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By: Alejandro Cano, Dani 
Martínez, Sergio Núñez & 
Carmen Barbero
• Gravity has an important 
role in this theme 
• As you all know, gravity 
is the force of attraction 
that we feel when we are 
near of an astronomical 
object 
• This was described by Sir. 
Isaac Newton in the Laws 
of Universal Gravitation
• It does not interact with electromagnetic 
spectrum. 
• It is not visible but the amount of it in the 
universe is much bigger than the amount of 
matter that is visible 
• Matter visible are planets, stars, galaxies.. 
• The only explanation for its existance is the 
gravitational pull.
Gravitational Pull 
• Appreciated in spiral 
galaxies 
• Stars at the center 
should rotate at a 
higher speed than the 
ones outside 
• The speed is mostly the 
same 
• As a conclusion the 
ones outside are feeling 
a gravitational pull.
Galaxy Clusters 
• If we look to one of this 
we can see that there is 
10 times more mass than 
the one we can account 
for 
• Coma Galaxy Cluster is 
one example 
• In this clusters we can 
see that it always 
remains the same but 
galaxies move at high 
speed
• Mass 
• Orbital speed
• Coma Cluster
• GALAXY-GALAXY CLUSTER-OBSERVER 
• Einstein´s ring
• Opposite effect: 
Negative pressure; repulsion of matter.
Expectation: slowing down, GRAVITY 
WINS!
Expectation: slowing down, GRAVITY 
WINS!
Space´s expansion is 
accelerating
Galaxies!
• EEuucclliidd ssppaaccee mmiissssiioonn:: measure the expanding universe’s 
acceleration. 
• FFeerrmmii GGaammmmaa--rraayy SSppaaccee TTeelleessccooppee:: gamma-ray 
observations from low Earth orbit.
• LLaarrggee HHaaddrroonn CCoolllliiddeerr ((LLHHCC)):: it might produce dark 
matter particles. It’s only evidence would be its missing 
energy. 
• CCDDMMSS ((CCrryyooggeenniicc DDaarrkk MMaatttteerr SSeeaarrcchh)):: detect 
particle dark matter in the form of WIMPs (weakly 
interactive massive particles).
Dark matter and dark energy (1)

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Dark matter and dark energy (1)

  • 1. By: Alejandro Cano, Dani Martínez, Sergio Núñez & Carmen Barbero
  • 2.
  • 3.
  • 4. • Gravity has an important role in this theme • As you all know, gravity is the force of attraction that we feel when we are near of an astronomical object • This was described by Sir. Isaac Newton in the Laws of Universal Gravitation
  • 5. • It does not interact with electromagnetic spectrum. • It is not visible but the amount of it in the universe is much bigger than the amount of matter that is visible • Matter visible are planets, stars, galaxies.. • The only explanation for its existance is the gravitational pull.
  • 6. Gravitational Pull • Appreciated in spiral galaxies • Stars at the center should rotate at a higher speed than the ones outside • The speed is mostly the same • As a conclusion the ones outside are feeling a gravitational pull.
  • 7. Galaxy Clusters • If we look to one of this we can see that there is 10 times more mass than the one we can account for • Coma Galaxy Cluster is one example • In this clusters we can see that it always remains the same but galaxies move at high speed
  • 8. • Mass • Orbital speed
  • 10. • GALAXY-GALAXY CLUSTER-OBSERVER • Einstein´s ring
  • 11. • Opposite effect: Negative pressure; repulsion of matter.
  • 12. Expectation: slowing down, GRAVITY WINS!
  • 13. Expectation: slowing down, GRAVITY WINS!
  • 14. Space´s expansion is accelerating
  • 16. • EEuucclliidd ssppaaccee mmiissssiioonn:: measure the expanding universe’s acceleration. • FFeerrmmii GGaammmmaa--rraayy SSppaaccee TTeelleessccooppee:: gamma-ray observations from low Earth orbit.
  • 17. • LLaarrggee HHaaddrroonn CCoolllliiddeerr ((LLHHCC)):: it might produce dark matter particles. It’s only evidence would be its missing energy. • CCDDMMSS ((CCrryyooggeenniicc DDaarrkk MMaatttteerr SSeeaarrcchh)):: detect particle dark matter in the form of WIMPs (weakly interactive massive particles).