The Transmission Spectrum of the Potentially Rocky Planet L 98-59 c

Abstract We present observations of the 1.35 ± 0.07 Earth radius planet L 98-59 c, collected using Wide Field Camera 3 on the Hubble Space Telescope (HST). L 98-59 is a nearby (10.6 pc), bright ( H = 7.4 mag) M3V star that harbors three small, transiting planets. As one of the closest known transiting multi-planet systems, L 98-59 offers one of the best opportunities to probe and compare the atmospheres of rocky planets that formed in the same stellar environment. We measured the transmission spectrum of L 98-59 c, and the extracted spectrum showed marginal evidence (2.1 σ ) for wavelength-dependent transit depth variations that could indicate the presence of an atmosphere. We forward-modeled possible atmospheric compositions of the planet based on the transmission spectrum. Although L 98-59 was previously thought to be a fairly quiet star, we have seen evidence for stellar activity, and therefore we assessed a scenario where the source of the signal originates with inhomogeneities on the stellar surface. We also see a correlation between transits of L 98-59 c and L 98-59 b collected 12.5 hr apart, which is suggestive (but at <2 σ confidence) of a contaminating component from the star impacting the exoplanet spectrum. While intriguing, our results are inconclusive and additional data are needed to verify any atmospheric signal. Fortunately, additional data have been collected from both the HST and James Webb Space Telescope. Should this result be confirmed with additional data, L 98-59 c would be the first planet smaller than 2 Earth radii with a detected atmosphere.

Authors

Publication Details

Journal
The Astronomical Journal
Published
2025-04-02
DOI
https://doi.org/10.3847/1538-3881/ada5f6
Citations
2
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
2.31

Funders

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article

The Transmission Spectrum of the Potentially Rocky Planet L 98-59 c

Joshua E. Schlieder, Laura D. Vega, James Mang, Christina Hedges et al.
2 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
2.31
article

The Transmission Spectrum of the Potentially Rocky Planet L 98-59 c

Joshua E. Schlieder, Laura D. Vega, James Mang, Christina Hedges, Francesco Gallo, Mario Damiano, Kyle Sheppard, Laura Kreidberg, Susan E. Mullally, Stefano Fiscale, Ian J. M. Crossfield, Eric Lopez, Daria Pidhorodetska, Shawn Domagal‐Goldman, Emily A. Gilbert, Renyu Hu, Veselin B. Kostov, Jonathan Brande, Daniel D. B. Koll, Ravi Kopparapu, Edwin S. Kite, Giuliano Liuzzi, Knicole D. Colón, Gerónimo Villanueva, G. Covone, Thomas Barclay, Natasha Latouf, Sebastian Zieba, Caroline Morley, Avi M. Mandell, Elisa V. Quintana, Thomas J. Fauchez, Giada Arney, Allison Youngblood
article en
2 citations

Abstract

Abstract We present observations of the 1.35 ± 0.07 Earth radius planet L 98-59 c, collected using Wide Field Camera 3 on the Hubble Space Telescope (HST). L 98-59 is a nearby (10.6 pc), bright ( H = 7.4 mag) M3V star that harbors three small, transiting planets. As one of the closest known transiting multi-planet systems, L 98-59 offers one of the best opportunities to probe and compare the atmospheres of rocky planets that formed in the same stellar environment. We measured the transmission spectrum of L 98-59 c, and the extracted spectrum showed marginal evidence (2.1 σ ) for wavelength-dependent transit depth variations that could indicate the presence of an atmosphere. We forward-modeled possible atmospheric compositions of the planet based on the transmission spectrum. Although L 98-59 was previously thought to be a fairly quiet star, we have seen evidence for stellar activity, and therefore we assessed a scenario where the source of the signal originates with inhomogeneities on the stellar surface. We also see a correlation between transits of L 98-59 c and L 98-59 b collected 12.5 hr apart, which is suggestive (but at <2 σ confidence) of a contaminating component from the star impacting the exoplanet spectrum. While intriguing, our results are inconclusive and additional data are needed to verify any atmospheric signal. Fortunately, additional data have been collected from both the HST and James Webb Space Telescope. Should this result be confirmed with additional data, L 98-59 c would be the first planet smaller than 2 Earth radii with a detected atmosphere.

The Astronomical JournalVol. 169(5)
Space Telescope Science Institute
Openalex Percentile: Top 12%
Stellar, planetary, and galactic studies
2.31
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