From AAS NOVA: “Opportunities from a Newly Discovered Planetary System”



26 August 2020
Susanna Kohler

Artist’s illustration of two small planets orbiting their host star. Planets such as these tend to fall into two categories: rocky like Earth, or gaseous like Neptune. [NASA/Ames/JPL-Caltech]

Less than 250 light-years from Earth lie two newly found planets orbiting a star not unlike our own. A new study introduces these discoveries and explores what we may learn from future observations of their puffy atmospheres.

Identifying Ideal Targets

The Transiting Exoplanet Survey Satellite (TESS) mission was specifically designed to search for transiting planets smaller than 4 Earth radii around bright stars — and it’s already found more than 1,000 planet candidates, with 10,000 expected by mission end. These discoveries will help us to better understand the transition between rocky planets like Earth, which have compact atmospheres, and gaseous sub-Neptunes, which have extended, puffy atmospheres.

With the upcoming launch of the James Webb Space Telescope (JWST), we’d especially like to identify TESS discoveries that make ideal candidates for transit spectroscopy with JWST. Transit spectroscopy allows us to study the atmospheres of nearby planets as they orbit across the face of their bright host star.

NASA/MIT TESS replaced Kepler in search for exoplanets

TESS light curves showing the phase-folded transits for TOI-421 b (top) and c (bottom). [Adapted from Carleo et al. 2020]

In a new publication, a team of scientists led by Ilaria Carleo (Wesleyan University; INAF-Astronomical Observatory of Padua, Italy) detail TESS’s identification of a transiting planet candidate in the nearby system TOI-421. By conducting a comprehensive follow-up campaign with ground-based photometry, adaptive optics imaging, and spectroscopy, Carleo and collaborators not only confirmed the TESS candidate, but also discovered a second planet orbiting in the same system.

A Pair of Puffy Planets

We find planets all the time — so what makes TOI-421 b and c worth talking about? Carleo and collaborators’ detailed characterization of the planets shows intriguing properties that could help us learn more about the transition between rocky Earths and gaseous Neptunes.

The inner planet, TOI-421 b, has a low density that’s similar to that of Neptune — despite the fact that the planet’s mass is less than half of Neptune’s. Using atmospheric loss models, Carleo and collaborators demonstrate that this puzzling planet — which lies on a blistering 5-day orbit very close to its toasty host star — should have lost all of its hydrogen-dominated atmosphere early in its lifetime. In spite of this, the TOI-421 b’s low bulk density strongly points to the presence of a puffy hydrogen atmosphere. More study will clearly be needed to better understand what we’re missing about this mysterious planet.

TOI-421 b and c lie among the 30 most favorable targets for atmospheric characterization, based on their predicted signal to noise with future observations. [Carleo et al. 2020]

As for TOI-421 c, this outer planet has roughly the same mass as Neptune, but its bulk density is extremely low — TOI-421 c’s density is less than half of Neptune’s. The authors show that the large radius of this planet and the quietness of its host star should make it an ideal target for followup atmospheric characterization.

Carleo and collaborators’ models suggest that these planets’ extended atmospheres can be probed with ultraviolet observations like those from Hubble; the authors also provide detailed predictions of what we expect to find in the transmission spectra of the two planets from JWST.

Comparison of these predictions to future observations of the TOI-421 system is sure to provide valuable insight from these intriguing, puffy planets.


“The Multiplanet System TOI-421,” Ilaria Carleo et al 2020 AJ 160 114.

See the full article here .


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