Now, new data has led scientists to develop a theory of how this "hell planet" came to be.
With a mass about eight times that of our planet, the rocky exoplanet 55 Cancri e (shortened to 55 Cnc e and formally called Janssen) is considered a super-Earth, but its surface conditions couldn't be more different from those we enjoy. Janssen orbits its star, called 55 Cancri or Copernicus, at a distance of just 1.4 million miles (2.4 million kilometers), making the planet's year just 18 hours long. By comparison, Mercury orbits about 36 million miles (58 million km) away from the sun. That proximity, of course, is what makes 55 Cancri e so hot — hot enough that the surface of the planet is an ocean of lava and its interior may be filled with diamonds.
Because of Janssen's tight orbit, astronomers have had difficulty studying the planet. But using data from the new Extreme Precision Spectrometer (EXPRES) at the Lowell Observatory's Lowell Discovery Telescope in Arizona, astronomers have for the first time been able to determine the planet's orbital plane, influencing their theory for how the planet formed.
Unlike the other planets in the system, Janssen orbits around Copernicus' equator. Researchers now believe the planet initially formed in a more distant — and thus cooler — location, then was later pulled into its current orbit by Copernicus' gravity.
"We've learned about how this multi-planet system — one of the systems with the most planets that we've found — got into its current state," Lily Zhao, an astrophysicist at the Flatiron Institute in New York and lead author of a new study on the observations, said in a statement.
The research into Janssen could unveil new discoveries about the formation and movement of planetary systems, which in turn could help scientists determine whether or not life might exist elsewhere in the universe. And that's exactly what the team plans to study next.
"We're hoping to find planetary systems similar to ours and to better understand the systems that we do know about," said Zhao.