Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation.

Two >130-meter-diameter impact craters formed on Mars during the later half of 2021. These are the two largest fresh impact craters discovered by the Mars Reconnaissance Orbiter since operations started 16 years ago. The impacts created two of the largest seismic events (magnitudes greater than 4) recorded by InSight during its 3-year mission. The combination of orbital imagery and seismic ground motion enables the investigation of subsurface and atmospheric energy partitioning of the impact process on a planet with a thin atmosphere and the first direct test of martian deep-interior seismic models with known event distances. The impact at 35°N excavated blocks of water ice, which is the lowest latitude at which ice has been directly observed on Mars.

Surface waves and crustal structure on Mars.

We detected surface waves from two meteorite impacts on Mars. By measuring group velocity dispersion along the impact-lander path, we obtained a direct constraint on crustal structure away from the InSight lander. The crust north of the equatorial dichotomy had a shear wave velocity of approximately 3.2 kilometers per second in the 5- to 30-kilometer depth range, with little depth variation. This implies a higher crustal density than inferred beneath the lander, suggesting either compositional differences or reduced porosity in the volcanic areas traversed by the surface waves. The lower velocities and the crustal layering observed beneath the landing site down to a 10-kilometer depth are not a global feature. Structural variations revealed by surface waves hold implications for models of the formation and thickness of the martian crust.

Suppression of the osmoinduced proline response of rapeseed leaf discs by polyamines.

Rapeseed leaf discs (RLD) subjected to upshock osmotic stress accumulate proline (Pro). Di- and polyamines (PA) supplied to the external medium suppressed Pro accumulation. These effects were dependent not only on diamine and PA concentrations but also on their cationic charge. The suppression of Pro accumulation required that diamine and PA be taken up and further accumulated in the leaf tissues. Glycine betaine (GB) also inhibited Pro accumulation, with the effects of GB and PA being additive. Experiments to elucidate the mechanism(s) responsible for the inhibitory effect of spermine (Spm) indicated that it could be simulated with methionine sulfoximine (MSO), a potent inhibitor of glutamine synthetase. The inhibitory effects of Spm and MSO were both alleviated by supplying glutamine to the RLD. In addition, Spm as well as MSO increased glutamate content, indicating that these compounds could inhibit the conversion of glutamate to proline. A comparison of the changes in chlorophyll and protein content of RLD osmotreated with or without added Spm indicates that this PA behaves as an antisenescent compound, preventing chlorophyll breakdown and proteolysis and hence the conversion of amino acids to Pro. Since the PA concentrations used in this work were much higher than the endogenous concentrations in RLD, the significance of PA under osmotic stress remains unclear. This study shows, however, that PA can suppress Pro accumulation.