(CNN)“I want to find another Earth. That’s what I’m living for.”
MIT astrophysicist Sara Seager has been looking at planets beyond our solar system, known as exoplanets, for almost 20 years.
When the first ones were discovered in the 1990s, many questioned the finding and didn’t think it was real. But since then, with better technology, we have observed more than 6,000 of them, most of which are giant balls of gas.
Today, the list grows every week.
With so many planets now coming out of hiding, the race is on to identify one that resembles Earth: a rocky world with liquid water just like ours, and suitable to host life.
Seager believes she knows how to make that discovery.
‘These aren’t planets!’
It’s not easy to see exoplanets as you can’t just look at them through a telescope. This is due to the blinding light coming from their host stars, which can be very different in size and features compared to our sun. The process is often described as trying to spot a firefly circling a lighthouse, from thousands of miles away.
The first ones were discovered indirectly, in 1995, by just looking at stars to see if they would wobble slightly, responding to the pull of another object’s gravity
At this time, Seager was a graduate student at Harvard searching for a topic for her Ph.D. and she was intrigued by the newborn field of faraway planets.
“Since the planets were discovered indirectly, most people didn’t believe that the discoveries were real. They’d say to me ‘Why are you doing this? These aren’t planets!’,” says Seager.
The contrarians weren’t entirely wrong: the wobble can be caused by other factors such as another star and several planet discoveries have been retracted over time for this reason.
But then a different technique was found to make their hunt easier, called transit. This is when a planet moves in front of its host star and causes the star’s light to dim slightly.
“One of the planets from the wobble technique showed transit: it went in front of the star at exactly the time it was predicted to and that was basically incontrovertible,” says Seager.
Exoplanets were real.
In 2014, NASA found the first Earth-sized planet orbiting a star in the habitable zone. This was named Kepler-186f — after the Kepler space telescope, used to spot it — and is about 500 light-years away in the constellation Cygnus, the galactic equivalent of our neighbourhood since the Milky Way is about 100,000 light years across. This planet is 10% larger than Earth.
Described by NASA as “a significant step toward finding worlds like our planet Earth,” Kepler-186f orbits around a type of common star known as a red dwarf, which is about half the size of our sun.
Then, in 2015, astronomers found the first Earth-like planet orbiting a star just like our sun, called Kepler-452b. This was dubbed Earth’s “bigger, older cousin,” as the planet is 60% larger than Earth and completes one orbit in 385 days, making its years remarkably close to our own
With our current technology, however, it’s hard to know much more than the size of an exoplanet and how far it is from its star.
But that’s about to change.
New eyes in the sky
The majority of exoplanet discoveries have been made by the Kepler space telescope, after which most of them have been named. Launched in 2009, the telescope has now entered emergency mode 75 million miles away from Earth, due to a malfunction.
To study the atmospheres of potential Earth twins, scientists need new eyes in the sky.
To date, Seager has only been able to study the atmospheres of a handful of exoplanets — all gas giants — but she’s involved in a new NASA program launching in 2017 to just scout the brightest nearby stars for small rocky planets in the habitable zone.
Called TESS (Transiting Exoplanet Survey Satellite), the two-year mission will accumulate data that will then be fed into the James Webb Space Telescope, the next Hubble, which is due to launch in 2018: “It’s going to be amazing,” says Seager.
The James Webb telescope — named after the head of NASA during the pioneering era of the 1960s — will look at the cosmos with unprecedented clarity thanks to its use of a primary mirror about five times larger than Hubble’s. It will also offer direct imaging of exoplanets by blocking the blinding light of their host stars with special instruments that make them more visible. This will allow Seager and other astronomers to study exoplanets like never before.
Seager believes many of the planets in their search will be the rocky, watery worlds she’s been looking for.
“I’m absolutely confident they’re out there.”