The Effect of Cosmic Rays on Cometary Nuclei. II. Impact on Ice Composition and Structure

Maggiolo, R.; Gronoff, G.; Cessateur, G.; Moore, W. B.; Airapetian, V. S.; De Keyser, J.; Dhooghe, F.; Gibbons, A.; Gunell, H.; Mertens, C. J.; Rubin, M.; Hosseini, S. (2020). The Effect of Cosmic Rays on Cometary Nuclei. II. Impact on Ice Composition and Structure. Astrophysical journal, 901(2), p. 136. Institute of Physics Publishing IOP 10.3847/1538-4357/abacc3

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Since their formation in the protosolar nebula some ∼4.5 billion years ago, comets are in storage in cold distant regions of the solar system, the Kuiper Belt/scattered disk or Oort Cloud. Therefore, they have been considered as mostly unaltered samples of the protosolar nebula. However, a significant dose of energy is deposited by galactic cosmic rays (GCRs) into the outermost tens of meters of cometary nuclei during their stay in the Oort Cloud or Kuiper Belt. We investigate the impact of energy deposition by GCRs on cometary nuclei. We use experimental results from laboratory experiments and the energy deposition by GCRs estimated by Gronoff et al. (2020), to discuss the depth down to which the cometary nucleus is altered by GCRs. We show that GCRs do not significantly change the isotopic composition of cometary material but modify the chemical composition and the ice structure in the outer layers of the nucleus, which cannot be considered as pristine solar nebula material. We discuss the effect of the collisional history of comets on the distribution of processed material inside the nucleus and its implication on the observation of comets.

Item Type:

Journal Article (Original Article)


08 Faculty of Science > Physics Institute > Space Research and Planetary Sciences
08 Faculty of Science > Physics Institute

UniBE Contributor:

Rubin, Martin


500 Science > 520 Astronomy
600 Technology > 620 Engineering
500 Science > 530 Physics




Institute of Physics Publishing IOP




Dora Ursula Zimmerer

Date Deposited:

05 Nov 2020 08:52

Last Modified:

06 Jan 2021 13:38

Publisher DOI:





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