The planet, known as Kepler-453b, is located within its host stars' "habitable zone," the area around the stars in which life could potentially exist.
And the somewhat fortuitous nature of its discovery indicates there could be more like it than previously believed, according to Stephen Kane, an assistant professor of physics and astronomy at San Francisco State University and member of the team that made the discovery.
"If we had observed this planet earlier or later than we did, we would have seen nothing and assumed there was no planet there," Kane said.
Researchers typically detect "exoplanets" - planets outside our solar system - by observing the decrease in starlight as the planet passes, or "transits," between its host star and Earth.
This method is known as the "transit method." But because Kepler-453b is affected by the gravitational pull of two stars, not just one, its orbit is more erratic - "like a spinning top," said Kane. As a result, its transits are only visible to astronomers 9 per cent of the time.
"It's amazing how fortunate we were in catching it at the right time. It's a good reminder that there's always a value in checking again," Kane said.
Kepler-453b blocked 0.5 per cent of its host stars' light during the transit, which enabled researchers to calculate that the planet's radius is 6.2 times that of Earth, or about 60 per cent larger than Neptune.
Its size indicates it is a gas giant, rather than a rocky planet, and thus unable to have life despite being in the habitable zone, researchers said.
Any inhabitants of the system would see two suns in their sky - much like the view from the planet Tatooine in the movie "Star Wars" - orbiting each other every 27 days.
The larger star is about 94 per cent the size of our sun, the smaller star only 20 per cent the size of our sun and much cooler, emitting less than 1 per cent of the larger star's energy. Kepler-453b takes 240 days to orbit its host stars.
The research appears in the Astrophysical Journal.
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