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EPIC211351816.01: The First Known Re-Inflated Planet(?)

skgrunblatt
September 05, 2016
16

EPIC211351816.01: The First Known Re-Inflated Planet(?)

Presented at Morning Tea at the University of Sydney, Sydney, Australia.

skgrunblatt

September 05, 2016
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  1. EPIC 211351816.01: THE FIRST RE-INFLATED PLANET(?) SAM GRUNBLATT, UNIVERSITY OF

    HAWAII DAN HUBER2, ERIC GAIDOS1, ERIC LOPEZ3, BJ FULTON1, ANDREW VANDERBURG4, TOM BARCLAY5, JONATHAN FORTNEY6, ANDREW HOWARD7, HOWARD ISAACSON8, ANDREW MANN9, ERIK PETIGURA7, VICTOR SILVA AGUIRRE10, EVAN SINUKOFF1 1. UNIVERSITY OF HAWAII, 2. UNIVERSITY OF SYDNEY, 3. UNIVERSITY OF EDINBURGH, 4. HARVARD UNIVERSITY, 5. NASA AMES, 6. UNIVERSITY OF CALIFORNIA, SANTA CRUZ, 7. CALIFORNIA INSTITUTE OF TECHNOLOGY, 8. UNIVERSITY OF CALIFORNIA, BERKELEY, 9. UNIVERSITY OF TEXAS, AUSTIN, 10. AARHUS UNIVERSITY Image credit: C. Carreau / ESA
  2. Inflated Hot Jupiters are ubiquitous. Lopez & Fortney (2016) maximum

    expected radius highly inflated not inflated
  3. The Mechanism of Planet Inflation eg. Batygin & Stevenson (2010)

    Wu & Lithwick (2013) Class I: planet inflated directly by increased stellar irradiation Class II: delayed cooling after planet formation
  4. How to distinguish between Classes I and II? Lopez &

    Fortney (2016) Class I Class II red giant host star
  5. K2: Extension to Kepler Mission - ~80 day observing campaigns

    - community chosen targets: Giants Orbiting Giants target stars observed in Campaigns 4, 5, 6, 7, 8, 10 (Huber 2015)
  6. Searching for Planets around Red Giant Stars with K2 D.

    Huber (2015) Planets K2 can detect
  7. Searches for Planets around Red Giant Stars with K2 D.

    Huber (2015) re-inflation regime
  8. Searches for Planets around Red Giant Stars with K2 D.

    Huber (2015) re-inflation regime EPIC 2113 Grunblatt et al., accepted (arXiv.org/abs/1606.05818)
  9. Gaussian process + transit fit individual transits phased lightcurve Grunblatt

    et al., submitted (arXiv:1606.05818) before GP fit
  10. Gaussian process + transit fit individual transits phased lightcurve after

    GP fit Grunblatt et al., submitted (arXiv:1606.05818)
  11. Asteroseismology Rs = 4.18 +/- 0.2 R⊙ Ms = 1.15

    +/- 0.15 M⊙ Rp = 1.29 +/- 0.11 RJ Grunblatt et al., submitted (arXiv:1606.05818)
  12. Planet mass determination: radial velocity measurements Mp = 1.10 +/-

    0.12 MJ Grunblatt et al., submitted (arXiv:1606.05818)
  13. Planet irradiation history average incident flux on main sequence: 170

    +140-60 F Grunblatt et al., submitted (arXiv:1606.05818)
  14. Planet irradiation history typical incident flux for ~1.3 RJ planets

    average incident flux on main sequence: 170 +140-60 F Grunblatt et al., submitted (arXiv:1606.05818)
  15. Result suggests re-inflation! Inconsistent with no external heating after formation

    Class II ] Class I Evidence for ~0.2% heating efficiency Grunblatt et al., submitted (arXiv:1606.05818)
  16. Energetic outlier on the MS! Currently typical of inflated planets

    Grunblatt et al., submitted (arXiv:1606.05818)
  17. Energetic outlier on the MS! Currently typical of inflated planets

    Grunblatt et al., submitted (arXiv:1606.05818) but an outlier assuming MS flux.
  18. Summary The first planet found orbiting an oscillating star with

    K2: 1.3 RJ, 1.1 MJ, 8.4 day period Suggests planet inflation during RGB phase: irradiation on main sequence could not inflate planet to current size. EPIC 211351816.01: The First Re-Inflated* Planet *probably. Grunblatt et al., submitted (arXiv:1606.05818)
  19. Future Work: Red Giant Planet Occurrence EPIC 2113 ? ?

    ? ? ? ? Expected yield: 20 +/- 10 planets.