Astronomer’s just discovered the Biggest 'Tatooine' planet yet orbiting two Suns - Physics-Astronomy.org

Astronomer’s just discovered the Biggest 'Tatooine' planet yet orbiting two Suns

Located about 3,700 light-years gone, in the direction of the Cygnus constellation, lies a distant planet called Kepler–1647b, which at approximately 4.4 billion years of age is roughly as older as Earth.But that's about where the similarities end, because Kepler–1647b turns out to hold a pretty sensational point of difference: this newly identified world is the biggest planet ever discovered that orbits two stars. Known as circumbinary planets, these strange cosmic phenomena are often called 'Tatooine' planets, after Luke Skywalker's dusty desert home.
An international team of Scientists led by NASA's Goddard Space Flight Centre just announced the discovery of Kepler–1647b, which has a mass and radius that are nearly identical to Jupiter's. But just because this circumbinary planet might be the biggest of its kind that we currently know about, that didn't make locating it any easier.
"[F]inding circumbinary planets is much harder than finding planets around single stars," said astronomer William Welsh from San Diego State University (SDSU). "The transits are not regularly spaced in time and they can vary in duration and even depth."
The team recognized the planet using data recorded by the Kepler space observatory, and adding to the challenge was Kepler–1647b's other remarkable feature – the immense length of its orbital period. At 1,107 days, this is the longest of any confirmed transiting exoplanet astronomers have yet found.
This means it takes over three years for Kepler–1647b to orbit its host stars - both of which are similar in size to our Sun, with one being slightly smaller, and the other being slightly bigger.
That epic orbital period is the result of Kepler–1647b being located further away from its host stars than other circumbinary planets, which usually hold relatively tight orbits. In the image below, you can see just how much wider Kepler–1647b's orbit (in red) is compared to its circumbinary counterparts (in grey), with Earth's orbit (in blue) added in for reference.
"It's a bit curious that this largest planet took so long to confirm, since it is easier to find big planets than small ones," said SDSU astronomer Jerome Orosz. "But it is because its orbital period is so long."
Evidence for Kepler–1647b's existence was first found back in 2011, when one of the team, Laurance Doyle from the SETI Institute, spotted the planet transit in front of one of its stars. But it took several extra years of analysis and observations – supported by amateur astronomers using the Kilodegree Extremely Little Telescopes in the US and South Africa – before the Scientists confirmed that Kepler–1647b was a circumbinary planet.
While Kepler–1647b's distance from its stars is greater than usual for a circumbinary planet, it's actually within the habitable zone – the distance from a star at which liquid water could exist on a planet's surface, not being so far away that it would freeze, nor so close that it would evaporate.

But, in this case, since Kepler–1647b is a gas giant like Jupiter, the researchers think it's unlikely to host life – although there's a possibility any as-yet-undiscovered moons orbiting the planet could provide a suitable environment for it. Sadly, this means there's probably nobody looking up to see a beautiful two-star sunset like the one Luke Skywalker watches in Star Wars.
Astronomer’s just discovered the Biggest 'Tatooine' planet yet orbiting two Suns


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