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News Release 05-097

Astronomers Announce the Most Earth-Like Planet Yet Found Outside the Solar System

An artist's conception of the new planet

This artist's conception of the new planet shows a hot, rocky, geologically active world.


June 13, 2005

Attention Broadcasters: animations will be available on Betacam SP. Contact Dena Headlee, (703) 292-7739, dheadlee@nsf.gov

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Arlington, Va.--Taking a major step forward in the search for Earth-like planets beyond our own solar system, a team of astronomers has announced the discovery of the smallest extrasolar planet yet detected. About seven-and-a-half times as massive as Earth, with about twice the radius, it may be the first rocky planet ever found orbiting a normal star not much different from our Sun.

All of the nearly 150 other extrasolar planets discovered to date around normal stars have been larger than Uranus, an ice-giant planet in our own solar system that is about 15 times the mass of the Earth.

"We keep pushing the limits of what we can detect, and we're getting closer and closer to finding Earths," said team member Steven Vogt, a professor of astronomy and astrophysics at the University of California, Santa Cruz.

The newly discovered "super-Earth" orbits the star Gliese 876, located just 15 light years away in the direction of the constellation Aquarius. This star also possesses two larger, Jupiter-size planets. The new planet whips around the star in a mere two days, and is so close to the star's surface that its dayside temperature probably tops 400 to 750 degrees Fahrenheit (200 to 400 degrees Celsius)--oven-like temperatures far too hot for life as we know it.

Nevertheless, the ability to detect the tiny wobble the planet induces in the star gives astronomers confidence that they will be able to detect even smaller rocky planets in orbits more hospitable to life.

"This is the smallest extrasolar planet yet detected and the first of a new class of rocky terrestrial planets," said team member Paul Butler of the Carnegie Institution of Washington. "It's like Earth's bigger cousin."

The team measures a minimum mass for the planet of 5.9 Earth masses, orbiting Gliese 876 with a period of 1.94 days at a distance of 0.021 astronomical units (AU), or 2 million miles.

Though the team has no direct proof the planet is rocky, they believe its low mass precludes it from retaining gas like Jupiter. Three other purported rocky planets have been reported outside the solar system, but they orbit a pulsar, the flashing corpse of an exploded star.

"This planet answers an ancient question," said team leader Geoffrey Marcy, professor of astronomy at the University of California, Berkeley. "Over 2,000 years ago, the Greek philosophers Aristotle and Epicurus argued about whether there were other Earth-like planets. Now, for the first time, we have evidence for a rocky planet around a normal star."

"Today's results are an important step toward answering one of the most profound questions that mankind can ask: Are we alone in the universe?" said Michael Turner, head of the Mathematical and Physical Sciences directorate at the National Science Foundation (NSF), which provided partial funding for the research.

The team's work, conducted at the Keck Observatory in Hawaii, was also supported by the National Aeronautics and Space Administration (NASA), the University of California and the Carnegie Institution of Washington.

Marcy, Butler, theoretical astronomer Jack Lissauer of NASA's Ames Research Center, and post-doctoral researcher Eugenio J. Rivera of the University of California Observatories/Lick Observatory at UC Santa Cruz presented their findings today (Monday, June 13) during a press conference at NSF in Arlington, Va.

A paper detailing their results has been submitted to The Astrophysical Journal. Coauthors on the paper are Steven Vogt and Gregory Laughlin of the Lick Observatory at the University of California, Santa Cruz; Debra Fischer of San Francisco State University; and Timothy M. Brown of NSF's National Center for Atmospheric Research in Boulder, Colorado.

Gliese 876 is a small, red star known as an M dwarf--the most common type of star in the galaxy. It is located in the constellation Aquarius, and, at about one-third the mass of the sun, is the smallest star around which planets have been discovered. Butler and Marcy detected the first planet there in 1998; it was a gas giant about twice the mass of Jupiter. Then, in 2001, they reported a second planet, another gas giant about half the mass of Jupiter. The two are in resonant orbits, the outer planet taking 60 days to orbit the star, twice the period of the inner giant planet.

Lissauer and Rivera have been analyzing Keck data on the Gliese 876 system in order to model the unusual motions of the two known planets, and three years ago got an inkling that there might be a smaller, third planet orbiting the star. In fact, if they hadn't taken account of the resonant interaction between the two known planets, they never would have seen the third planet.

"We had a model for the two planets interacting with one another, but when we looked at the difference between the two-planet model and the actual data, we found a signature that could be interpreted as a third planet," Lissauer said.

A three-planet model consistently gave a better fit to the data, added Rivera. "But because the signal from this third planet was not very strong, we were very cautious about announcing a new planet until we had more data," he said.

Recent improvements to the Keck Telescope's high-resolution spectrometer (HIRES) provided crucial new data. Vogt, who designed and built HIRES, worked with the technical staff in the UC Observatories/Lick Observatory Laboratories at the University of California, Santa Cruz, to upgrade the spectrometer's CCD (charge-coupled device) detectors last August.

"It is the higher precision data from the upgraded HIRES that gives us confidence in this result," Butler said.

The team now has convincing data for the planet orbiting very close to the star, at a distance of about 10 stellar radii. That's less than one-tenth the size of Mercury's orbit in our solar system.

"In a two-day orbit , it's about 200 degrees Celsius too hot for liquid water," Butler said. "That tends to lead us to the conclusion that the most probable composition of this thing is like the inner planets of this solar system--a nickel-iron rock, a rocky planet, a terrestrial planet."

"A planet seven and a half times the mass of the Earth could easily hold onto an atmosphere," noted Laughlin, an assistant professor of astronomy at UC Santa Cruz. "It would still be considered a rocky planet, probably with an iron core and a silicate mantle. It could even have a dense steamy water layer. I think what we are seeing here is something that's intermediate between a true terrestrial planet like the Earth and a hot version of the ice giants Uranus and Neptune."

Combined with improved computer software, the new CCD detectors designed by this team for Keck's HIRES spectrometer can now measure the Doppler velocity of a star to within one meter per second--human walking speed--instead of the previous precision of three meters per second. This improved sensitivity will allow the planet-hunting team to detect the gravitational effect of an Earth-like planet within the habitable zone of M dwarf stars like Gliese 876.

"We are pushing a whole new regime at Keck to achieve one meter per second precision, triple our old precision, that should also allow us to see Earth-mass planets around sun-like stars within the next few years," Butler said.

"Our UC Santa Cruz and Lick Observatory team has done an enormous amount of optical and technical and detector work to make the Keck telescope a rocky planet hunter, the best one in the world," Marcy added.

Lissauer also is excited by another feat reported in the paper submitted to the journal. For the first time, he, Rivera and Laughlin have determined the line-of-sight inclination of the orbit of the stellar system solely from the observed Doppler wobble of the star. Using dynamical models of how the two Jupiter-size planets interact, they were able to calculate the masses of the two giant planets from the observed shapes and precession rates of their oval orbits. Precession is the slow turning of the long axis of a planet's elliptical orbit.

They showed that the orbital plane is tilted 40 degrees to our line of sight. This allowed the team to estimate the most likely mass of the third planet as seven and a half Earth masses.

"There's more dynamical modeling involved in this study than any previous study, much more," Lissauer said.

The team plans to continue to observe the star Gliese 876, but is eager to find other terrestrial planets among the 150 or more M dwarfs they observe regularly with Keck.

"So far we find almost no Jupiter-mass planets among the M dwarf stars we've been observing, which suggests that, instead, there is going to be a large population of smaller mass planets," Butler noted.

-NSF-

Media Contacts
 M. Mitchell Waldrop, NSF, (703) 292-7752, email: mwaldrop@nsf.gov
Tim Stephens, University of California, Santa Cruz, (831) 459-4352, email: stephens@ucsc.edu
Susanne Garvey, Carnegie Institution of Washington, (202) 939-1128, email: sgarvey@pst.ciw.edu
Robert Sanders, University of California, Berkeley, (510) 643-6998, email: rsanders@berkeley.edu

Program Contacts
 Michael Briley, NSF, (703) 292-4901, email: mbriley@nsf.gov
Michael S. Turner, NSF, (703) 292-8800, email: mturner@nsf.gov

B-Roll Contacts
 Dena Headlee, NSF, (703) 292-7739, email: dheadlee@nsf.gov

Co-Investigators
 Paul Butler, Carnegie Institution of Washington, (202) 478-8866, email: paul@dtm.ciw.edu
Steven Vogt, University of California, Santa Cruz, (831) 459-2151, email: vogt@ucolick.org
Jack Lissauer, NASA Ames Research Center, (650) 604-2293, email: jlissauer@mail.arc.nasa.gov
Geoffrey Marcy, University of California, Berkeley, (510) 642-8400, email: gmarcy@astro.berkeley.edu
Eugenio Rivera, NASA Ames Research Center and Lick Observatory, (831) 459-2277, email: rivera@ucolick.org
Gregory Laughlin, Lick Observatory and University of California, Santa Cruz:, (831) 459-3208, email: laughlin@ucolick.org

Related Websites
Press briefing webcast: http://www.nsf.gov/news/newsmedia/planetdiscovery.jsp
Geoffery Marcy's web page on the new planet: http://www.exoplanets.org/index_gl.html
NASA's PlanetQuest site: http://planetquest.jpl.nasa.gov/
The California & Carnegie Planet Search site: http://exoplanets.org/

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