The document summarizes the origins of the universe, Earth, and life. It describes how the Big Bang created matter, light elements, and forces. As the universe expanded and cooled, hydrogen and helium fused to form heavier elements. Gravity caused matter to accumulate into stars and planets. On Earth, early atmospheric gases trapped water and the water cycle began. Over billions of years, conditions became suitable for the development of life.
Slide presentation for MS chemistry unit describing formation of the elements. Presentation uses photos from Hubble Space Telescope. Ends with open writing exercise.
Slide presentation for MS chemistry unit describing formation of the elements. Presentation uses photos from Hubble Space Telescope. Ends with open writing exercise.
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
The twelfth and final part in our survey of emerging New Energy technologies. Pioneered by Nikolai Kozyrev in the Soviet Union and popularized more recently by Richard Hoagland, Torsion Physics draws our attention to the twisting, spinning motion of objects and energy fields in the Universe. Understanding torsion physics may be important not only for humanity's future, but for understanding our ancient past as well.
The sixth area of New Energy science that we think is key to tapping energy from the quantum vacuum. This is electrogravitics, which was pioneered by Alfred Biefeld and Thomas Townsend Brown. Long used in covert military projects for super-fast aviation and aerospace propulsion, this is a science that is slowly attracting mainstream attention.
This PowerPoint is one small part of the Astronomy Topics unit from www.sciencepowerpoint.com. This unit consists of a five part 3000+ slide PowerPoint roadmap, 12 page bundled homework package, modified homework, detailed answer keys, 8 pages of unit notes for students who may require assistance, follow along worksheets, and many review games. The homework and lesson notes chronologically follow the PowerPoint slideshow. The answer keys and unit notes are great for support professionals. The activities and discussion questions in the slideshow and meaningful. The PowerPoint includes built-in instructions, visuals, and follow up questions. Also included are critical class notes (color coded red), project ideas, video links, and review games. This unit also includes four PowerPoint review games (110+ slides each with Answers), 38+ video links, lab handouts, activity sheets, rubrics, materials list, templates, guides, and much more. Also included is a 190 slide first day of school PowerPoint presentation. Teaching Duration = 5+ weeks. Areas of Focus in the Astronomy Topics Unit: The Solar System and the Sun, Order of the Planets, Our Sun, Life Cycle of a Star, Size of Stars, Solar Eclipse, Lunar Eclipse, The Inner Planets, Mercury, Venus, Earth, Moon, Craters, Tides, Phases of the Moon, Mars and Moons, Rocketry, Asteroid Belt, NEOs, The Torino Scale, The Outer Planets and Gas Giants, Jupiter / Moons, Saturn / Moons, Uranus / Moons, Neptune / Moons, Pluto's Demotion, The Kuiper Belt, Oort Cloud, Comets / Other, Beyond the Solar System, Types of Galaxies, Blackholes, Extrasolar Planets, The Big Bang, Dark Matter, Dark Energy, The Special Theory of Relativity, Hubble Space Telescope, Constellations, Spacetime and much more. If you have any questions please feel free to contact me. Thanks again and best wishes. Sincerely, Ryan Murphy M.Ed www.sciencepowerpoint@gmail.com
The twelfth and final part in our survey of emerging New Energy technologies. Pioneered by Nikolai Kozyrev in the Soviet Union and popularized more recently by Richard Hoagland, Torsion Physics draws our attention to the twisting, spinning motion of objects and energy fields in the Universe. Understanding torsion physics may be important not only for humanity's future, but for understanding our ancient past as well.
The sixth area of New Energy science that we think is key to tapping energy from the quantum vacuum. This is electrogravitics, which was pioneered by Alfred Biefeld and Thomas Townsend Brown. Long used in covert military projects for super-fast aviation and aerospace propulsion, this is a science that is slowly attracting mainstream attention.
How much of the human body is made up of stardust,Does atoms age and what is ...Healthcare consultant
How much of the human body is made up of stardust,Does atoms age and what is the age of atoms. If an atom or molecule becomes electrically charged by gaining or losing one or more electrons, it becomes an ion. If the atom gains electrons, it has a negative charge. If it loses electrons, it has a positive charge.
Universe and the Solar System (Lesson 1).pptxJoenelRubino3
SHS Earth and Life Grade 11 Lesson 1. This lesson discusses the compos of the universe, the origin of the universe, different hypotheses of the origin of the universe
Astronomy- State of the art is a course covering the hottest topics in astronomy. In this section, the exotic end states of stars are discussed, including pulsars, neutron stars, and black holes.
HOW RELATIONSHIPS MADE THE UNIVERE & HUMANSPaul H. Carr
-Einstein’s General Relativity (1916) frames modern cosmology.
-Big-Bang energetic beginning: interactive relationships of matter particles created our universe.
-Explains origin of 92 elements in the Periodic Table
- We are made of stardust.
- Symbiotic relations between cells led to the Cambrian explosion of complex and human life.
-BIG HISTORY: 13.8 BILLION YEARS
“Each of us is as old as the universe and experiences our greater self in the larger story of the universe.” Thomas Berry.
My collogues often asked me what I was so absorbed in my free time reading books.
I made this PPT to educate them.
I did not include my views in the PPT but only what great minds had to say on the subject.
These slides are prepared for giving a quick lecture to any kind of Astro freak audience. It will demonstrate a brief overview of our visible universe (cosmos) and some very basic idea of our cosmological aspects.
Visit: www.ahmedsanny.com for more lectures, notes, articles, and contents.
Operation “Blue Star” is the only event in the history of Independent India where the state went into war with its own people. Even after about 40 years it is not clear if it was culmination of states anger over people of the region, a political game of power or start of dictatorial chapter in the democratic setup.
The people of Punjab felt alienated from main stream due to denial of their just demands during a long democratic struggle since independence. As it happen all over the word, it led to militant struggle with great loss of lives of military, police and civilian personnel. Killing of Indira Gandhi and massacre of innocent Sikhs in Delhi and other India cities was also associated with this movement.
Instructions for Submissions thorugh G- Classroom.pptxJheel Barad
This presentation provides a briefing on how to upload submissions and documents in Google Classroom. It was prepared as part of an orientation for new Sainik School in-service teacher trainees. As a training officer, my goal is to ensure that you are comfortable and proficient with this essential tool for managing assignments and fostering student engagement.
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
Dive into the world of AI! Experts Jon Hill and Tareq Monaur will guide you through AI's role in enhancing nonprofit websites and basic marketing strategies, making it easy to understand and apply.
Macroeconomics- Movie Location
This will be used as part of your Personal Professional Portfolio once graded.
Objective:
Prepare a presentation or a paper using research, basic comparative analysis, data organization and application of economic information. You will make an informed assessment of an economic climate outside of the United States to accomplish an entertainment industry objective.
Model Attribute Check Company Auto PropertyCeline George
In Odoo, the multi-company feature allows you to manage multiple companies within a single Odoo database instance. Each company can have its own configurations while still sharing common resources such as products, customers, and suppliers.
Synthetic Fiber Construction in lab .pptxPavel ( NSTU)
Synthetic fiber production is a fascinating and complex field that blends chemistry, engineering, and environmental science. By understanding these aspects, students can gain a comprehensive view of synthetic fiber production, its impact on society and the environment, and the potential for future innovations. Synthetic fibers play a crucial role in modern society, impacting various aspects of daily life, industry, and the environment. ynthetic fibers are integral to modern life, offering a range of benefits from cost-effectiveness and versatility to innovative applications and performance characteristics. While they pose environmental challenges, ongoing research and development aim to create more sustainable and eco-friendly alternatives. Understanding the importance of synthetic fibers helps in appreciating their role in the economy, industry, and daily life, while also emphasizing the need for sustainable practices and innovation.
Acetabularia Information For Class 9 .docxvaibhavrinwa19
Acetabularia acetabulum is a single-celled green alga that in its vegetative state is morphologically differentiated into a basal rhizoid and an axially elongated stalk, which bears whorls of branching hairs. The single diploid nucleus resides in the rhizoid.
Unit 8 - Information and Communication Technology (Paper I).pdfThiyagu K
This slides describes the basic concepts of ICT, basics of Email, Emerging Technology and Digital Initiatives in Education. This presentations aligns with the UGC Paper I syllabus.
How to Make a Field invisible in Odoo 17Celine George
It is possible to hide or invisible some fields in odoo. Commonly using “invisible” attribute in the field definition to invisible the fields. This slide will show how to make a field invisible in odoo 17.
A Strategic Approach: GenAI in EducationPeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
2. Origin of the Cosmos—3
Options
Option 1: Someone made the universe
(Big Bang or creationist theory)
Option 2: The universe made itself
(Inflationary or evolutionist theory)
Option 3: The universe has always been
here (Steady State Theory)
Scientists now know that the cosmos had
a beginning (proton decay and galactic
motion)
Therefore only options 1 and 2 are viable
3. THE Big Bang/Nucleosynthesis
13.7 billion years agoMass of universesize of
head of a pin (singularity)
Unimaginable release of energy (an expansion
not a traditional explosion)trillions of degrees
Nobody knows how/why it happened
Created space and time
Created the 4 main forces: gravity, strong, weak
and electromagnetic forces.
http://hyperphysics.phy-astr.gsu.edu/hbase/forces/fu
Electrons, quarks and gluons created (building
blocks for all atoms)
5. Sounds a little “Quarky” to me…
Strong Force
http://tinyurl.com/3jjnw
http://www2.slac.stanford.edu/vvc/theory/quarks.html
6. Wave Characteristics
Wavelength: distance from the
beginning of one crest to the
beginning of another
Frequency: number of waves in a
given time period and distance
Amplitude: distance from the
midpoint of a wave to the crest or
trough
9. Cosmic Microwave Background
(CMB)
Discovered by the Hubble Space
Telescope
Originally discovered in the 1960’s
Mapped out in 1990 at Berkley
Energy waves (photons) left over
from the original Big Bang in the
form of microwaves
Thought to prove the BBT
10. So….What’s The MATTER?
Baryonic Matter (10% of universe): Matter
composed of protons/neutrons and
electrons (solid, liquid and gases)
Non-Baryonic or Dark Matter (90% of
universe): composed of WIMP (weakly
interacting massive particles)
Neutrinos: elementary particles with none
or very little mass
11. It’s All Elemental My Dear
Watson!
Expanding universe = stuff slowly
cools down (space is cold dude!!)
Nucleus protons + neutrons
Early space: mostly hydrogen and
helium atoms (He formed from H)
14. Atomic Number/Isotopes
Isotopes
Hydrogen atomssingle proton and a single
electron
Isotopes of Hydrogensame number of protons
and electrons….different number of NEUTRONS
Protium1+, 1- and O neutrons (atomic number
of 1)
Deuterium1+, 1- and 1 neutron (atomic
number of 2)
Tritium1+, 1- and 2 neutrons (atomic number
of 3)
16. Ions
Atoms with more or less electrons
than they are supposed to have
Formed when atoms gain or lose
electrons (bonding and fusion)
Anions: have more than the normal
amount of electrons (negative ions)
Cations: have less than the normal
amount of electrons (positive ions)
17. Formation of the Earth/Solar
System
50-100 million years pass
Gravityclumpingcoolingformed
all the masses in the universe
Stars begin to form(Our sun—5
billion years ago)
Planets (ie. Our solar system)
All still very very very hot!!
Too hot for ANYTHING to last
19. Expanding/Contracting Universe
TheoryWhich One?
Blue Shift of Lightgalaxies moving
toward us (contracting universe)
Faster move toward usmore blueshifted
Red Shift of Lightgalaxies would be
moving away from us (expanding
universe)
Faster move away from usmore
redshifted
Ambulance example (eeee ummm)
20. Hubble Expansion
Galaxies in our local group are
moving away from us
ThereforeRed Shifting
Proves our universe is still expanding
21. The Big Crunch and Cycling
Stuff is still red shifting today
Eventually gravity will slow junk
down
Crap will stop and then slowly begin
to blue shift
Blue shifting will speed up
Stuff, junk and crap will then form
another singularity
BIG CRUNCH = Another Big Bang
22. Origin of the Atmosphere
http://www.env.leeds.ac.uk/envi1280/lecture_notes_carsla
23. That’s Some Ha-High Quality
H2O!!
Water originated in the original formation
of the universe (heavy elements bonded
together)and solar system
water on earth also came from comets
melting as they enter the atmosphere
Over billions of yearsenough melted ice
and rain to fill up the crevices in the earth
Oceans, lakes and rivers formed
24. Water/Atmosphere Relationship
Surface originally too hotNo
atmosphere present to reflect heat
from sun
No atmosphere to hold it near the
surface
Evaporated into space
Molecules escaped faster than
gravity could hold them
25. OK…..Cool!!
Earth cools as time goes on (took a
billion years or so)
Early atmosphere forms (outgassing)
Ozone forms
Traps water from outgassing and
comet impacts
Water cycle begins
