Exoplanets for the Masses: Crowdsourcing the Search for New Worlds
1. Exoplanets for the Masses:
Crowdsourcing the Search
for New Worlds
Dr. Joshua Schlieder
NASA Goddard Space Flight Center
CSW2018 - Oct. 27, 2018 joshua.e.schlieder@nasa.gov
2.
3. (Sizes to scale - Separations NOT to scale)
Asteroids
What about planets around other stars?
4. Why Study Exoplanets?
1. Planet Formation
- From gas and dust to planets —> how?
2. Planet Demographics
- Are there diverse planets orbiting the diversity of stars?
3. Habitability
- How common are planets that can potentially support life?
5. Finding Exoplanets - The Transit Method
Monitor the brightness of a star while a planet
crosses in front and measure a characteristic drop
https://svs.gsfc.nasa.gov/
6. Kepler and K2 -
Measuring Transits
From Space
NASA
Kepler measured the brightness
of about 150,000 stars, every
30 minutes, over 4 years
Kepler discovered more than
2,500 exoplanets and taught us
something fundamental about the
Universe – Planets are common
and most stars host them!
7. A Sad Day for Exoplaneteers
May 2013 – hardware failures lead to
the loss of Kepler pointing control
Kepler becomes K2 and
continues discovering
exoplanets – more than 300 as
of September 2018!
8. Kepler and K2 – A Wealth of Data
The data from Kepler/K2 is represented as a light curve
Time (days)
Brightness
Brightness
Brightness
Petigura et al. 2016
9. Kepler and K2 – A Wealth of Data
Kepler and K2 have provided a very large number of light curves
Kepler light curves - >150,000
K2 light curves - >500,000 and counting
The large data set and nature of the
light curves make Kepler/K2 prime
for crowdsourced citizen science!
10. Exoplanet Citizen Science Projects
hosted on the Zooniverse citizen science platform
(www.zooniverse.org)
www.planethunters.org www.exoplanetexplorers.org
14. Planet Hunters - www.planethunters.org
What have Planet Hunters citizen scientists discovered?
A planet in a quadruple
star system
“The most mysterious star
in the Galaxy”
Schwamb et al. 2013, Haven Giguere/Yale; Boyajian et al. 2016, NASA/JPL
19. What’s next for Exoplanet Citizen Science?
Transiting Exoplanet Survey Satellite
TESS
An MIT led NASA Astrophysics Mission
launched in April 2018
20. Transiting Exoplanet Survey Satellite
TESS
-Four telescopes
-High precision brightness
measurements of the closest stars
-All-sky survey over 2 years
-Designed to detect transiting planets in the
Solar Neighborhood
21. TESS - four small telescopes
working together
24o
96o
22. TESS’s First Planet Candidate
Huang et al. 2018, Gandolfi et al. 2018
By the end of its mission, TESS
will provide light curves for
>20,000,000(!) stars
Citizen scientists will be needed and
astronomers are getting ready with new
crowdsourcing platforms – stay tuned!
23. Exoplanet Citizen Science
-Kepler /K2 provided data for exoplanet discovery via
crowdsourcing
-Citizen scientists used Planet Hunters and
Exoplanet Explorers to make high impact discoveries
-TESS will provide tens of millions of light curves
for crowdsourced citizen science
26. Kepler - What did we learn?
A planetary censusPlanets are
COMMON and
most stars
host at least one
Super-Earths and
Sub-Neptunes are
the most
frequent planets
NASA, Petigura+2013
Earth size planets
in habitable zones?
Some detected, but
very hard!
27. The road to launch
Observatory fully integrated and tested
28. The road to launch
Complete TESS space craft sent to Kennedy Space
Center to undergo final preparation for launch
Micron sized dust grains grow 13 orders of magnitude in size and 40 orders of magnitude in mass in millions of years
Introduce Light curves, Show examples, Describe that there is more to be found – large data volume, biases in planet detection algorithms, prime for crowd sourcing
Introduce Light curves, Show examples, Describe that there is more to be found – large data volume, biases in planet detection algorithms, prime for crowd sourcing
Star Gazing Live
Chris Lintott, Brian Cox, Julia Zemiro
TESS - 200,000 bright targets @2 min cadence, Full Frame Images - 20,000,000 stars @30 min cadence
JWST - transmission spectroscopy from 1 - 11 microns using NIRISS, 2 NIRCam grism settings, and MIRI - emission spectroscopy also an option
TESS - 200,000 bright targets @2 min cadence, Full Frame Images - 20,000,000 stars @30 min cadence
Known planet is on a 2000 day orbit and is ~10 Jupiter masses.