SLIDE 1
Exoplanets: the cosmic context Sprial Galaxy NGC 1352 Sprial Galaxy - - PowerPoint PPT Presentation
Exoplanets: the cosmic context Sprial Galaxy NGC 1352 Sprial Galaxy - - PowerPoint PPT Presentation
Exoplanets: the cosmic context Sprial Galaxy NGC 1352 Sprial Galaxy NGC 1352 100,000 light years Sprial Galaxy NGC 1352 100,000 light years billions of stars in a 1000 ly radius every star we see at night is in the Milky Way The surface of a
SLIDE 2
SLIDE 3
Sprial Galaxy NGC 1352
100,000 light years
SLIDE 4
Sprial Galaxy NGC 1352
100,000 light years
billions of stars in a 1000 ly radius
SLIDE 5
every star we see at night is in the Milky Way
SLIDE 6
The surface of a planet is good place for life to...live
SLIDE 7
a nearby star provides energy; atmosphere and water may be key ingredients
SLIDE 8
Curiosity rover on Mars
SLIDE 9
Jupiter’s moon Europa: salt-water oceans
SLIDE 10
How common are habitable worlds?
Artist’s rendition: Lynette Cook
SLIDE 11
Galactic context for planets and life
SLIDE 12
Dense, cold clouds of gas and dust
SLIDE 13
Eagle Nebula (10s of light years across)
SLIDE 14
Star (and planet?) formation
SLIDE 15
SLIDE 16
“Debris disk” around the young star beta Pictoris
note: coronograph image; direct light from the star is physically blocked in front of the telescope
SLIDE 17
What is a planet?
break: mass limits on blackboard...
SLIDE 18
“Debris Disk” around the young star beta Pictoris
SLIDE 19
Our Solar System (sizes to scale)
Inner, terrestrial, planets: small, close together, rocky and metallic Outer, Jovian, planets: large, spread out, gaseous
SLIDE 20
Coplanar, most angular momentum vectors are aligned
SLIDE 21
Nebula collapsing under its own gravity -- spins faster – is is flattened into a disk
SLIDE 22
How common are other planetary systems? What properties do they have? How can we detect them and measure their properties?
SLIDE 23
Planets (and moons) shine by reflected sun/star-light
SLIDE 24
Direct imaging
SLIDE 25
Fomalhaut b - is it a planet?
SLIDE 26
Center of mass: common orbital motion
SLIDE 27
Radial velocity method
we’ll discuss this later...
iron lithium calcium
SLIDE 28
Venus transiting the Sun
SLIDE 29
SLIDE 30
SLIDE 31
SLIDE 32
Kepler Mission (2009)
SLIDE 33
SLIDE 34
SLIDE 35
Some early Kepler results
SLIDE 36
SLIDE 37
SLIDE 38
SLIDE 39
SLIDE 40
SLIDE 41