Characterization of Hyper-velocity Particle Impact Craters on Apollo 11 Lunar Soil

1970 ◽  
Vol 28 ◽  
pp. 20-21
Author(s):  
John R. Devaney ◽  
Kenneth Evans
Keyword(s):  
Lunar Soil ◽  
Impact Craters ◽  
Particle Impact ◽  
List Type ◽  
The Moon ◽  
Lunar Orbiter ◽  
Lunar Material ◽  
Resolution Limits ◽  
Continuous Range

There exists on the visible surface of the moon, a continuous range of impact craters from the very large to those below the resolution limits of terrestrial telescopes. The RANGER, SURVEYOR and LUNAR ORBITER programs extended the knowledge of existent craters down to those several centimeters in diameter. Prior to the actual examination of lunar material returned by the Apollo 11 mission, a debate was being carried on as to whether craters from hyper-velocity particles existed in the microscopic realm. Soon after the first samples were examined via Scanning Electron Microscopy, the point in question was settled with a definite affirmative.The initial effort in conjunction with Caltech scientist G. J. Wasserberg had as its goal the solution of two problems: (1) Can impact craters be differentiated from bubble bursts?(2) What are the characteristics of impact craters?To pursue the first problem initial efforts were designed to study samples with low possibility of bubbles or voids. This resulted in the examination of a chip of lunar feldspar with a large pit on its exposed surface.

Thematic maps in the scientific studies of the moon

2019 ◽  
Vol 943 (1) ◽  
pp. 68-75
Author(s):  
S.G. Pugacheva ◽  
E.A. Feoktistova ◽  
V.V. Shevchenko
Keyword(s):  
Natural Resources ◽  
Thermal Inertia ◽  
High Growth ◽  
Lunar Soil ◽  
Nature Management ◽  
The Moon ◽  
Surface Cooling ◽  
Laser Altimeters ◽  
Space Infrastructure ◽  
The Impact

The article presents the results of astrophysical studies of the Moon’s reflected and intrinsic radiation. We studied the intensity of the Moon’s infrared radiation and, thus, carried out a detailed research of the brightness temperature of the Moon’s visible disc, estimated the thermal inertia of the coating substance by the rate of its surface cooling, and the degree of the lunar soil fragmentation. Polarimetric, colorimetric and spectrophotometric measurements of the reflected radiation intensity were carried out at different wavelengths. In the article, we present maps prepared based on our measurement results. We conducted theresearch of the unique South Pole – Aitken basin (SPA). The altitude profiles of the Apollo-11 and Zond-8 spacecrafts and the data of laser altimeters of the Apollo-16 and Apollo-15 spacecrafts were used as the main material. Basing upon this data we prepared a hypsometric map of SPA-basing global relief structure. A surface topography map of the Moon’s Southern Hemisphere is given in the article. The topography model of the SPA topography surface shows displacement centers of the altitude topographic rims from the central rim. Basing upon the detailed study of the basin’s topography as well as its “depth-diameter” ratio we suggest that the basin originated from the impact of a giant cometary body from the Orta Cloud. In our works, we consider the Moon as a part of the Earth’s space infrastructure. High growth rates of the Earth’s population, irrational nature management will cause deterioration of scarce natural resources in the near future. In our article, we present maps of the natural resources on the Moon pointing out the most promising regions of thorium, iron, and titanium. Probably in 20 or 40 years a critical mining level of gold, diamonds, zinc, platinum and other vital rocks and metals will be missing on the Earth.

scholarly journals Self-Secondaries Formed by Cold Spot Craters on the Moon

2021 ◽  
Vol 13 (6) ◽  
pp. 1087
Author(s):  
Yiren Chang ◽  
Zhiyong Xiao ◽  
Yang Liu ◽  
Jun Cui
Keyword(s):  
Systematic Investigation ◽  
Impact Craters ◽  
Spatial Density ◽  
Cold Spot ◽  
The Moon ◽  
Potential Threat ◽  
Frequency Distributions ◽  
Crater Size ◽  
The Impact ◽  
Density Pattern

Self-secondaries are a population of background secondaries, and they have been observed on top of impact melt and ballistically emplaced ejecta deposits on various planetary bodies. Self-secondaries are formed by impacts of sub-vertically launched ejecta, but the launch mechanism is not confirmed. The potential threat of self-secondaries to the theoretical and applicable reliability of crater chronology has been noted, but not constrained. Hitherto discovered self-secondaries were located around complex impact craters, but their potential existence around simple craters has not been discovered. Here we report the first discovery of self-secondaries around lunar cold spot craters, which are an extremely young population of simple craters formed within the past ~1 million years on the Moon. Self-secondaries are widespread on layers of cascading flow-like ejecta deposits around cold spot craters. The spatial density of self-secondaries dwarfs that of potential primary craters. The spatial distribution of self-secondaries is highly heterogeneous across the ejecta deposits. With respect to the impactor trajectory that formed cold spot craters, self-secondaries formed at the downrange of the ejecta deposits have the largest spatial density, while those at the uprange have the smallest density. This density pattern holds for all cold spot craters that were formed by non-vertical impacts, but self-secondaries do not exhibit other systematic density variations at different radial distances or at other azimuths with respect to the impactor trajectory. Among known mechanics of ejecting materials to the exterior of impact craters, impact spallation is the most likely scenario to account for the required large ejection velocities and angles to form self-secondaries. The production population of self-secondaries is estimated based on the highly diverse crater size-frequency distributions across the ejecta deposits of cold spot craters. For a better understanding of the impact history on the Moon, a systematic investigation for the effect of self-secondaries on lunar crater chronology is required.

scholarly journals Characterization of bacteriocin and chitinase producing bacterial isolates with broad-spectrum antimicrobial activities

2021 ◽  
Vol 3 (8) ◽  
Author(s):  
Muhammad Yasir ◽  
Basit Zeshan ◽  
Nur Hardy A. Daud ◽  
Izzah Shahid ◽  
Hafza Khalid
Keyword(s):  
Antimicrobial Activity ◽  
Inhibitory Activity ◽  
Antifungal Drugs ◽  
Proteinase K ◽  
Diffusion Method ◽  
List Type ◽  
Bacterial Isolates ◽  
E Coli ◽  
Inhibitory Potential

Abstract There is a need for more efficient and eco-friendly approaches to overcome increasing microbial infections. Bacteriocins and chitinases from Bacillus spp. can be powerful alternatives to conventional antibiotics and antifungal drugs, respectively. The purpose of this study was to assess the inhibitory potential of bacteriocins and chitinase enzymes against multiple resistant bacterial and fungal pathogens. Bacterial isolates were selected by growth on minimal salts medium and after that were morphologically and biochemically characterized. The physiochemical characterization of bacteriocins was carried out. The inhibitory potential of bacteriocins towards six pathogenic bacteria was determined by the well diffusion assay while chitinase activity towards three fungal strains was determined by the dual plate culture assay. Two bacterial strains (WW2P1 and WRE4P2), out of nine showed inhibition of K. pneumonia, P. aeruginosa, E. coli and MRSA while WW4P2 was positive against S. typhimurium and E. coli and WRE10P2 against P. aeruginosa, S. pneumoniae. Two bacterial isolates (WW3P1 and WRE10P2) were chosen for further study on the basis of their antifungal activities. Of these, WW3P1 isolate was more effective against A. fumigatus as well as A. niger. The proteinaceous nature of the bacteriocins was confirmed by treatment of the crude extract with proteinase K. It was found that the inhibitory activity of strain WW3P1 against E. coli was highest at 20 °C, and against S. pneumoniae it was at 20 °C and pH 10 after treatment with EDTA. Inhibition by strain the WRE10P2 against P. aeruginosa was highest at 20 °C and pH 14. It was found that EDTA increased the inhibitory activity of strain WW2P1 against P. aeruginosa, K. pneumoniae and E. coli by 2 ± 0.235, 3.5 ± 0.288, 2.5 ± 1.040 times, respectively, of strain WRE4P2 against P. aeruginosa and E. coli by 2.5 ± 0.763, 2.7 ± 0.5 times, respectively, and of strain WRE10P2 against S. pneumoniae by 3 ± 0.6236 times. The isolates have promising inhibitory activity, which should be further analyzed for the commercial production of antimicrobials. Article highlights The current study aimed to isolate the microbiome from wheat plant (Triticum aestivum L.), to screen for bacteriocin production and to assess its antimicrobial activity against human pathogens. Forty-one phenotypically different bacterial colonies were subjected to bacteriocin purification from which 25 colonies showed positive reactions. These 25 bacterial isolates were screened against six different human bacterial pathogens using the well diffusion method to check the antimicrobial activity. Out of nine bacterial isolates, WW3P1 and WRE10P2 were able to degrade the chitin and utilize it as their sole energy source. Strain WRE4P2 exhibited partial inactivation in its activity against MRSA after treatment with proteinase K.

Abstract 1372: Characterization Of The Rejuvenation Of Cardiac Sympathetic Nerves In Cardiac Hypertrophy

Circulation ◽  
2007 ◽  
Vol 116 (suppl_16) ◽  
Author(s):  
Kensuke Kimura ◽  
Masaki Ieda ◽  
Hideaki Kanazawa ◽  
Takahide Arai ◽  
Takashi Kawakami ◽  
...  
Keyword(s):  
Cardiac Hypertrophy ◽  
Fluorescent Protein ◽  
Sympathetic Neurons ◽  
Weight Ratio ◽  
Sympathetic Nerves ◽  
Marker Genes ◽  
List Type ◽  
Stellate Ganglia ◽  
Immature Neuron

Background : Cardiac hypertrophy induces the fetal isoform of genes (rejuvenation), including contractile proteins, ion channels, and natriuretic peptides. Cardiac sympathetic nerve function is known to be altered in cardiac hypertrophy and congestive heart failure. We recently reported that alteration of cardiac sympathetic nerves (CSN) was caused by their rejuvenation (Circ Res, 2007). The present study was designed to examine the precise characterization of the rejuvenation of CSN in cardiac hypertrophy. Methods and Results : RV hypertrophy was produced by consistent hypoxia (10% O 2 ) in C57/BL6 mice. RV pressure increased to 47 mmHg, and RV/(body weight) ratio increased by 1.6 fold. Nerve growth factor protein was augmented in hypertrophic RV, but was unchanged in LV. Double-transgenic mice, which specifically express eGFP (enhanced green fluorescent protein) in the sympathetic neurons, was generated by crossing dopamine β-hydroxylase (DBH)-Cre mice with Floxed-eGFP mice. The eGFP-positive CSN were markedly increased in hypertrophic RV, but not in LV. Nerve density, quantitated by immunostained area with eGFP and GAP43 (growth-associated corn marker), increased by 8.1 and 9.3 fold, respectively, in RV, but not in LV. (4) Catecholamine content was attenuated in RV. (5) Western blot revealed that tyrosine hydroxylase was markedly down-regulated in RV. (6) Immunostaining clearly demonstrated that the immature neuron markers, PSA-NCAM (highly polysialylated neural cell adhesion molecule) and Ulip-1 (Unc-33-like phosphoprotein 1), were expressed in CSN in hypertrophic RV and stellate ganglia. Basic helix-loop-helix transcription factor, Mash-1 (mammalian achaete-scute complex homolog 1) was strongly expressed in the stellate ganglia. (7) Immature neuron marker-immunopositive cells in stellate ganglia had a markedly decreased TH expression. Conclusion : The rejuvenated CSN showed various immature and fetal neuron marker genes at not only the peripheral axons but also the cellular bodies at the stellate ganglia. Rejuvenation of CSN might be critically involved in the alteration of sympathetic neuronal function in cardiac hypertrophy, including depressed norepinephrine synthesis and hyperinnervation.

scholarly journals 2.2.4 Lunar Soil Movement Registered by the Apollo 17 Cosmic Dust Experiment

1976 ◽  
Vol 31 ◽  
pp. 233-237 ◽  
Author(s):  
Otto E. Berg ◽  
Henry Wolf ◽  
John Rhee
Keyword(s):  
Lunar Surface ◽  
Lunar Soil ◽  
Cosmic Dust ◽  
Dust Particles ◽  
The Moon ◽  
Normal Impact ◽  
Soil Movement ◽  
Impact Parameters

In December, 1973, a Lunar Ejecta and Meteorites (LEAM) experiment was placed in the Taurus-Littrow area of the moon by the Apollo 17 Astronauts. Objectives of the experiment were centered around measurements of impact parameters of cosmic dust on the lunar surface. During preliminary attempts to analyze the data it became evident that the events registered by the sensors could not be attributed to cosmic dust but could only be identified with the lunar surface and the local sun angle. The nature of these data coupled with post-flight studies of instrument characteristics, have led to a conclusion that the LEAM experiment is responding primarily to a flux of highly charged, slowly moving lunar surface fines. Undoubtedly concealed in these data is the normal impact activity from cosmic dust and probably lunar ejecta, as well. This paper is based on the recognition that the bulk of events registered by the LEAM experiment are not signatures of hypervelocity cosmic dust particles, as expected, but are induced signatures of electrostatically charged and transported lunar fines.

Transitional impact craters on the Moon: Insight into the effect of target lithology on the impact cratering process

2018 ◽  
Author(s):  
Gordon R. Osinski ◽  
Elizabeth A. Silber ◽  
Jacqueline Clayton ◽  
Richard A. F. Grieve ◽  
Kayle Hansen ◽  
...  
Keyword(s):  
Impact Craters ◽  
The Moon ◽  
Impact Cratering ◽  
The Impact ◽  
Insight Into
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