variations in 94 aqr with tess metcalfe.pdfk3v g8iv 85% 9% 6% t. reinhold / r. egeland....

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Deciphering Rotation and Activity Deciphering Rotation and Activity Variations in 94 Aqr with TESS Variations in 94 Aqr with TESS Travis Metcalfe Travis Metcalfe Space Science Institute Space Science Institute @palebluedotguy @palebluedotguy +TESS Asteroseismic +TESS Asteroseismic Science Consortium Science Consortium Working Group 2 Working Group 2

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Page 1: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Deciphering Rotation and ActivityDeciphering Rotation and ActivityVariations in 94 Aqr with TESS Variations in 94 Aqr with TESS

Travis MetcalfeTravis MetcalfeSpace Science InstituteSpace Science Institute@palebluedotguy@palebluedotguy

+TESS Asteroseismic +TESS Asteroseismic Science ConsortiumScience Consortium

Working Group 2Working Group 2

Page 2: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Spin-down stalls near middle-age

van Saders+ (2016, Nature)

standard spin-down

stalledbraking

Page 3: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Activity cycle grows longer and weaker

Metcalfe & van Saders (2017)

(4 Gyr)

(5.5 Gyr)

(7 Gyr)

Page 4: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

BAa

Ab0.2”0.2”

13” K2V

K3V

G8IV9%85%

6%

Page 5: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

BAa

Ab0.2”0.2”

13” K2V

K3V

G8IV9%85%

6%

T. Reinhold / R. Egeland

Page 6: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

BAa

Ab0.2”0.2”

13” K2V

K3V

G8IV9%85%

6%

T. Reinhold / R. Egeland

Page 7: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Asteroseismic properties from TESS

R = 2.06 ± 0.05 Rsun

M = 1.22 ± 0.02 Msun

Age = 6.2 ± 0.4 Gyr

⬆ D. Buzasi M. Lund / R. Handberg ⬇

⬇ D. Huber / P. Gaulme + S. Basu ⬆

Prot

~ 44 days

Page 8: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Asteroseismic properties are accurate

Spectral Energy Distribution →

Binary Orbit (astrom.+ RVs) →

Gyrochronology of 94 Aqr B →

K. Stassun T. Appourchaux

R = 2.05 ± 0.04 Rsun

M = 1.24 ± 0.08 Msun

Age = 6.3 ± 0.6 Gyr

Page 9: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Rotation modeling requires stalled braking

• Given stellar properties of subgiant, predict current rotation period (47 ± 4 d)

• Stalled magnetic braking beyond stellar middle-age yields: P

rot= 48 ± 4 days

• Standard spin-down for complete main-sequence yields: P

rot= 78 ± 7 days

J. van Saders

Page 10: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Subgiant has a “born-again dynamo”

• Subgiant mass suggests that it was an F-type star on the main-sequence

• After losing any original cycle, rotation slowed as it expanded and cooled

• Convection zone became deeper, longer timescale reinvigorated the dynamo

Page 11: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

Subgiant has a “born-again dynamo”

• Subgiant mass suggests that it was an F-type star on the main-sequence

• After losing any original cycle, rotation slowed as it expanded and cooled

• Convection zone became deeper, longer timescale reinvigorated the dynamo

critical value

no dynamo action

dynamo action

Page 12: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

• Rotation and cycle periods from Mount Wilson data can be attributed to the subgiant based on amplitude

• Asteroseismic properties from TESS are consistent with SED (radius), binary orbit (mass), and gyro (age)

• Evolution models only reproduce rotation period with stalled magnetic braking – standard spin-down fails

• After stalled braking and cycle shutdown on the main sequence, subgiant exhibits a “born-again dynamo”

Summary of conclusions

Page 13: Variations in 94 Aqr with TESS Metcalfe.pdfK3V G8IV 85% 9% 6% T. Reinhold / R. Egeland. Asteroseismic properties from TESS R = 2.06 ± 0.05 R sun M = 1.22 ± 0.02 M sun Age = 6.2 ±

tess.adoptastar.org