[Redbook4:163-164][19871121:1310b]{Star
Cycles (III) [continued
(3)]
– The Main Sequence}[21st
November 1987]
19871121.1310
[continued]
I
have misunderstood Chartrand#** (p48): thinking that the labels
'early-type Stars' (O, B, A) and 'late-type Stars' (K, M) referred to
development of the individual Stars along a main-sequence lifetime.
In fact, the description of a typical life (on Chartrand p. 50-51)
makes much more sense (and I am sure that I had understood it
before):
[Text
of ms diagram above.]
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Gravity
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R[~]
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[+]C[I~]
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S[~]
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(Creating
Iron)
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{Closed
Groups}
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White
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White
Dwarf
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Yellow
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Red
Supergiant
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A
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Blue
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F
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B
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#*
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c.10
billion yrs life
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G
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The
Sun
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Early
type Stars***
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O
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A
few million years life
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Supernova?
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Weak
Nuclear Force*
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G[~]
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Orange
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K
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Late
type Stars****
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☼
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(Indigo)
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M[~]
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Strong
Nuclear Force**
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c.10,000
billion year life
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(H→He)
Nuclear
fusion
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M
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(R,N,S?)
<880111>
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Protostar
Nebula
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Red
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Interstellar
Cloud
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(Violet)
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↑
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Gravitat-ional
Attraction
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Black
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J[~]
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A[~]
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Dark
Cinder or
Neutron Star (Pulsar /Black Hole)
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U[~]
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Electro[-]
magnetic Force
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#
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#**
*Weak
Nuclear Force:
form
lightest element (H)
gets
rid of electric charge
so
E[lectro]M[agnetic]F[orce] does not prevent
creation
of Helium etc.
i.e.
Changes
electrically
charged protons
into
electrically neutral neutrons.
**Strong
Nuclear Force:
Creating
heavier elements (> iron)
(in
massive Stars at higher temperature
(Supernova)
(more protons per nucleus)
against
more powerful electric repulsion.
***Early
type Stars:
More
massive,
hotter,
larger,
brighter;
short-lived.
****Late
type Stars:
Less
massive,
cooler,
smaller,
duller;
longer-lived.
#Later
lives:
All become red giant; then:
F5
and cooler
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More
massive
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White
Dwarfs
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Red
Supergiants (some)
Explode
as Supernova
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\
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Dark
Cinders
|
Neutron
Star
(=
Pulsar/Black Hole)
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}(only
the most massive)
/
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#*cf.
S&C.20-2 [presumably
original full-length paper version]
<930506>
#*[Amateur
Astronomy Pocket Skyguide (Newnes)]
#**For
Star lives,
this circle is unconvincing; for Star types,
it is uninformative. <891018> {Try [Clockwise
circle from and to +CI~]?
– cf. VI.327.}
[continues]
[PostedBlogger06for08022017]
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