Hydroxylated Mg-rich Amorphous Silicates: A New Component of the 3.2 μm Absorption Band of Comet 67P/Churyumov

Hydroxylated Mg-rich Amorphous Silicates: A New Component of the 3.2 μm Absorption Band of Comet 67P/Churyumov–Gerasimenko

Published:2020-07-14 Issue:2 Volume:897 Page:L37
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Mennella V.^ORCID,Ciarniello M.^ORCID,Raponi A.^ORCID,Capaccioni F.,Filacchione G.^ORCID,Suhasaria T.,Popa C.,Kappel D.^ORCID,Moroz L.,Vinogradoff V.^ORCID,Pommerol A.,Rousseau B.,Istiqomah I.,Bockelee-Morvan D.,Carlson R. W.,Pilorget C.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab919e/pdf

Reference46 articles.

1. Carbon-rich dust in comet 67P/Churyumov-Gerasimenko measured by COSIMA/Rosetta

2. Detection of exposed H2O ice on the nucleus of comet 67P/Churyumov-Gerasimenko

3. Estimate of the erosion rate from H2O mass-loss measurements from SWAN/SOHO in previous perihelions of comet 67P/Churyumov-Gerasimenko and connection with observed rotation rate variations

4. An Astronomical 2175 Å Feature in Interplanetary Dust Particles

5. Chemically Anomalous, Preaccretionally Irradiated Grains in Interplanetary Dust from Comets

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