The document summarizes key characteristics of the sun, including its diameter being 109 times larger than Earth, surface temperature of 5100-6000°C, and composition of 70-80% hydrogen gas. It describes the sun's three-layer atmosphere - the corona, chromosphere, and photosphere - and details their temperatures and appearances. Solar phenomena like sunspots, prominences, and solar flares are discussed in relation to their effects on Earth and technologies. The energy generation process within the sun's core through hydrogen fusion to helium is also summarized.
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Tingkatan 5 / SPM
KOMSAS Bahasa Malaysia
Novel TIRANI karya Beb Sabariah mengandungi 24 bab
Nota dipermudahkan dalam bentuk peta I-think / mind map / peta minda
[UPDATED] beserta Analisis Novel (Tema, Persoalan, Plot, Watak & perwatakan, Latar masa, tempat & masyarakat, Nilai & pengajaran, gaya bahasa)
[UPDATED] sinopsis mengikut bab..
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 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.
Ethnobotany and Ethnopharmacology:
Ethnobotany in herbal drug evaluation,
Impact of Ethnobotany in traditional medicine,
New development in herbals,
Bio-prospecting tools for drug discovery,
Role of Ethnopharmacology in drug evaluation,
Reverse Pharmacology.
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 Create Map Views in the Odoo 17 ERPCeline George
The map views are useful for providing a geographical representation of data. They allow users to visualize and analyze the data in a more intuitive manner.
The French Revolution, which began in 1789, was a period of radical social and political upheaval in France. It marked the decline of absolute monarchies, the rise of secular and democratic republics, and the eventual rise of Napoleon Bonaparte. This revolutionary period is crucial in understanding the transition from feudalism to modernity in Europe.
For more information, visit-www.vavaclasses.com
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.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
2. Characteristic of the sun
Diameter : 109 times larger than earth
Mass : 33 420 times the mass of earth
Density :1485kg/m3 (0.27 x earth)
Surface temperature : 5100-6000o
C
Composition : Hydrogen gas (70-80%) & Helium
Structure of the sun
Sun’s atmosphere divided into 3 layers :
Corona,
Chromosphere
Photosphere
3. Corona :
Thin layer of gas, visible during total solar eclipse
Bluish white layer
Temperature : 2,000,000o
C
Chromosphere
9600km thick
Temperature 15,000o
C
Reddish during solar eclipse
Photosphere
Can be seen from earth
400km thick
Temperature 6000o
C
Core
Temperature 15 000 000o
C
Hydrogen is changed to helium
4.
5. Sunspots
Dark patches
Magnetically active spots
Cause changes in earth climate; e.g extreme drought
Prominences
Many thousand kilometres from the surface
Gases (hydrogen & helium which consists of energetic
& electrically charged particles) escape to the outer
space, causes solar wind that will affect :
satellite, radio, television, telegraph and telephone
communications
Climatic disturbances on earth
Aurora (the sky in the polar regions apperas
colourful)
6.
7.
8.
9. Solar flares
Huge cloud of hydrogen that causes violent
explosions
Causes
disturbances to telecommunication signals
Changes in earth climate
Magnet to malfunction in large solar flares
Energy is generated from the sun when the
hydrogen gas is changed into helium gas.
Energy is carried to the sun’s surface where
it is released as heat and light
10. Star : made up of dust and gases (hydrogen
and helium)
Sun is a star because it is made up of
hydrogen and helium
Stars can be compared by :
Size (neutron star -> supergiant star)
Brightness : depends on surface temperature,
size & distance from earth
Colour & Temperature: blue coloured has highest
temperature, red coloured have the lowest
temperature
11. Nebulae is made up of dust and gases
(hydrogen & helium)
Gravitational attraction will pull them
together and become stronger till a star is
formed
The attractive force causes the star to
expand & the temperature rise
The star will become stable if there is a
balance between the force pulling the star
together and the heat pushing the star apart.
12.
13. When the nuclear fusion of hydrogen and helium
has been completed, the core of the star will
getting smaller and smaller
A lot of heat is generated and heat up the
outermost layer of the star.
Hydrogen starts to burn, star will expand and
appears red in colour
If red giant is not massive, white dwarf is formed
If red giant is big, a supernova will occur n
neutron star formed
If the original star is superlarge star, a black hole
will be formed.
14.
15. Galaxies is a gathering of billions of stars and
planets, dusts and gases.
3 types of galaxies:
Spiral
Elliptical
Irregular
Our solar system is in the Milky Way, a spiral
shaped galaxy
The solar system occupies only a small part of
the Milky Way
The universe consists of all the matter, energy
and space that exist. It contain billion of
galaxies, stars, planets and particles.