Top Banner
50

The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Aug 26, 2018

Download

Documents

lyphuc
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 2: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

The retrograde motion of Mars lasts for about 3 months.

Page 3: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Ptolemy’s solution to the problem of the retrograde motion ofMars as viewed from above. (Drastically out of scale)

Page 4: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Ptolemaic Mars

The period ofMars is about 2terrestrial years.The retrogrademotion shown tothe left is roughlyscale, occurringover about 1/8 ofthe cycle. Theangular velocitiesof both thedeferent (thelarge circle) andthe epicycle arethe same.(The epicycle on the epicycle isnot functional. Think of it asMars itself.)

Page 5: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

ca. 26,000 year cycle. Here Polaris is shown as the North Star.

Page 6: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

This map of the cosmos

actually shows most of

what has been discussed

so far.

The 10+ spheres.

The 4 elements.

The planets.

Precession adjustments:

The outer ring is the

astrological coordinate

system and the 2 rings

lower are the actual

constellations. As you

can see, at about 3:00,

Pisces is in Aries. This

is from the 16th century.

Now things have

changed a bit and the sun

is dawning in Aquarius,

Aqu-air-ee-us.

Page 7: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Claudius Ptolemaeus

Claudius Ptolemy

Klaudion Ptolemaion

Ptolemus

Tolomaeus

Ptolemeo

!"#$%&'( )*'"+µ#&'(

Tolomi

Ptolemeus

Tolomeo

and Arabic …

and others…

fl. 150 A.D. in Alexandria

fl. ca. 800 Damascus

fl. ca. 1200 England

fl. ca. 1400 Italy

fl. ca. 1600 China

fl. ca. 1700 Germany

fl. ca. 1900 United States

Planetary Hypothesis

Syntaxis Mathematica

Harmonics

Tetrabiblos

Quatripartitum

On Music in Three Books

!"#$# %"&'()'$#

*+µ,#'-$# %'%('" .

Almagest

Geography

Handy Tables

Mathmatical Treatise

in Four Books

Optics

Table or Reigns

De Anelemmate

Planisphaerium

Centiloquium

‘/0,1)&)'2

and Arabic…

and others…

Page 8: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Go to Lindberg PDF…

The

Equant:

Copernic

us hated

this idea.

Page 9: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 10: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

There is some

unresolved

confusion over

whether these

should really be

considered spheres

in Ptolemy’s

theory or just

hypothetical

spheres for easier

visualization.

Similarly, the

circles and

epicycles are

difficult to

imagine as real.

Page 11: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 12: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 13: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 14: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 15: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

From Bruno’s

Cena de le

ceneri - Ash

Wed. Supper,

1584

Page 16: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

The first written heleocentric “academic paper” by Copernicus was the

Commentariolus written and distributed ca. 1510-1514

No details but a general presentation of the theory.

1. Not all heavenly bodies revolve around the same center.

2. The earth is the center only for the moon.

3. The sun is the center of the rest.

4. The earth is quite close to the sun as compared with the stars.

5. Earth’s daily rotation on its axis accounts for apparent star motions.

6. The sun’s motion amongst the stars is due to earth orbit of sun.

7. Retrograde motions are due to earth and planets orbit of the sun.

34 circles needed to explain the solar system: Mercury with 7, Venus

with 5, Earth with 3, Moon with 4, Mars with 5, Jupiter with 5, and

Saturn with 5.

Page 17: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

In 1539 Rheticus wrote the Narratio Prima, a very good

summary of Copernican theory. Copernicus only

identified as Dr. Nicolaus and “my Teacher.”

It was printed in 1540.

Rheticus stayed with Copernicus until 1541 and copied by

hand the masterwork, De revolutionibus, and made

corrections and checked the math… etc.

Page 18: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Narratio Prima…

From The Motion of the Fixed Stars (p. 111) in N.p. Copernicus/Rheticus

discusses the precession of the equinoxes. Copernicus thought that this

motion was irregular and thus made it much more complicated that it needed

to be. But the last line of this section sums up the story, “the mean motion of

the stars in an Egyptian year [he’s arguing from Ptolemy’s data] is about 50”,

and the complete revolution of the mean motion will take 25,816 Egyptian

years.” This figure is still generally accepted.

Precession changes the locations in the Earth's orbit at which the equinoxes

and solstices occur. The sun appears to move a bit west each year. For

example, the spring equinox today occurs when the Sun appears in the

direction of the constellation Pisces and Aquarius. In another 600 years,

precession will move this point fully into the constellation Aquarius, while

2000 years ago, this point was in the constellation Aries.

Page 19: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Copernican Precession Animation

Page 20: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

De revolutionibus orbium

coelestium 1542/3

On the revolutions of the

heavenly spheres

Page 21: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 22: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 23: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

This is from Kepler’s copy, which is titled in translation,

On the revolutions of the the celestial/heavenly spheres,

or

On the revolutions of the spheres of the heavenly bodies.

Copernicus’ original title was De revolutinibus orbium mundi.

“Mundi” is a tricky word.

This could be translated as

On the revolutions of the spheres of the universe/heavens/world

Page 24: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

The Sol-ar

System of

Copernicus-

Note that the

last sphere is

of the fixed

stars and that

it is

immobilis

and finite.

Page 25: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

I. Immobile sphere of the

fixed stars

II. Saturn, is turned in 30

years

III. Twelve-year revolution of

Jupiter

IV. Two-year revolution of

Mars

V. Earth (Tellus), with the orb

of the moon …[?] …

VI. Venus nine month return

VII. Mercury … [?] …80 days

[VIII]. The Sun

Page 26: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

This comment made ca. 1533.

Not everybody loved this new idea.

Although, to be honest, most didn’t care one way or the other.

The following is by someone who was annoyed by it.

Page 27: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

“Perhaps there will be babblers who claim to be judges of astronomy

although completely ignorant of the subject and, badly distorting

some passage of Scripture to their purpose, will dare to find fault with

my undertaking and censure it. I disregard them even to the extent of

despising their criticism as unfounded. For it is not unknown that

Lactantius, otherwise an illustrious writer but hardly an astronomer,

speaks quite childishly about the earth's shape, when he mocks those

who declared that the earth has the form of a globe. Hence scholars

need not be surprised if any such persons will likewise ridicule me.

Astronomy is written for astronomers.”

From De rev, 1543. The part called “To His Holiness, Pope Paul III…”

Page 28: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

To make things confusing, we also have Osiander’s preface.

At the very end Osiander writes,

“Therefore alongside the ancient hypotheses, which are no

more probable, let us permit these new hypotheses

[Copernicus’] also to become known, especially since

they are admirable as well as simple and bring with them

a huge treasure of very skillful observations. So far as

hypotheses are concerned, let no one expect anything

certain from astronomy, which cannot furnish it, lest he

accept as the truth ideas conceived for another purpose,

and depart from this study a greater fool than when he

entered it. Farewell.”

Page 29: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Osiander’s Preface

from the first edtion.

Note how the typeface

of “Andreas Osiander”

appears to be hand

written.

Page 30: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Jerome Schreiber of Nuremberg penned in Osiander’s name in his

edition later owned by Kepler. [Kepler is aware of this.]

Page 31: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

“D. Heironymo Schr/[ei]

ber petreius dd

1543”

Given to Jerome Schreiber by

Petreius in 1543.

Page 32: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Schreiber’s library was sold to a book dealer after his death.

This book dealer happened to be a relative of Johannes Kepler.

Kepler obtained these books and they became a part of his

personal library. Along with De rev. he also had a copy of a

collection of astronomical/astrological, meteorlogical

observations which had numerous notes scribbled in the

margins by Schreiber. From these notes, Kepler was able to

compare the handwriting to the “Andreas Osiander” written in

his copy of De rev. CSI – Renaissance Europe.

In Kepler’s second major work, Astronomia nova, he outed

Osiander as the writer of the preface in De rev. Despite this

public and published detail, the mystery of the writer of the

preface continued on for about 150 years. Clearly people

didn’t read Astronoma nova all that closely.

Page 33: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Summer in Northern

Hemisphere

Page 34: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

The retrograde motion of Mars lasts for about 3 months.

Page 35: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Copernican Retrograde Motion

Page 36: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 37: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 38: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Commentariolus had 34 circles (38 if you count precession and

some lunar issues that he didn’t count for his total). In order to

account for some speed variations that Copernicus discovered in

the data he added more circles to De rev in the end having 48.

Copernicus exagerated Ptolemy’s circles, claiming that Ptolemy

had ca. 80. The actual number of circles in the most modern

version of the Ptolemaic system by Perubach had it at about 40.

Copernicus’ system was really not simpler than Ptolemy’s. But

Copernicus said it was. Who really felt like checking? It also

wasn’t any more accurate if you compare it to modernized versions

of Ptolemy’s theory.

All the same, people slowly heard of it… (Kepler in particular.)

Page 39: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 40: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

The

Diggesian

Cosmos(1576)

http://math.dartmouth.edu/~matc/Readers/re

naissance.astro/1.1.Revol.html

Page 41: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 42: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Background trivia for next class…

Page 43: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 44: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 45: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

This person (an Aries) was born in the Spring near the equinox.

The moon was full (in Libra), but Venus cannot possibly be in

Capricorn because Venus is sort of tied to the sun. (It’s the

morning and evening star.) But replace Venus with Saturn, evil

Saturn, and you can start making sense of astrology. A 3:2 (P5)

cosmic ratios is indicated in the diagram on the left.

Page 46: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 47: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

Giorgi’s

Vitruvian Man

ca. 1525

Page 48: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos
Page 49: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos

…more macro-micro

Page 50: The retrograde motion of Mars lasts for about 3 months. · PtolemyÕs solution to the problem of the retrograde motion of Mars as viewed from above. (Drastically out ... Tetrabiblos