The TRAPPIST-1 system has been of great interest to observers and planetary scientists because it seems to contain seven planets that are all roughly Earth-sized.
"Because the TRAPPIST-1 star is very old and dim, the surfaces of the planets have relatively cool temperatures by planetary standards, ranging from 126 degrees Celsius, which is cooler than Venus, to minus 106 degrees Celsius, which is colder than Earths poles," said Amy Barr, a scientist at Planetary Science Institute in the US.
"The planets also orbit very close to the star, with orbital periods of a few days. Because their orbits are eccentric - not quite circular - these planets could experience tidal heating just like the moons of Jupiter and Saturn," said Mr Barr.
"Assuming the planets are composed of water ice, rock, and iron, we determine how much of each might be present, and how thick the different layers would be," he said.
"Because the masses and radii of the planets are not very well-constrained, we show the full range of possible interior structures and interior compositions," Mr Barr said.
The teams results show that improved estimates of the masses of each planet can help determine whether each of the planets has a significant amount of water.
Analyses show that planets d and e are the most likely to be habitable due to their moderate surface temperatures, modest amounts of tidal heating, and because their heat fluxes are low enough to avoid entering a runaway greenhouse state.
A global water ocean likely covers planet d, researchers said.
The team calculated the balance between tidal heating and heat transport by convection in the mantles of each planet.
Results show that planets b and c likely have partially molten rock mantles. The paper also shows that planet c likely has a solid rock surface, and could have eruptions of silicate magmas on its surface driven by tidal heating, similar to Jupiters moon Io