SlideShare una empresa de Scribd logo
1 de 17
Big Bang)



            13,700




Universe)


              10,000,000,000


                     Stars)
Star clusters)          Nebulae)
            Cosmic dust)




                            ''




                      big-bang theory
        G.Lemaitre)


6,400           4,000
Primeval Atom)                                      2




                           G.Gamow)



              3 x 10^9          3,000,000,000
                            5                            10^9
      1,000,000,000                             3 x 10^8
300,000,000                              200


                                                          2472
      Edwin P.Hubble)                                       20
                                20




                    2.5                         38,000




                      Exploding Universe)
globula cluster)                12,000



                                                    r       v
                                                    t=r/v


v=hr
       1/h                                      H
             hubble constant
)
1929                      3
                         200                                H
                        5,000
                                       12,000



                                Cepheid variabie star)
1948



            BIG BANG




            18,000
                ''



big bang)
quantum mechanics)




               1980




“   ” (Big Bang Theory)
,




           Inflationary period)
                                               Plasma
period)




                          “       ” (Galaxy)




“         ” (Milky Galaxy)
“    ” (COBE)




   ,


                                “       ”




            “      ”(dark matter)



Stephen Hawking)


                                            Evolution
Theory)               Charles Darwin)



                                        “     ”
(Emergent Evolution)


                       “       ”




1964


                                             1965




                                   1.1 x 1010-1.8x1010




                           3


1
1


protogalaxy)
15
2498            3
(




                    4




         2520


    *   2523            23"
*   2527




*   2539




*   2520 -   1
                 3
*   2520 -       3
                 25
*   2522 -   2
                 4
*   2536 -



*   2537 -


*   2538 -




*   2543 -
o
                50
    o




                     “
        ”                1
3




            ,
“   ”




                “
”




    5
,
กำเนิดเอกภพ

Más contenido relacionado

Similar a กำเนิดเอกภพ

เอกภพ Universe
เอกภพ Universeเอกภพ Universe
เอกภพ Universeyokyoi
 
เอกภพ Universe
เอกภพ Universe เอกภพ Universe
เอกภพ Universe yokyoi
 
พายุสุริยะคืออะไร
พายุสุริยะคืออะไรพายุสุริยะคืออะไร
พายุสุริยะคืออะไรNUMFON13
 
The Evolution of Elliptical Galaxies in Rich Clusters
The Evolution of Elliptical Galaxies in Rich ClustersThe Evolution of Elliptical Galaxies in Rich Clusters
The Evolution of Elliptical Galaxies in Rich ClustersRobert Berrington
 
Faltenbacher - Simulating the Universe
Faltenbacher - Simulating the UniverseFaltenbacher - Simulating the Universe
Faltenbacher - Simulating the UniverseCosmoAIMS Bassett
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศtrongjaitt
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศtrongjaitt
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศtrongjaitt
 
Colafrancesco - Dark Matter Dectection 1
Colafrancesco - Dark Matter Dectection 1Colafrancesco - Dark Matter Dectection 1
Colafrancesco - Dark Matter Dectection 1CosmoAIMS Bassett
 
Ccmc Universo
Ccmc UniversoCcmc Universo
Ccmc Universodiegotrap
 
Ccmc Universo
Ccmc UniversoCcmc Universo
Ccmc Universodiegotrap
 
A short introduction to massive gravity... or ... Can one give a mass to the ...
A short introduction to massive gravity... or ... Can one give a mass to the ...A short introduction to massive gravity... or ... Can one give a mass to the ...
A short introduction to massive gravity... or ... Can one give a mass to the ...CosmoAIMS Bassett
 
N.28 di martino-impact-and-non-impact-craters-in-eastern-sah
N.28 di martino-impact-and-non-impact-craters-in-eastern-sahN.28 di martino-impact-and-non-impact-craters-in-eastern-sah
N.28 di martino-impact-and-non-impact-craters-in-eastern-sahIAPS
 
37.pptx
37.pptx37.pptx
37.pptxzeex60
 
Roe_Summer_Lecture------------------.ppt
Roe_Summer_Lecture------------------.pptRoe_Summer_Lecture------------------.ppt
Roe_Summer_Lecture------------------.pptlily rosemary masilang
 
Origin of Universe (Twin)
Origin of Universe (Twin)Origin of Universe (Twin)
Origin of Universe (Twin)omsai_999
 
mrm Bristol-Flow Visualisation-(2008)
mrm Bristol-Flow Visualisation-(2008)mrm Bristol-Flow Visualisation-(2008)
mrm Bristol-Flow Visualisation-(2008)malcolmmackley
 

Similar a กำเนิดเอกภพ (19)

เอกภพ Universe
เอกภพ Universeเอกภพ Universe
เอกภพ Universe
 
เอกภพ Universe
เอกภพ Universe เอกภพ Universe
เอกภพ Universe
 
พายุสุริยะคืออะไร
พายุสุริยะคืออะไรพายุสุริยะคืออะไร
พายุสุริยะคืออะไร
 
The Evolution of Elliptical Galaxies in Rich Clusters
The Evolution of Elliptical Galaxies in Rich ClustersThe Evolution of Elliptical Galaxies in Rich Clusters
The Evolution of Elliptical Galaxies in Rich Clusters
 
Faltenbacher - Simulating the Universe
Faltenbacher - Simulating the UniverseFaltenbacher - Simulating the Universe
Faltenbacher - Simulating the Universe
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศ
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศ
 
เทคโนโลยีอวกาศ
เทคโนโลยีอวกาศเทคโนโลยีอวกาศ
เทคโนโลยีอวกาศ
 
Colafrancesco - Dark Matter Dectection 1
Colafrancesco - Dark Matter Dectection 1Colafrancesco - Dark Matter Dectection 1
Colafrancesco - Dark Matter Dectection 1
 
Ccmc Universo
Ccmc UniversoCcmc Universo
Ccmc Universo
 
Ccmc Universo
Ccmc UniversoCcmc Universo
Ccmc Universo
 
A short introduction to massive gravity... or ... Can one give a mass to the ...
A short introduction to massive gravity... or ... Can one give a mass to the ...A short introduction to massive gravity... or ... Can one give a mass to the ...
A short introduction to massive gravity... or ... Can one give a mass to the ...
 
N.28 di martino-impact-and-non-impact-craters-in-eastern-sah
N.28 di martino-impact-and-non-impact-craters-in-eastern-sahN.28 di martino-impact-and-non-impact-craters-in-eastern-sah
N.28 di martino-impact-and-non-impact-craters-in-eastern-sah
 
Cps Hokudai
Cps HokudaiCps Hokudai
Cps Hokudai
 
Science and NASA's Human Space Flight Program
Science and NASA's Human Space Flight ProgramScience and NASA's Human Space Flight Program
Science and NASA's Human Space Flight Program
 
37.pptx
37.pptx37.pptx
37.pptx
 
Roe_Summer_Lecture------------------.ppt
Roe_Summer_Lecture------------------.pptRoe_Summer_Lecture------------------.ppt
Roe_Summer_Lecture------------------.ppt
 
Origin of Universe (Twin)
Origin of Universe (Twin)Origin of Universe (Twin)
Origin of Universe (Twin)
 
mrm Bristol-Flow Visualisation-(2008)
mrm Bristol-Flow Visualisation-(2008)mrm Bristol-Flow Visualisation-(2008)
mrm Bristol-Flow Visualisation-(2008)
 

กำเนิดเอกภพ

  • 1. Big Bang) 13,700 Universe) 10,000,000,000 Stars)
  • 2. Star clusters) Nebulae) Cosmic dust) '' big-bang theory G.Lemaitre) 6,400 4,000
  • 3. Primeval Atom) 2 G.Gamow) 3 x 10^9 3,000,000,000 5 10^9 1,000,000,000 3 x 10^8 300,000,000 200 2472 Edwin P.Hubble) 20 20 2.5 38,000 Exploding Universe)
  • 4. globula cluster) 12,000 r v t=r/v v=hr 1/h H hubble constant ) 1929 3 200 H 5,000 12,000 Cepheid variabie star)
  • 5. 1948 BIG BANG 18,000 '' big bang)
  • 6.
  • 7. quantum mechanics) 1980 “ ” (Big Bang Theory)
  • 8. , Inflationary period) Plasma period) “ ” (Galaxy) “ ” (Milky Galaxy)
  • 9. ” (COBE) , “ ” “ ”(dark matter) Stephen Hawking) Evolution Theory) Charles Darwin) “ ”
  • 10. (Emergent Evolution) “ ” 1964 1965 1.1 x 1010-1.8x1010 3 1
  • 12. 15 2498 3 ( 4 2520 * 2523 23"
  • 13. * 2527 * 2539 * 2520 - 1 3 * 2520 - 3 25 * 2522 - 2 4 * 2536 - * 2537 - * 2538 - * 2543 -
  • 14. o 50 o “ ” 1 3 ,
  • 15. ” “ ” 5
  • 16. ,