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A Transi)ng Circumbinary Planet in a Quadruple Star System Meg Schwamb (Yale University) [email protected] Image Credit: Haven Giguere

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A  Transi)ng  Circumbinary  Planet  in  a  Quadruple  Star  System  

Meg  Schwamb  (Yale  University)    [email protected]  

Image  Credit:  Haven  Giguere  

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Discovery  and  Confirma)on  of  PH1:  A  Circumbinary  Planet  in  a  Four  Star  System  

 •  Planet  spoDed  by  ciEzen  scienEsts  

reviewing  Kepler  light  curves  on  the  Planet  Hunters  (planethunters.org)  website  

 •   Combining  the  Kepler  light  curve  +  

measured  radial  velociEes,  we  have  confirmed  the  planet  and  the  properEes  of  its  host  stars    

•  First  planet  discovered  in  a  four  star  system  

 

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Transits  spoBed  in  Kepler  light  curve  of  eclipsing  binary  KIC  4862625  

Primary Eclipse

Secondary Eclipse

Planet Transit

Primary Eclipse

Secondary Eclipse Secondary Eclipse

Planet Transit

Quarter 2 Quarter 4

Days from Start of Quarter 1 Days from Start of Quarter 1

Robert  Gagliano     Kian  Jek  

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Schwamb  et  al.  (ApJ  submiDed)  

Circumbinary  planet,  orbi)ng  both  stars  in  binary  star  system  

 

Time (BJD-2455000)

Nor

mal

ized

Flu

x x1

000

Nor

mal

ized

Flu

x x1

000

Q2 Q4 Q5 Q7

Q8 Q11Q10

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Keck  HIRES  Radial  Veloci)es    

Schwamb  et  al.  (ApJ  submiDed)  

Phase (P =20.000251025, T!=54967.8195)

Radi

al V

eloc

ity (k

m s"

#)

Binary  has  20  day  orbital  period  

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Adap)ve  Op)cs  Keck  Observa)ons  N

E

0.5"Schwamb  et  al.  (ApJ  submiDed)  

Column Column

Row

0.7’’ Contaminator KIC 4862625

Column Column

Row

0.07’’ Contaminator KIC 4862625

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•  PH1  is  a  6.18  ±  0.17    Earth  radii  planet  orbits  its  parent  stars  every  138.3  days  (semimajor  axis  =0.65  AU)  

 

•  PH1  is  <  0.53  Jupiter  masses    

•  The  parent  eclipsing  stars  are  1.7  &  0.4  Solar  radii  (1.5  &  0.41  Solar  masses)    

 

•  The  second  pair  of  stars  at  ~1000  AU  is  bound  to  the  planetary  system  

 

•  We  esEmate  an  age  of  ~2  Gyr  for  the  system  

Planet  Hunters’  First  Confirmed  Planet  

Image  Credit:  Haven  Giguere/Yale    

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PH1

To

Ea

rth

Aa

Ab

b

0.5 AU

Aa

Ab b

Kepler−47

To

Ea

rth

A

B

b

c

0.5 AU

AB

b

c

0.5 AU0.5 AU 0.5 AUKepler-16Kepler-35Kepler-34

Kepler-38

b

A

B

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This  work  is  supported  by  the  NSF  Astronomy  &    Astrophysics  Postdoctoral  Fellowship  program  and  NASA  

PresentaEon  slides,  images  &  paper  preprint:      

hBp://www.planethunters.org/dpspress2012    

Username:  planet            Password:  hunters  

[email protected]