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Proximity of new planets stuns even astronomers

June 21, 2012
Yale University
One is a rocky planet 1.5 times the size of Earth. The other is a gaseous world nearly four times Earth's size. Together they form a spectacular system in which two planets orbit closer to each other than any yet discovered.

Artist's conception showing Kepler-36c as it might look from the surface of Kepler-36b.
Credit: David Aguilar, Harvard-Smithsonian Center for Astrophysics

One is a rocky planet 1.5 times the size of Earth. The other is a gaseous world nearly four times Earth's size. Together they form a spectacular system in which two planets orbit closer to each other than any yet discovered.

"We've never known of planets like this," said Yale University astronomer Sarbani Basu, a member of the research team that analyzed the system. "If you were on the smaller planet looking up, the larger planet would seem more than twice the size of Earth's full moon. It would be jaw-dropping."

Basu's research focused on determining the properties of the planets' host star -- work that was essential for discerning the characteristics of the orbiting planets.

The 46-member, international team, led by astronomers at Harvard and the University of Washington, report their discovery June 21 in Science Express, the early release version of the journal Science.

"These two worlds are having close encounters," said Josh Carter, lead author of the paper and a Hubble Fellow at the Harvard-Smithsonian Center for Astrophysics.

Located about 1200 light years away, the two-planet system -- now called Kepler-36 -- orbits a star similar to Earth's sun, but bigger and older.

The larger outer planet, Kepler-36c, is a hot, gaseous, Neptune-like planet. The smaller inner planet, Kepler-36b, is rocky and subject to quakes and volcanic eruptions caused by the interplay of the planets' gravitational forces on each other.

Like our sun, Kepler-36 pulsates constantly. Data on its quakes enabled the team to determine its size, weight, and age (all greater than those of our sun). Knowing the star's radius and mass enabled the calculation of the sizes and masses of the planets. From this information, astronomers could determine the planets' densities and characteristics: the smaller planet is denser than Earth and hence must be rocky; the larger planet is much less dense, in fact less dense than water, suggesting it is gaseous.

"The precise determination of the planets' properties was possible because the star around which they revolve could be characterized precisely," said Basu.

The planets' proximity to each other is astonishing, according to the researchers. The rocky inner planet orbits its star every 14 days, at an average distance of 11 million miles. The outer gaseous planet orbits every 16 days, at an average distance of 12 million miles.

Every 97 days they move into perfect alignment, a position known as conjunction. At that point they are separated by a mere 1.2 million miles -- less than five times the distance between Earth and its moon. By contrast, Venus, Earth's nearest neighbor, never comes closer than 26 million miles.

The research team identified the planets by analyzing data from NASA's Kepler satellite. Kepler detects planets by measuring variations in the brightness of stars; dips in brightness may indicate a planet passing in front the star.

This discovery poses new challenges to the theories of planet formation. Astronomers are now trying to understand how planets with markedly different compositions and densities fell into remarkably close orbit.

NASA and the National Science Foundation supported the research. The national research councils of the United Kingdom, Denmark and the Netherlands also provided support.

Eric Agol of the University of Washington is a co-lead author of the paper.

Story Source:

The above post is reprinted from materials provided by Yale University. Note: Materials may be edited for content and length.

Journal Reference:

  1. Joshua A. Carter, Eric Agol, William J. Chaplin, Sarbani Basu, Timothy R. Bedding, Lars A. Buchhave, Jørgen Christensen-Dalsgaard, Katherine M. Deck, Yvonne Elsworth, Daniel C. Fabrycky, Eric B. Ford, Jonathan J. Fortney, Steven J. Hale, Rasmus Handberg, Saskia Hekker, Matthew J. Holman, Daniel Huber, Christopher Karoff, Steven D. Kawaler, Hans Kjeldsen, Jack J. Lissauer, Eric D. Lopez, Mikkel N. Lund, Mia Lundkvist, Travis S. Metcalfe, Andrea Miglio, Leslie A. Rogers, Dennis Stello, William J. Borucki, Steve Bryson, Jessie L. Christiansen, William D. Cochran, John C. Geary, Ronald L. Gilliland, Michael R. Haas, Jennifer Hall, Andrew W. Howard, Jon M. Jenkins, Todd Klaus, David G. Koch, David W. Latham, Phillip J. MacQueen, Dimitar Sasselov, Jason H. Steffen, Joseph D. Twicken, and Joshua N. Winn. Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities. Science, 21 June 2012 DOI: 10.1126/science.1223269

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Yale University. "Proximity of new planets stuns even astronomers." ScienceDaily. ScienceDaily, 21 June 2012. <>.
Yale University. (2012, June 21). Proximity of new planets stuns even astronomers. ScienceDaily. Retrieved May 30, 2016 from
Yale University. "Proximity of new planets stuns even astronomers." ScienceDaily. (accessed May 30, 2016).

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