Not
What's an exo-planet?
- Planets must orbit the Sun
- Planets must be large enough that their gravity forces their shape to be spherical
- Planets must clear their orbits of other material, so they are the largest body near their orbit
What's a planet?
Planets must orbit the Sun- Planets must be large enough that their gravity forces their shape to be spherical
- Planets must clear their orbits of other material, so they are the largest body near their orbit
Finding exoplanets
All we have to measure is light from a distant star.....so how can we find a planet that we can't see?
flux
spectra
position
wavefront
What can we measure from light?
Characteristics
-
Intensity ("flux")
-
photometry
- magnitudes
- transits
-
photometry
-
Wavelength ("color")
-
spectrum
- radial velocity
- composition
- incandescence
- emission
- absorption
-
spectrum
- Interference
- Polarization
- Timing
Transits
Transits rely on chance alignments
Radial Velocity
Radial velocity favors cooler stars.
Current visible-light RV instrument operate at the ≈ 10cm/s precision thanks to extreme wavelength stability and calibration.
Astrometry
Astrometry favors hotter stars and nearby stars.
Astrometric detection of exoplanets requires sub-μarcsecond position measurement. Equivalent to seeing 1mm on the moon.
Gravitational microlensing
Microlensing relies on chance alignments
Direct Imaging
The star to planet contrast varies from 1e7 (10 μm thermal IR) to 1e10 (visible light),
"The multiple observation techniques are scientifically complementary, and several approaches are required for characterization of exoplanets.
For example, direct imaging is key to measure the exoplanet’s atmospheric composition (spectroscopy), but does not measure exoplanet radius (measured by transit) or mass (measured by radial velocity or astrometry)."
TESS camera apertures
Kepler primary mirror
~ 100,000 stars over several years
TESS
Most stars aren' t single
~50% of the stars you see are binaries
~25% are triples
-on avg there's an exoplanet per star
~10% of Sun-like stars likely host rocky exoplanets, more for lower-mass stars
but atmospheric turbulence limit resolution to
The problem of the atmosphere
details = color ÷ telescope size
details = color ÷ atmosphere turbulence (~10cm)
Classifying
exoplanets
- Hot Jupiters
- lava planets
- rogue planets
- lethal rain
- devoured planets
- evaporating planets
- eccentric orbits
- ocean planets
- zombie planets
Tidally locked planets
Eyeball planets
Multiple-habitable worlds in a single system?
Circumbinary planets
Kepler-16
Super-Earth or mini-Neptune?
Garnet planets
Plate tectonics & magnetic fields - these are important for life
We know the compositions of the stars.....the same elements likely go into the planets that form
Atmospheres
&
Biosignatures?
Oxygen
- get transmission spectrum of the atmosphere
- measure different radii at different wavelegnths to give clues to composition
Giordano Bruno
(1548 – 1600)
Italian Friar
Oct 1995
links:
The Sun:
https://www.youtube.com/watch?v=6tmbeLTHC_0
black holes:
https://www.wikiwand.com/en/Black_hole
https://www.youtube.com/watch?v=4YzWosQYg6Q
https://www.youtube.com/watch?v=if2opecmev8
https://www.youtube.com/watch?v=wyuj7-XE8RE
https://www.youtube.com/watch?v=TF8THY5spmo
exoplanets:
https://exoplanets.nasa.gov/interactable/11/
https://en.wikipedia.org/wiki/List_of_exoplanet_extremes
https://www.quora.com/What-is-the-farthest-exoplanet
https://www.space.com/29120-alien-planet-among-farthest-known.html
https://www.nasa.gov/feature/jpl/20-intriguing-exoplanets
http://seagerexoplanets.mit.edu/research.htm
known universe/scales:
https://neal.fun/size-of-space/
https://www.youtube.com/watch?v=17jymDn0W6U&list=PLrfcruGtplwHQB7fGpuohlVkRDhPaJfJt
Scale of the Solar system: http://joshworth.com/dev/pixelspace/pixelspace_solarsystem.html
https://www.space.com/30610-scale-of-solar-system-amazing-video.html
https://www.youtube.com/watch?v=GoW8Tf7hTGA
Scale of the universe: http://htwins.net/scale2/
Sizes of stars: https://www.youtube.com/watch?v=kBkNhMfrxuk&feature=youtu.be
How many exoplanets have been found?
https://exoplanetarchive.ipac.caltech.edu/
Light
Solar system
-
Why does Saturn have rings? What are the rings?
Moons that are other worlds:
Stars
Stellar Evolution
<0.08
0.08-0.4
0.4-8
>8
>20
>3
1.4-3
>1.4
Solar Masses
Scales and galaxies
Oumuamua
Random
-
How does climate change affect NASA? (if the world is going to end, if climate change is such a big problem, wont that affect our study of other planets)
Why is the government underfunding NASA? Are there other ways for NASA to get money?
Was the moon landing fake?
- photos from LRO
- photos from the missions:
- equipment on the moon
- seismometers
- laser retroreflectors
- lunar samples
- broadcast tracking -inc Soviets
Exoplanets & how to find them
By Nic Scott
Exoplanets & how to find them
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