stellar activity in the kepler era tom ayres (casa)

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Stellar Activity in the Kepler Era Tom Ayres (CASA)

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Stellar Activity in the Kepler Era Tom Ayres (CASA). Talk deals with lower rungs of Drake’s Ladder, where, sadly, sexiness is low, but on positive side, knowledge content is high Note that main focus of Kepler mission is much higher on ladder!. Activity XXXXXXXXX. Outline. - PowerPoint PPT Presentation

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Page 1: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Stellar Activity in the Kepler Era

Tom Ayres (CASA)

Page 2: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Talk deals with lower rungs of

Drake’s Ladder, where, sadly,

sexiness is low, but on positive side, knowledge content is high

Note that main focus of Kepler mission is much

higher on ladder!

Activity

XXXXXXXXX

Page 3: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Outline• What is “Activity?” (Sun-like stars)• Stellar Cycles & Irradiances• Spots & Rotation (A.Brown: Fri;

Meibom: Tues; Garcia: Fri; Soderblom: Wed [flares])

• Seismology (T.Brown: Thur [LCOGT])

Guiding question:Is Sun ‘normal’ in cosmic scheme of

things?

Page 4: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Solar Activity

Solar minimum at left; maximum at right; dramatic changes in sunspot counts over 11 yr cycle

Page 5: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Sunspots are regions of multi-kilogauss magnetic fields

Page 6: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Sunspot numbers vary (erratically) over 11-yr period, with polarity reversals over 22-yr Hale cycle, and migrate from high latitudes to low (“butterfly diagram”)

Page 7: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Surface magnetic activity strongly influences solar outer atmosphere,

including 1 MK corona

Page 8: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Fe XII 195 (1 MK) coronal emission persists at spot minimum (left ; max at right). ‘Fuzzy ball ’ devolves from magnetic carpet: small clumps

of flux built by local dynamo, independent of deep seated el jefe dynamo responsible for

sunspots and their decadal cycling: lack of spots doesn’t mean lack of activity

Page 9: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Activity H-R Diagram Activity appears

confined to ‘cool stars’, in

convective half of H-R diagram

Not coincidence! Originally thought to signal lack of acoustic energy,

but dynamo needs convection

too(and rotation)

Page 10: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Stellar Activity Cycles

Long term Ca II emissions of nearby field star closely mimic Sun’s cycle. Visible brightness changes of Sun

only few milli-mags, in positive correlation with sunspots (Radick, Lockwood, Skiff, & Baliunas 1998)

Page 11: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

More examples (from SSS: Hall et al. 2008)

Page 12: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Most late-type stars of near-solar color show long term variations in Ca II

emission, many cyclic. Others, typically low RHK and often subgiants, are ‘flat activity’ (Radick et al. 1998)

Page 13: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Solar variations on long (and short)

timescales fall close to stars of similar activity (Radick et al. ’98; Lockwood et al. 2007)

Page 14: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Case Study: Alpha Cen AB Alpha Centauri triple system. Two solar-like stars about 20 au apart (Sun-Uranus); dim red dwarf 10,000 au away

Slightly metal rich compared with Sun, slightly older by ~1 Gyr. G2V primary

(“A”) is near twin of our own star

Page 15: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

In 2005, XMM reported complete disappearance of Alpha Cen A corona. Since

‘00 Alpha Cen orbital separation closing rapidly: no longer easily resolvable by

XMM, still trivial for Chandra. HRC campaign (since Oct ‘05) captures both

stars.

Page 16: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)
Page 17: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Rotation-Age-Activity Connection

’Skumanich laws’ confirm importance of dynamo, creating high levels of activity in

fast rotating stars, but also root of magnetic braking, which ultimately

quenches activity.

Page 18: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Week in life of Sun as seen by

SDO/HMI. Sunspot passages create dimmings

in visible light curves, but

surrounding plage regions cause

overall increase in irradiance.

Page 19: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Kepler can measure rotation

periods, diff rotation, and photometric

changes associated with

starspot evolution…trick is to disentangle

latter two effects.

Page 20: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Evolution of sunspot fields often accompanied by significant super-rotational motions

Page 21: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Starspot modeling for two Kepler objects

Page 22: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Key issue in contemporary solar physics: “flux emergence”…will be tricky for Kepler to make any progress in this area.

Page 23: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

What about seismology?

Here are 1-min measurements from Virgo instrument on SOHO (vs. ~50 mmag changes seen in spotted stars).

Page 24: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Asteroseismology Impact

• Mode frequencies sensitive to magnetic structure: cycle induced frequency shifts? (Garcia et al. 2010, Science, CoRot)

• Rotation/differential rotation from mode splittings (Karnoff et al. 2009, MNRAS)

• Convection zone depth (ibid); age (Mathur)

• Highly demanding on precision of acoustic frequencies; requires bright stars; Sun in the “sour spot”

Page 25: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

GONG Solar torsional

oscillations; equatorial

branch originates several yrs

before appearance

of first sunspots of new cycle; Cycle 25??

Page 26: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Measurements of large scale

coronal topology using

green line (forbidden

iron); “rush to the poles”

seen in previous

cycles is late or absent.

Page 27: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Left: Mean field strength of sunspots, and temperature

contrast, declining: all this together suggests approaching Maunder

minimum? Right: solar oxygen in trouble too

Page 28: Stellar Activity in  the Kepler Era Tom Ayres  (CASA)

Conclusions Kepler will make fundamental

contributions to the understanding of stellar activity by exploiting two complementary aspects of the

precision photometry: spot modulations (surface activity, rotation

& diff rotation, flares) and asteroseismology (rotation, diff

rotation [?], internal structure, age, cycles). A third possibility –

correlations of luminosity with spottedness – will be possible if absolute accuracy is achieved.