Cited by 34Stellar, planetary, and galactic studiesAstro and Planetary ScienceSpace Science and Extraterrestrial Life

Identifiable acetylene features predicted for young Earth-like exoplanets with reducing atmospheres undergoing heavy bombardment

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Rimmer, P. B., Ferus, M., Waldmann, I. P., Knížek, A., Kalvaitis, D., Ivanek, O., Kubelík, P., Yurchenko, S. N. +9 more·2020·The Astrophysical Journal

Abstract

Abstract The chemical environments of young planets are assumed to be largely influenced by the impacts of bodies lingering on unstable trajectories after the dissolution of the protoplanetary disk. We explore the chemical consequences of impacts within the context of reducing planetary atmospheres dominated by carbon monoxide, methane, and molecular nitrogen. A terawatt high-power laser was selected in order to simulate the airglow plasma and blast wave surrounding the impactor. The chemical results of these experiments are then applied to a theoretical atmospheric model. The impact simulation results in substantial volume mixing ratios within the reactor of 5% hydrogen cyanide (HCN), 8% acetylene (C2H2), 5% cyanoacetylene (HC3N), and 1% ammonia (NH3). These yields are combined with estimated impact rates for the early Earth to predict surface boundary conditions for an atmospheric model. We show that impacts might have served as sources of energy that would have led to steady-state surface quantities of 0.4% C2H2, 400 ppm HCN, and 40 ppm NH3. We provide simulated transit spectra for an Earth-like exoplanet with this reducing atmosphere during and shortly after eras of intense impacts. We predict that acetylene is as observable as other molecular features on exoplanets with reducing atmospheres that have recently gone through their own “heavy bombardments,” with prominent features at 3.05 and 10.5 μm.

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  • Conditions of very low total atmospheric surface pressures and H2O dissociation at least periodically existed during the Archean, as derived from approximately 2.4 Ga old micrometeorites oxidized in the upper atmosphere.

    “That such conditions at least periodically existed and H 2 Owas then indeed dissociated can be derived from ≈ 2.4 Ga old micrometeorites which were oxidized in the upper atmosphere (Tomkins et al. 2016; Zahnle and Buick 2016; Rimmer et al. 2020).”

    From The young Sun's XUV-activity as a constraint for lower CO2-limits in the Earth's Archean atmosphere (2021) · cites this paper as Rimmer et al. 2020

    The Introduction discusses possible Hadean atmospheric compositions, and §5.2 models a reducing atmosphere, but neither addresses the claimed evidence from approximately 2.4 Ga micrometeorites. Searches for micrometeorites, very low surface pressure, and H2O dissociation found no passage linking them to Archean conditions; page numbers are unavailable in our copy. (LLM, conf=0.75)

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Research works printed but not linked: 2

  1. Juha, L., & Civiš, S. 2008, Lasers in Chemistry (Weinheim: Wiley-VCH), 899
  2. Wyatt, M., Kral, Q., & Sinclair, C. 2019, MNRAS, in press (arXiv:1910. 10731)

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Authors
Rimmer, P. B., Ferus, M., Waldmann, I. P., Knížek, A., Kalvaitis, D., Ivanek, O., Kubelík, P., Yurchenko, S. N., Burian, T., Dostál, J., Juha, L., Dudžák, R., Krůs, M., Tennyson, J., Civiš, S., Archibald, A. T., & Granville-Willett, A.
Affiliations
  • MRC Laboratory of Molecular Biology (GB)
  • Czech Academy of Sciences (CZ)
  • University College London (GB)
  • University of Cambridge (GB)
Venue
The Astrophysical Journal
Published
2019-12-30
Volume
888
Issue
1
Pages
21
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2988582677
Cited by
34
References
89
Citations by year
2026: 1 · 2025: 1 · 2024: 6 · 2023: 7 · 2022: 11 · 2021: 6 · 2020: 2
FWCI
2.54
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • UCL Discovery (University College London) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • Simons Foundation (SCOL awards 59963)
  • ERDF/ESF (CZ.02.1.01/0.0/0.0/16_019/0000778)
  • Czech Ministry of Education (LTT17015)
  • UK STFC (ST/M001334/1)
  • European Research Council (European Union Horizon 2020 Grant 758892)
  • Natural Environment Research Council (National Centre for Atmospheric Science)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
Keywords
acetylene, reducing atmosphere, heavy bombardment, hydrogen cyanide, HC3N, ammonia, carbon monoxide, methane, nitrogen molecule, blast wave, transit spectra, early Earth, protoplanetary disks, atmospheric modeling

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