Figure 1: Comets are pristine remnants from the early Solar System. Comets are mostly made of ice and dust, but are also known to be rich in organic materials. If "complex" organic molecules like amino acids are enriched in comets and the meteoroids of cometary origin, the meteor showers might have delivered water and complex organic materials to the ancient Earth. (An artist's illustration. Credit: Kyoto Sangyo University)
Using the Cooled Mid-Infrared Camera and Spectrometer (COMICS) on the
Subaru Telescope, astronomers have detected an unidentified infrared
emission band from comet 21P/Giacobini-Zinner (hereafter, comet 21P/G-Z)
in addition to the thermal emissions from silicate and carbon grains.
These unidentified infrared emissions are likely due to complex organic
molecules, both aliphatic and aromatic hydrocarbons, contaminated by N-
or O-atoms. Considering the properties of the dust and organic
molecules, comet 21P/G-Z might have originated from the circumplanetary
disk of a giant planet (like Jupiter or Saturn) where it was warmer than
the typical comet-forming regions.
Comet 21P/G-Z is a Jupiter-family comet with an orbital period of
about 6.6 years and is thought to be the parent body of the October
Draconids meteor shower. Compared to other comets, this comet is
peculiar in terms of its volatile content (depleted in carbon-chain
molecules, NH2, and highly volatile species) and the
properties of its dust grains, and is categorized as "G-Z type" (~6% of
surveyed comets). Based on previous studies, it was proposed that comet
21P/G-Z originated in a different region than other comets, but we
didn’t have any information about the specific region in the
protoplanetary disk. A negative trend of linear polarization in the
optical wavelength region is also reported for the dust continuum of
comet 21P/G-Z. It is suggested that this negative wavelength gradient of
polarization might be explained by a higher content of organic
materials in the dust grains of 21P/G-Z. If complex organic molecules
like amino acids are enriched in comet 21P/G-Z and in the meteoroids of
the October Draconids, this meteor shower might have delivered complex
organic materials to the ancient Earth. However, complex
high-molecular-weight organic molecules have never been detected clearly
in comets, except in comet 67P/Churyumov-Gerasimenko by the in-situ
measurements of the Rosetta spacecraft. How much and how complex of
organic molecules are contained in comet 21P/G-Z is still an open
question.
Figure 2: Comet 21P/Giacobini-Zinner observed in the optical on August 22, 2018
Credit: Michael Jaeger
A team of astronomers from the Institute of Space and Astronautical
Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Kyoto Sangyo
University (KSU), National Astronomical Observatory of Japan (NAOJ), and
Okayama University of Science (OUS) conducted mid-infrared
spectroscopic and imaging observations of comet 21P/G-Z using COMICS on
UT July 5, 2005 (when the comet was 1.04 au from the Sun, near its
perihelion). The obtained spectrum of comet 21P/G-Z shows emission peaks
of crystalline silicate grains, which are usually also seen in many
other comets. In addition to these silicate features, the researchers
found that the spectrum of comet 21P/G-Z exhibits unidentified infrared
emission features, which could be attributed to a mixture of aliphatic
and aromatic hydrocarbons (such as polycyclic aromatic hydrocarbons or
hydrogenated amorphous carbons contaminated by N- or O-atoms).
Comet 21P/G-Z is enriched in complex organic molecules. The
enrichment of complex organic molecules requires a warm temperature or
high energetic particle environment around the comet in the early solar
nebula. The presence of these complex organic molecules suggests that
comet 21P/G-Z originated from a warmer region in the protoplanetary disk
than the typical comet-forming region. Considering that the derived
mass fraction of crystalline silicates in comet 21P/G-Z is typical of
comets, we propose that the comet originated from the circumplanetary
disk of a giant planet (like Jupiter or Saturn) where it was warmer than
the typical comet-forming region (5–30 au from the Sun) and was
suitable for the formation of complex organic molecules. Comets from
circumplanetary disks might be enriched in complex organic molecules,
similar to comet 21P/G-Z, and may have provided pre-biotic molecules to
ancient Earth by direct impact or meteor showers.
Figure 3: Blackbody normalized mid-infrared spectra of
comets. The spectrum of comet 21P/G-Z (black filled circles) is
different from other comets, and exhibits unidentified infrared emission
features. The features at ~8.2 microns, ~8.5 microns, and ~11.2 microns
could be attributed to PAHs (or HACs) contaminated by N- or O-atoms,
although part of the feature at ~11.2 microns comes from crystalline
olivine. The feature at ~9.2 microns might originate from aliphatic
hydrocarbons. (Credit: Ootsubo et al.).
These results were published on November 18, 2019 in Icarus (Ootsubo et al., "Unidentified Infrared Emission Features in Mid-infrared Spectrum of Comet 21P/Giacobini-Zinner"). This research paper is also available as a preprint (Ootsubo et al., arXiv:1910.03485)
on arxiv.org. This study is financially supported by MEXT Supported
Program for the Strategic Research Foundation at Private Universities,
2014-2018 (No. S1411028). T.O. is supported by JSPS KAKENHI
Grants-in-Aid for Scientific Research (C) JP17K05381 and (A) JP19H00725.
Link
Source: Subaru Telescope
