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Kepler telescope spies details of TRAPPIST-1 system’s outermost planet

last modified May 22, 2017 05:32 PM
Kepler telescope spies details of TRAPPIST-1 system’s outermost planet

Artist impression of the TRAPPIST-1 system. Credits: IoA/Amanda Smith)

University of Cambridge astronomers joined an international team that used data gathered by the Kepler Space Telescope to observe and confirm details of the outermost of seven exoplanets orbiting the star TRAPPIST-1. The observations confirm, as had been predicted, that the seventh and outermost planet, TRAPPIST-1h, orbits its star every 18.77 days. 

Rodrigo Luger, a PhD student at the University of Washington, is lead author on a paper published May 22 in the journal Nature Astronomy.

"TRAPPIST-1h was exactly where our team predicted it to be," Luger said. The researchers discovered a mathematical pattern in the orbital periods of the inner six planets, which was strongly suggestive of an 18.77 day period for planet h. 

TRAPPIST-1A is a middle-aged, ultra cool dwarf star, much less luminous than the Sun and only a bit larger than the planet Jupiter. The star, which is nearly 40 light-years away in the constellation of Aquarius, is named after the ground-based Transiting Planets and Planetesimals Small Telescope (TRAPPIST), the facility that first found evidence of planets around it in 2015.

The TRAPPIST survey is led by Michaël Gillon of the University of Liège, Belgium, who is also a co-author on this research. In 2016, Gillon’s team announced the detection of three planets orbiting TRAPPIST-1 and this number was upped to seven in a subsequent 2017 paper. All seven planets are deemed temperate, meaning that under certain geologic and atmospheric conditions, water could exist in a liquid form. Three of the planets are particularly optimal. In addition the TRAPPIST-1 system is currently the most convenient to remotely explore the atmospheres of planets with sizes similar to Earth.

Such exoplanets are detected when they transit, or pass in front of, their host star, blocking a measurable portion of the light. Kavli Exoplanet fellow Amaury Triaud, from the University of Cambridge, and a contributor to the various discovery announcements about TRAPPIST-1 reflects: “We only captured one transit of TRAPPIST-1h last autumn. However, the resonant pattern formed by the other six planets, and the time TRAPPIST-1h takes to pass in front of its star, allowed the team to deduce its orbital period with a precision of a few minutes.” He continues: “This is absolutely remarkable! TRAPPIST-1h represents a perfect illustration of the power of the scientific method, of its ability to make predictions that can later be verified.”

The inner six planets occupy orbits consistent with being in “resonance”. All orbital periods are mathematically related and slightly influence each other. Orbital resonances can also be found in the Solar system. For instance, Jupiter's moons Io, Europa and Ganymede are set in a 1:2:4 resonance, meaning that while Ganymede orbits Jupiter once, Europa does so twice, and Io four times. The prediction of TRAPPIST-1h’s orbital period principally relied on extrapolating

the known resonant configuration of the inner six planets, to the seventh. This prediction was later confirmed. 

The team analysed 79 days of observation data from K2, the second mission of the Kepler Space Telescope, and was able to recover four transits of TRAPPIST-1h across its star. The K2 data was also used to further characterize the orbits of the other six planets, help rule out the presence of additional transiting planets, and learn the rotation period and activity level of the star. 

TRAPPIST-1's seven-planet chain of resonances establishes a record among known planetary systems. The resonances strengthen the long-term stability of the planetary system. It is also likely that these orbital connections were forged early in the life of the TRAPPIST-1 system, when the planets and their orbits were not fully formed.  

 “Observing TRAPPIST-1 with K2 was an ambitious task,” said Marko Sestovic, a PhD student at the University of Bern and second author of the study. In addition to the complicated signals introduced by the spacecraft’s wobble, the faintness of the star in the optical (the range of wavelengths where K2 observes) placed TRAPPIST-1h “near the limit of what we could detect with K2,” he said. To make matters worse, Sestovic said, one transit of the planet coincided with a transit of TRAPPIST-1b, and one happened during a stellar flare, adding to the difficulty of the observation. “Finding the planet was really encouraging,” Luger said, “since it showed we can still do high-quality science with Kepler despite significant instrumental challenges.”

Contributing to this discovery are researchers at the University of Bern in Switzerland; Paris Diderot and Paris Sorbonne Universities in France; the University of Liège in Belgium; the University of Chicago; the University of California, San Diego; California Institute of Technology; the University of Bordeaux in France; the University of Cambridge in England; NASA's Ames Research Center, Goddard Space Flight Center, and Johnson Space Center; Massachusetts Institute of Technology; the University of Central Lancashire in England; King Abdulaziz University in Saudi Arabia; Cadi Ayyad University in Morocco; and the University of Geneva in Switzerland. 

The research was funded by the NASA Astrobiology Institute via the UW-based Virtual Planetary Laboratory as well as a National Science Foundation Graduate Student Research Fellowship, the Swiss National Science Foundation, the European Research Council and the UK Science and Technology Facilities Council, among other agencies. This work was partially supported by a grant from the Simons Foundation (PI Queloz, grant number 327127)

Based on a press release prepared by the University of Washington. For more information, visit or contact Amaury Triaud at