Here is what scientists know about the planet:

• The planet is known as HD 63433d and it’s the third planet found in orbit around a star called HD 63433.
• HD 63433d is so close to its star, it completes a trip all the way around every 4.2 days.
• “Even though it’s really close-orbiting, we can use follow-up data to search for evidence of outgassing and atmospheric loss that could be important constraints on how terrestrial worlds evolve,” Soares-Furtado says. “But that’s where the similarities end — and end dramatically.”
• Based on its orbit, the astronomers are relatively certain HD 63433d is tidally locked, which means one side is perpetually facing its star.
• That side can reach a brutal 2,300 degrees Fahrenheit and may flow with lava, while the opposite side is forever dark.

What you should know about the planet’s star:

• HD 63433 is roughly the same size and star type as our sun, but (at about 400 million years old) it’s not even one-tenth our sun’s age.
• The star is about 73 light years away from our own sun and part of the group of stars moving together that make up the constellation Ursa Major, which includes the Big Dipper.
• “On a dark night in Madison,” Soares-Furtado says, “you could see [HD 63433] through a good pair of binoculars.”

How the scientists found the planet:

• The study’s authors are collaborating on a planet-hunting project called THYME. In 2020, they used data from NASA’s Transiting Exoplanet Survey Satellite to identify two mini-Neptune-sized planets orbiting HD 63433.
• Since then, TESS took four more looks at the star, compiling enough data for the researchers to detect HD 63433d crossing between the star and the satellite.

What comes next:

• The researchers, including UW–Madison study co-authors graduate student Andrew C. Nine, undergraduate Alyssa Jankowski and Juliette Becker, a UW–Madison astronomy professor, think there is plenty to learn from HD 63433d.
• The planet is uniquely situated for further study. Its peppy young star is visible from both the Northern and Southern hemispheres, increasing the number of instruments, like the South African Large Telescope or WIYN Observatory in Arizona (both of which UW–Madison helped design and build) that can be trained on the system.
• And the star is orders of magnitude closer than many Soares-Furtado has studied, possibly affording opportunities to develop new methods to study gasses escaping from the planet’s interior or measure its magnetic field.

“This is our solar backyard, and that’s kind of exciting,” Soares-Furtado says. “What sort of information can a star this close, with such a crowded system around it, give away? How will it help us as we move on to look for planets among the maybe 100 other, similar stars in this young group it’s part of?”