Astronomers Pinpoint Two New Double-Star Planetary Systems
The discoveries include the first circumbinary planet revealed by observations from NASAs TESS mission, which will search nearly the entire sky.
Astronomers announced the first discovery made by NASA's TESS mission of a two-star planetary system. Led by researchers at the Goddard Space Flight Center and San Diego State University, with other collaborators, the telescope satellite’s finding marks the start of a much better understanding of such planetary systems.
On behalf of the international team of 60 investigators, including SDSU astronomers William Welsh and Jerome Orosz, the work was presented by researcher Veselin Kostov at the 235th meeting of the American Astronomical Society in Honolulu on January 6.
The new planet, called TOI-1338 b, is about 6.9 times larger than Earth. It orbits its pair of host stars every 95 days. One of the stars is more massive and much brighter than the other, and as the planet orbits around, it blocks some of the light from the brighter star. This transit allows astronomers to measure the size of the planet. The transit was first found in the TESS data by a high school student working at NASA with Kostov over the summer.
“Our analysis confirmed the transit was caused by a circumbinary planet and we were able to measure the planet's properties,” said SDSU astronomer Jerome Orosz.
A dozen such Tatooine-like planets—so named for the desert world in “Star Wars”—were found with NASA's Kepler Mission, which ended in 2013. The orbiting TESS telescope, launched in 2018, will cover nearly the whole sky and enable many more discoveries, perhaps as many as 100 new circumbinary planets. A sample size that large will allow a statistical analysis of the population, which to date has not been possible because too few systems are known.
New Kepler planet
Helping to boost the numbers, SDSU astronomers at the AAS meeting also revealed a new Kepler circumbinary planet, called KOI-3152 b.
“We first noted convincing evidence for this planet in 2012, but confirmation required additional data and improvements in computer modeling,” said SDSU astronomer William Welsh. “In particular, star spots on the primary host star and a weak eclipse signal from the second star made the analysis difficult.”
In 2019, Welsh's master's thesis student Quentin Socia accepted the challenge and spearheaded the investigation.
KOI-3152 b is located 1,347 light-years away and is 3.9 times the size of the Earth. It orbits its binary stars every 175 days. Although KOI-3152 b straddles the hot edge of the habitable zone, it is a low-density gaseous planet and not able to support life as we know it. This work has been accepted for publication in The Astronomical Journal.
This finding marks the latest discovery made by the SDSU team using Kepler Mission data. Their work established this new type of planet and includes the discovery of the most interesting of the circumbinary planets, the Kepler-47 system, consisting of three planets orbiting two stars.
The work was supported in part by grants from NASA and the National Science Foundation, and by a gift to SDSU from John Hood, Jr.
