Properties of periodic table by Saliha RaisSaliha Rais
The presentation "Properties of Periodic Table" is prepared for grade IX students. The slide show includes a brief description on the properties of elements in the periodic table, that shifts periodically, hence explaining the concept of periodicity. the main topics include Atomic Radii, Ionization energy, Electron affinity and Electronegativity.
Properties of periodic table by Saliha RaisSaliha Rais
The presentation "Properties of Periodic Table" is prepared for grade IX students. The slide show includes a brief description on the properties of elements in the periodic table, that shifts periodically, hence explaining the concept of periodicity. the main topics include Atomic Radii, Ionization energy, Electron affinity and Electronegativity.
This is a revised PowerPoint on five families of the periodic table I put together for my HS chemistry 9 class after taking a course on visual literacy, inclusive of effective PowerPoint presentations. It could still be much better but I hope some improvement between the two PowerPoints is evident.
Specifically designed for Leaving Cert Chemistry students. A simplified explanation of all the trends in the periodic Table. It includes details such as atomic radius, electronegativity and ionisation energy
This is a revised PowerPoint on five families of the periodic table I put together for my HS chemistry 9 class after taking a course on visual literacy, inclusive of effective PowerPoint presentations. It could still be much better but I hope some improvement between the two PowerPoints is evident.
Specifically designed for Leaving Cert Chemistry students. A simplified explanation of all the trends in the periodic Table. It includes details such as atomic radius, electronegativity and ionisation energy
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.
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.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
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.
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.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
17. The History of the Modern Periodic
Glenn T. Seaborg
1912 - 1999
Table
He is the only person to have an element
named after him while still alive.
"This is the greatest honor ever
bestowed upon me - even better, I think,
than
winning the Nobel Prize."
18. Key in the Periodic Table
Elements are organized on the table
according to their atomic number, usually
found near the top of the square.
-The atomic number refers to how
many protons an atom of that element
has.
-For instance, hydrogen has 1 proton,
so it’s atomic number is 1.
-The atomic number is unique to that
element. No two elements have the
same atomic number.
19.
20. Key in the Periodic Table
Atomic Number
This refers to how many protons an atom
of that element has.
No two elements, have the same number
of protons.
Wave Model
21. Key in the Periodic Table
Atomic Mass
Atomic Mass refers to the “weight” of the
atom.
It is derived at by adding the number of protons
with the number of neutrons.
This is a helium atom. Its atomic mass is 4
(protons plus neutrons).
What is its atomic number?
22. Key in the Periodic Table
Atomic Mass and Isotopes
While most atoms have the
same number of protons and
neutrons, some don’t.
Some atoms have more or less
neutrons than protons. These
are called isotopes.
An atomic mass number with a
decimal is the total of the
number of protons plus the
average number of neutrons.
23. Key in the Periodic Table
Atomic Mass Unit (AMU)
The unit of measurement for an atom
is an AMU. It stands for atomic mass
unit.
One AMU is equal to the mass of one
proton.
24. Key in the Periodic Table
Atomic Mass Unit (AMU)
There are
6 X 1023 or
600,000,000,000,000,000,000,000
amus in one gram.
(Remember that electrons are 2000
times smaller than one amu).
25. Key in the Periodic Table
Symbols
All elements
have their own
unique symbol.
It can consist
of a single
capital letter,
or a capital
letter and one
or two lower
case letters.
26.
27. Key in the Periodic Table
Valence Electrons
The number of valence electrons an
atom has may also appear in a square.
Valence electrons are the electrons in
the outer energy level of an atom.
These are the electrons that are
transferred or shared when atoms
bond together.
28. Key in the Periodic Table
Where to elements come from?
The ‘Big Bang’ theory suggests that all the
fundamental particles in the universe were
formed over a very short time (a few seconds or
less) in a huge explosion that occurred some 15
billion years ago.
Explain the fourth state of matter – plasma.
How is He formed?
What is the difference between nuclear fission
and nuclear fusion?
29. Key in the Periodic Table
Where to elements come from?
Once a star has converted a large fraction of
its core mass to iron, it has almost reeached
the end of its life
The core of the star then begins to cool,
causing a violent gravitational collapse, or
implosion.
Eventually the star explodes, spreading its
products throughout the universe.
An exploding star is called a supernova
A supernova can produce heavier elements
up to the size of the iron nucleus by nuclear
fusion reactions. Larger stars can produce
heavier atoms
32. Periodic Table Geography
The elements in any group of the
periodic table have similar physical and
chemical properties.
The vertical columns of the periodic
table are called GROUPS, or FAMILIES.
33. Periodic Table Geography
Periodic Law
When elements are arranged in order of
increasing atomic number, there is a
periodic pattern in their physical and
chemical properties.
40. Groups and Block
Based upon the electron configuration of the
elements the table can be divided into four
blocks. These blocks represent the different
sublevels of electron configuration.
Group A elements are called
representative elements
Group B elements are called transition
elements.
41. Groups and Block
The s and p block elements
are called
REPRESENTATIVE ELEMENTS.
The d block elements
are called
TRANSITION ELEMENTS
42. Groups and Block
The s-block elements:
Groups 1-2
Electron configuration: ns1,2 (valence
electrons in the s subshell)
Contains the alkali metals (Group 1), and
alkaline-earth metals (Group 2)
Very reactive metals; Group 1 is more
reactive than Group 2, but both do not
exist in nature as free elements because
they are too reactive.
He has a filled s subshell of the innermost
K shell of the atom rendering it
unreactive.
43. Groups and Block
The d-block elements:
Groups 3-12
Electron configuration: (n-1)d1-10ns0-2
(valence electrons in the p subshell)
transition elements: typical metallic
properties
Good Conductors of electricity and have a
high luster; less reactive than the s-block
elements; many exist in nature as free
elements.
44. The f-block elements:
Groups and Block
Lanthanides and Actinides
Between Groups 3 and 4.
Between Periods 6 and 7.
14 in each; highly similar properties;
resemble Group 2 elements.
f subshells progressivley filled
47. Properties of Metals
Metals are good conductors of heat
and electricity.
Metals are shiny.
Metals are ductile (can be stretched
into thin wires).
Metals are malleable (can be
pounded into thin sheets).
A chemical property of metal is its
reaction with water which results in
corrosion.
48. Properties of Non-Metals
Non-metals are poor
conductors of heat and
electricity.
Non-metals are not
ductile or malleable.
Solid non-metals are
brittle and break easily.
They are dull.
Many non-metals are
gases.
Sulfur
49. Properties of Metalloids
Silicon (Si)
Metalloids (metal-like)
have properties of both
metals and non-metals.
They are solids that can
be shiny or dull.
They conduct heat and
electricity better than
non-metals but not as
well as metals.
They are ductile and
malleable.
63. HYDROGEN
The hydrogen square sits atop Family AI, but it
is not a member of that family. Hydrogen is in a
class of its own.
It’s a gas at room temperature.
It has one proton and one electron in its one
and only energy level.
Hydrogen only needs 2 electrons to fill up its
valence shell.
64. Alkali Metals
The alkali family is found in
the first column of the periodic
table.
Atoms of the alkali metals
have a single electron in their
outermost level, in other
words, 1 valence electron.
They are shiny, have the
consistency of clay, and are
easily cut with a knife.
65. Alkali Metals
They are the most reactive
metals.
They react violently with
water.
Alkali metals are never found
as free elements in nature.
They are always bonded with
another element.
66. Alkaline Earth Metals
They are never found
uncombined in nature.
They have two valence
electrons.
Alkaline earth metals include
magnesium and calcium,
among others.
67. Transition Metals
Transition Elements
include those elements in
the B families.
These are the metals you
are probably most
familiar: copper, tin,
zinc, iron, nickel, gold,
and silver.
They are good
conductors of heat and
electricity.
68. Transition Metals
The compounds of transition metals are usually
brightly colored and are often used to color
paints.
Transition elements have 1 or 2 valence
electrons, which they lose when they form
bonds with other atoms. Some transition
elements can lose electrons in their next-to-outermost
level.
69. Transition Elements
Transition elements have properties similar to
one another and to other metals, but their
properties do not fit in with those of any other
family.
Many transition metals combine chemically
with oxygen to form compounds called oxides.
70. Boron Family
The Boron Family is named after the first
element in the family.
Atoms in this family have 3 valence electrons.
This family includes a metalloid (boron), and
the rest are metals.
This family includes the most abundant metal
in the earth’s crust (aluminum).
71. Nitrogen Family
The nitrogen family is named
after the element that makes up
78% of our atmosphere.
This family includes non-metals,
metalloids, and metals.
Atoms in the nitrogen family
have 5 valence electrons. They
tend to share electrons when
they bond.
Other elements in this family are
phosphorus, arsenic, antimony,
and bismuth.
72. Oxygen Family
Atoms of this family have
6 valence electrons.
Most elements in this
family share electrons
when forming compounds.
Oxygen is the most
abundant element in the
earth’s crust. It is
extremely active and
combines with almost all
elements.
73. Halogen Family
The elements in this family are fluorine,
chlorine, bromine, iodine, and astatine.
Halogens have 7 valence electrons, which
explains why they are the most active non-metals.
They are never found free in nature.
Halogen atoms only need to gain 1 electron to
fill their outermost energy level.
They react with alkali metals to form salts.
74. Noble Gas
Noble Gases are colorless gases that
are extremely un-reactive.
One important property of the noble
gases is their inactivity. They are
inactive because their outermost
energy level is full.
Because they do not readily combine
with other elements to form
compounds, the noble gases are called
inert.
The family of noble gases includes
helium, neon, argon, krypton, xenon,
and radon.
All the noble gases are found in small
amounts in the earth's atmosphere.
75. The thirty rare earth elements
are composed of the lanthanide
and actinide series.
One element of the lanthanide
series and most of the elements
in the actinide series are called
trans-uranium, which means
synthetic or man-made.