Chapter 5 - The World of Atoms
The classification of the stars
Personal
REU Report, Nicholas Reshetnikov
Archival Publication,Reshetnikov et al
I. Stellar Classifications
The puzzle
Twinkle?
Early Hindu model of the Universe
Hipparchus
Ptolemy's Almagest
The Library
of Alexandria
Hypatia
Measurement of Kirchhoff & Bunsen
August Comte on stellar composition
Fr. Angelo Secchi
The Vatican observatory
The grand fact
Hipparchus to Secchi
Stellar classifications
The atmospheric windows
The cast of characters
The heros
Interesting fact
Matthew
Brady's Civil War photos
Long exposure astronomical photography
Caroline
Herschel
John Herschel
Annie Russell Maunder
E. C. Pickering
Henrietta
Swan Leavitt
Harlow Shapley
Picture - p.124
Edwin Hubble
Walter Baade
The solution
Spectra of the star types
Hydrogen Grotrian diagram
Inert gas
structure
Sodium Grotrian diagram
The Ladies of Observatory Hill
Harvard group photo
Annie Cannon & Cecilia Payne
Temperature range
Fermi-Dirac population distribution
Balmer line absorption
Ca+ Grotrian
diagram
Fraunhofer line absorption
Intra shell dominates from f-sum rule
Studies of Hydrogen and the H-K lines
Relationship to temperature
Cosmic abundances
Hertzsprung-Russell diagram
Characteristic regions
Mass relationship
Path of stellar evolution
Eddington and Russell
Sir Arthur Eddington
Thumbnail sketch
Anecdotes
Russell's story
The
truth
Henry Norris Russell & Lyman Spitzer
Lyman
Spitzer
Iron?
Bias and Censorship
Galileo
James Hansen
On the other side
Crichton
Provenance
Textbook summary
II. The Solar Corona
The nature and history of the corona
Eclipse photo
Per chance the same solid angle just now?
Solar corona before 1930: the "element"coronium
New elements on the sun?
Helium
Viewed from the Lagrange point
UV
CDS on SOHO
Highly ionized atoms
Coronium and Edlén
Grotrian
Creating an artificial eclipse
Lyot solar camera
Coronagraph spectrum
Bengt Edlén
Bengt Edlén and King Gustaf VI Adolf,
1951
Why Edlén abandoned his thesis work
Green earth?
Gröna jorden?
Ground configuration fine structures
Ground configurations
Fine structures
M1 transitions
Ground state fine structures
Hydrogenlike splitting
Screening parametrization
Isoelectronic sequence
M1 decay rates
Identified lines
Consequences
Temperature broadening
Solar temperatures
Why is the Corona
so hot?
Highly ionized lab spectra
HZE particles in space
Semiempirical studies of atomic structure
U 90+
Textbook summary
III. Nebulium
Nebulium and the O III ground configuration
Chapter 6
Black holes
John Michell's prediction of the black hole
Laplace's prediction of the black hole
When was the Big Bang?
Ultimate limits: the Planck Length
General Relativity
The Triplets of Belleville
continued
Various answers
Geometry
Wente torii
E = mc2 proven?
Misleading article
The black swan
problem
Self-consistent fields for complex atoms
Superimpose dwell time patterns in a complex
atom
Compare QM with classical