This chapter discusses chemical bonds and mixtures. It introduces electron-dot structures to show valence electrons and how they are involved in bonding. Ionic bonds form when ions with opposite charges are attracted to each other. Covalent bonds form when atoms share electrons. Polar covalent bonds result when electrons are shared unevenly. Molecular polarity arises if the polar bonds in a molecule do not cancel out. Most materials are mixtures that can be separated into pure substances. Solutions are homogeneous mixtures where one substance dissolves evenly throughout another. Concentration, molarity, and solubility are measures used to describe solutions.
It's very good for SPM students . You have to learn the ionic bond thoroughly. If you understand well you can explain it vividly. For other chemistry notes can email me puterizamrud@gmail.com or facebook Pusat Tuisyen Zamrud .
Chemical Structure: Chemical Bonding. Ionic, Metallic & Coordinate Bondsulcerd
Lecture materials for the Introductory Chemistry course for Forensic Scientists, University of Lincoln, UK. See http://forensicchemistry.lincoln.ac.uk/ for more details.
It's very good for SPM students . You have to learn the ionic bond thoroughly. If you understand well you can explain it vividly. For other chemistry notes can email me puterizamrud@gmail.com or facebook Pusat Tuisyen Zamrud .
Chemical Structure: Chemical Bonding. Ionic, Metallic & Coordinate Bondsulcerd
Lecture materials for the Introductory Chemistry course for Forensic Scientists, University of Lincoln, UK. See http://forensicchemistry.lincoln.ac.uk/ for more details.
Ionic bond seminar by Mohammad Nasih
in Kurdistan -Iraq
Kurdistan regional government
Ministry of higher education & scientific research
University scientific
Part chemistry
Introduction
Some Information & Properties about Ionic Bonding
Write Chemical Formula about this substance
Atoms gain or lose
Formation of Ions from Metals
Ions from Nonmetal Ions
Some Typical Ions with Positive Charges (Cations)
Unit 2, Lesson 2.6 - Elements and Compoundsjudan1970
Unit 2, Lesson 2.6 - Elements and Compounds
Lesson Outline:
1. Matter: An Overview
2. Pure Substance
3. Element vs. Compound
4. Metals, Metalloids, Nonmetals
5. Law of Definite Composition
chromatograpIn any chemical or bioprocessing industry, the need to separate and purify a product from a complex mixture is a necessary and important step in the production line. Today, there exists a wide market of methods in which industries can accomplish these goals. Chromatography is a very special separation process for a multitude of reasons! First of all, it can separate complex mixtures with great precision. Even very similar components, such as proteins that may only vary by a single amino acid, can be separated with chromatography.
Ionic bond seminar by Mohammad Nasih
in Kurdistan -Iraq
Kurdistan regional government
Ministry of higher education & scientific research
University scientific
Part chemistry
Introduction
Some Information & Properties about Ionic Bonding
Write Chemical Formula about this substance
Atoms gain or lose
Formation of Ions from Metals
Ions from Nonmetal Ions
Some Typical Ions with Positive Charges (Cations)
Unit 2, Lesson 2.6 - Elements and Compoundsjudan1970
Unit 2, Lesson 2.6 - Elements and Compounds
Lesson Outline:
1. Matter: An Overview
2. Pure Substance
3. Element vs. Compound
4. Metals, Metalloids, Nonmetals
5. Law of Definite Composition
chromatograpIn any chemical or bioprocessing industry, the need to separate and purify a product from a complex mixture is a necessary and important step in the production line. Today, there exists a wide market of methods in which industries can accomplish these goals. Chromatography is a very special separation process for a multitude of reasons! First of all, it can separate complex mixtures with great precision. Even very similar components, such as proteins that may only vary by a single amino acid, can be separated with chromatography.
This presentation explains the various correction and caveats related to using dermal fillers. The intended audience is medical professionals. Dr. Scheiner is a Plastic Surgeon and the President of ASAMP (The American Society of Aesthetic Medical Professionals). ASAMP certifies medical professionals for cosmetic injection procedures (Botox; Dermal Fillers) and is accredited through the American Academy of Family Physicians (up to 14 CME credits).
Classifying Life
The Three Domains of Life
Bacteria
Archaea
Protists
Plants
Moving Water Up a Tree
Fungi
Animals
How Birds Fly
Viruses and Prions
Science and Society: Swine Flu
Chapter 17
Evoution of Life
The Origin of Life
Did Life on Earth Originate on Mars?
Early Life on Earth
Charles Darwin and The Origin of Species
How Natural Selection Works
Adaptation
Staying Warm and Keeping Cool
Evolution and Genetics
How Species Form
Evidence of Evolution
Fossils: Earth's Tangible Evidence of Evolution
The Evolution of Humans
History of Science: The Peppered Moth
Science and Society: Antibiotic-Resistant Bacteria
Chapter 16 Genetics
What Is a Gene?
Chromosomes: Packages of Genetic Information
The Structure of DNA
DNA Replication
How Proteins Are Built
Genetic Mutations
How Radioactivity Causes Genetic Mutations
Meiosis and Genetic Diversity
Mendelian Genetics
More Wrinkles: Beyond Mendelian Genetics
The Human Genome
Cancer: Genes Gone Awry
Environmental Causes of Cancer
Transgenic Organisms and Cloning
DNA Technology—What Could Possibly Go Wrong?
History of Science: Discovery of the Double Helix
Technology: Gene Therapy
Science and Society: Genetic Counseling
Science and Society: DNA Forensics
Chapter 15
The basic unit of life
Characteristics of Life
Macromolecules Needed for Life
Cell Types: Prokaryotic and Eukaryotic
The Microscope
Tour of a Eukaryotic Cell
The Cell Membrane
Transport into and out of Cells
Cell Communication
How Cells Reproduce
How Cells Use Energy
ATP and Chemical Reactions in Cells
Photosynthesis
Cellular Respiration and Fermentation
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.
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.
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.
Richard's entangled aventures in wonderlandRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
2. This lecture will help you understand:
• Electron-Dot Structures
• The Formation of Ions
• Ionic Bonds
• Metallic Bonds
• Covalent Bonds
• Polar Covalent Bonds
• Molecular Polarity
• Molecular Attractions
• Most Materials Are Mixtures
• The Chemist's Classification of Matter
• Solutions
• Solubility
3. Electron-Dot Structures
• Atoms bond together through their electrons. To
learn about bonding, therefore, we need to know
something about how the electrons in an atom are
organized.
• Electrons behave as though they are contained
within seven concentric shells.
4. Electron-Dot Structures
• The numbers indicate the maximum number of
electrons each shell may contain.
Note:
• This is a "conceptual model"
and not a representation of
what an atom "looks like."
• Rather, it helps us to
understand how the
electrons in atoms behave.
5. Electron-Dot Structures
• The shells are more easily
drawn in two dimensions.
• Each atom has its own
configuration of electrons.
Elements in the same group
have similar configurations,
which is why they have
similar properties.
6. Electron-Dot Structures
• Valence electrons are electrons in the outermost
shell of an atom. These are the ones that can
participate in chemical bonding.
• An electron-dot structure is a notation that shows
the valence electrons surrounding the atomic
symbol.
7. Kr
Electron-Dot Structures
• Special Note
– For heavier atoms, some valence electrons are
more available than others. Krypton, for example,
has 18 valence electrons, but only eight of these
are typically shown in an electron-dot structure.
These are the eight that extend farthest away
from the nucleus.
12. Na+ F-
Ionic Bonds
• An ionic bond is the electrical force of attraction
between oppositely charged ions.
13.
14.
15. Ionic Bond Formation
1) An electrically neutral sodium atom loses its valence
electron to an electrically neutral chlorine atom.
2) This electron transfer results in two oppositely charged ions
3) The ions are held together by an ionic bond.
16.
17. Metallic Bonds
• Outer electrons in metal atoms are held only weakly
by the nucleus.
• This weak attraction allows the electrons to move
about quite freely.
• This mobility of electrons accounts for many metallic
properties.
19. Covalent Bonds
A covalent bond is the type of electrical attraction in
which atoms are held together by their mutual
attraction for shared electrons.
20. F — FF F
Covalent Bonds
• There are two electrons in a single covalent bond.
• The covalent bond is represented using a straight
line.
21. Covalent Bonds
• The number of covalent bonds an atom can form
equals its number of unpaired valence electrons.
24. Polar Covalent Bonds
• Electrons in a covalent bond are shared evenly
when the two atoms are the same.
25. Polar Covalent Bonds
• Electrons in a covalent bond may be shared
unevenly, however, when the bonded atoms are
different.
26. High
Low
Polar Covalent Bonds
• Electronegativity is the ability of a bonded atom to
pull on shared electrons. Greater electronegativity
means greater "pulling power."
32. Molecular Attractions
• An dipole-dipole attraction is the attraction between
two dipoles.
– Example: cohesive forces within water
33. Molecular Attractions
• A dipole–induced dipole attraction is the attraction
between a dipole and an induced dipole.
34. Molecular Attractions
• A fourth molecular attraction is the induced dipole–
induced dipole, which occurs between nonpolar
molecules.
35. Nonpolar atoms are attracted to each other by these "momentary" dipoles.
Molecular Attractions
36. The larger the atom, the stronger the "momentary" dipole.
Molecular Attractions
37. Molecular Attractions
The tiny nonpolar fluorine atoms in Teflon provide very weak
attractions, which is why Teflon provides a "nonstick" surface.
38. So, how do the gecko's sticky feet stay so clean?
Molecular Attractions
39. Most Materials Are Mixtures
• A pure substance is a material that consists of only
one type of element or compound.
• A mixture is a collection of two or more pure
substances.
• It can be separated by physical means.
42. The Chemist's Classification of Matter
• Pure materials consist of a single element or
compound.
• Impure materials consist of two or more elements or
compounds.
• Mixtures may be heterogeneous or homogeneous.
43. The Chemist's Classification of Matter
• In heterogeneous mixtures, the different
components can be seen as individual substances.
• In homogeneous mixtures, the composition is the
same throughout.
45. The Chemist's Classification of Matter
• Homogeneous mixtures:
– Solution: all components in the same phase
– Suspension: different components in different
phases
47. Concentration
Amount of solute
Amount of solution
Solutions
• Concentration is a measure of the amount of solute
dissolved in solution.
• A solution with more solute than solution is called
concentrated.
• A solution with more solution than solute is called
dilute.
=
48. The formula mass of a
substance expressed in
grams contains 1 mole.
Substance Formula Mass
Carbon, C 12
Oxygen, O2 32
Carbon dioxide, CO2 44
Sucrose, C12H22O11 342
Solutions
• A mole is a super-large number, 6.02 × 1023
, used to
measure numbers of atoms or molecules, also
called Avogadro's number.
50. Molarity
moles of Solute
liter of Solution
Solutions
• Molarity is a unit of concentration expressed in
moles of solute per liter of solution.
=
51. 1 ppm
1 part solute
1,000,000 parts solution
1 milligram solute
1 liter solution
=
Solutions
• ppm is a unit of concentration expressed in
milligrams of solute in per liters of solution.
=
52. Solubility
• Solubility is the ability of a solute to dissolve in a
solvent.
• A solute that has appreciable solubility is said to be
soluble.