Issue |
A&A
Volume 643, November 2020
|
|
---|---|---|
Article Number | A50 | |
Number of page(s) | 8 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201526964 | |
Published online | 02 November 2020 |
Organic matter in interstellar dust lost at the approach to the heliosphere
Exothermic chemical reactions of free radicals ignited by the Sun
1
Planetary Exploration Research Center (PERC), Chiba Institute of Technology,
Tsudanuma 2-17-1,
Narashino,
Chiba
275-0016, Japan
e-mail: hiroshi_kimura@perc.it-chiba.ac.jp
2
Institut für Geologische Wissenschaften, Freie Universität Berlin,
Malteserstr. 74-100,
12249
Berlin, Germany
3
Institute of Earth Sciences, University of Heidelberg,
Im Neuenheimer Feld 234-236,
69120
Heidelberg, Germany
4
Solar System Science Operation Division, Directorate of Science and Robotic Exploration,
ESA-ESAC - PO Box 78,
28691
Villanueva de la Cañada,
Madrid, Spain
5
Klaus Tschira Laboratory for Cosmochemistry, University of Heidelberg,
Im Neuenheimer Feld 234-236,
69120
Heidelberg, Germany
Received:
15
July
2015
Accepted:
15
September
2020
Aims. We tackle the conundrums of organic materials missing from interstellar dust when measured inside the Solar System, while undoubtedly existing in the local interstellar cloud (LIC), which surrounds the Solar System.
Methods. We present a theoretical argument that organic compounds sublimate almost instantaneously by exothermic reactions, when solar insolation triggers the recombination of free radicals or the rearrangement of carbon bonds in the compounds.
Results. It turns out that the triggering temperature lies in the range of 20–50 K by considering that sublimation of organic materials takes place beyond the so-called filtration region of interstellar neutral atoms. We find that in-situ measurements of LIC dust in the Solar System result in an overestimate for the gas-to-dust mass ratio of the LIC, unless the sublimation of organic materials is taken into account. We also find that previous measurements of interstellar pickup ions have determined the total elemental abundances of gas and organic materials, instead of interstellar gas alone.
Conclusions. We conclude that LIC organic matter suffers from sublimation en route to the heliosphere, implying that our understanding of LIC dust from space missions is incomplete. Since space missions inside the orbit of Saturn cannot give any information on the organic substances of LIC dust, one must await a future exploration mission to the inner edge of the Oort cloud for a thorough understanding of organic substances in the LIC. Once our model for the sublimation of interstellar organic matter by exothermic chemical reactions of free radicals is confirmed, the hypothesis of panspermia from the diffuse interstellar medium is ruled out.
Key words: dust, extinction / ISM: abundances / ISM: clouds / ISM: individual objects: the local interstellar cloud (LIC)
© ESO 2020
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