Cited by 100Stellar, planetary, and galactic studiesPlanetary Science and ExplorationSpace Science and Extraterrestrial Life

DETECTING AND CONSTRAINING N2ABUNDANCES IN PLANETARY ATMOSPHERES USING COLLISIONAL PAIRS

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Schwieterman, Edward W., Robinson, Tyler D., Meadows, Victoria S., Misra, Amit, Domagal-Goldman, Shawn·2015·The Astrophysical Journal

Abstract

Characterizing the bulk atmosphere of a terrestrial planet is important for determining surface pressure and potential habitability. Molecular nitrogen (N 2 ) constitutes the largest fraction of Earth's atmosphere and is likely to be a major constituent of many terrestrial exoplanet atmospheres. Due to its lack of significant absorption features, N 2 is extremely difficult to remotely detect. However, N 2 produces an N 2 –N 2 collisional pair, (N 2 ) 2 , which is spectrally active. Here we report the detection of (N 2 ) 2 in Earth's disk-integrated spectrum. By comparing spectra from NASA's EPOXI mission to synthetic spectra from the NASA Astrobiology Institute's Virtual Planetary Laboratory three-dimensional spectral Earth model, we find that (N 2 ) 2 absorption produces a ∼35% decrease in flux at 4.15 μ m. Quantifying N 2 could provide a means of determining bulk atmospheric composition for terrestrial exoplanets and could rule out abiotic O 2 generation, which is possible in rarefied atmospheres. To explore the potential effects of (N 2 ) 2 in exoplanet spectra, we used radiative transfer models to generate synthetic emission and transit transmission spectra of self-consistent N 2 –CO 2 –H 2 O atmospheres, and analytic N 2 –H 2 and N 2 –H 2 –CO 2 atmospheres. We show that (N 2 ) 2 absorption in the wings of the 4.3 μ m CO 2 band is strongly dependent on N 2 partial pressures above 0.5 bar and can significantly widen this band in thick N 2 atmospheres. The (N 2 ) 2 transit transmission signal is up to 10 ppm for an Earth-size planet with an N 2 -dominated atmosphere orbiting within the habitable zone of an M5V star and could be substantially larger for planets with significant H 2 mixing ratios.

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Research works printed but not linked: 3

  1. Dressing, C. D., & Charbonneau, D. 2013, ApJ, 797, 95 · DOI
  2. Krissansen-Totton, J., Bergsman, D. S., & Catling, D. C. 2015, AsBio, submitted (arXiv: 1503.08249) · arXiv
  3. Kurucz, R. L. 1995, in ASP Conf. Ser. 81, Laboratory and Astronomical High Resolution Spectra, ed. A. J. Sauval, R. Blomme & N. Grevesse (Brussells, Belgium: ASP), 17

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Authors
Schwieterman, E. W., Robinson, T. D., Meadows, V. S., Misra, A., & Domagal-Goldman, S.
Affiliations
  • NASA Astrobiology Institute (US)
  • Ames Research Center (US)
  • Goddard Space Flight Center (US)
Venue
The Astrophysical Journal
Published
2015-08-28
Volume
810
Issue
1
Pages
57
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2148711597
Cited by
100
References
72
Citations by year
2026: 4 · 2025: 5 · 2024: 8 · 2023: 7 · 2022: 12 · 2021: 8 · 2020: 10 · 2019: 6 · 2018: 21 · 2017: 6 · 2016: 10 · 2015: 3
FWCI
7.59
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • ResearchWorks at the University of Washington (University of Washington) (submittedVersion)
  • eScholarship (California Digital Library) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Aeronautics and Space Administration (NNA13AA93A, NNH12ZDA002C)
  • University of Washington
  • NASA Astrobiology Institute (NNH12ZDA002C, NNA13AA93A)
  • Ames Research Center
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
Keywords
nitrogen molecule, emission spectra, habitability, synthetic spectra, radiative transfer

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