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Total Eclipse of the Sun Dr Steve Barrett 1 15 May 2008 Total Eclipse of the Sun 1 Dr Steve Barrett 15 May 2008 Total Eclipse of the Sun Total Eclipse of the Sun 2 Dr Steve Barrett 15 May 2008 Total Eclipse of the Sun Total Eclipse of the Sun 3 Introduction The Sun Core Surface Atmosphere Eclipses Total Eclipse of 29 Mar 2006 Why? When? Total Eclipse of the Sun 4 000,000,000,000 watts Power ~ 400,000,000,000,000 Solar Vital Statistics Size ~ 100 x Earth ~ 400 x Moon Mass ~ 1,000,000 x Earth Composition ~ 75% hydrogen 25% helium 0.1% other stuff Distance ~ 370 410 x Moon Total Eclipse of the Sun 5 Power Source 1871 Hermann von Helmholtz Burning coal, one ton per hour per square foot of the Suns surface, would exhaust the fuel in a few million years 1919 Sir Arthur Eddington Conversion of hydrogen to helium could provide enough energy to power the Sun for billions of years Total Eclipse of the Sun 6 Fusion hydrogen helium + energy
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Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

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Page 1: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 1 15 May 2008

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Dr Steve Barrett 15 May 2008

TotalEclipse ofthe Sun

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Dr Steve Barrett 15 May 2008

Total Eclipseof the Sun

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3 Introduction

The Sun CoreSurfaceAtmosphere

Eclipses

Total Eclipse of 29 Mar 2006

Why?When?

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000,000,000,000 wattsPower ~ 400,000,000,000,000

Solar Vital Statistics

Size ~ 100 x Earth ~ 400 x Moon

Mass ~ 1,000,000 x EarthComposition ~ 75% hydrogen

25% helium0.1% other stuff

Distance ~ 370 – 410 x Moon

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5 Power Source

1871 Hermann von HelmholtzBurning coal, one ton per hour persquare foot of the Sun’s surface, wouldexhaust the fuel in a few million years

1919 Sir Arthur EddingtonConversion of hydrogen to helium couldprovide enough energy to power the Sunfor billions of years

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6 Fusion

hydrogen → helium + energy

Page 2: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 2 15 May 2008

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7 Fusion

Mass loss → energy thanks to E = mc 2

600 Mt of H → 596 Mt of He

Sun loses 4 million tons every second

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8 Internal Structure

core

radiationzone

convectionzone

photosphere

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9 Helioseismology (or “Star Quakes” )

Convection zone turbulence can be detected throughthe Doppler shift of the photosphere’s emission lines To

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10 Solar Spectrum

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11 Sunspots

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12 Sunspots

Page 3: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 3 15 May 2008

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13 Sunspots

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14 Sunspot Cycle

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15 Sunspot Cycle

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16 Sunspot Cycle

50 years of very low sunspot activity coincidedwith the ‘Little Ice Age’ period of very cold winters

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17 Magnetic Loops

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18 Magnetic Loops

Page 4: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 4 15 May 2008

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19 Magnetic Polarity

SN

34 d

30 d

25 d

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20 Flares and Prominences

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21 Corona

Temperature of surface ~ 6,000 K

Temperature of corona ~ 2,000,000 K

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22 Corona

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23 Solar Wind

400 km/s Tota

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24 Aurora Borealis

Page 5: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 5 15 May 2008

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25 Aurora Borealis

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26 Eclipses

EclipseThe passage of one object into theshadow cast by another.Thus an Eclipse of the Sun should becalled an Eclipse of the Earth.

OccultationThe passage of one object in front ofanother, hiding the latter from view.

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27 Moon

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28 Eclipses

Total Eclipse ( long )

Total Eclipse ( short )

Annular Eclipse

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29 Transit of Venus 2004

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30 Eclipse Geometry

An eclipse cannot occur at every New Moonbecause the Moon’s orbit is tilted by ~ 5°.

Page 6: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 6 15 May 2008

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31 Eclipse Geometry

The Moon crosses the plane of the Earth’sorbit (the Ecliptic) at a node.

Ecliptic

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32 Eclipse Timing

Synodic MonthNew Moon to New Moon

Draconic MonthNode to Node

Anomalistic MonthPerigee to Perigee

29.53 days

27.21 days

27.55 days

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33 The Saros Cycle

223 Synodic months =

242 Draconic months =

239 Anomalistic months =

6585.32 days

6585.36 days

6585.54 days

Over this time, the saros cycle, the Moon’sorbital periods are back in ‘synch’.

Two eclipses separated by one saros cyclehave similar geometries. To

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34 Saros 139

Date ØM/ØS Length Seen from

1988 Mar 18 1.046 3m 46s Asia

2006 Mar 29 1.052 4m 07s Africa

2024 Apr 08 1.057 4m 28s Americas

2042 Apr 20 1.061 4m 51s Asia

2060 Apr 30 1.066 5m 15s Africa

2078 May 11 1.070 5m 40s Americas

2096 May 22 1.074 6m 06s Asia

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35 Eclipses Coming Soon

Date Saros Length Seen from

2006 Mar 29 139 4m 07s Africa, Turkey

2008 Aug 01 126 2m 27s Greenland, Siberia

2009 Jul 22 136 6m 39s India, China

2010 Jul 11 146 5m 20s S Pacific, S America

2012 Nov 13 133 4m 02s Australia, S Pacific

2013 Nov 03 143 1m 40s Africa

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36 Eclipses

Page 7: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 7 15 May 2008

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37 Eclipses

1715

1724

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38 Total Eclipse of 29 Mar 2006

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39 Total Eclipse of 29 Mar 2006

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40 Total Eclipse of 29 Mar 2006

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41 Total Eclipse of 29 Mar 2006

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42 Eclipse Cruise

Page 8: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 8 15 May 2008

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43 Libya

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44 Libya

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45 Eclipse Track

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46 Eclipse Site

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47 Eclipse Track

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48 Setting Up in the Desert

Page 9: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 9 15 May 2008

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49 The Eclipse Starts…

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50 Totality!

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51 Catching the Corona

1/4000 s

1/1000 s

1/250 s

1/60 s

1/15 s

1/4 s

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52 Total Eclipse of the Sun 2006

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53 Total Eclipse of the Sun 2006

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54 Total Eclipse of the Sun 2006

Page 10: Total Eclipse of the Sun - University of Liverpoolsdb/Talks/Eclipse-IoP-MB.pdfTotal Eclipse of the Sun Dr Steve Barrett 6 15 May 2008 n 31 Eclipse Geometry The Moon crosses the plane

Total Eclipse of the Sun

Dr Steve Barrett 10 15 May 2008

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55 Viewing Totality

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56 Viewing Totality

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57 Shadow Bands

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58 Green Flash

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59 An African Experience

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60 http://www.liv.ac.uk/~sdb/ Talks

Dr Steve Barrett 15 May 2008