2. Extra-terrestrial life: Is there anybody out there?… Dr Martin Hendry University of Glasgow Star Wars Day May 4 th 2011

5. Liquid Water Oxygen Carbon Dioxide = life!

6. Is there life elsewhere in our Solar System?

7. Mars is the best bet:  Mars Express ( + Beagle 2)  Spirit + Opportunity

8. We can use spectral lines, like fingerprints, to identify the chemicals that stars and planets are made of.

9. Wavelength (microns) Strength of absorption

10. Signs of past running water in many Martian photographs

14. The moons of Jupiter

15. One of Jupiter’s moons, Europa, is another candidate The icy crust of the moon is covered in ‘cracks’ due to the tides, and beneath the crust we think friction has melted the ice, resulting in a thin ocean layer

16. Inside Europa

17. From Science (2002)

26. 2. How can we detect planets around other stars? This isn’t easy because: other stars (and their planets) are very far away planets don’t shine by themselves, they just reflect light from their star, so they get lost in the glare.

27. The distance from the Earth to the Sun is 150 million km. It takes sunlight more than eight minutes to travel this distance. The light from the next nearest star, Alpha Centauri, takes more than four years to reach the Earth.

28. Exoplanets are ‘drowned out’ by their parent star. That makes them very hard to see directly with current telescopes (~10m mirrors)… Keck telescopes on Mauna Kea, Hawaii

29. The European Extremely Large Telescope project 42m mirror: to be completed by 2020

30. The European Extremely Large Telescope project 42m mirror: to be completed by 2020 ‘Jupiter’ at 30 l.y.

31. How can we detect planets around other stars? This isn’t easy because: other stars (and their planets) are very far away planets don’t shine by themselves, they just reflect light from their star, so they get lost in the glare. We can tell that planets are there by the effect they have on their star.

32. Planets cause their parent star to ‘wobble’ Centre of gravity

33. Star + planet orbit about centre of gravity

34. Can see star ‘wobble’, even when we can’t see the planet.

35. Star + planet orbit about centre of gravity We can also see the motion of the star from its spectral lines.

36. Direction to Earth Suppose line of sight is in orbital plane Star has a periodic motion towards and away from Earth

37. Star Laboratory

38. In the past 16 years we have found many planets orbiting other stars in our galaxy…

39. Could some of those planets be like the Earth? Most planets we’ve found so far are ‘hot Jupiters’: gas giants, much bigger and closer to their parent star than the Earth is to the Sun. These are not good places to look for life like us: no water, no oxygen, much too hot!

40. No Earth-like planets, yet…. In the past 16 years we have found many planets orbiting other stars in our galaxy…

41. Transit of Mercury: May 7 th 2003 In recent years a growing number of exoplanets have been detected via transits

42. Kepler Launched: March 5 th 2009

43. Detecting exoplanets from transits Brightness Time Star Planet

46. Kepler If Earth-like planets exist around nearby stars, Kepler should find them

47. Could there be ET life like us on those planets? Finding water, carbon dioxide, and especially oxygen would be a very big clue, but we really don’t know!

48. Could there be ET life like us on those planets? Finding water, carbon dioxide, and especially oxygen would be a very big clue, but we really don’t know! If life does exist, what would it look like? How would this depend on the type of planet and star?...

49. 5. If ETs are out there, how would we communicate? What language could we use? What would we say?

50. If ETs are out there, how would we communicate? What language could we use? What would we say?

51. If ETs are out there, how would we communicate? What language could we use? What would we say?

52. Or we can just try listening!...

53. What would you say to ET?....

54. May the Fourth be with you

55. http://www.astro.gla.ac.uk/users/martin/etlife/