WIYN 3.5-meter Telescope at Kitt Peak Discovers Extremely Strange Orbit of Rare Exoplanet

Newswise — At present there are over 5600 confirmed exoplanets in just over 4000 star systems. Within this population, about 300–500 exoplanets fall into the curious class known as hot Jupiters — large, Jupiter-like exoplanets that orbit very close to their star, some even as close as Mercury is to our Sun. How hot Jupiters end up in such close orbits is a mystery, but astronomers postulate that they begin in orbits far from their star and then migrate inward over time. The early stages of this process have rarely been observed, but with this new analysis of an exoplanet with an unusual orbit, astronomers are one step closer to unraveling the hot Jupiter mystery.

The discovery of this exoplanet, named TIC 241249530 b, originated with the detection by NASA’s Transiting Exoplanet Survey Satellite (TESS) in January 2020 of a dip in a star’s brightness consistent with a single Jupiter-sized planet passing in front of, or transiting, it. To confirm the nature of these fluctuations and eliminate other possible causes, a team of astronomers used two instruments on the WIYN 3.5-meter Telescope at the U.S. National Science Foundation Kitt Peak National Observatory (KPNO), a Program of NSF NOIRLab.

The team first utilized the NASA-funded NN-EXPLORE Exoplanet and Stellar Speckle Imager (NESSI) in a technique that helps to ‘freeze out’ atmospheric twinkling and eliminate any extraneous sources that might confuse the signal’s source. Then, using the NASA-funded NEID spectrograph, the team measured the radial velocity of TIC 241249530 b by carefully observing how its host star’s spectrum, or wavelengths of its emitted light, shifted as a result of the exoplanet orbiting it.

Arvind Gupta, NOIRLab postdoctoral researcher and lead author of the paper published in Nature, praised NESSI and NEID as being critical to the team’s efforts to characterize and confirm the exoplanet’s signal. “NESSI gave us a sharper view of the star than would have been possible otherwise, and NEID precisely measured the star’s spectrum to detect shifts in response to the orbiting exoplanet,” explained Gupta. Gupta particularly noted the unique flexibility of NEID’s observation-scheduling framework as it allows for swift adaptation of the team’s observing plan in response to new data.

“The WIYN telescope is playing a crucial role in helping us understand why the planets found in other solar systems can be so different from system to system,” said NSF's Chris Davis, program director for NSF NOIRLab. “The collaboration between NSF and NASA on the NN-EXPLORE program continues to yield impressive results in exoplanet research.”

Detailed analysis of the spectrum confirmed that the exoplanet is approximately five times more massive than Jupiter. The spectrum also revealed that the exoplanet is orbiting along an extremely eccentric, or stretched-out, path. The eccentricity of a planet’s orbit is measured on a scale from 0 to 1, with 0 being a perfectly circular orbit and 1 being highly elliptical. This exoplanet has an orbital eccentricity of 0.94, making it more eccentric than the orbit of any other exoplanet ever found via the transiting method [1]. For comparison, Pluto’s highly elliptical orbit around the Sun has an eccentricity of 0.25; Earth’s eccentricity is 0.02.

If this planet was part of our Solar System its orbit would stretch from its closest approach ten times closer to the Sun than Mercury all the way out to its most distant extent at Earth’s distance. This extreme orbit would cause temperatures on the planet to vary between that of a summer’s day to hot enough to melt titanium.

To add to the unusual nature of the exoplanet’s orbit, the team also found that it’s orbiting backwards, meaning in a direction opposite to the rotation of its host star. This is not something that astronomers see in most other exoplanets, nor in our own Solar System, and it helps inform the team’s interpretation of the exoplanet’s formation history.

The exoplanet’s unique orbital characteristics also hint at its future trajectory. It’s expected that its initial highly eccentric orbit and extremely close approach to its host star will ‘circularize’ the planet’s orbit, since tidal forces on the planet sap energy from the orbit and cause it to gradually shrink and circularize. Discovering this exoplanet before this migration has taken place is valuable as it lends crucial insight into how hot Jupiters form, stabilize, and evolve over time.

“While we can’t exactly press rewind and watch the process of planetary migration in real time, this exoplanet serves as a sort of snapshot of the migration process,” Gupta said. “Planets like this are incredibly rare and hard to find, and we hope it can help us unravel the hot Jupiter formation story.”

"We’re especially interested in what we can learn about the dynamics of this planet's atmosphere after it makes one of its scorchingly close passages to its star," said Jason Wright, Penn State professor of astronomy and astrophysics who supervised the project while Gupta was a doctoral student at the university. "Telescopes like NASA's James Webb Space Telescope have the sensitivity to probe the changes in the atmosphere of the newly discovered exoplanet as it undergoes rapid heating, so there is still much more for the team to learn about the exoplanet."

TIC 241249530 b is only the second exoplanet ever discovered to demonstrate the hot Jupiter pre-migration phase. Together, these two examples observationally affirm the idea that higher-mass gas giants evolve to become hot Jupiters as they migrate from highly eccentric orbits toward tighter, more circular orbits.

“Astronomers have been searching for exoplanets that are likely precursors to hot Jupiters, or that are intermediate products of the migration process, for more than two decades, so I was very surprised — and excited — to find one,” Gupta said. “It’s exactly what I was hoping to find.”

Notes

[1] One exoplanet has been found with a higher eccentricity. HD 20782 b has an eccentricity of 0.956 but is not transiting, thus the orientation of its orbit compared to its host star cannot be determined. This emphasizes the importance of the discovery of TIC 241249530 b whose orbital characteristics could be determined thanks to its transiting its star.

More information

This research was presented in a paper entitled “A hot Jupiter progenitor on a super-eccentric, retrograde orbit” to appear in Nature. DOI: 10.1038/s41586-024-07688-3

NSF NOIRLab (U.S. National Science Foundation National Optical-Infrared Astronomy Research Laboratory), the U.S. center for ground-based optical-infrared astronomy, operates the International Gemini Observatory (a facility of NSF, NRC–Canada, ANID–Chile, MCTIC–Brazil, MINCyT–Argentina, and KASI–Republic of Korea), Kitt Peak National Observatory (KPNO), Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and Vera C. Rubin Observatory (operated in cooperation with the Department of Energy’s SLAC National Accelerator Laboratory). It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on I’oligam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawai‘i, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O’odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.

Links

• Research paper: A hot Jupiter progenitor on a super-eccentric, retrograde orbit
• Photos of WIYN 3.5-meter Telescope
• Videos of the WIYN 3.5-meter Telescope
• Check out other NOIRLab Science Releases

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