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A New Method to Validate Planets and the Discovery of Kepler-10c Francois Fressin Harvard-Smithsonian Center for Astrophysics [email protected]
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A New Method to Validate Planets a nd the Discovery of Kepler-10c

Mar 23, 2016

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A New Method to Validate Planets a nd the Discovery of Kepler-10c. Francois Fressin Harvard -Smithsonian Center for Astrophysics [email protected]. Kepler’s First Rocky Planet: Kepler-10b. Another signal in the data. - PowerPoint PPT Presentation
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Page 1: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

A New Method to Validate Planets and the Discovery of

Kepler-10c

Francois Fressin Harvard-Smithsonian Center for Astrophysics

[email protected]

Page 2: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Kepler’s First Rocky Planet: Kepler-10b

Page 3: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Another signal in the data

• There was a longer period signal, that could not be confirmed as a planet by the Doppler method.

• New technique to validate the discovery

Page 4: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Period = 45.29 days

• There was a longer period signal, that could not be confirmed as a planet by the Doppler method.

• New technique to validate the discovery

Kepler-10c

Page 5: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Planet or Blend?An observed periodic transit signal could be due to:

Blender is a light-curve fitting software• It attempts to explain Kepler candidates assuming they

are the result of two background eclipsing stars.

Transiting Planet Eclipsing Binary Stars

Page 6: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

PleiadesNASA’s fastest supercomputer

Page 7: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Validating Transiting PlanetsA large range of Eclipsing Binary Stars could mimic the transit.

Blender results show that only a very small fraction can actually reproduce the exact transit shape

Page 8: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Warm Spitzer ObservationsIf the system is a planet, transit depth is independent of the

color of light observed

In visible light

In Infrared

Page 9: A New Method  to  Validate Planets a nd the  Discovery  of  Kepler-10c

Validation of Kepler-10cThere is only 1 in 60,000 chance it’s not a planet

Period = 45.3 days2.23 Earth Radii< 20 Earth Masses

This technique will be used to validate planets that cannot otherwise be confirmed, like rocky planets in the

habitable zone. 9