Working with data from NASA’s Transiting Exoplanet Survey Satellite, or TESS, Michigan State University has helped discover an Earth-sized exoplanet — a planet outside of our solar system.
This planet, named TOI-700 e, falls within its star’s habitable zone, meaning the newfound planet could be capable of supporting life as we know it. The research team announced the finding Jan. 10 at the American Astronomical Society meeting in Seattle.
Astronomers believe that many such planets exist in our galaxy and across the universe. The discovery of TOI-700 e, along with the earlier confirmation of its host system, could provide unique opportunities to better explore exoplanets going forward.
“Even with more than 5,000 exoplanets discovered to date, TOI-700 e is a key example that we have a lot more to learn,” said Joey Rodriguez, an assistant professor in the Department of Physics and Astronomy at MSU, who helped make the discovery.
Rodriguez was one of the senior researchers on the project, led by Emily Gilbert, a postdoctoral fellow at NASA’s Jet Propulsion Laboratory in Southern California. The duo is also part of the original team that confirmed the TOI-700 system in 2020, finding it had at least three planets (named TOI-700 b, TOI-700 c and TOI-700 d).
With the new discovery, the team showed that the TOI-700 system has two Earth-sized planets within its habitable zone.
“This is one of only a few systems with multiple, small, habitable-zone planets that we know of,” said Gilbert. “That makes the TOI-700 system an exciting prospect for additional follow-up.”
Gilbert, Rodriguez and Andrew Vanderburg, an assistant professor of physics at the Massachusetts Institute of Technology, spearheaded the current project, which included researchers from dozens of
Rodriguez, an exoplanet expert at MSU, sat down to answer some questions to help explain this discovery and the research behind it.
What makes this discovery special?
The discovery of TOI-700 e provides a valuable opportunity for detailed follow-up studies, as it is one of the only systems known with two small planets in the star’s habitable zone. The host star, TOI-700, is well-suited for these characterization efforts.
This system is very accessible in comparison to other candidates or TESS Objects of Interest, TOIs. Some of those other systems are farther away and their stars are fainter. TOI-700 is really close to us — about 100 light years away.
Having a close and bright host star allows us to achieve the sensitivity needed to measure key aspects like the mass of the planets and the composition of a planet’s atmosphere.
How does one go about discovering an exoplanet?
With TESS, we are observing more than 100 million stars across the night sky. When we look at one of those stars, we can also see if a planet moves between the star and the satellite, blocking out just a little bit of the star’s light. We use the analogy of a fly moving in front of a spotlight.
You were also part of the team that originally confirmed the TOI-700 system in 2020. Can you share a little bit of the background there?
There are almost 10,000 exoplanet candidates, but those aren’t all going to turn out to be planets. A large fraction will be, though, and it’s our job to confirm them.
In 2020, there was a series of three papers that came out at the same time that confirmed the TOI-700 system. Emily Gilbert, who led this current effort, led one of those studies. That one looked at the star, its three planets known at the time — b, c and d — and the dynamics of the system.
I led another paper, which also used data from the Spitzer Space Telescope to confirm the system had a habitable-zone, Earth-sized planet. That was planet d.
At the time, we had some hints that there might be another planet, planet e, but on the outside of the system — like way, way outside. After we got in another year of observation with TESS, though, we discovered that planet e was actually inside the habitable zone, in between the orbits of planets b and c.
So TOI-700’s planets aren’t in alphabetical order?
No, and there’s a little bit of an easter egg in our new paper where we say, “Sorry, they are not in order.” But this demonstrates the power of something like TESS and the reason to continue observing systems with already discovered exoplanets. It shows that we have a lot more to learn and there may be surprises as we keep observing.
Can you talk about the names: planet b, c, d and e? Are those final or will you get to pick different ones?
I get this question all the time. People will ask if I can name an exoplanet “Joey-1 b” or if I could name one after my wife. I tell them I could call them that, but nobody else would.
There’s actually a convention and I don’t want to get too far in the weeds, but it is a combination of the discovery instrument or telescope and a catalog number. In the case of TOI-700, before they were confirmed, the candidate planets were designated TOI-700.01, TOI-700.02 and TOI-700.03. As we confirmed them, they became TOI-700 b, TOI-700 c and so on. The “a” gets reserved for the star, even though we just call it TOI-700.