The Sun
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The document summarizes key information about the sun. It begins by stating that the sun is an average sized star, located at the center of the solar system, composed primarily of hydrogen and helium. It then describes the various layers of the sun, including the core, radiation layer, convection layer, photosphere, chromosphere, and corona. It explains that nuclear fusion in the core converts hydrogen into helium, releasing energy in the process. This energy eventually makes its way to the surface of the sun and radiates out into space.
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臓is a star because it is made up of light and heat.
is the only star in the solar system.
As a star, it is a source of light and heat.
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- Convective Zone
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This is my report to Earth Science subject.
Please download it, to see the whole content.
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APM event hosted by the South Wales and West of England Network (SWWE Network)
Speaker: Aalok Sonawala
The SWWE Regional Network were very pleased to welcome Aalok Sonawala, Head of PMO, National Programmes, Rider Levett Bucknall on 26 February, to BAWA for our first face to face event of 2025. Aalok is a member of APMs Thames Valley Regional Network and also speaks to members of APMs PMO Interest Network, which aims to facilitate collaboration and learning, offer unbiased advice and guidance.
Tonight, Aalok planned to discuss the importance of a PMO within project-based organisations, the different types of PMO and their key elements, PMO governance and centres of excellence.
PMOs within an organisation can be centralised, hub and spoke with a central PMO with satellite PMOs globally, or embedded within projects. The appropriate structure will be determined by the specific business needs of the organisation. The PMO sits above PM delivery and the supply chain delivery teams.
For further information about the event please click here.South Hornsey: The Lost Local Authority that Merged with Stoke Newington by T...
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- Autonomy, Teams and Tension
- Oliver Randall & David Bovis
- Own Your Autonomy
Oliver Randall
Consultant, Tribe365
Oliver is a career project professional since 2011 and started volunteering with APM in 2016 and has since chaired the People Interest Network and the North East Regional Network. Oliver has been consulting in culture, leadership and behaviours since 2019 and co-developed HPTM速an off the shelf high performance framework for teams and organisations and is currently working with SAS (Stellenbosch Academy for Sport) developing the culture, leadership and behaviours framework for future elite sportspeople whilst also holding down work as a project manager in the NHS at North Tees and Hartlepool Foundation Trust.
David Bovis
Consultant, Duxinaroe
A Leadership and Culture Change expert, David is the originator of BTFA and The Dux Model.
With a Masters in Applied Neuroscience from the Institute of Organisational Neuroscience, he is widely regarded as the Go-To expert in the field, recognised as an inspiring keynote speaker and change strategist.
He has an industrial engineering background, majoring in TPS / Lean. David worked his way up from his apprenticeship to earn his seat at the C-suite table. His career spans several industries, including Automotive, Aerospace, Defence, Space, Heavy Industries and Elec-Mech / polymer contract manufacture.
Published in Londons Evening Standard quarterly business supplement, James Caans Your business Magazine, Quality World, the Lean Management Journal and Cambridge Universities PMA, he works as comfortably with leaders from FTSE and Fortune 100 companies as he does owner-managers in SMEs. He is passionate about helping leaders understand the neurological root cause of a high-performance culture and sustainable change, in business.
Session | Own Your Autonomy The Importance of Autonomy in Project Management
#OwnYourAutonomy is aiming to be a global APM initiative to position everyone to take a more conscious role in their decision making process leading to increased outcomes for everyone and contribute to a world in which all projects succeed.
We want everyone to join the journey.
#OwnYourAutonomy is the culmination of 3 years of collaborative exploration within the Leadership Focus Group which is part of the APM People Interest Network. The work has been pulled together using the 5 HPTM速 Systems and the BTFA neuroscience leadership programme.
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-Autonomy, Teams and Tension: Projects under stress
-Tim Lyons
-The neurological levels of
team-working: Harmony and tensions
With a background in projects spanning more than 40 years, Tim Lyons specialised in the delivery of large, complex, multi-disciplinary programmes for clients including Crossrail, Network Rail, ExxonMobil, Siemens and in patent development. His first career was in broadcasting, where he designed and built commercial radio station studios in Manchester, Cardiff and Bristol, also working as a presenter and programme producer. Tim now writes and presents extensively on matters relating to the human and neurological aspects of projects, including communication, ethics and coaching. He holds a Masters degree in NLP, is an NLP Master Practitioner and International Coach. He is the Deputy Lead for APMs People Interest Network.
Session | The Neurological Levels of Team-working: Harmony and Tensions
Understanding how teams really work at conscious and unconscious levels is critical to a harmonious workplace. This session uncovers what those levels are, how to use them to detect and avoid tensions and how to smooth the management of change by checking you have considered all of them.
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Historical instances like the 1938 FD&C Act and the Generic Drug Scandals underscore how crisis-triggered reforms often fail to address the fundamental issues, perpetuating inefficiencies and hazards.
The narrative advocates a shift from reactive crisis management to proactive, adaptable systems prioritizing continuous enhancement. Key hurdles involve challenging outdated assumptions regarding bioavailability, inadequately funded research ventures, and the impact of vague language in regulatory frameworks.
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Tackling these blind spots demands a holistic approach, embracing adaptive learning and a steadfast commitment to self-improvement. By nurturing curiosity, refining regulatory terminology, and judiciously harnessing new technologies, the pharmaceutical sector can progress towards better public health service delivery and ensure the safety, efficacy, and real-world impact of drug products.Rass MELAI : an Internet MELA Quiz Finals - El Dorado 2025
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The Sun
- 1. The Sun Chapter 6 Lesson 1 Ms. Aab Mrs. Avila
- 2. California State Standards and Objective 5 ES 5.a. Students know the Sun, an average star, is the central and largest body in the solar system and is composed primarily of hydrogen and helium. Objective : Students in grade five will be able to label and identify parts of the sun, identify the sun as a star , and explain the atomic process through which the sun releases energy.
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- 5. The Sun is a Star The sun is a Star made of hydrogen and helium. The sun is located at the center of the solar system and is also the largest object.
- 6. Vocabulary Star - is an object that produces it own energy, including heat and light. Astronomical Unit- the closest stars to the solar system are found in the Alpha Centauri star system.
- 7. The size of the Sun If the Sun were a hollow ball more then a million Earths could fit inside it! The Sun is an average size star and the largest object in the solar system. The Sun looks larger than the other stars that can be seen in the night sky because it is much closer to Earth.
- 8. What are the Parts of the Sun? The Sun is a huge sphere made up of mostly of two gases. 71% of the Suns mass is Hydrogen 27% of the Suns mass is Helium The remaining 2% is Oxygen and Carbon
- 9. Parts of the Sun!
- 10. The Core Most of the energy that the Sun produces is formed in its core. The Cores temperature is 10 million to 20 million degrees Celsius. The pressure is more than 1 billion times greater then the air pressure of Earth.
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- 12. Radiation Layer Next to the core Moves the energy produced in the core in every direction. It can take million of years for energy to move out of this layer.
- 13. Convection Layer Layer next to the radiation layer Gasses with different energies move in circles in a way similar to air with different densities. Energy moves out of this layer in about a week.
- 14. Photosphere Is the visible surface of the Sun. It is not a solid surface, but rather a layer of gasses. It is cooler then the core with a temperature of 10,346 F
- 15. Chromosphere Is the inner layer of the Suns atmosphere. When it can be seen it looks like a red circle around the Sun.
- 16. The Corona The outermost layer of the Suns atmosphere. The corona takes on different shapes around the Sun depending on changes in the temperature of the photosphere.
- 17. Solar Flares Are burst of heat and energy that stretch out from the corona and chromospheres into space. Sometimes the energy disrupts satallites, interfering with TV, radio, and cell phone communication systems.
- 18. Aurora Borealis Also called the Northern Lights Energy from the solar flares also causes displays of different-colored lights in the upper atmosphere. Most often seen in Alaska, Canada, and the Northern United States
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- 21. Sun Spots Solar Flares are also sometimes associated with sunspots They are dark spots on the Sun. They are regions of the photosphere that have a lower temperature then the surrounding regions.
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- 23. How does the Sun produce energy? 100 years ago, Albert Einstein discovered a relationship between energy and mass. E = MC 2 The E stands for energy, M stands for mass, the C represents the speed of light.
- 24. What happens inside the Sun? Hydrogen particles smash together to make helium. This smashing is called Fusion . A little bit of mass is a lost when hydrogen particles combine to make helium. The mass in turned into energy We see this energy as light and heat!