Abstract
The imminent launch of space telescopes designed to probe the
atmospheres of exoplanets has prompted new efforts to prioritize the
thousands of transiting planet candidates for follow-up
characterization. We report the detection and confirmation of TOI-1842b,
a warm Saturn identified by TESS and confirmed with ground-based
observations from Minerva-Australis, NRES, and the Las Cumbres Observatory Global Telescope. This planet has a radius of RJ, a mass of MJ, an orbital period of days, and an extremely low density (ρ = 0.252 ± 0.091 g cm−3). TOI-1842b has among the best known combinations of large atmospheric scale height (893 km) and host-star brightness (J
= 8.747 mag), making it an attractive target for atmospheric
characterization. As the host star is beginning to evolve off the main
sequence, TOI-1842b presents an excellent opportunity to test models of
gas giant reinflation. The primary transit duration of only 4.3 hr also
makes TOI-1842b an easily-schedulable target for further ground-based
atmospheric characterization.
| Original language | English |
|---|---|
| Article number | 82 |
| Journal | Astronomical Journal |
| Volume | 163 |
| Issue number | 2 |
| Number of pages | 15 |
| ISSN | 0004-6256 |
| DOIs | |
| Publication status | Published - 2022 |
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