gijs mulders, ilaria pascucci, daniel apai university of arizona an increase in planet formation...
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Gijs Mulders, Ilaria Pascucci, Daniel ApaiUniversity of Arizona
An Increase in Planet Formation Efficiency around Low-Mass Stars
EOS (PI: Daniel Apai)
a NASA NexSS program
Planet Formation Efficiency
Mul
ders
et a
l. 20
15b.
Dis
k m
ass:
And
rew
s et
al.
2013
Low-Mass Stars have more planets?
How
ard
et a
l. 20
12
Johnson et al. 2007
Stellar Mass vs. Effective Temperature
Hub
er e
t al.
2014
, Dre
ssin
g &
Cha
rbon
neau
201
3
K2: talk by Ian Crossfield
Planet Candidates: Q1-Q16
KOIs from
Mullally et al. 2014
3. Detection efficiency
(Chr
istian
sen
et a
l. 20
15)
Transit Probability
Detection efficiency
(S/N)
Planet Occurrence
Mul
ders
et a
l. 20
15a,
b
Planet Radius
Distribution
Planet Period
Distribution
Planet Period Distribution (Q1-Q8)See Mulders et al. 2015a for details
Mul
ders
et a
l. 20
15a
Planet Radius Distribution (Q1-Q16)
Mul
ders
et a
l. 20
15b
Planet Radius Distribution (Q1-Q16)
Mul
ders
et a
l. 20
15b
Planet Radius Distribution (Q1-Q16)
Mul
ders
et a
l. 20
15b
4x
2x
Estimating Planet Heavy Element Mass
Wei
ss &
Mar
cy 2
014
Heavy element mass from Miller & Fortney 2011
Heavy Elements Mass in Planets P<50 days
Mul
ders
et a
l. 20
15b
Heavy Elements <150 days
Mul
ders
et a
l. 20
15b.
Dis
k m
ass:
And
rew
s et
al.
2013
More Efficient Migration of Disk Material?
?
The Planet Population around Low-Mass Stars from Kepler Prime
• Contains more small planets (<3 R_earth)• Contains fewer giant planets• Contains more heavy-metals• Extends closer in to their host stars
Indicates solid migration is the dominant factor in planet formation
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