SlideShare a Scribd company logo
1 of 4
"The Sun: Our Closest Star" appearing
Introduction
Did you know that the sun is not just a big ball of fire? It's
much more fascinating than that! The sun is composed of gas
and lacks a solid surface. But that's just the beginning!
The Core: Where Magic Happens
Right at the heart of the sun lies its core, which makes up a
staggering 25% of its radius. This core is where all the magic
happens. Now, let's talk about something mind-blowing—
nuclear fusion! It's the powerhouse behind the sun's
brilliance.
Yes, Nuclear fusion is a process where hydrogen atoms fuse
together to form helium, releasing an enormous amount of
energy in the process. This energy is what makes the sun
shine so brilliantly and provides us with warmth and light.
The Radiative Zone: A Bouncing Journey
But wait, there's more! Beyond the core lies the radiative
zone, which comprises a whopping 45% of the sun's radius.
In the radiative zone, energy from the core gradually makes
its way outwards, bouncing around like a pinball game,
before eventually reaching the sun's surface. It's an
incredible journey.
The Sun's Atmosphere: A Multilayered Marvel
Now, let's shift our focus to the sun's atmosphere. It's not
just a single layer; it's divided into three distinct parts. Up
here, above the surface, we have the photosphere,
chromosphere, and the enigmatic corona.
1. The Photosphere: The Visible Surface
The photosphere is like the sun's visible surface, the part
we're most familiar with. It's where sunspots and solar flares
occur.
2. The Chromosphere: A Red-Hued Beauty
Just above the photosphere, we have the chromosphere—a
layer of red-hued gas that's absolutely stunning during a solar
eclipse.
3. The Corona: The Crown Jewel
And finally, the crown jewel, the corona! This outermost
layer is incredibly hot, and it extends for millions of miles into
space. Can you imagine that?
The corona is a place of extreme temperatures and magnetic
activity, making it one of the most mysterious parts of our
sun.
Conclusion
The incredible structure of our sun—composed of gas,
powered by nuclear fusion, and surrounded by layers of
wonder. The sun may be our closest star, but it's also our
most mysterious one.
To watch more. Click the link
https://www.youtube.com/watch?v=0sliStRE_Dg

More Related Content

Similar to sun composition.docx (20)

Astronomy project
Astronomy projectAstronomy project
Astronomy project
 
Sun
SunSun
Sun
 
sun properties.ppt
sun properties.pptsun properties.ppt
sun properties.ppt
 
The sun
The sun The sun
The sun
 
The sun
The sunThe sun
The sun
 
The Universe and the Stars
The Universe and the StarsThe Universe and the Stars
The Universe and the Stars
 
SUN
SUNSUN
SUN
 
C. the solar system
C. the solar systemC. the solar system
C. the solar system
 
Sun
SunSun
Sun
 
6.Sun.ppt
6.Sun.ppt6.Sun.ppt
6.Sun.ppt
 
6.sun
6.sun6.sun
6.sun
 
The Sun
The SunThe Sun
The Sun
 
sun
sunsun
sun
 
Sun (2)
Sun (2)Sun (2)
Sun (2)
 
Form 3 PMR Science Chapter 9 Stars and Galaxies
Form 3 PMR Science Chapter 9 Stars and GalaxiesForm 3 PMR Science Chapter 9 Stars and Galaxies
Form 3 PMR Science Chapter 9 Stars and Galaxies
 
Stars print
Stars printStars print
Stars print
 
Nebulae & Galaxies
Nebulae & GalaxiesNebulae & Galaxies
Nebulae & Galaxies
 
Nebula & Galaxies
Nebula & GalaxiesNebula & Galaxies
Nebula & Galaxies
 
04 The Sun Mc Neely
04 The Sun Mc Neely04 The Sun Mc Neely
04 The Sun Mc Neely
 
Dtu10e lecture ppt_ch10 2
Dtu10e lecture ppt_ch10 2Dtu10e lecture ppt_ch10 2
Dtu10e lecture ppt_ch10 2
 

Recently uploaded

Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.
Cherry
 
ONLINE VOTING SYSTEM SE Project for vote
ONLINE VOTING SYSTEM SE Project for voteONLINE VOTING SYSTEM SE Project for vote
ONLINE VOTING SYSTEM SE Project for vote
RaunakRastogi4
 
LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.
Cherry
 
development of diagnostic enzyme assay to detect leuser virus
development of diagnostic enzyme assay to detect leuser virusdevelopment of diagnostic enzyme assay to detect leuser virus
development of diagnostic enzyme assay to detect leuser virus
NazaninKarimi6
 
Lipids: types, structure and important functions.
Lipids: types, structure and important functions.Lipids: types, structure and important functions.
Lipids: types, structure and important functions.
Cherry
 
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
Cherry
 
POGONATUM : morphology, anatomy, reproduction etc.
POGONATUM : morphology, anatomy, reproduction etc.POGONATUM : morphology, anatomy, reproduction etc.
POGONATUM : morphology, anatomy, reproduction etc.
Cherry
 
Reboulia: features, anatomy, morphology etc.
Reboulia: features, anatomy, morphology etc.Reboulia: features, anatomy, morphology etc.
Reboulia: features, anatomy, morphology etc.
Cherry
 

Recently uploaded (20)

Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.Phenolics: types, biosynthesis and functions.
Phenolics: types, biosynthesis and functions.
 
ONLINE VOTING SYSTEM SE Project for vote
ONLINE VOTING SYSTEM SE Project for voteONLINE VOTING SYSTEM SE Project for vote
ONLINE VOTING SYSTEM SE Project for vote
 
Selaginella: features, morphology ,anatomy and reproduction.
Selaginella: features, morphology ,anatomy and reproduction.Selaginella: features, morphology ,anatomy and reproduction.
Selaginella: features, morphology ,anatomy and reproduction.
 
Efficient spin-up of Earth System Models usingsequence acceleration
Efficient spin-up of Earth System Models usingsequence accelerationEfficient spin-up of Earth System Models usingsequence acceleration
Efficient spin-up of Earth System Models usingsequence acceleration
 
GBSN - Biochemistry (Unit 2) Basic concept of organic chemistry
GBSN - Biochemistry (Unit 2) Basic concept of organic chemistry GBSN - Biochemistry (Unit 2) Basic concept of organic chemistry
GBSN - Biochemistry (Unit 2) Basic concept of organic chemistry
 
Cyanide resistant respiration pathway.pptx
Cyanide resistant respiration pathway.pptxCyanide resistant respiration pathway.pptx
Cyanide resistant respiration pathway.pptx
 
Terpineol and it's characterization pptx
Terpineol and it's characterization pptxTerpineol and it's characterization pptx
Terpineol and it's characterization pptx
 
LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.LUNULARIA -features, morphology, anatomy ,reproduction etc.
LUNULARIA -features, morphology, anatomy ,reproduction etc.
 
development of diagnostic enzyme assay to detect leuser virus
development of diagnostic enzyme assay to detect leuser virusdevelopment of diagnostic enzyme assay to detect leuser virus
development of diagnostic enzyme assay to detect leuser virus
 
Dr. E. Muralinath_ Blood indices_clinical aspects
Dr. E. Muralinath_ Blood indices_clinical  aspectsDr. E. Muralinath_ Blood indices_clinical  aspects
Dr. E. Muralinath_ Blood indices_clinical aspects
 
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
Human & Veterinary Respiratory Physilogy_DR.E.Muralinath_Associate Professor....
 
Lipids: types, structure and important functions.
Lipids: types, structure and important functions.Lipids: types, structure and important functions.
Lipids: types, structure and important functions.
 
Method of Quantifying interactions and its types
Method of Quantifying interactions and its typesMethod of Quantifying interactions and its types
Method of Quantifying interactions and its types
 
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
Major groups of bacteria: Spirochetes, Chlamydia, Rickettsia, nanobes, mycopl...
 
FS P2 COMBO MSTA LAST PUSH past exam papers.
FS P2 COMBO MSTA LAST PUSH past exam papers.FS P2 COMBO MSTA LAST PUSH past exam papers.
FS P2 COMBO MSTA LAST PUSH past exam papers.
 
POGONATUM : morphology, anatomy, reproduction etc.
POGONATUM : morphology, anatomy, reproduction etc.POGONATUM : morphology, anatomy, reproduction etc.
POGONATUM : morphology, anatomy, reproduction etc.
 
Reboulia: features, anatomy, morphology etc.
Reboulia: features, anatomy, morphology etc.Reboulia: features, anatomy, morphology etc.
Reboulia: features, anatomy, morphology etc.
 
Adaptive Restore algorithm & importance Monte Carlo
Adaptive Restore algorithm & importance Monte CarloAdaptive Restore algorithm & importance Monte Carlo
Adaptive Restore algorithm & importance Monte Carlo
 
Concept of gene and Complementation test.pdf
Concept of gene and Complementation test.pdfConcept of gene and Complementation test.pdf
Concept of gene and Complementation test.pdf
 
GBSN - Microbiology (Unit 5) Concept of isolation
GBSN - Microbiology (Unit 5) Concept of isolationGBSN - Microbiology (Unit 5) Concept of isolation
GBSN - Microbiology (Unit 5) Concept of isolation
 

sun composition.docx

  • 1. "The Sun: Our Closest Star" appearing Introduction Did you know that the sun is not just a big ball of fire? It's much more fascinating than that! The sun is composed of gas and lacks a solid surface. But that's just the beginning! The Core: Where Magic Happens Right at the heart of the sun lies its core, which makes up a staggering 25% of its radius. This core is where all the magic happens. Now, let's talk about something mind-blowing— nuclear fusion! It's the powerhouse behind the sun's brilliance.
  • 2. Yes, Nuclear fusion is a process where hydrogen atoms fuse together to form helium, releasing an enormous amount of energy in the process. This energy is what makes the sun shine so brilliantly and provides us with warmth and light. The Radiative Zone: A Bouncing Journey But wait, there's more! Beyond the core lies the radiative zone, which comprises a whopping 45% of the sun's radius. In the radiative zone, energy from the core gradually makes its way outwards, bouncing around like a pinball game, before eventually reaching the sun's surface. It's an incredible journey. The Sun's Atmosphere: A Multilayered Marvel Now, let's shift our focus to the sun's atmosphere. It's not just a single layer; it's divided into three distinct parts. Up here, above the surface, we have the photosphere, chromosphere, and the enigmatic corona. 1. The Photosphere: The Visible Surface
  • 3. The photosphere is like the sun's visible surface, the part we're most familiar with. It's where sunspots and solar flares occur. 2. The Chromosphere: A Red-Hued Beauty Just above the photosphere, we have the chromosphere—a layer of red-hued gas that's absolutely stunning during a solar eclipse. 3. The Corona: The Crown Jewel And finally, the crown jewel, the corona! This outermost layer is incredibly hot, and it extends for millions of miles into space. Can you imagine that? The corona is a place of extreme temperatures and magnetic activity, making it one of the most mysterious parts of our sun. Conclusion
  • 4. The incredible structure of our sun—composed of gas, powered by nuclear fusion, and surrounded by layers of wonder. The sun may be our closest star, but it's also our most mysterious one. To watch more. Click the link https://www.youtube.com/watch?v=0sliStRE_Dg