Monthly Archives: May 2025

From Kepler to Ptolemy 16

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Kepler

Kepler wrote five major astronomical works. Chronologically:

the Mysterium cosmographicum (1596)

the Astronomia nova (1609)

the Epitome astronomiae Copernicanae (1618–1622)

the Harmonice mundi (1619)

and the Tabulae Rudolphinae (1627).

The Mysterium cosmographicum (Cosmographical Mystery) expresses Kepler’s youthful enthusiasm and sounds the leading notes to themes that would persist throughout his career. Kepler’s elliptical orbits and the area speed law make their debut in the Astronomia nova (New Astronomy). (Although at this point Kepler regarded the area law as just an approximation to the inverse speed law.) The Epitome astronomiae Copernicanae (Epitome of Copernican Astronomy) completes and refines his theory. The Harmonice mundi (Harmonies of the World) contains the statement of Kepler’s 3rd law, its main scientific claim to fame. The Tabulae Rudolphinae (Rudolphine Tables) ultimately led to the widespread acceptance of Keplerian astronomy.

He also wrote several lesser astronomical works, and treatises on optics, on computing volumes, on the philosophy of science, a pamplet on snowflakes… The critical edition of his collected works runs to 22 volumes. I will focus just on the Mysterium cosmographicum and the Astronomia nova.

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Set Theory Jottings 9. Cantor Normal Form

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Suppose β>1, and let ζ>0 be arbitrary. Then ζ has a unique representation in so-called Cantor normal form:

ζ α1 χ1+···+βαk χk
α1>···>αk, 1≤χi<β for all i
(1)

Stillwell gives an illustration, close to a proof, in §2.6 (pp.46–47)1, for the most important special case: β=ω and ζ<ε0. (The Cantor normal form for ε0 is just ωε0, not helpful.)

Here’s a more formal proof of the full theorem. First generalize division to all ordinals. If β>1, then any ζ has a unique representation in the form

ζ= βχ+ρ,   ρ<β

Proof: since β>1, β(ζ+1)≥ζ+1, and so there is a least χ′ such that βχ′>ζ. Furthermore χ′ cannot be a limit ordinal: if βξ≤ζ for all ξ<λ, then βλ≤ζ by continuity of multiplication. Set χ=χ′−1, so

βχ≤ζ<β(χ+1)

Now write (by equation (7) of post 8)

ζ=βχ+(−βχ+ζ)=βχ+ρ

setting ρ=−βχ+ζ. We cannot have ρ≥β, otherwise

ζ=βχ+ρ≥βχ+β=β(χ+1)>ζ

Uniqueness needs to be done just right, since ordinal addition has cancellation on the left but not on the right. Suppose

βχ11=βχ22,    ρ12

If χ12 then χ21+γ for some γ>0. So

βχ11=β(χ1+γ)+ρ2=βχ1+βγ+ρ2

Cancelling on the left,

ρ1=βγ+ρ2≥βγ≥β

contradicting the definition of ρ1. So χ12=χ (say), and we can cancel βχ on the left to get ρ12.

The proof of Cantor normal form starts out in a similar fashion. First prove by induction that βα≥α for all α. Since βζ+1>ζ, it follows that there is a least α with βα>ζ. Furthermore α cannot be a limit ordinal by continuity of exponentiation (in the exponent). Set α1=α−1. So

βα1≤ζ<βα1+1

Now we divide ζ by βα1:

ζ=βα1χ11,    ρ1α1

We cannot have χ1≥β, otherwise

ζ=βα1χ11≥βα1β=βα1+1

Repeat with ρ1:

ρ1α2χ22,   χ2<β,   ρ2α2

We must have α21 because βα2≤ρ1α1. Continuing we get a descending sequence of αi’s which must terminate in finitely many steps, because ordinals. This establishes (1).

The proof of uniqueness provides a bonus: a criterion for which of two normal forms is larger. It’s what you’d expect from decimal notation. Suppose

ζ α1 χ1+···+βαk χk
ζ′ = βα1 χ1′+···+ βαm χm

are two unequal normal forms. Because cancellation on the left holds for addition, we can remove any equal terms on the left, and assume either α11′ or α11′ and χ11′ (for the reverse inequalities, just flip things around). Then ζ<ζ′. I will call this the first difference criterion for the ordering of Cantor normal forms.

The proof resembles a decimal computation. To show that 999<1000 (for example), we add 1 and do the carries. Here, we begin by combining the last two terms of ζ, using the facts that χk<β and αk−1k:

βαk-1 χk-1αk χk αk-1 χk-1αk+1
≤βαk-1 χk-1αk-1
αk-1k-1+1)

Next we combine with the previous term, using the fact that χk−1+1≤β and αk−2k−1:

βαk-2 χk-2αk-1k-1+1) ≤βαk-2 χk-2αk-1+1
≤βαk-2k-2+1)

We keep going, until eventually we have

ζ<βα11+1)

If α11′ and χ11′, then we have βα11+1)≤βα1 χ1′. Thus ζ is less than the first term of ζ′. If α11′ then we use the fact that χ1+1≤β, concluding that βα11+1)≤βα1+1≤βα1, and hence ζ is again less than the first term of ζ′. A fortiori, ζ<ζ′.

Uniqueness follows. These ordering criteria are needed for the Goodstein and Hydra theorems.

[1] However, Stillwell messes up at the end of the example. In the last bullet he says, “This means that α is a term in the following sequence with limit ωω2·7+ω·4+11+ω= ωω2·7+ω·4+12.” This equation is incorrect; the last “+ω’’ should be “·ω’’. The sequence on the next line should have “·1’’, “·2’’, etc., instead of “+1’’, “+2’’, etc. So he has many more steps to go.

Another point. When he says that α “falls between” two terms in a sequence, he’s not entitled to assume it falls strictly between. He should say instead that there are two consecutive terms with α greater than or equal to the first and less than the second.

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Set Theory Jottings 8. Ordinal Arithmetic

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Usually one defines the ordinal operations via transfinite induction:

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From Kepler to Ptolemy 15

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The Planetary Hypotheses

In the Planetary Hypotheses, Ptolemy lays out his cosmology: that is, the structure and arrangement of the universe. This work answers the question, did Ptolemy believe in the physical truth of the Almagest’s celestial geometry?—with an unambiguous Yes. Contrary to an opinion often expressed by earlier historians, he did not regard it just as a calculational scheme for predicting planetary positions.

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Set Theory Jottings 7. The (Cantor-Dedekind-Schröder)-Bernstein Theorem

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The trichotomy of cardinals says that for any 𝔪 and 𝔫, exactly one of these holds: 𝔪<𝔫, 𝔪=𝔫, or 𝔪>𝔫. It’s equivalent to the conjunction of these two propositions, for any two cardinals 𝔪 and 𝔫:

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From Kepler to Ptolemy 14

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Cycle Counts

You may have heard that Ptolemaic systems grew to have 80 spheres or cycles, while the Copernican system had only 34. This is a myth.

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Set Theory Jottings 6. Zorn’s Lemma

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Zermelo’s 1904 proof of the well-ordering theorem got a lot of blowback, as we’ve seen. On the other hand, the very next year Hamel used it to prove the existence of a so-called Hamel basis. In 1910, Steinitz made numerous applications in the theory of fields. He wrote:

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