Astronomers have detected a record seven Earth-sized planets orbiting a single star.
The researchers said that all seven could potentially support liquid water on the surface, depending on the other properties of those planets.
Three of these worlds were within the "habitable" zone where life was considered a possibility.
The compact system of exoplanets orbits Trappist-1, a low-mass, cool star located 40 light-years away from Earth.
The planets were detected using Nasa's Spitzer Space Telescope and several ground-based observatories are described in the journal Nature.
"The planets are all close to each other and very close to the star, which is very reminiscent of the moons around Jupiter," said lead author Michaël Gillon, from Belgium's University of Liège.
"Still, the star is so small and cold that the seven planets are temperate, which means that they could have some liquid water - and maybe life, by extension - on the surface."
Three of the Trappist-1 planets fall within the traditional habitable zone definition, where surface temperatures could support the presence of liquid water - given sufficient atmospheric pressure.
Dr Gillon said this was the largest number of Earth-sized planets found in a single habitable zone.
Co-author Amaury Triaud, from the University of Cambridge, UK, said that if the planet furthest from the parent star, Trappist-1h, had an atmosphere that efficiently trapped heat, more like Venus's atmosphere than Earth's, it might be habitable.
'Much we don't know'
The six inner planets have orbital periods that are organised in a "near-resonant chain". This means that in the time that it takes for the innermost planet to make eight orbits, the second, third and fourth planets revolve five, three and two times around the star, respectively.
This appears to be an outcome of interactions early in the evolution of the planetary system.
The astronomers say it should be possible to study the planets' atmospheric properties with telescopes.
"The James Webb Space Telescope, Hubble's successor, will have the possibility to detect the signature of ozone if this molecule is present in the atmosphere of one of these planets," said co-author Prof Brice-Olivier Demory, from the University of Bern in Switzerland.
"This could be an indicator for biological activity on the planet."
But the astrophysicist also warns that we must remain extremely careful about inferring biological activity from afar.
Some of the properties of cooler, low mass stars could make life a more challenging prospect. For example, some are known to emit large amounts of radiation in the form of flares, which has the potential to sterilise the surfaces of nearby planets.
In addition, the habitable zone is located closer to the star to receive the heating necessary for liquid water to persist. This also causes planets to become tidally locked, so they always show the same face to their star.
This might have the effect of making one side of the planet hot, and the other cold.
Amaury Triaud said UV light might be vital for producing the chemical compounds that can later be assembled into biological systems. Similarly, if life emerges on the permanent night side of a tidally locked planet, it might be sheltered from any flares.
He said the Trappist-1 star was not particularly active, something it has in common with other "ultra cool dwarfs" the team has surveyed.
"It is fair to say there is much we don't know. Where I am hopeful is that we will know if flares are important, we will know if tidal locking is relevant to habitability and maybe to the emergence of biology," he explained.
"Many of the arguments in favour or disfavour of habitability can be flipped in that way. First and foremost we need observations."
- BBC / NASA