Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
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(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
Beyond The Earth and How The Solar System EvolvedLJAshleyDigamon
This is our PowerPoint Presentation for our report in Science Subject and I want it to share with you. This would be useful for your studies! Hope I can help! Thank you and God Bless!
The curiosity to find earth-like planet can be dated to long time ago. But because of the incapability of the available technologies, it was a dream to detect planets beyond our solar system. After the time stated, the space research have taken a new leap and opened a new era of information. The concept of Exoplanet born. It can also be referred to as Extra Solar Planet. Any planet which is not within our solar system is Exoplanet. But an absolute definition is quite complex and problematic. So some of the important characteristics of an Exoplanet is it has to be earth-like environment, it can be giant or terrestrial type
Chiotelis Ioannis, Theodoropoulou Maria, “Searching for Black Holes. Photometry in our Classrooms”, Hellenic Conference on Innovating STEM Education, 16-18 December 2016, Athens, Greece.
Um belo ebook para você aprender tudo sobre os asteroides, aprender sobre possíveis ameaças de colisão com a Terra e como estão os planos de desviar um asteroide que possa colidir com o planeta.
Hi !
I have made this presentation for you so that you know what is space and what is space technology.The one who will download it will be the one who has got 95% knowledge of space and
FOR MORE KNOWLEDGE JUST EMAIL ME ON THIS EMAIL ADDRESS
workplaceid154@gmail.com
Thanks for your downloading
(please spread this presentation to all schools and all institute so that the students or people can get to know about space)
NOTE:THIS IS MICROSOFT 2013 PRESENTATION)
I WILL UPLOAD LOWER VERSIONS OF THIS FILE
THANKS (MADE BY IRTAZA ZAFAR AND
HASEEB AHMED FROM THE CITY SCHOOL CHENAB CAMPUS FSD
Beyond The Earth and How The Solar System EvolvedLJAshleyDigamon
This is our PowerPoint Presentation for our report in Science Subject and I want it to share with you. This would be useful for your studies! Hope I can help! Thank you and God Bless!
The curiosity to find earth-like planet can be dated to long time ago. But because of the incapability of the available technologies, it was a dream to detect planets beyond our solar system. After the time stated, the space research have taken a new leap and opened a new era of information. The concept of Exoplanet born. It can also be referred to as Extra Solar Planet. Any planet which is not within our solar system is Exoplanet. But an absolute definition is quite complex and problematic. So some of the important characteristics of an Exoplanet is it has to be earth-like environment, it can be giant or terrestrial type
Chiotelis Ioannis, Theodoropoulou Maria, “Searching for Black Holes. Photometry in our Classrooms”, Hellenic Conference on Innovating STEM Education, 16-18 December 2016, Athens, Greece.
Um belo ebook para você aprender tudo sobre os asteroides, aprender sobre possíveis ameaças de colisão com a Terra e como estão os planos de desviar um asteroide que possa colidir com o planeta.
The 12 biggest objects in the universe presented in a 5 inch screen, how crazy is that?. Be amazed of what the universe holds, be ready to blow your minds.
Education Material about Astronomy Presentation Template
If you want to buy this presentation template, please visit http://madlis.com
Good design gets out of the way of the content you are sharing. It helps your audience focus on the content itself instead of the design.
But, it's no secret that most people dislike giving presentations. The dread of public speaking consistently ranks among the greatest fears in public surveys.
This presentation slides can help you reduce the anxiety involved with giving a presentation. Well-designed slides not only build your own confidence, they make your key points clearer to the audience.
Education Material about Astronomy Presentation Template
If you want to buy this presentation template, please visit http://madlis.com
Good design gets out of the way of the content you are sharing. It helps your audience focus on the content itself instead of the design.
But, it's no secret that most people dislike giving presentations. The dread of public speaking consistently ranks among the greatest fears in public surveys.
This presentation slides can help you reduce the anxiety involved with giving a presentation. Well-designed slides not only build your own confidence, they make your key points clearer to the audience.
When earth will die? Scientists agree that the sun will die within 10 billion years, but they weren’t sure – until recently – what would happen to it next.
Space telescopes (2/3) - NASA's Active Orbiting SatellitesSteven Belaire
The second of a 3 part series exploring currently active space telescopes. This installment covers NASA's active orbiting satellites (excluding solar telescopes).
This article seeks to present the future of the Universe, as well as to point out the measures that lead to the survival of humanity in the face of the numerous threats that may occur at the level of the solar system and the Universe as a whole.
Astronomy Impact
Astronomy Essay
Astronomy Essay
Astronomy Essay
Astronomy Essay
Essay about Telescopes in Astronomy
Socrates On Astronomy
Ancient Greek Astronomy Essay
History of Astronomy
Similar to Cosmic monster' star spits energy with the force of a billion suns (20)
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
The increased availability of biomedical data, particularly in the public domain, offers the opportunity to better understand human health and to develop effective therapeutics for a wide range of unmet medical needs. However, data scientists remain stymied by the fact that data remain hard to find and to productively reuse because data and their metadata i) are wholly inaccessible, ii) are in non-standard or incompatible representations, iii) do not conform to community standards, and iv) have unclear or highly restricted terms and conditions that preclude legitimate reuse. These limitations require a rethink on data can be made machine and AI-ready - the key motivation behind the FAIR Guiding Principles. Concurrently, while recent efforts have explored the use of deep learning to fuse disparate data into predictive models for a wide range of biomedical applications, these models often fail even when the correct answer is already known, and fail to explain individual predictions in terms that data scientists can appreciate. These limitations suggest that new methods to produce practical artificial intelligence are still needed.
In this talk, I will discuss our work in (1) building an integrative knowledge infrastructure to prepare FAIR and "AI-ready" data and services along with (2) neurosymbolic AI methods to improve the quality of predictions and to generate plausible explanations. Attention is given to standards, platforms, and methods to wrangle knowledge into simple, but effective semantic and latent representations, and to make these available into standards-compliant and discoverable interfaces that can be used in model building, validation, and explanation. Our work, and those of others in the field, creates a baseline for building trustworthy and easy to deploy AI models in biomedicine.
Bio
Dr. Michel Dumontier is the Distinguished Professor of Data Science at Maastricht University, founder and executive director of the Institute of Data Science, and co-founder of the FAIR (Findable, Accessible, Interoperable and Reusable) data principles. His research explores socio-technological approaches for responsible discovery science, which includes collaborative multi-modal knowledge graphs, privacy-preserving distributed data mining, and AI methods for drug discovery and personalized medicine. His work is supported through the Dutch National Research Agenda, the Netherlands Organisation for Scientific Research, Horizon Europe, the European Open Science Cloud, the US National Institutes of Health, and a Marie-Curie Innovative Training Network. He is the editor-in-chief for the journal Data Science and is internationally recognized for his contributions in bioinformatics, biomedical informatics, and semantic technologies including ontologies and linked data.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
The ASGCT Annual Meeting was packed with exciting progress in the field advan...
Cosmic monster' star spits energy with the force of a billion suns
1. 'Cosmic monster' star spits energy with
the force of a billion suns
High energy outbursts in this type of neutron star — a magnetar — are
thought to be caused by "starquakes."
A powerful X-ray burst erupts from a magnetar — a supermagnetized version of
a stellar remnant known as a neutron star — in this illustration. (Image credit:
NASA Goddard Space Flight Center/Chris Smith (USRA))
A dense, magnetic star violently erupted and spat out as much energy as a billion
suns — and it happened in a fraction of a second, scientists recently reported.
This type of star, known as a magnetar, is a neutron star with an exceptionally
strong magnetic field, and magnetars often flare spectacularly and without
warning. But even though magnetars can be thousands of times brighter than our
sun, their eruptions are so brief and unpredictable that they're challenging for
astrophysicists to find and study.
However, researchers recently managed to catch one of these flares and calculate
oscillations in the brightness of a magnetar as it erupted. The scientists found that
the distant magnetar released as much energy as our sun produces in 100,000
years, and it did so in just 1/10 of a second, according to a statement translated
from Spanish.
2. A neutron star forms when a massive star collapses at the end of its life. As the
star dies in a supernova, protons and electrons in its core are crushed into a
compressed solar mass that combines intense gravity with high-speed rotation
and powerful magnetic forces, according to NASA. The result, a neutron star, is
approximately 1.3 to 2.5 solar masses — one solar mass is the mass of our sun,
or about 330,000 Earths — crammed into a sphere measuring just 12 miles (20
kilometers) in diameter.
Matter in neutron stars is so densely packed that an amount the size of a sugar
cube would weigh more than 1 billion tons (900 million metric tons), and a
neutron star's gravitational pull is so intense that a passing marshmallow would
hit the star's surface with the force of 1,000 hydrogen bombs, according to
NASA.
Magnetars are neutron stars with magnetic fields that are 1,000 times stronger
than those of other neutron stars, and they are more powerful than any other
magnetic object in the universe. Our sun pales in comparison to these bright,
dense stars even when they aren't erupting, study lead author Alberto J. Castro-
Tirado, a research professor with the Institute for Astrophysics of Andalucía at
the Spanish Research Council, said in the statement.
"Even in an inactive state, magnetars can be 100,000 times more luminous than
our sun," Castro-Tirado said. "But in the case of the flash that we have studied
— GRB2001415 — the energy that was released is equivalent to that which our
sun radiates in 100,000 years."
A "giant flare"
The magnetar that produced the brief eruption is located in the Sculptor Galaxy,
a spiral galaxy about 13 million light-years from Earth, and is "a true cosmic
monster," study co-author Victor Reglero, director of UV's Image Processing
Laboratory, said in the statement. The giant flare was detected on April 15, 2020
by the Atmosphere–Space Interactions Monitor (ASIM) instrument on the
International Space Station, researchers reported Dec. 22 in the journal Nature.
Artificial intelligence (AI) in the ASIM pipeline detected the flare, enabling the
researchers to analyze that brief, violent energy surge; the flare lasted just 0.16
seconds and then the signal decayed so rapidly that it was nearly
indistinguishable from background noise in the data. The study authors spent
more than a year analyzing ASIM's two seconds of data collection, dividing the
event into four phases based on the magnetar's energy output, and then
3. measuring variations in the star's magnetic field caused by the energy pulse
when it was at its peak.
It's almost as if the magnetar decided to broadcast its existence "from its cosmic
solitude" by shouting into the void of space with the force "of a billion suns,"
Reglero said.
Only about 30 magnetars have been identified from approximately 3,000 known
neutron stars, and this is the most distant magnetar flare detected to date.
Scientists suspect that eruptions such as this one may be caused by so-called
starquakes that disrupt magnetars' elastic outer layers, and this rare observation
could help researchers unravel the stresses that produce magnetars' energy
burps, according to the study.
Our Milky Way Galaxy
(Image credit: ESA/NASA/JPL-Caltech)
How much do you know about the city you live in? Sure, you've got your favorite
restaurants and the best way to avoid traffic during rush hour, but it's unlikely
you know the details of every urban nook and cranny. The same goes for the
galaxy you live in, the Milky Way.
Our celestial home is an awe-inspiring place full of stars, supernovas, nebulas,
energy and dark matter, but many aspects of it remain mysterious, even to
scientists. For those seeking to better know their own place in the universe, here
are 11 enlightening facts about the Milky Way.
4. We're not sure exactly how many stars are in the Milky Way
(Image credit: Two Micron All-Sky Survey)
Counting stars is a tedious business. Even astronomers argue over the best way
to do it. Their telescopes see only the brightest stars in our galaxy, and many are
hidden by obscuring gas and dust. One technique to estimate the stellar
population of the Milky Way is to look at how fast stars are orbiting within it,
which gives an indication of the gravitational tug, and therefore the mass, of the
galaxy. Divide the galactic mass by the average size of a star and you should have
your answer. But as David Kornreich, an astronomer at Ithaca College in New
York, told Live Science's sister site Space.com, these numbers are all
approximations. Stars vary widely in size, and many assumptions go into
estimating the number of stars residing in the Milky Way. The European Space
Agency's Gaia satellite has mapped the location of 1 billion stars in our galaxy,
and its scientists believe this represents 1 percent of the total, so perhaps the
Milky Way contains about 100 billion stars. [Large Numbers That Define the
Universe].
5. Nobody knows how much the Milky Way weighs
On a related note, astronomers are still unsure exactly how much our galaxy
weighs, with estimates
ranging from 700 billion to
2 trillion times the mass of
our sun. Getting a better
grasp is no easy task. Most
of the Milky Way's mass —
perhaps 85 percent — is in
the form of dark matter,
which gives off no light and
so is impossible to directly
observe, according to
astronomer Ekta Patel of the University of Arizona in Tucson. Her recent study
looked at how strongly our galaxy's humongous mass gravitationally tugs on
smaller galaxies orbiting it and updated the estimate of the Milky Way's mass to
960 billion times the mass of the sun, Live Science previously reported.
The Milky Way is probably in a big, empty spot in the universe
Several studies have
indicated that the Milky Way
and its neighbors are living
out in the boonies of the
cosmos. From afar, the large-
scale structure of the
universe looks like a colossal
cosmic web, with string-like
filaments connecting dense regions separated by enormous, mostly empty
voids. The emphasis in that last sentence should be on "mostly empty," since
our own galactic abode seems to be an inhabitant of the Keenan, Barger and
Cowie (KBC) Void, named after three astronomers who identified it in a 2013
study in The Astrophysical Journal. Last year, a separate team looked at the
motion of galaxies in the cosmic web to provide additional confirmation
that we're floating in one of the big, empty areas, Live Science previously
reported.
6. Astronomers are trying to photograph the monster black hole at the
Milky Way's center
(Image credit: NASA/CXC/Columbia Univ. /C. Hailey et al.)
Lurking in the heart of our galaxy is a hungry behemoth, a gigantic black hole
with the weight of 4 million suns. Scientists know that it's there because they
can trace the paths of stars in the Milky Way's center and see that they seem to
orbit a supermassive object that can't be seen. But in recent years, astronomers
have been combining observations from multiple radio telescopes to try and get
a glimpse of the environment surrounding the black hole, which is packed with
gas and dust spinning around the black hole's maw. The project, called the Event
Horizon Telescope, expects to have preliminary images of the black hole's edge
in the coming months, according to the team's blog. [Stephen Hawking's Most
Far-Out Ideas About Black Holes]
7. Small galaxies orbit the Milky Way and sometimes crash into it
(Image credit: Juan Carlos Muñoz/ESO)
When Portuguese explorer Ferdinand Magellan sailed through the Southern
Hemisphere in the 16th century, he and his crew were among the first
Europeans to report on circular clusters of stars in the night sky, according to
the European Southern Observatory. These clusters are actually small galaxies
that orbit our Milky Way like planets around a star, and they have been named
the Small and Large Magellanic clouds. Many such dwarf galaxies orbit ours —
and sometimes they get eaten by our massive Milky Way. Earlier this year,
astronomers used new data from the Gaia satellite that showed millions of stars
in our galaxy moving in similar narrow, "needle-like" orbits, suggesting they all
originated from an earlier dwarf galaxy dubbed "the Gaia Sausage," as Live
Science reported at the time.