Presentation is loading. Please wait.

Presentation is loading. Please wait.

Observing the Universe

Similar presentations


Presentation on theme: "Observing the Universe"— Presentation transcript:

1 Observing the Universe
Expanding Universe? Observing the Universe

2 Can you remember the two pieces of evidence?
Red shift They have seen it!!!!! Also remember that the expanding universe is evidence for the Big Bang……Why?

3 Red Shift When Hubble looked at the absorption spectra of the stars in the galaxies the light was “shifted” towards the red end of the spectrum, a so called red shift This was the pattern produced from a star This was the same star but some time later. The lines have moved towards the red end…red shift!

4 The Hubble Constant The more distant the galaxy, the greater its speed of recession ( recession means moving away) Speed of recession = Hubble constant x distance

5 Hubble Constant Hubble worked on this for a while and his constant changed a few times. Now its accepted to be 72 km/s per Mpc This means that a galaxy 1Mpc would be moving at a speed of 72 km/s

6 P73 Lesson 7 Hubble’s constant
Calculate the speed of recession of a galaxy that is at a distance of 100 Mpc, if the Hubble constant is 70 km/s per Mpc. Using the same value of the Hubble constant given in question 1, calculate the distance of a galaxy whose speed of recession is 2000 km/s. A galaxy lies at a distance of 40 Mpc from Earth. Measurements show its speed of recession is 3000 km/s. What value does this suggest for the Hubble constant?

7 The answers 1) Speed of recession = Hubble constant × distance.
Speed of recession = 70 km/s per Mpc ×100 Mpc = 7000 km/s 2) Distance = speed of recession/Hubble constant = 2000 km/s/70 km/s per Mpc = 29 Mpc 3) Hubble constant = speed of recession/distance = 3000 km/s/40 Mpc = 75 km/s per Mpc


Download ppt "Observing the Universe"

Similar presentations


Ads by Google