Influence of collisions on ion dynamics in the inner comae of four comets

CONTEXT

Collisions between cometary neutrals in the inner coma of a comet and cometary ions that have been picked up into the solar wind flow and return to the coma lead to the formation of a broad inner boundary known as a collisionopause. This boundary is produced by a combination of charge transfer and chemical reactions, both of which are important at the location of the collisionopause boundary. Four spacecraft measured ion densities and velocities in the inner region of comets, exploring the part of the coma where an ion-neutral collisionopause boundary is expected to form.

AIMS

The aims are to determine the dominant physics behind the formation of the ion-neutral collisionopause and to evaluate where this boundary has been observed by spacecraft.

METHODS

We evaluated observations from three spacecraft at four different comets to determine if a collisionopause boundary was observed based on the reported ion velocities. We compared the measured location of the ion-neutral collisionopause with measurements of the collision cross sections to evaluate whether chemistry or charge exchange are more important at the location where the collisionopause is observed.

RESULTS

Based on measurements of the cross sections for charge transfer and for chemical reactions, the boundary observed by Rosetta appears to be the location where chemistry becomes the more probable result of a collision between H2O and H2O+ than charge exchange. Comparisons with ion observations made by Deep Space 1 at 19P/Borrelly and Giotto at 1P/Halley and 26P/Grigg-Skjellerup show that similar boundaries were observed at 19P/Borrelly and 1P/Halley. The ion composition measurements made by Giotto at Halley confirm that chemistry becomes more important inside of this boundary and that electron-ion dissociative recombination is a driver for the reported ion pileup boundary.

Comparison of neutral outgassing of comet 67P/Churyumov-Gerasimenko inbound and outbound beyond 3 AU from ROSINA/DFMS

CONTEXT

Pre-equinox measurements of comet 67P/Churyumov-Gerasimenko with the mass spectrometer ROSINA/DFMS on board the Rosetta spacecraft revealed a strongly heterogeneous coma. The abundances of major and various minor volatile species were found to depend on the latitude and longitude of the nadir point of the spacecraft. The observed time variability of coma species remained consistent for about three months up to equinox. The chemical variability could be generally interpreted in terms of surface temperature and seasonal effects superposed on some kind of chemical heterogeneity of the nucleus.

AIMS

We compare here pre-equinox (inbound) ROSINA/DFMS measurements from 2014 to measurements taken after the outbound equinox in 2016, both at heliocentric distances larger than 3 AU. For a direct comparison we limit our observations to the southern hemisphere.

METHODS

We report the similarities and differences in the concentrations and time variability of neutral species under similar insolation conditions (heliocentric distance and season) pre- and post-equinox, and interpret them in light of the previously published observations. In addition, we extend both the pre- and post-equinox analysis by comparing species concentrations with a mixture of CO₂ and H₂O.

RESULTS

Our results show significant changes in the abundances of neutral species in the coma from pre- to post-equinox that are indicative of seasonally driven nucleus heterogeneity.

CONCLUSIONS

The observed pre- and post-equinox patterns can generally be explained by the strong erosion in the southern hemisphere that moves volatile-rich layers near the surface.

6-phosphofructo-2-kinase/fructose 2,6-bisphosphatase from rat liver

Rat liver 6-phosphofructo-2-kinase/fructose 2,6-bisphosphatase was phosphorylated by [gamma-32P]ATP plus fructose-6-P or [2-32P]fructose-2,6-P2. The radioactivity co-migrated with homogeneous 6-phosphofructo-2-kinase/fructose 2,6-bisphosphatase during sodium dodecyl sulfate-disc gel electrophoresis and the phosphoenzyme was acid-labile and base-stable. Hydrolysis of the phosphate group from phosphoenzyme prepared with either donor and the hydrolysis of their tryptic phosphopeptides depended on pH similarly. The pH dependence suggested that phosphate was linked to the N3 of a histidine residue. Co-electrophoresis and co-chromatography of alkaline hydrolysates of the labeled phosphoenzyme prepared from either substrate allowed the definitive identification of 3-phosphohistidine in the degradation products. Modification of the enzyme with diethylpyrocarbonate inactivated both the phosphotransferase and phosphohydrolase activities and suppressed the phosphorylation of the enzyme by ATP and fructose-6-P or by fructose-2,6-P2. Trypsin digestion of the phosphoenzyme formed upon incubation with ATP or fructose-2,6-P2 yielded an identical phosphopeptide after high pressure liquid chromatography. All the above data are consistent with this enzyme catalyzing both phosphohydrolase and phosphotransferase reactions with the mediation of phosphohistidine in the reaction scheme(s).

The synthesis of deuterium-substituted, spin-labeled analogues of AMP and NAD+ and their use in ESR studies of lactate dehydrogenase

Two spin-labeled analogues of AMP and NAD+ were synthesized, in which a perdeuterated nitroxide radical (4-amino-2,2,6,6-tetramethylpiperidine-1-oxyl, TEMPAMINE) was attached to C-6 or C-8 position of the adenine ring. The ESR spectra of these derivatives exhibit a 4-fold increase in sensitivity and a concomitant decrease in line-width as compared to the corresponding protonated analogues. The improved resolution of composite spectra consisting of freely tumbling and immobilized components is demonstrated in ternary complexes of the spin-labeled NAD+ derivatives with lactate dehydrogenase (L-lactate:NAD+ oxidoreductase, EC 1.1.1.27) and oxalate.