Nondetection of helium in the upper atmospheres of TRAPPIST-1b, e, and f

Vigneshwaran Krishnamurthy*, Teruyuki Hirano, Gumundur Stefánsson, Joe P. Ninan, Suvrath Mahadevan, Eric Gaidos, Ravi Kopparapu, Bunei Sato, Yasunori Hori, Chad F. Bender, Caleb I. Cañas, Scott A. Diddams, Samuel Halverson, Hiroki Harakawa, Suzanne Hawley, Fred Hearty, Leslie Hebb, Klaus Hodapp, Shane Jacobson, Shubham KanodiaMihoko Konishi, Takayuki Kotani, Adam Kowalski, Tomoyuki Kudo, Takashi Kurokawa, Masayuki Kuzuhara, Andrea Lin, Marissa Maney, Andrew J. Metcalf, Brett Morris, Jun Nishikawa, Masashi Omiya, Paul Robertson, Arpita Roy, Christian Schwab, Takuma Serizawa, Motohide Tamura, Akitoshi Ueda, Sébastien Vievard, John Wisniewski

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We obtained high-resolution spectra of the ultracool M-dwarf TRAPPIST-1 during the transit of its planet "b"using two high-dispersion near-infrared spectrographs, the Infrared Doppler (IRD) instrument on the Subaru 8.2m telescope, and the Habitable Zone Planet Finder (HPF) instrument on the 10 m Hobby-Eberly Telescope. These spectroscopic observations are complemented by a photometric transit observation for planet "b"using the APO/ARCTIC, which assisted us in capturing the correct transit times for our transit spectroscopy. Using the data obtained by the new IRD and HPF observations, as well as the prior transit observations of planets "b,""e"and "f"from IRD, we attempt to constrain the atmospheric escape of the planet using the He i triplet 10830 Å absorption line. We do not detect evidence for any primordial extended H-He atmospheres in all three planets. To limit any planet-related absorption, we place an upper limit on the equivalent widths of <7.754 mÅ for planet "b,"<10.458 mÅ for planet "e,"<4.143 mÅ for planet "f"at 95% confidence from the IRD data, and <3.467 mÅ for planet "b"at 95% confidence from HPF data. Using these limits along with a solar-like composition isothermal Parker wind model, we attempt to constrain the mass-loss rates for the three planets. For TRAPPIST-1b, our models exclude the highest possible energy-limited rate for a wind temperature <5000 K. This nondetection of extended atmospheres with low mean-molecular weights in all three planets aids in further constraining their atmospheric composition by steering the focus toward the search of high-molecular-weight species in their atmospheres.

    Original languageEnglish
    Article number82
    Pages (from-to)1-8
    Number of pages8
    JournalAstronomical Journal
    Volume162
    Issue number3
    DOIs
    Publication statusPublished - Sep 2021

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