They are about half the distance from their source star as Jupiter and Saturn are from our sun, but the two new planets are the same distance apart as Jupiter and Saturn are to each other.

Because this is just the fifth exoplanetary system found via microlensing, the finding suggests that our galaxy hosts many solar systems like our own.

"This is the first time something analogous to our solar system has been found," said Kem Cook, one of three LLNL researchers on the team and a pioneer in gravitational microlensing. "This indicates that our kind of planetary system is relatively common and that in and of itself is exciting."

The research appears in the Feb. 15 issue of the journal, Science.

The two planets were seen when the star they orbit crossed in front of a more distant star as seen from Earth (gravitational microlensing). For a two-week period from late March through early April 2006, the nearer star's gravity magnified the light shining from the farther star. The planets altered this magnification in a distinctive manner.

The gravitational microlensing planet search method is sensitive to multiple-planet systems containing analogs of all of our solar system planets except Mercury.

The new planets resemble a scaled-down version of our solar system, because the mass ratio, separation ratio and equilibrium temperatures are similar to those of Jupiter and Saturn. The planets' masses are about 71 percent and 90 percent, respectively, of Jupiter and Saturn; their sun is about 50 percent the mass of our sun.

"It looks more like our solar system than any other system we've seen so far," said Bruce Macintosh, another of the Livermore authors. "This system resembles our own and it has room in it for a planet like Earth."

The Optical Gravitational Lensing Experiment (OGLE) first detected the event, dubbed OGLE-2006-BLG-109, on March 28, 2006. The Microlensing Follow Up Network (MicroFUN), led by Andrew Gould, professor of astronomy at Ohio State, then joined with OGLE to organize astronomers worldwide to gather observations of it. Analyzing the data in real time, Ohio State Professor Scott Gaudi (the lead author) realized that this observation was likely to be a two-planet event, instead of the hoped for single-planet event, making the discovery even more exciting.

To confirm the existence of the two planets, Livermore researchers went a step further. LLNL's Sergei Nikolaev used the Lab's supercomputer Zeus to run codes that would constrain the parameters of the microlensing model and would allow the planetary motions to be included in the solution in a reasonable amount of calendar time. The result: The code confirmed the existence of the two scaled-down Jupiter and Saturn-like planets. Notre Dame University's David Bennett (another author of the paper) developed the code and helped in the analysis.

Macintosh used the adaptive optics (AO) system at the Keck Observatory in Hawaii to isolate the lens star (the star of the new planetary system) from other stars in the extremely crowded region toward the center of our galaxy. Adaptive optics allow astronomers to minimize the blurring effects of the Earth's atmosphere, producing images with unprecedented detail and resolution. The Keck adaptive optics image allowed a direct measurement of the source system's brightness and color, helping constrain the source system's mass. Cook, in addition to belonging to one of the follow-up teams (Probing Lensing Anomalies NETwork or PLANET), analyzed the Keck AO data.

The current discovery relied on 11 different ground-based telescopes in countries around the world, including New Zealand, Tasmania, Israel, Chile, the Canary Islands and the United States.

The planetary system represents a scaled down version of our own solar system, with a less-massive sun. However, the scaling down is consistent with the core-accretion paradigm in which giant planets form near the snow line- thepoint in the protoplanetary disk beyond which ices are stable. Planet mass decreases as the distance beyond the snow lineincreases.

earlier related report
Astronomers Discover Scaled-Down Jupiter And Saturn In A Faraway Solar System Like Our Own

Columbus OH - An international team of astronomers has discovered two planets that resemble smaller versions of Jupiter and Saturn in a solar system nearly 5,000 light years away.

The find suggests that our galaxy hosts many planetary systems like our own, said Scott Gaudi, assistant professor of astronomy at Ohio State University.

He and his colleagues reported their results in the February 15 issue of the journal Science.

The two planets were revealed when the star they orbit crossed in front of a more distant star as seen from Earth. For a two-week period from late March through early April of 2006, the nearer star magnified the light shining from the farther star.

The phenomenon is called gravitational microlensing, and this was a particularly dramatic example: the light from the more distant star was magnified 500 times.

The Optical Gravitational Lensing Experiment (OGLE) first detected the event, dubbed OGLE-2006-BLG-109, on March 28, 2006. The Microlensing Follow Up Network (MicroFUN), led by Andrew Gould, professor of astronomy at Ohio State, then joined with OGLE to organize astronomers worldwide to gather observations of it. Andrzej Udalski, professor of astronomy at Warsaw University Observatory, is the leader of OGLE.

Gaudi took the lead in analyzing the data as they came in. As he studied the light signal, he saw a distortion that he thought was caused by a Saturn-mass planet. Then, less than a day later, came an additional distortion he wasn't expecting: a "blip" in the signal that appeared to be caused by a second, larger planet orbiting the same star.

Over the next few months, Gaudi demonstrated that this two-planet interpretation was correct. Then David Bennett, a research associate professor of astrophysics and cosmology at the University of Notre Dame, refined Gaudi's preliminary model using sophisticated software, and revealed additional details about the system.

This is the third time a Jupiter-mass planet was found by microlensing, Gaudi explained. In the previous two cases, additional planets would have been very difficult to detect, had they been there.

"This is the first time we had a high-enough magnification event where we had significant sensitivity to a second planet -- and we found one." Gaudi said. "You could call it luck, but I think it might just mean that these systems are common throughout our galaxy."

Astronomers have found two planets at once before, "but using other techniques that don't pick up on solar systems like ours," he said.

The newly-discovered planets appear to be gaseous planets like Jupiter and Saturn -- only about 80 percent as big -- and they orbit a star about half the size of the sun. The star is dim and cold compared to ours, issuing only five percent as much light. Still, the new solar system appears to be a smaller analog of our own. The larger planet is about as massive compared to its star as Jupiter is to ours. The smaller planet shares a similar mass ratio with Saturn.

Also, the smaller planet is roughly twice as far from its star as the larger one, just as Saturn is roughly twice as far away from the sun as Jupiter. Although the star is much dimmer than our sun, temperatures at both planets are likely to be similar to that of Jupiter and Saturn, because they are closer to their star.

"The temperatures are important because these dictate the amount of material that is available for planet formation," Gaudi said. "Most theorists think that the biggest planet in our solar system formed at Jupiter's location because that is the closest to the sun that ice can form. Saturn is the next biggest because it is in the next location further away, where there is less primordial material available to form planets."

"Theorists have wondered whether gas giants in other solar systems would form in the same way as ours did. This system seems to answer in the affirmative."

The fact that astronomers found the planets during the first event that allowed such a detection suggests that these scaled-down versions of our solar system are very common, he added.

Previously, astronomers had found four planets using microlensing; two of those were found by the Ohio State University-based MicroFUN group. The latest two planets make six, and he expects that number to double over the next year as other teams publish new findings.

"We're just getting better at what we do," Gaudi said. "We've hit our stride with this technique."

He has also calculated that the next generation of microlensing experiments -- using telescopes on the ground and in space -- will likely be able to detect analogs to all of our solar system's planets, except for the tiniest one, Mercury.

The current discovery relied on 11 different ground-based telescopes in countries around the world, including New Zealand, Tasmania, Israel, Chile, the Canary Islands, and the United States.

Both professional and amateur skywatchers joined in. People from three other microlensing collaborations -- the Microlensing Observations in Astrophysics (MOA) Collaboration, the Probing Lensing Anomalies NETwork (PLANET), and the RoboNet Collaboration -- all contributed observations and are co-authors of the study with MicroFUN and OGLE.

Gaudi described this microlensing event as the most complicated one ever studied. The astronomers carefully modeled their data on computers, and explored all possible explanations for the light signal. A year and a half later, they were confident that they'd found two planets. In part, their confidence came from additional observations from the W.M. Keck Observatory in Hawaii, which they used to calculate the mass of the star.

Ohio State coauthors on the Science paper included Darren DePoy and Richard Pogge, both professors of astronomy; and Subo Dong and Stephan Frank, both graduate students. Other coauthors hailed from the University of Notre Dame, Warsaw University Observatory, Auckland Observatory, Tel-Aviv University, Farm Cove Observatory, Mt. John Observatory, Lawrence Livermore National Laboratory, Princeton University Observatory, Universidad de Concepcion, University of Cambridge, Chungbuk National University, Korea Astronomy and Space Science Institute, Campo Catino Astronomical Observatory, Nagoya University, Massey University, University of Auckland, University of Canterbury, Victoria University, Konan University, Nagano National College of Technology, University of Manchester, Tokyo Metropolitan College of Aeronautics, University of Exeter, Universite Pierre et Marie Curie, Liverpool John Moores University, University of St. Andrews, University of Tasmania, Universite Paul Sabatier-Toulouse, Dartmouth College, and the University of Oxford.

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