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How Eclipses Occur, and the 2017 Great American Solar Eclipse
Dr. Bill Blair JHU Quarknet Presentation July 25, 2017 (with thanks to the STScI Office of Public Outreach for some of the graphics)
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Eclipses through History...
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Moon Phases and Orbit NOAO
Credit: T.A.Rector, I.P.Dell'Antonio, NOAO/AURA/NSF NOAO
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SUN Synodic Month = days
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Lunar Phases and Geometry
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Lunar Eclipse Sun Earth Moon
Approx. Relative Size of Earth and Moon: Moon fits in earth’s shadow with room to spare!
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Lunar eclipse – visible from anywhere on the night-side of earth
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Lunar Eclipse Time Series
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Penumbra Umbra
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Why is the moon red in Lunar Eclipse?
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Solar Eclipse Sun Earth Moon
Angular Size of Sun and Moon are nearly the same! (Only a small portion of the sunlit side of earth can see, however.)
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...but of course not to scale!
This is the geometry... What else is wrong with this picture? ...but of course not to scale!
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Earth’s diameter (8000 miles) is about
Earth’s diameter (8000 miles) is about 4 times the Moon’s diameter (2200 miles)
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The Moon is located about 240,000 miles (30 Earth diameters) away.
(Now think about the shadows needed to cause eclipses!) (Yardstick demo)
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(sun)
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Why Not Eclipses Every Month?
Eclipse Ingredients Moon Phase Full moon (lunar) or new moon (solar) Orbital plane alignment Moon crossing Earth-Sun plane Earth-Moon Distance (apogee, perigee, or inbetween) Affects apparent (angular) size of moon
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Moon’s orbital plane is tipped ~5o to Earth’s
Need full or new moon to occur along the intersection of the orbit planes for eclipses!
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Otherwise the shadows miss their targets!
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Moon’s orbit is slightly elliptical, so its angular size changes during its orbit.
a > b a b
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Anthony Ayiomamitis
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Annular Eclipse (February 2017)
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Annular Solar Eclipse Views
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Solar Eclipse Phenomenology
NASA
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Partial eclipse showing large sunspot group
Partial phases last about 3 hours total. (Totality is in the middle of this time if you are on the center line.)
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Partial eclipse showing large sunspot group
Earth to scale
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Diamond Ring Effect
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“Baily’s Beads” (Sunlight passing through lunar valleys on the moon’s limb) Pierre Arpin
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Baily’s Beads Time Series
Richard Nugent
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Total Eclipse showing solar corona
Klaus Kemmerich
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Coronal structure depends on solar activity level
HAO / NCAR
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Solar Chromosphere and Prominences
Luc Viatour
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A Realistic Naked Eye View...
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Solar Eclipse Viewed from Space
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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March 9 2016 Pacific Solar eclipse captured by DISCOVR [Deep Space Climate Observatory] (NASA)
DSCOVR / NASA
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August 21, 2017 – Where Will You Be?
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Total Solar Eclipse – August 21, 2017
Greatest eclipse at 18:25 UT Duration 2 min 40 sec Totality path is 71 miles wide Partial eclipse across North America
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Eclipse calculator by city: fractional coverage and timing:
Observing the Eclipse Eclipse calculator by city: fractional coverage and timing:
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Eclipse calculator by city: fractional coverage and timing:
Observing the Eclipse Eclipse calculator by city: fractional coverage and timing:
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Safety First Looking directly at the Sun is unsafe! Only one exception
Use certified solar filters, or eclipse glasses SUNGLASSES ARE NOT ENOUGH! Only one exception Can look directly at Sun during total eclipse Don’t look directly at Sun during partial eclipse!
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Indirect Viewing (Partial phases)
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For pinhole cameras, the image is inverted.
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Use what you have available to create your own pinhole cameras….
Lucia Garcia
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The Eclipse of 1919 and General Relativity
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General Relativity 1915 – Einstein: “mass warps space”
Light that passes near the Sun will bend Background star positions should shift slightly due to the mass of the sun
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(Effect is greatly exaggerated in this example!)
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Background stars could not be seen or measured until the sun was blocked!
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General Relativity Tested
1915 – Einstein “mass warps space” Light that passes near the Sun will bend 1919 – Expeditions to measure star positions during total solar eclipse and compare to earlier pictures of the field. Result: Deviations matched predictions General Relativity passed eclipse test!
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Gravitational lens example as observed with Hubble
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August eclipse planets and stars
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Questions?
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