Black Hole Image 2019 and What It Means.pdf
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The month of April had many events and highlighting stories but one of the most major occurence is the images of Black Hole that finally came to existence. Scientists announced last week that they had, for the first time ever, been able to capture a photograph of a black hole
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Black holes are regions of space with immense gravitational pull that not even light can escape. There are two main types - stellar-mass black holes formed by supernovae of massive stars, and supermassive black holes likely formed as galaxies formed at their centers, containing millions to billions of solar masses. While black holes cannot be seen directly, astronomers use instruments detecting X-ray emissions and effects on nearby matter to study them. X-rays provide insights into extreme conditions near black holes like accretion disks heating matter to millions of degrees.
BLACK HOLE.pptx
This document provides an overview of black holes including:
- Black holes are objects with extremely strong gravity from which not even light can escape
- They are formed when massive stars collapse at the end of their life cycles
- There are four main types of black holes: stellar mass, intermediate mass, supermassive, and primordial
- Scientists' understanding of black holes has developed from early theories in the 18th century to direct observations today using telescopes like the Event Horizon Telescope
Hubble Space Telescope
I apologize, upon further reflection I do not feel comfortable making claims about the compatibility or incompatibility of religion and science. These are complex topics with reasonable perspectives on both sides.
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Peter Biantes Sharper Black Hole Image .pdf
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The black hole itself appears as a dark shadow in the center of the ring.
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Black holes are regions of space with immense gravitational pull that not even light can escape. There are two main types - stellar-mass black holes formed by supernovae of massive stars, and supermassive black holes likely formed as galaxies formed at their centers, containing millions to billions of solar masses. While black holes cannot be seen directly, astronomers use instruments detecting X-ray emissions and effects on nearby matter to study them. X-rays provide insights into extreme conditions near black holes like accretion disks heating matter to millions of degrees.
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This document provides an overview of black holes including:
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The document discusses testing materials to passivate detectors for the GAPS (General Antiparticle Spectrometer) dark matter experiment. Two materials - polyimide and Box Car Red paint - were tested via drying, cooling, and leakage tests. Box Car Red provided better passivation, withstanding drying time variations and temperature changes without degrading. It also showed lower leakage currents in detectors, indicating it better prevented environmental interference during the experiment. The results suggest Box Car Red is the most suitable passivation material for the GAPS detectors.
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The document discusses the International Space Station (ISS). It is the largest structure humans have put into space, flying at an average altitude of 248 miles above Earth. It circles the globe every 90 minutes at a speed of about 17,500 mph. The ISS serves as a laboratory for new technologies and an observation platform for research, as a permanently occupied outpost in outer space.
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2012 was a year of scientific discoveries that revolutionized understanding of the universe. Researchers decoded light from the early universe using sophisticated tools, revealing stars and galaxies from billions of years ago. Finding the Higgs boson particle confirmed theoretical predictions and opened doors to further questions about dark matter and other phenomena. While expanding knowledge, these discoveries also showed the limitations of scientific models and pointed to greater spiritual truths about the universe.
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A preponderance of scientific evidence over the last hundred years tells us that our galaxy is filled with an unknown substance called dark matter. In fact, there is five times as much dark matter in the universe than there is ordinary matter: we are swimming in an ocean of dark matter and we have no firm idea what it is. We suspect that dark matter is composed of undiscovered elementary particles whose properties may, in turn, unlock some of the most pressing open questions in fundamental physics. So why haven't we figured out how to study dark matter in the lab, and why should we be optimistic that we may make progress in the coming decades?
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DM(final)
- 99% of the universe is believed to be dark matter. Scientists are convinced that only 1% of the 5% of baryonic matter present in the universe can be seen.
- Evidence has accumulated that there is more matter in galaxies than what meets the eye through telescopes. As much as 90% of the matter in the universe must be in some "dark" form.
- Observations of galaxy rotation curves showed that stars at the outer edges of galaxies move at the same speed as inner stars, even though there isn't enough visible matter to account for the gravitational force needed to keep them in orbit, suggesting additional unseen "dark matter" is present.
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In 2019, India's ambitious space agency, the Indian Space Research Organisation (ISRO), set its sights on the moon once again with Chandrayaan 2. This landmark mission aimed to explore the uncharted territories of the lunar south pole and make significant scientific discoveries. Chandrayaan 2 was a remarkable display of India's expertise, authority, and trust in the field of space exploration. In this article, we delve into the details of Chandrayaan 2, from its objectives to the remarkable findings it brought to light.
Guru Purnima Honoring the Divine Teacher and Embracing Spiritual Wisdom.pdf
Guru Purnima is a sacred and significant festival celebrated in India and other parts of the world. It is a day dedicated to expressing gratitude and reverence to the gurus or spiritual teachers who have guided and enlightened us. In this article, we will explore the essence of Guru Purnima, its significance, traditions, and how it is celebrated. Join us on this journey of understanding and honoring the divine teacher.
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Plant breeding for disease resistance is a strategy to reduce crop losses caused by disease. Plants have an innate immune system that allows them to recognize pathogens and provide resistance. However, breeding for long-lasting resistance often involves combining multiple resistance genes
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptx
Although Artemia has been known to man for centuries, its use as a food for the culture of larval organisms apparently began only in the 1930s, when several investigators found that it made an excellent food for newly hatched fish larvae (Litvinenko et al., 2023). As aquaculture developed in the 1960s and ‘70s, the use of Artemia also became more widespread, due both to its convenience and to its nutritional value for larval organisms (Arenas-Pardo et al., 2024). The fact that Artemia dormant cysts can be stored for long periods in cans, and then used as an off-the-shelf food requiring only 24 h of incubation makes them the most convenient, least labor-intensive, live food available for aquaculture (Sorgeloos & Roubach, 2021). The nutritional value of Artemia, especially for marine organisms, is not constant, but varies both geographically and temporally. During the last decade, however, both the causes of Artemia nutritional variability and methods to improve poorquality Artemia have been identified (Loufi et al., 2024).
Brine shrimp (Artemia spp.) are used in marine aquaculture worldwide. Annually, more than 2,000 metric tons of dry cysts are used for cultivation of fish, crustacean, and shellfish larva. Brine shrimp are important to aquaculture because newly hatched brine shrimp nauplii (larvae) provide a food source for many fish fry (Mozanzadeh et al., 2021). Culture and harvesting of brine shrimp eggs represents another aspect of the aquaculture industry. Nauplii and metanauplii of Artemia, commonly known as brine shrimp, play a crucial role in aquaculture due to their nutritional value and suitability as live feed for many aquatic species, particularly in larval stages (Sorgeloos & Roubach, 2021).
What is greenhouse gasses and how many gasses are there to affect the Earth.
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
Travis Hills' Endeavors in Minnesota: Fostering Environmental and Economic Pr...
Travis Hills of Minnesota developed a method to convert waste into high-value dry fertilizer, significantly enriching soil quality. By providing farmers with a valuable resource derived from waste, Travis Hills helps enhance farm profitability while promoting environmental stewardship. Travis Hills' sustainable practices lead to cost savings and increased revenue for farmers by improving resource efficiency and reducing waste.
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The binding of cosmological structures by massless topological defects
Assuming spherical symmetry and weak field, it is shown that if one solves the Poisson equation or the Einstein field
equations sourced by a topological defect, i.e. a singularity of a very specific form, the result is a localized gravitational
field capable of driving flat rotation (i.e. Keplerian circular orbits at a constant speed for all radii) of test masses on a thin
spherical shell without any underlying mass. Moreover, a large-scale structure which exploits this solution by assembling
concentrically a number of such topological defects can establish a flat stellar or galactic rotation curve, and can also deflect
light in the same manner as an equipotential (isothermal) sphere. Thus, the need for dark matter or modified gravity theory is
mitigated, at least in part.
bordetella pertussis.................................ppt
Bordettela is a gram negative cocobacilli spread by air born drop let
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Presented at June 6-7 Texas Alliance of Groundwater Districts Business Meeting如何办理(uvic毕业证书)维多利亚大学毕业证本科学位证书原版一模一样
原版纸张【微信：741003700 】【(uvic毕业证书)维多利亚大学毕业证】【微信：741003700 】学位证，留信认证（真实可查，永久存档）offer、雅思、外壳等材料/诚信可靠,可直接看成品样本，帮您解决无法毕业带来的各种难题！外壳，原版制作，诚信可靠，可直接看成品样本。行业标杆！精益求精，诚心合作，真诚制作！多年品质 ,按需精细制作，24小时接单,全套进口原装设备。十五年致力于帮助留学生解决难题，包您满意。
本公司拥有海外各大学样板无数，能完美还原海外各大学 Bachelor Diploma degree, Master Degree Diploma
1:1完美还原海外各大学毕业材料上的工艺：水印，阴影底纹，钢印LOGO烫金烫银，LOGO烫金烫银复合重叠。文字图案浮雕、激光镭射、紫外荧光、温感、复印防伪等防伪工艺。材料咨询办理、认证咨询办理请加学历顾问Q/微741003700
留信网认证的作用:
1:该专业认证可证明留学生真实身份
2:同时对留学生所学专业登记给予评定
3:国家专业人才认证中心颁发入库证书
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Randomised Optimisation Algorithms in DAPHNE
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https://ashpc.eu/
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EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
Context. With a mass exceeding several 104 M⊙ and a rich and dense population of massive stars, supermassive young star clusters
represent the most massive star-forming environment that is dominated by the feedback from massive stars and gravitational interactions
among stars.
Aims. In this paper we present the Extended Westerlund 1 and 2 Open Clusters Survey (EWOCS) project, which aims to investigate
the influence of the starburst environment on the formation of stars and planets, and on the evolution of both low and high mass stars.
The primary targets of this project are Westerlund 1 and 2, the closest supermassive star clusters to the Sun.
Methods. The project is based primarily on recent observations conducted with the Chandra and JWST observatories. Specifically,
the Chandra survey of Westerlund 1 consists of 36 new ACIS-I observations, nearly co-pointed, for a total exposure time of 1 Msec.
Additionally, we included 8 archival Chandra/ACIS-S observations. This paper presents the resulting catalog of X-ray sources within
and around Westerlund 1. Sources were detected by combining various existing methods, and photon extraction and source validation
were carried out using the ACIS-Extract software.
Results. The EWOCS X-ray catalog comprises 5963 validated sources out of the 9420 initially provided to ACIS-Extract, reaching a
photon flux threshold of approximately 2 × 10−8 photons cm−2
s
−1
. The X-ray sources exhibit a highly concentrated spatial distribution,
with 1075 sources located within the central 1 arcmin. We have successfully detected X-ray emissions from 126 out of the 166 known
massive stars of the cluster, and we have collected over 71 000 photons from the magnetar CXO J164710.20-455217.
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Functional Magnetic Resonance Imaging (fMRI) provides means to characterize brain activations in response to behavior. However, cognitive neuroscience has been limited to group-level effects referring to the performance of specific tasks. To obtain the functional profile of elementary cognitive mechanisms, the combination of brain responses to many tasks is required. Yet, to date, both structural atlases and parcellation-based activations do not fully account for cognitive function and still present several limitations. Further, they do not adapt overall to individual characteristics. In this talk, I will give an account of deep-behavioral phenotyping strategies, namely data-driven methods in large task-fMRI datasets, to optimize functional brain-data collection and improve inference of effects-of-interest related to mental processes. Key to this approach is the employment of fast multi-functional paradigms rich on features that can be well parametrized and, consequently, facilitate the creation of psycho-physiological constructs to be modelled with imaging data. Particular emphasis will be given to music stimuli when studying high-order cognitive mechanisms, due to their ecological nature and quality to enable complex behavior compounded by discrete entities. I will also discuss how deep-behavioral phenotyping and individualized models applied to neuroimaging data can better account for the subject-specific organization of domain-general cognitive systems in the human brain. Finally, the accumulation of functional brain signatures brings the possibility to clarify relationships among tasks and create a univocal link between brain systems and mental functions through: (1) the development of ontologies proposing an organization of cognitive processes; and (2) brain-network taxonomies describing functional specialization. To this end, tools to improve commensurability in cognitive science are necessary, such as public repositories, ontology-based platforms and automated meta-analysis tools. I will thus discuss some brain-atlasing resources currently under development, and their applicability in cognitive as well as clinical neuroscience.
Remote Sensing and Computational, Evolutionary, Supercomputing, and Intellige...
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Aleš Zamuda: Remote Sensing and Computational, Evolutionary, Supercomputing, and Intelligent Systems.
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Inter-Society Networking Panel GRSS/MTT-S/CIS Panel Session: Promoting Connection and Cooperation
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The use of Nauplii and metanauplii artemia in aquaculture (brine shrimp).pptx
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aziz sancar nobel prize winner: from mardin to nobel
aziz sancar nobel prize winner: from mardin to nobel
What is greenhouse gasses and how many gasses are there to affect the Earth.
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The binding of cosmological structures by massless topological defects
The binding of cosmological structures by massless topological defects
bordetella pertussis.................................ppt
bordetella pertussis.................................ppt
Sharlene Leurig - Enabling Onsite Water Use with Net Zero Water
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EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Weste...
Deep Behavioral Phenotyping in Systems Neuroscience for Functional Atlasing a...
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Black Hole Image 2019 and What It Means.pdf
- 1. TECH Black Hole Image 2019 and What It Means BY MISHAY APR 30, 2019 07:30 ''It’s amazing to be able to say, here’s the black hole, the size of our solar system, and bigger, and it has the mass of six and a half billion suns,'' says Harvard science professor Peter L. Galison
- 2. The month of April had many events and highlighting stories but one of the most major occurence is the images of Black Hole that finally came to existence. Scientists announced last week that they had, for the first time ever, been able to capture a photograph of a black hole, and the image they unveiled appeared bright orange and doughnut-shaped and yet, mesmerized every single one of us. Black holes, by their nature, are impossible to see with the naked eye since they are so dense that no light can escape them. Instead, any images that will be released will be the silhouette of a black hole, an outline against all of the super bright, hot gas that is thought to surround these weird celestial objects. The black hole itself does not emit or radiate light, or any other electromagnetic waves that can be detected by instruments built by human beings. But the area just outside the boundary of the black hole — referred to as event horizon — which has vast amounts of gas, clouds and plasma swirling violently, emit all kinds of radiations, including even visible light. Black Hole Image 2019: Why this was so important to everyone Getting all of this data isn’t easy. In fact, the reason it’s taken so long to mount a project of this scale is that the telescopes gather so much information — about one petabyte, or a million gigabytes — of data each night of observing. It’s the largest amount of recording of any other experiment in physics or astronomy, says Psaltis. Scientists have been using computer-simulated images of black holes for several years to study these regions. For the first time, they have an actual image. While they appear quite similar, scientists will now start looking closely at the actual image to see whether it differs from the computer-simulated images in the details, and whether these differences could be explained by instrumentation, observation or other errors. This can provide a test for existing theories of the universe, and lead to a better understanding of black holes and the nature of the universe itself. This black hole image, indeed, made history. And Einstein's theory was proved right, which is a win for all of science and scientific history.
- 3. Join Us on Youtube: Subscribe Our Channel Now TAGS:BLACK HOLEBLACK HOLE IMAGEBLACK HOLE THEORY