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Twice the size of Earth

Comparison (left to right) of the size of Earth, Wolf 503b, and Neptune. The blue color of Wolf 503b is presumed; nothing is known yet about the planet's atmosphere or surface. (Credit: NASA Goddard/Robert Simmon (Earth), NASA/JPL (Neptune))
Comparison (left to right) of the size of Earth, Wolf 503b, and Neptune. The blue color of Wolf 503b is presumed; nothing is known yet about the planet's atmosphere or surface. (Credit: NASA Goddard/Robert Simmon (Earth), NASA/JPL (Neptune))

A young Canadian student at Université de Montréal discovers new exoplanet ideal for detailed characterization.

Wolf 503b, an exoplanet twice the size of Earth, has been discovered by an international team using data from NASA’s Kepler Space Telescope. The find is described in a new study led by Merrin Peterson, who just started her master’s degree at the Institute for Research on Exoplanets (iREx), at Université de Montréal (UdeM). Wolf 503b is about 145 light years from Earth in the Virgo constellation and orbits its star ten times closer than Mercury is to the Sun. Scientists are excited about this discovery because Wolf-503b presents an excellent opportunity to study a planet of this size in great detail.

“The discovery and confirmation of this new exoplanet was very rapid, thanks to the collaboration that my advisor, Björn Benneke, and I are a part of,” Peterson said. “In May, I just started my graduate studies when the latest release of Kepler K2 data came in. We were able to quickly analyze the new data quickly and found many interesting candidate exoplanets. Wolf 503b was one of them.”

The team identified distinct, periodic dips that appear in the light curve of the star when the planet passes in front of it. In order to better characterize the star and planet, the astronomers first obtained a spectrum of the host star at the NASA Infrared Telescope Facility. This confirmed that the star is an old ‘orange dwarf’, slightly less luminous than the Sun, and allowed a precise determination of the radius of both the star and its companion. Finally, to confirm the companion was indeed a planet and to avoid making a false positive identification, the team obtained high-resolution images from the Palomar Observatory and also examined archival data to rule out background stars and other companions in the same planetary system.

Size of Wolf 503b compared to the distribution of planets found by the Kepler Telescope. Wolf 503b falls just to the right of the ‘Fulton Gap’, a still poorly understood lack of planets between 1.5 and 2 times the radius of the Earth. (Credit: B.J. Fulton, using data from  NASA Ames, Caltech and University of Hawaii)

Wolf 503b is interesting, firstly, because of its size. Thanks to the Kepler telescope, we know that most of the planets in the Milky Way that orbit close to their stars are about as big as Wolf 503b, somewhere between that the size of the Earth and Neptune (which is 4 times bigger than Earth). Since there is nothing like them in our solar system, astronomers wonder whether these planets are small and rocky ‘super-Earths’ or gaseous mini versions of Neptune. One recent discovery also shows that there are significantly fewer planets that are between 1.5 and 2 times the size of Earth than those either smaller or larger than that. This drop, called the Fulton gap, could be what distinguishes the two types of planets from each other, researchers say in their study of the discovery, published in 2017.

“Wolf 503b is one of the only planets with a radius (near the gap that has a star that is bright enough to be amenable to more detailed study that will better constrain its true nature,” explained Björn Benneke, an UdeM professor and member of iREx and CRAQ. “It provides a key opportunity to better understand the origin of this radius gap as well as the nature of the intriguing populations of ‘super-Earths’ and ‘sub-Neptunes’ as a whole.”

The second reason for interest in the Wolf 503b system is that the star is relatively close to Earth, and thus very bright. One of the possible follow-up studies for bright stars is the measurement of their radial velocity to determine the mass of the planets in orbit around them. A more massive planet will have a greater gravitational influence on its star, and the variation in line-of-sight velocity of the star over time will be greater. The mass, together with the radius determined by Kepler’s observations, gives the bulk density of the planet, which in turn tells us something about its composition. For example, at its radius, if the planet has a composition similar to Earth, it would have to be about 14 times its mass. If, like Neptune, it has an atmosphere rich in gas or volatiles, it would be approximately half as massive.

Because of its brightness, Wolf 503 will also be a prime target for the upcoming James Webb Space Telescope. Using a technique called transit spectroscopy, it will be possible to study the chemical content of the planet’s atmosphere, and to detect the presence of molecules like hydrogen and water. This is crucial to verify if it is similar to that of the Earth, Neptune or completely different from the atmospheres of planets in our solar system.

Similar observations can’t be made of most planets found by Kepler, because their host stars are usually much fainter. As a result, the bulk densities and atmospheric compositions of most exoplanets are still unknown.

“By investigating the nature of Wolf 503b, we’ll understand more about the structure of planets near the radius gap and more generally about the diversity of exoplanets present in our galaxy,” said Peterson. “I look forward to learning more about it.”


About this study

The article “A 2 Earth Radius Planet Orbiting the Bright Nearby K-Dwarf Wolf 503” was published on xxxx xxx, 2018 in The Astronomical Journal. In addition to Merrin Peterson and her advisor Björn Benneke (iREx, Université de Montréal), the research team included Courtney D. Dressing and Howard Isaacson (University of California, Berkeley); Trevor J. David and Eric E. Mamajek (Jet Propulsion Laboratory, California Institute of Technology); David Ciardi; Jessie L. Christiansen, Benjamin J. Fulton and Charles Beichman (Caltech/IPAC-NASA Exoplanet Science Institute); Joshua E. Schlieder (NASA Goddard Space Flight Center); Erik A. Petigura, Andrew W. Howard and Evan Sinukoff  (California Institute of Technology); Sam Quinn and David W. Latham (Harvard-Smithsonian Center for Astrophysics); Ian J. M. Crossfield, Liang Yu, Avi Shporer, Chelsea X. Huang and Jason Dittmann (Massachusetts Institute of Technology); Thomas Henning (Max Planck Institute for Astronomy);Molly R. Kosiarek (University of California, Santa Cruz); and Nicole Arango (College of the Canyons).



Merrin Peterson and Björn Benneke
Institute for Research on Exoplanets, Université de Montréal,



Marie-Eve Naud and Merrin Peterson
Institute for Research on Exoplanets, Université de Montréal



Link to the scientific article
Link to a free version of the scientific article
Link to UdeM press release