the effects of birth environment on planetary...

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The effects of birth environment on planetary systems Melvyn B. Davies Department of Astronomy and Theoretical Physics Lund Observatory www.astro.lu.se

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Page 1: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

The effects of birth environment

on planetary systems

Melvyn B. DaviesDepartment of Astronomy and Theoretical Physics

Lund Observatory

www.astro.lu.se

Page 2: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

Five things to remember about

exoplanetary systems

Melvyn B. DaviesDepartment of Astronomy and Theoretical Physics

Lund Observatory

www.astro.lu.se

Page 3: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

1) The Solar System

2) Lovis et al. (2010) list of multiple systems

3) Kepler systems

Lissauer et al. 2011; Tremaine & Dong 2012; Johansen et al. 2012; Fang & Margot 2012

There are many flat and/or low eccentricity planetary systems

Page 4: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

Making everything from 3p systems

0 5 10 15 20 25 301t3p/3t3p

0

2

4

6

8

10

2t3p

/3t3

p

2.0 3.0

4.0 5.0

6.0 7.0

8.0 9.0

0.0

10.0

Kepler

Increasinginclinationspread

Kepler seesmore 1t than come from 3p

(Johansen, Davies, Church & Holmelin 2012)

Page 5: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

1) The Solar System

2) Lovis et al. (2010) list of multiple systems

3) Kepler systems

Lissauer et al. 2011; Tremaine & Dong 2012; Johansen et al. 2012; Fang & Margot 2012

There are many flat and/or low eccentricity planetary systems

But some exoplanets are also observed on eccentric orbits... are they de-stabilised by encounters?

Page 6: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

Encounters within birth environments happen interestingly often

Timescale for a given star to undergo an encounter is

τenc ' 3.3⇥107yr✓100 pc�3

n

◆✓V∞

1 km/s

◆✓103AURmin

◆✓M�Mt

Beware of the average: lumpiness can make a difference.

(e.g. Malmberg et al. 2007; Davies et al. 2014)

Page 7: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

Close fly-by Binary earlier Binary today

WS-10 ~0.10 ~0.05 ~0.03CL-10 ~0.15 ~0.20 ~0.15WS-all ~0.20 ~0.20 ~0.03CL-all ~0.20 ~0.50 ~0.10

In other words: fly-bys and exchanges into binary systems can happen interestingly often.

Fraction of solar-like stars suffering encounters

(Church, Davies & Bonnerot, in prep.)

Page 8: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

Encounters can mess up planetary systems

Page 9: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

The four gas giants 108 years after fly-by (rMin < 100 AU)

(Malmberg, Davies & Heggie 2011; see also Scharf & Menou 2009; Veras, Crepp & Ford 2009)

Page 10: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

The four gas giants in a binary

(Malmberg, Davies & Chambers 2007;Malmberg & Davies 2009)

Page 11: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

In Kepler zone many planetary systems are multiple but most hot Jupiters are single

Page 12: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

(Mustill, Davies & Johansen 2015)

Page 13: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

3p+J=np or J3p+np=p?

Injecting planets in from further out can mess up inner system

(Mustill, Davies & Johansen 2015;Mustill, Davies & Johansen in prep.)

Page 14: The effects of birth environment on planetary systemsinterferometer.osupytheas.fr/colloques/OHP2015/slides/Melvyn_Davi… · 1 km/s 103 AU R min ... WS-10 ~0.10 ~0.05 ~0.03 CL-10

1. Planetary systems are often flat

2. Encounters happen in birth environments

3. Encounters mess up planetary systems

4. Kepler sees multiple p, single J, or single p

5. 3p+J or 3p+np may make what we see

Summary