439 research outputs found
Hall Effect in the coma of 67P/Churyumov-Gerasimenko
Magnetohydrodynamics simulations have been carried out in studying the solar
wind and cometary plasma interactions for decades. Various plasma boundaries
have been simulated and compared well with observations for comet 1P/Halley.
The Rosetta mission, which studies comet 67P/Churyumov-Gerasimenko, challenges
our understanding of the solar wind and comet interactions. The Rosetta Plasma
Consortium observed regions of very weak magnetic field outside the predicted
diamagnetic cavity. In this paper, we simulate the inner coma with the Hall
magnetohydrodynamics equations and show that the Hall effect is important in
the inner coma environment. The magnetic field topology becomes complex and
magnetic reconnection occurs on the dayside when the Hall effect is taken into
account. The magnetic reconnection on the dayside can generate weak magnetic
filed regions outside the global diamagnetic cavity, which may explain the
Rosetta Plasma Consortium observations. We conclude that the substantial change
in the inner coma environment is due to the fact that the ion inertial length
(or gyro radius) is not much smaller than the size of the diamagnetic cavity.Comment: 23 pages, 6 figur
Interpretation of the ion mass spectra in the mass range 25-35 obtained in the inner coma of Halley's comet by the HIS-sensor of the Giotto IMS Experiment
The IMS-HIS double-focussing mass spectrometer that flew on the Giotto spacecraft covered the mass per charge range from 12 to 56 (AMU/e). By comparing flight data, calibration data, and results of model calculations of the ion population in the inner coma, the absolute mass scale is established, and ions in the mass range 25 to 35 are identified. Ions resulting from protonation of molecules with high proton affinity are relatively abundant, enabling us to estimate relative source strengths for H2CO, CH3OH, HCN, and H2S, providing for the first time a positive in situ measurement of methanol. Also, upper limits for NO and some hydrocarbons are derived
Origin of molecular oxygen in Comet 67P/Churyumov-Gerasimenko
Molecular oxygen has been detected in the coma of comet
67P/Churyumov-Gerasimenko with abundances in the 1-10% range by the ROSINA-DFMS
instrument on board the Rosetta spacecraft. Here we find that the radiolysis of
icy grains in low-density environments such as the presolar cloud may induce
the production of large amounts of molecular oxygen. We also show that
molecular oxygen can be efficiently trapped in clathrates formed in the
protosolar nebula, and that its incorporation as crystalline ice is highly
implausible because this would imply much larger abundances of Ar and N2 than
those observed in the coma. Assuming that radiolysis has been the only O2
production mechanism at work, we conclude that the formation of comet
67P/Churyumov-Gerasimenko is possible in a dense and early protosolar nebula in
the framework of two extreme scenarios: (1) agglomeration from pristine
amorphous icy grains/particles formed in ISM and (2) agglomeration from
clathrates that formed during the disk's cooling. The former scenario is found
consistent with the strong correlation between O2 and H2O observed in 67P/C-G's
coma while the latter scenario requires that clathrates formed from ISM icy
grains that crystallized when entering the protosolar nebula.Comment: The Astrophysical Journal Letters, in pres
A protosolar nebula origin for the ices agglomerated by Comet 67P/Churyumov-Gerasimenko
The nature of the icy material accreted by comets during their formation in
the outer regions of the protosolar nebula is a major open question in
planetary science. Some scenarios of comet formation predict that these bodies
agglomerated from crystalline ices condensed in the protosolar nebula.
Concurrently, alternative scenarios suggest that comets accreted amorphous ice
originating from the interstellar cloud or from the very distant regions of the
protosolar nebula. On the basis of existing laboratory and modeling data, we
find that the N/CO and Ar/CO ratios measured in the coma of the Jupiter
family comet 67P/Churyumov-Gerasimenko by the ROSINA instrument aboard the
European Space Agency's Rosetta spacecraft match those predicted for gases
trapped in clathrates. If these measurements are representative of the bulk
N/CO and Ar/CO ratios in 67P/Churyumov-Gerasimenko, it implies that the
ices accreted by the comet formed in the nebula and do not originate from the
interstellar medium, supporting the idea that the building blocks of outer
solar system bodies have been formed from clathrates and possibly from pure
crystalline ices. Moreover, because 67P/Churyumov-Gerasimenko is impoverished
in Ar and N, the volatile enrichments observed in Jupiter's atmosphere
cannot be explained solely via the accretion of building blocks with similar
compositions and require an additional delivery source. A potential source may
be the accretion of gas from the nebula that has been progressively enriched in
heavy elements due to photoevaporation.Comment: The Astrophysical Journal Letters, in pres
Future thruster application: combination of numerical simulation of ECR zone and plasma X-ray Bremsstrahlung measurement of the SWISSCASE ECR ion source
We present the combination of the numerical 3D magnetic field simulation of SWISSCASE, the new 10 GHz ECR ion source at the University of Bern in Switzerland, and the experimental X-ray Bremsstrahlung measurement of the same ion source, to determine the hot electron and the total electron number densities of its ECR plasma. The results, which are in excellent agreement with literature, demonstrate the quality of the numerical simulation, the X-ray Bremsstrahlung measurement and the method of combination to calculate these particle densities. The revealed key parameters of the ECR plasma such as geometry, particle densities and Bremsstrahlung emission, may enable the development of a microwave ECR plasma model, yet to be defined, which can be integrated into a Finite Difference Time Domain (FDTD) simulation to reproduce realistic microwave-plasma interaction. The presented method of 3D magnetic field modeling, X-ray Bremsstrahlung measurement and the subsequent determination of the electron densities is not limited to the SWISSCASE ion source but can further be used for detailed investigation and optimization of current and future electric propulsion concepts
Identification and characterization of a new ensemble of cometary organic molecules.
In-situ study of comet 1P/Halley during its 1986 apparition revealed a surprising abundance of organic coma species. It remained unclear, whether or not these species originated from polymeric matter. Now, high-resolution mass-spectrometric data collected at comet 67P/Churyumov-Gerasimenko by ESA's Rosetta mission unveil the chemical structure of complex cometary organics. Here, we identify an ensemble of individual molecules with masses up to 140 Da while demonstrating inconsistency of the data with relevant amounts of polymeric matter. The ensemble has an average composition of C1H1.56O0.134N0.046S0.017, identical to meteoritic soluble organic matter, and includes a plethora of chain-based, cyclic, and aromatic hydrocarbons at an approximate ratio of 6:3:1. Its compositional and structural properties, except for the H/C ratio, resemble those of other Solar System reservoirs of organics-from organic material in the Saturnian ring rain to meteoritic soluble and insoluble organic matter -, which is compatible with a shared prestellar history
Is there a future for genome-editing technologies in conservation?
In a recent review, Pimm et al. (2015) highlight emerging technologies in protecting biodiversity. While their list is noteworthy, the authors’ exclusion of innovations in genomic research, with the exception of single-species DNA barcoding methods, was surprising given recent advances in genome-editing technology and its potential application to conservation. Taylor & Gemmell (2016) address that deficiency in a subsequent commentary identifying three avenues where emerging genomic technologies have great potential for increasing our ability to conserve biodiversity. Those areas include the use of next-generation sequencing technologies and methods such as RADseq for monitoring genetic diversity, effective population size, and introgression (Andrews et al., 2016); the use of environmental DNA (eDNA) and metabarcoding approaches to map species occurrence and interaction networks (Evans et al., 2016); and the use of genomic data and gene-editing technology to identify and alter regions of the genome that may impact fitness and limit survival in endangered taxa (Taylor & Gemmell, 2016). Here, we extend that the theme with additional discussion on how genome-editing technologies can benefit the conservation of threatened and endangered species
Is there a future for genome-editing technologies in conservation?
In a recent review, Pimm et al. (2015) highlight emerging technologies in protecting biodiversity. While their list is noteworthy, the authors’ exclusion of innovations in genomic research, with the exception of single-species DNA barcoding methods, was surprising given recent advances in genome-editing technology and its potential application to conservation. Taylor & Gemmell (2016) address that deficiency in a subsequent commentary identifying three avenues where emerging genomic technologies have great potential for increasing our ability to conserve biodiversity. Those areas include the use of next-generation sequencing technologies and methods such as RADseq for monitoring genetic diversity, effective population size, and introgression (Andrews et al., 2016); the use of environmental DNA (eDNA) and metabarcoding approaches to map species occurrence and interaction networks (Evans et al., 2016); and the use of genomic data and gene-editing technology to identify and alter regions of the genome that may impact fitness and limit survival in endangered taxa (Taylor & Gemmell, 2016). Here, we extend that the theme with additional discussion on how genome-editing technologies can benefit the conservation of threatened and endangered species
Observation of a New Type of Low Frequency Waves at Comet 67P/Churyumov-Gerasimenko
We report on magnetic field measurements made in the innermost coma of
67P/Churyumov-Gerasimenko in its low activity state. Quasi-coherent,
large-amplitude (), compressional magnetic field
oscillations at 40 mHz dominate the immediate plasma environment of the
nucleus. This differs from previously studied comet-interaction regions where
waves at the cometary ion gyro-frequencies are the main feature. Thus classical
pick-up ion driven instabilities are unable to explain the observations. We
propose a cross-field current instability associated with newborn cometary ion
currents as a possible source mechanism.Comment: 6 pages, 3 Figure
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