the electromagnetic spectrum, which lies between infrared light and radio waves.

The astronomers see the effect of the large planet on the dust, and infer the planet's existence from the asymmetrical dust. The distribution of the dust is shaped by the gravitational field of the unseen planet.

Holland's team used the James Clerk Maxwell Telescope (JCMT) at the summit of Mauna Kea, Hawaii, the world's largest telescope dedicated to the study of light at submillimeter wavelengths. With a specially cooled camera called SCUBA, they were able to measure the tiny amounts of heat radiated by the dust particles that make up the disk.

SCUBA (Submillimeter Common User Bolometer Array), which was built at the Royal Observatory, Edinburgh, has detectors that are cooled to just one-tenth of a degree above absolute zero (-273 degrees Celsius). It has already found young nurseries where stars are being born and has discovered distant galaxies near the edge of the Universe.

The research team is now analyzing SCUBA pictures of additional bright stars, including Vega -- in the constellation of Lyra and the brightest star in our summer sky -- which also show very clear evidence of gravitationally disturbed dusty disks. It is the dusty structures visible in the SCUBA images that indicate that massive planets having orbits as large as or larger than those of Saturn, Uranus and Neptune must exist around many other stars, Zuckerman and Holland concluded. Even though no such planet has yet been imaged directly, the SCUBA images yield the first good observational evidence that massive planets with big orbits "are really out there," Zuckerman said.

The disk appears a bit like a doughnut with a hole in the center around the star. "The Fomalhaut disk is close to edge-on as we see it, and in the image it looks like the ends of the 'doughnut' are brighter," Greaves said. "The disk is about the same size as the sun's Kuiper Belt of comets which orbits outside Neptune and Pluto, so we may be seeing a region near Fomalhaut that has many millions of comets."

Implications for other planets like Earth?

Is the universe filled with planets like Earth?

Solar systems like the ones containing the "hot-Jupiters" are not hospitable to Earth-like planets that can sustain life, Zuckerman said, because these giant planets have orbits too close to their stars; the gravitational fields of these giant planets would disturb the orbits of Earth-like planets and make life as we know it impossible.

While the new data do provide strong evidence for massive planets at a much more desirable location for Earth-like planets to exist, Zuckerman still believes intelligent life in the universe is extremely rare, and perhaps unique to Earth.

The astronomers plan a new survey of more than 100 nearby stars. Holland is also leading a team to build a new, more powerful camera ("SCUBA-2").

"SCUBA-2 will be able to image disks, such as the one around Fomalhaut, in just a few minutes, instead of the many tens of hours it currently takes," said Ian Robson, deputy director of the UK ATC.

The research team also includes UK ATC astronomers Mark Wyatt and William Dent, and Iain Coulson, with the Joint Astronomy Centre in Hawaii.

Zuckerman's research is funded by the UCLA Astrobiology Institute, which is supported by NASA. Holland's team received funding from The Particle Physics and Astronomy Research Council (PPARC), the UK's strategic science investment agency. PPARC funds research, education and public understanding in particle physics, astronomy, cosmology and space science.

Online resources

The Particle Physics and Astronomy Research Council: http://www.pparc.ac.uk/

James Clerk Maxwell Telescope: http://www.jach.hawaii.edu/JACpublic/JCMT/

Benjamin Zuckerman: http://www.physics.ucla.edu/people/faculty_members/zuckerman.html


Story Source:

The above story is based on materials provided by University Of California - Los Angeles. Note: Materials may be edited for content and length.


Cite This Page:

University Of California - Los Angeles. "UCLA, British Astronomers Discover The Wake Of A Planet Around A Nearby Star – Strong Evidence For Solar Systems Like Ours." ScienceDaily. ScienceDaily, 11 October 2002. <www.sciencedaily.com/releases/2002/10/021011071404.htm>.
University Of California - Los Angeles. (2002, October 11). UCLA, British Astronomers Discover The Wake Of A Planet Around A Nearby Star – Strong Evidence For Solar Systems Like Ours. ScienceDaily. Retrieved September 1, 2014 from www.sciencedaily.com/releases/2002/10/021011071404.htm
University Of California - Los Angeles. "UCLA, British Astronomers Discover The Wake Of A Planet Around A Nearby Star – Strong Evidence For Solar Systems Like Ours." ScienceDaily. www.sciencedaily.com/releases/2002/10/021011071404.htm (accessed September 1, 2014).

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