First Planets Found Around Sun-Like Stars in a Cluster

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Sept. 14, 2012

J.D. Harrington 
Headquarters, Washington 
202-358-5241 
j.d.harrington@xxxxxxxx 

Whitney Clavin 
Jet Propulsion Laboratory, Pasadena, Calif. 
818-354-4673 
whitney.clavin@xxxxxxxxxxxx 

RELEASE: 12-322

FIRST PLANETS FOUND AROUND SUN-LIKE STARS IN A CLUSTER

WASHINGTON -- NASA-funded astronomers have, for the first time, 
spotted planets orbiting sun-like stars in a crowded cluster of 
stars. The findings offer the best evidence yet planets can sprout up 
in dense stellar environments. Although the newfound planets are not 
habitable, their skies would be starrier than what we see from Earth. 


The starry-skied planets are two so-called hot Jupiters, which are 
massive, gaseous orbs that are boiling hot because they orbit tightly 
around their parent stars. Each hot Jupiter circles a different 
sun-like star in the Beehive Cluster, also called the Praesepe, a 
collection of roughly 1,000 stars that appear to be swarming around a 
common center. 

The Beehive is an open cluster, or a grouping of stars born at about 
the same time and out of the same giant cloud of material. As such, 
the stars share a similar chemical composition. Unlike the majority 
of stars, which spread out shortly after birth, these young stars 
remain loosely bound together by mutual gravitational attraction. 

"We are detecting more and more planets that can thrive in diverse and 
extreme environments like these nearby clusters," said Mario R. 
Perez, the NASA astrophysics program scientist in the Origins of 
Solar Systems Program. "Our galaxy contains more than 1,000 of these 
open clusters, which potentially can present the physical conditions 
for harboring many more of these giant planets." 

The two new Beehive planets are called Pr0201b and Pr0211b. The star's 
name followed by a "b" is the standard naming convention for planets. 


"These are the first 'b's' in the Beehive," said Sam Quinn, a graduate 
student in astronomy at Georgia State University in Atlanta and the 
lead author of the paper describing the results, which was published 
in the Astrophysical Journal Letters. 

Quinn and his team, in collaboration with David Latham at the 
Harvard-Smithsonian Center for Astrophysics, discovered the planets 
by using the 1.5-meter Tillinghast telescope at the Smithsonian 
Astrophysical Observatory's Fred Lawrence Whipple Observatory in 
Arizona to measure the slight gravitational wobble the orbiting 
planets induce upon their host stars. Previous searches of clusters 
had turned up two planets around massive stars but none had been 
found around stars like our sun until now. 

"This has been a big puzzle for planet hunters," Quinn said. "We know 
that most stars form in clustered environments like the Orion nebula, 
so unless this dense environment inhibits planet formation, at least 
some sun-like stars in open clusters should have planets. Now, we 
finally know they are indeed there." 

The results also are of interest to theorists who are trying to 
understand how hot Jupiters wind up so close to their stars. Most 
theories contend these blistering worlds start out much cooler and 
farther from their stars before migrating inward. 

"The relatively young age of the Beehive cluster makes these planets 
among the youngest known," said Russel White, the principal 
investigator on the NASA Origins of Solar Systems grant that funded 
this study. "And that's important because it sets a constraint on how 
quickly giant planets migrate inward. And knowing how quickly they 
migrate is the first step to figuring out how they migrate." 

The research team suspects planets were turned up in the Beehive 
cluster because it is rich in metals. Stars in the Beehive have more 
heavy elements such as iron than the sun has. 

According to White, "Searches for planets around nearby stars suggest 
that these metals act like a 'planet fertilizer,' leading to an 
abundant crop of gas-giant planets. Our results suggest this may be 
true in clusters as well." 

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages NASA's 
Exoplanet Exploration Program office. More information about 
exoplanets and NASA's planet-finding program is available at: 

http://planetquest.jpl.nasa.gov 

	
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