Heliocentrism
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Discussion
early
Aristarchus a.k.a. Αρίσταρχος (310-230 BCE) Greece (Samos)
- the earth is bigger than the moon (~3 times larger - 8:3 to be more exact) can be seen from the shadow of the earth on the moon during a lunar eclipse
- the sun is very much farther away than the moon, as can be seen by the fact the time separating first quarter and third quarter moons is the same as the time between the third quarter and the first quarter
- the sun is also very much larger than the moon as can be seen during a solar eclipse
- the sun must be the center of the universe, since it is so very, very large
- the stars are very far away since there is no apparent parallax
However, Aristarchus' only remaining work on the topic, On the Sizes and Distances
of the Sun and Moon, is geocentric!
Pythagoras a.k.a. Πυθαγόρας (582 BC-496 BCE) Greece (Ionia)
copernicus
Nicolaus Copernicus (1473-1543) Poland (latinized version of Mikołaj Kopernik). De Revolutionibus Orbium Cœlestium (On the Revolutions of Heavenly Spheres) 1543.
| In medio uero omnium residet Sol. |
|
In the center of all rests the sun. |
|
Quotes
- People gave ear to an upstart astrologer who strove to show that the earth
revolves, not the heavens or the firmament, the sun and the moon…. This fool wishes to reverse the entire science of astronomy; but sacred
scripture tells us that Joshua commanded the sun to stand still, and
not the earth.
Martin Luther, referring to Joshua 10:13, in his series of "Table Talks" (1539)
- The eyes are witnesses that the heavens revolve in the space of twenty-four
hours. But certain men, either from the love of novelty, or to make a
display of ingenuity, have concluded that the earth moves; and they maintain
that neither the eighth sphere nor the sun revolves…. Now, it is a want of honesty and decency to assert such notions publicly,
and the example is pernicious. It is the part of a good mind to accept
the truth as revealed by God and to acquiesce in it.
Melanchthon, emphasizing Ecclesiastes 1:4-5
- Who will venture to place the authority of Copernicus above that of the Holy
Spirit?
John Calvin, citing Psalm 93:1 in his Commentary on Genesis
- … And whereas it has also come to the knowledge of the said Congregation that
the Pythagorean doctrine -- which is false and altogether opposed to
the Holy Scripture -- of the motion of the Earth and the immobility of
the Sun, which is also taught by Nicolaus Copernicus in De Revolutionibus Orbium Cœlestium, and by Diego de Zuñiga On Job, is now being spread
abroad and accepted by many… Therefore, in order that this opinion may not insinuate itself any further
to the prejudice of Catholic truth, the Holy Congregation has decreed
that the said Nicolaus Copernicus, De Revolutionibus Orbium, and Diego
de Zuñiga, On Job, be suspended until they are corrected.
The Roman Catholic Church, from The Decree of the Roman Catholic Congregation
of the Index which condemned De Revolutionibus on March 5, 1616
Notes
- heliocentric with circular orbits and a few (48?) epicycles
- The outermost sphere of the fixed stars is made immobile. Previously it was the prime mover?
- Moving the sun to the center made calculations easier.
- It did not work as well as Ptolemy's geocentric system, which was at the time, more accurate.
- No observational evidence that the earth moved, therefore it was not taken seriously. (Before you laugh at these "foolish people", look at the ground. Do you see it moving? Prove to me that the earth is not fixed.)
How heliocentrism deals with retrograde motion.

[magnify]

[magnify]
bruno
Giordano Bruno a.k.a. Filippo Bruno a.k.a. Bruno Nolano (1548-1600) Italy (Naples)
- La Cena de le Ceneri (The Ash Wednesday Supper). 1584
- De l'Infinito, Universo, e Mondi (On the Infinite Universe and Worlds). 1584
- In space there are countless constellations, suns and planets; we see only the suns because they give light; the planets remain invisible, for they are small and dark. There are also numberless earths circling around their suns, no worse and no less than this globe of ours. For no reasonable mind can assume that heavenly bodies that may be far more magnificent than ours would not bear upon them creatures similar or even superior to those upon our human earth.
- De Immenso (On Immensity). 1591
- unknown
- Open wide the door for us, so that we may look out into the immeasurable starry universe; show us that other worlds like ours occupy the ethereal realms.
galileo
Galileo Galilei (1564-1642) Italy
Notes and Quotes
- Siderius Nuncius
(Starry Messenger). 1610
telescopic evidence for the heliocentric model, the first printing sold
out within days (March 12)
- mountains on the moon -- moon was supposed to be perfect
" From observations …
repeated many times I have been led to the opinion and conviction
that the surface of the moon is not smooth, uniform, and precisely
spherical as a great number of philosophers believe it (and other
heavenly bodies) to be, but is uneven, rough, and full of cavities
and prominence's, being not unlike the face of the earth, relieved
by chains of mountains and deep valleys."
- milky way made of stars -- there are things invisible to the naked eye
"I have observed the nature and the material of the Milky Way. With the aid
of a telescope this has been scrutinized so directly and with such ocular
certainty that all disputes which have vexed philosophers through so many
ages have been resolved, and we are at last freed from worldly debates about
it The galaxy is, in fact, nothing but a congress of innumerable stars grouped
together in clusters. Upon whatever part of it the telescope is directed,
a vast crowd of stars is immediately presented to view. Many of them are
rather large and quite bright, while the number of smaller ones is quite
beyond calculation."
- moons of jupiter -- was thought that moon could not keep up with moving earth
(first sighted January 7, realized they were moons on January 15),
Jupiter shares something in common with the earth, both are satellites
of the sun
" On the seventh day of January in this present year 1610, at the first hour
of night, when I was viewing the heavenly bodies with a telescope, Jupiter
presented itself to me; and because I had prepared a very excellent instrument
for myself, I perceived (as I had not before, on account of the weakness
of my previous instrument) that beside the planet there were three starlets,
small indeed, but very bright. Though I believed them to be among a host
of fixed stars, they aroused my curiosity somewhat by appearing to lie in
an exact straight line parallel to the ecliptic, and by their being more
splendid than others of their size. Their arrangement with respect to Jupiter
and each other was the following:"
[Descriptive text removed between diagrams. Galileo uses a tipped-over
zero or and "O" to represent Jupiter and asterisks to represent the "starlets".]
| 7 |
January |
East |
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* |
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| 8 |
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East |
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* |
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| 9 |
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"everywhere covered with clouds" |
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| 10 |
January |
East |
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O |
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January |
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| 14 |
January |
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"the weather was cloudy" |
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| 15 |
January |
East |
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O |
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* |
* |
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* |
West |
| 16 |
January |
East |
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| 23 |
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| 26 |
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| 27 |
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East |
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* |
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O |
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| 28 |
January |
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"nothing could be observed
because of interposed
clouds." |
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| 31 |
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| 1 |
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East |
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[*] |
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| 2 |
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| 3 |
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| 4 |
February |
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| 5 |
February |
East |
"the sky was cloudy" |
West |
| 6 |
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[*] |
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| 14 |
February |
East |
"the sky was covered by clouds" |
West |
| 15 |
February |
East |
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"the sky was cloudy" |
West |
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O |
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| 22 |
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"the sky was covered by clouds"
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West |
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| 24 |
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"Such are the observations concerning the four Medicean planets recently first
discovered by me …."
Galileo then goes on to describe how these "starlets" wander around the bright dot that is Jupiter. First appearing ahead then
behind the planet, they follow Jupiter no matter which way it moves
across the sky, be it in direct or retrograde motion. Like a miniature
solar system (a concept that did not really exist at the time), each
dot shifts from side to side within a restricted orbit, the closest
one in having the shortest period and the farthest one out having
the longest period. Galileo named them the "Medicean planets" after his benefactor Cosimo II de' Medici, the Grand Duke of Tuscany. He
is using the word "planet" with its original meaning of "wandering star", which is what these objects look like when viewed from the earth -- bright
flecks of light that move relative to the other "fixed stars". The meaning of the word has shifted, so that nowadays the word "planet" refers only to the eight or nine major bodies orbiting the sun -- a shift
in meaning almost entirely due to the observations of Galileo. The "Medicean planets" are now the "Galilean moons".
Galileo discovered something new and hugely important -- satellites
of a satellite; bodies orbiting a body orbiting another, more significant,
body. Moons! The comparison is earth-shaking. Jupiter is a planet
(in current language, a major body orbiting the sun). It has bodies
that orbit it. The earth has a body that orbits it. We call it the
moon. The earth has one moon. Jupiter has many moons. Galileo saw
four, but that was just the beginning. Jupiter is now known to have
nearly sixty moons. This means that Jupiter and the earth are similar
and maybe even equal in stature. Jupiter is a planet and so is the
earth. (Gasp!)
"Here we have a fine and elegant argument for quieting the doubts of those
who, while accepting with tranquil mind the revolutions of the planets about
the sun in the Copernican system, are mightily disturbed to have the moon
alone revolve about the earth and accompany it in an annual rotation about
the sun."
Given what we now know about the cosmos, it gets even worse for the
geocentrists. The earth is certainly something, but now Jupiter is
more than the earth, and the sun is even more than all of them combined.
The earth has one moon, one satellite, one thing that orbits it.
Jupiter had four in Galileo's day and about sixty in our day. The
sun had six in Galileo's day -- Mercury, Venus, Mars, Jupiter, Saturn,
and now the earth too. When you include all the objects known today
-- planets, asteroids, comets, Kuiper belt objects, and the Oort
cloud -- you up the number to about a thousand. The earth goes from
the center of all things to just one rock among many orbiting a bigger
ball of fire.
"[N]ow we have not just one planet rotating about another while both run through
a great orbit around the sun; our own eyes show us four stars which wander
around Jupiter as does the moon around the earth, while all together trace
out a grand revolution about the sun …."
- Istoria e dimostrazioni intorno alle Macchie Solari e loro accidenti. (History and Demonstrations Concerning Sunspots and Their Phenomena.)
1613 -- commonly called The Letters on Sunspots, further evidence for a heliocentric system
- sunspots -- sun is not perfect and it rotates
- phases of venus -- verifies heliocentric geometry
- Dialogo sopra i due massimi sistemi del mondo, Tolemaico, e Copernicano. (Dialogue Concerning the Two Chief World Systems, Ptolemaic and Copernican.) 1632.
- Salviati argues for the Copernican position and presents some of Galileo's
views directly, calling him the "Academician" in honor of Galileo's membership in the Academia dei Lincei. He is named
after Galileo's friend Filipo Salviati (1582-1614).
- Sagredo is an intelligent layman who is initially neutral. He is named after
Galileo's friend Giovanfrancesco Sagredo (1571-1620).
- Simplicio is a dedicated follower of Ptolemy and Aristotle, who presents
the traditional views and the arguments against the Copernican position.
He is modeled after Ludovico delle Colombe (1565-1616) and Cesare
Cremonini (1550-1631), both of whom were conservative philosophers.
The character's name is not "Simpleton", but is taken from the sixth-century philosopher Simplicius, who wrote notable
commentaries on Aristotle. [Maffeo Barberini - Pope Urban VII (1623-1644)?]
- on the Index of Prohibited Books from 1616 to 1835 (with De Revolutionibus)
- held under house for eight years arrest until his death
- condemned in 1633, condemnation reversed gradually (last word in 1992)
Just Quotes
- If the sacred scribes had meant to teach men astronomy, then why did they
leave it out?
Galileo
- The Galileo affair was unique and contrary to the history of the Catholic
Church, which has always supported scholarship, and founded universities.
God can do anything God wants.
Guy Consolmagno, Vatican Astronomer. Hazel Muir, Heaven's Observer, New
Scientist 2231, 23 March 2000.
tycho
Tycho Brahe (1546-1601) Denmark
Notes
- Compromise system
- Uraniborg (Castle of the Heavens) 1576-1597
- moved to Prague in 1597 at the request of Emperor Rudolph of Bohemia
- Rightly determined that comets are beyond the moon, must have an orbit of
some strange sort.
- There are no spheres that carry the planets.
- Since comets travel on an orbit that crosses the orbits of the planets, they
could not be affixed to solid, crystalline spheres. Either the comet
would stop or the spheres would shatter.
- Crystalline spheres would refract light, but we do not see the position of
the fixed stars shift.
- Sometimes the planet Mars is nearer to the earth than the sun. Thus the sphere
of Mars and the sphere of the sun must overlap -- something that
is not possible were they solid.
Quotes
- Now it is quite clear to me that there are no solid spheres in the heavens,
and those that have been devised by authors to save the appearances,
exist only in their imagination, for the purpose of permitting the mind
to conceive the motion which the heavenly bodies trace in their courses.
Quoted in A L Mackay, Dictionary of Scientific Quotations (London 1994)
- Those who study the stars have God for a teacher.
kepler
Johannes Kepler (1571-1630) Holy Roman Empire (now Austria)
Kepler was a terrible high school teacher.
Kepler's first attempt fails
Mysterium Cosmographicum (Cosmic Mystery) 1596.
Before the universe was created, there were no numbers except the Trinity,
which is God himself… For, the line and the plane imply no numbers: here infinitude itself reigns.
Let us consider, therefore, the solids. We must first eliminate the
irregular solids, because we are only concerned with orderly creation.
There remain six bodies, the sphere and the five regular polyhedra.
To the sphere corresponds the heaven. On the other hand, the dynamic
world is represented by the flat-faces solids. Of these there are
five: when viewed as boundaries, however, these five determine six
distinct things: hence the six planets that revolve about the sun.
This is also the reason why there are but six planets.
I have further shown that the regular solids fall into two groups: three
in one, and two in the other. To the larger group belongs, first
of all, the Cube, then the Pyramid, and finally the Dodecahedron.
To the second group belongs, first, the Octahedron, and second, the
Icosahedron. That is why the most important portion of the universe,
the Earth -- where God's image is reflected in man -- separates the
two groups. For, as I have proved next, the solids of the first group
must lie beyond the earth's orbit, and those of the second group
within… Thus I was led to assign the Cube to Saturn, the Tetrahedron to Jupiter,
the Dodecahedron to Mars, the Icosahedron to Venus, and the Octahedron
to Mercury.
[magnify]
Kepler decided the observations of the planets were wrong, not his model
of nested platonic solids.
This model was rendered useless when Uranus (the seventh planet) was discovered
in 1781, Neptune (the eighth planet) in 1846, Ceres (the first asteroid)
in 1801, and Pluto (the first Kuiper belt object) in 1930. More than 10,000
objects orbiting the sun have been identified.
The counter reformation steps in and Kepler is driven out of Graz.
rather make a desert of the country than rule over heretics
Philip III (1598-1621) Son of Philip II becomes leader of Spanish house
of Hapsburg
says to Pope: "I would rather lose a hundred lives, if I had them, than consent to rule
over heretics."
This rebellion would drag on until 1648, become part of the wider European
struggle known as the Thirty Years War (1618-1648)
Kepler's Good Stuff
- Astronomia Nova seu Physica Cœlestis (New Astronomy or Celestial Physics) 1609
- Law of Elliptical Orbits: The orbit of a planet about the sun is an ellipse
with the sun at one focus.
- Law of Equal Areas: A line joining a planet and the sun sweeps out equal
areas during equal intervals of time.
- Planets move with variable speed.
- Added the recently discovered Galilean moons of Jupiter to his system (and
the "supporting stars"
of Saturn, which we now recognize as the rings). There are the six "primary" planets that orbit the sun and the "secondary" planets that orbit the primary planets and move along with them. We would
call these secondary planets satellites.
- Laws also apply to satellite orbits (constant depends on mass of object being
orbited)
- Harmonices Mundi (Harmonies of the World) 1619
- Harmonic Law: The square of the sidereal period of a planet is directly proportional
to the cube of the orbit's semimajor axis (r3 ∝ T2).
- Empirical not theoretical in origin (also included "music of the planets"and platonic solids)
- Originally tried a geometric description, 5 nested platonic solids give 6
planetary orbits, model fails since there are many more than 6 objects
orbiting the sun
- On how he discovered his Third law:
… and if you want the exact moment in time, it was conceived mentally
on 8th March in this year one thousand six hundred and eighteen,
but submitted to calculation in an unlucky way, and therefore rejected
as false, and finally returning on the 15th of May and adopting
a new line of attack, stormed the darkness of my mind. So strong
was the support from the combination of my labor of seventeen years
on the observations of Brahe and the present study, which conspired
together, that at first I believed I was dreaming, and assuming
my conclusion among my basic premises. But it is absolutely certain
and exact that the proportion between the periodic times of any
two planets is precisely the sesquialterate proportion of their
mean distances …
Harmonices mundi (Linz, 1619) Book 5, Chapter 3, trans. Aiton, Duncan and Field, p. 411.
Quoted in J. Koenderink, Solid Shape, Cambridge MA: MIT Press, 1990.
- Dritte Keplersche Gesetz: "Die Quadrate der Umlaufszeiten zweier Planeten verhalten sich wie die dritten
Potenzen ihrer mittleren Abstände." [The squares of the rotating times
of two planets behave like the third powers of their middle distances.]
- Epitome Astronomiæ Copernicanæ (Summary of Copernican Astronomy) 1618-1621
Additional Quotes
| Ubi materia, ibi geometria. |
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Where there is matter, there is geometry. |
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| Geometria una et æterna est in mente Dei refulgens: cuius consortium hominibus tributum inter causas est, cur homo sit imago Dei. |
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Geometry is one and eternal shining in the mind of God: that share in it accorded to men is one of the reasons that Man is the image of God. |
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| Mensus eram cœlos, nunc Terræ metior umbras. Mens cœlestis erat, corporis umbra jacet. |
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I used to measure the Heavens, now I measure the shadows of Earth. The mind belonged to Heaven, the body's shadow lies here. |
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Geometry existed before the Creation. It is co-eternal with the mind of God. Geometry provided God with a model for the Creation. Geometry is God Himself. |
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Geometry, which before the origin of things was coeternal with the divine mind and is God himself (for what could there be in God which would not be God himself?), supplied God with patterns for the creation of the world, and passed over to Man along with the image of God. |
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My brain gets tired when I try to understand what I wrote, and I
find it hard to rediscover the connexion between the figures and the
text, that I established myself. |
|
Kepler wrote the first work of science fiction -- the Somnium (1634) -- published
by Kepler's son Ludwig, four years after his death.
Summary
Problems
practice
- Geosynchronous Satellite
There is a special class of satellites that orbit the earth with a period of one day.
- Determine the orbital radius at which the period of a satellite's orbit will
equal one day. State your answer as …
- an approximate fraction of the moon's orbital radius
- an approximate multiple of the earth's radius
- an "exact" number of kilometers
- How will the satellite's motion appear when viewed from the surface of the
earth?
- What type of satellites use this orbit and why is it important for them to
be located in this orbit? (Keep in mind that this is a relatively high
orbit. Satellites not occupying this band are normally kept in much lower
orbits.)
Solutions …
- Use Kepler's third law of planetary motion: the square of the period of a satellite in a circular orbit is proportional to the cube of its radius.
| |
|
|
| r3satellite |
= |
r3moon |
| T2satellite |
T2moon |
| |
|
|
(This problem can also be solved using Newton's law of universal gravitation
with the centripetal force formula. That solution is presented in the
section called Orbital Mechanics I.)
- Compare the radius and period of the geosynchronous satellite's orbit to
the radius and period of the moon's orbit. Use convenient "approximate" values.
| |
|
|
|
|
|
|
| r3satellite |
= |
r3moon |
⇒ |
r3satellite |
= |
r3moon |
| T2satellite |
T2moon |
(1 day)2 |
(27 days)2 |
| |
|
|
|
|
|
|
| rsatellite ≈ |
1 |
earth-moon distance |
| 9 |
| |
|
- The earth-moon distance is about sixty times the radius of the earth.
| |
|
|
| rsatellite ≈ |
60 |
≈ 7 earth radii |
| 9 |
| |
|
- Repeat the first part of this problem using more "exact" values.
| |
|
|
|
| r3satellite |
= |
r3moon |
|
| T2satellite |
T2moon |
| |
|
|
|
| r3satellite |
= |
(3.944 × 108 m)3 |
|
| (0.9973 day)2 |
(27.32 day)2 |
| |
|
|
|
| rsatellite |
= |
4.230 × 107 m ≈ |
42,000 km |
| |
|
|
|
You might have noticed some odd values in this solution.
- The period of the earth's rotation is approximately equal to the mean solar day (1 day = 24 x 3600 = 86,400 s), but for best results the sidereal day (86,164 s or 0.9973 days) should be used. A mean solar day is the time between local noon one
day and local noon the next day. (Local noon is the time when the
sun is at its highest position in the sky when viewed from a particular
location on the earth.) The sidereal day is the time it takes for
the earth to return to its original orientation with respect to the
distant stars. The mean solar day is a bit longer since the earth
is moving around the sun. After the earth has completed one rotation
relative to the stars, it has to spin for an extra four minutes to
line up with the sun again.
- The period of the moon's orbit used above was not the 30 days found in a
typical calendar month, nor was it the 28 day lunar cycle familiar
to 51% of the earth's population, nor was it the more precise 29.5
day period between full moons. These numbers are all related to the synodic period of the moon -- the time it takes for the sun, earth, and moon to line up
in the same relative positions. The number we used was the sidereal period -- the time it takes for the moon to return to its same orientation with
respect to the distant stars. The moon has to travel an additional
2⅙ days after it has already completed one orbit in order to catch up with
the moving earth.
- The answer appears elsewhere in this book.
- The answer appears elsewhere in this book.
- Kirkwood Gaps
The asteroids are a group of small rocky bodies orbiting the sun in relatively
circular orbits. (In comparison, comets are small icy bodies orbiting the
sun in highly elliptical orbits.) The number of asteroids currently identified
is something on the order of 200,000 but only about half of these are in
orbits that are known with enough certainty to receive an official catalog
entry in the Minor
Planet Center Orbit Database (MPCORB). The vast majority of asteroids lie in the region between the orbits
of mars and jupiter known as the main asteroid belt. The graph below shows the distribution of asteroids in the densest part
of this region. The values highlighted in red show orbital radii for which
there are few or even no corresponding asteroids. The values highlighted
in blue show the effective edges of this part of the main belt. These features
were discovered by the American astronomer Daniel Kirkwood (1814-1895)
in the Nineteenth Century and are now known as Kirkwood gaps.
These orbits are empty because they share a simple harmonic relationship
with the orbit of jupiter; that is, the ratio of the period of an unoccupied
or under-occupied orbit in a Kirkwood gap forms a simple whole number ratio
with the period of an orbit of jupiter (something like 2:1 or 3:2 or 5:3).
Because of this synchrony the point of closest approach between the two bodies
-- the moment when their mutual gravitational attraction is the greatest
-- will always take place at the same phase in the asteroid's orbit. Small
perturbations applied at just the right moment over and over again reinforce
one another until eventually the asteroid enters a new orbit. Repeat this
procedure for many simple harmonic ratios and a series of gaps will open
up in an asteroid belt that would otherwise be randomly populated.
Using a statistical or spreadsheet application determine …
- the radii of all possible resonant orbits that can be generated using the numbers 1 through 9
- the resonance ratios responsible for each of the seven Kirkwood gaps identified above
Solutions …
- Start with Kepler's harmonic law. Use the orbital radius of jupiter (5.2 AU) and let x and y be the orbital periods of the asteroid and jupiter respectively.
| |
|
|
|
|
|
|
|
|
⎛ ⎝ |
rresonant orbit |
⎞ ⎠ |
3 |
= |
⎛ ⎝ |
x |
⎞ ⎠ |
2 |
| 5.2 AU |
|
y |
|
| |
|
|
|
|
|
|
|
|
| |
|
|
|
|
| rresonant orbit = 5.2 AU |
⎛ ⎝ |
x |
⎞ ⎠ |
⅔ |
| y |
|
| |
|
|
|
|
Cycle both x and y through all possible combinations of the whole numbers from 1 to 9. The
results are compiled in the table below. The values nearest to the
observed gap radii are highlighted in red and blue. Repeated ratios
like 2:2 (which is a repeat of 1:1) or 3:9 (which is a repeat of 1:3)
have been grayed out.
| |
| Resonant Orbits with Jupiter (AU) |
| x |
1:x |
2:x |
3:x |
4:x |
5:x |
6:x |
7:x |
8:x |
9:x |
| 1 |
5.200
|
3.276 |
2.500 |
2.064 |
1.778 |
1.575 |
1.421 |
1.300 |
1.202 |
| 2 |
8.254 |
5.200 |
3.968
|
3.276 |
2.823 |
2.500 |
2.256
|
2.064 |
1.908 |
| 3 |
10.816 |
6.814 |
5.200 |
4.293
|
3.699 |
3.276 |
2.956 |
2.704 |
2.500 |
| 4 |
13.10 |
8.254 |
6.299 |
5.200 |
4.481 |
3.968 |
3.581
|
3.276 |
3.028 |
| 5 |
15.20 |
9.578 |
7.310 |
6.034 |
5.200 |
4.605 |
4.155 |
3.801 |
3.514 |
| 6 |
17.17 |
10.82 |
8.254 |
6.814 |
5.872 |
5.200 |
4.692 |
4.293 |
3.968 |
| 7 |
19.03 |
11.99 |
9.148 |
7.551 |
6.508 |
5.763 |
5.200 |
4.757 |
4.398 |
| 8 |
20.80 |
13.10 |
10.00 |
8.254 |
7.113 |
6.299 |
5.684 |
5.200 |
4.807 |
| 9 |
22.50 |
14.17 |
10.82 |
8.929 |
7.695 |
6.814 |
6.148 |
5.625 |
5.200 |
| |
- Filter out all the extra junk and make a new table …
| |
| Kirkwood Gaps and Their Ratios |
| orbital radius (AU) |
number of orbital periods |
| observed |
theoretical |
asteroid |
: |
jupiter |
| 2.060 |
2.064 |
4 |
: |
1 |
| 2.500 |
2.500 |
3 |
: |
1 |
| 2.710 |
2.704 |
8 |
: |
3 |
| 2.822 |
2.823 |
5 |
: |
2 |
| 2.956 |
2.956 |
7 |
: |
3 |
| 3.030 |
3.028 |
9 |
: |
4 |
| 3.280 |
3.276 |
2 |
: |
1 |
| |
and a new graph …
Some additional comments:
- Not all resonant orbits produce gaps and sometimes the exact opposite happens.
Certain harmonic ratios seem to attract asteroids resulting in the formation
of groups at some resonant orbits. The most famous of these are the Trojan
asteroids, which are locked in a 1:1 resonance with jupiter and are clumped
60° on either side of it at the Lagrange points. (Lagrange orbits will be discussed
in more detail in the two sections on orbital mechanics in this book.) The second most important example of this effect is the Hilda
group, which occupies the 3:2 resonant orbit at 3.58 AU. Why some resonances produce groups while others produce gaps is a subject
that still hasn't been fully resolved.
- Some resonant orbits appear to have only one occupant. The asteroid 279 Thule is the lone member of the Thule group in 4:3 resonance with jupiter.
It is also one of only a half dozen or so objects which lie in an otherwise
big empty region from 4.2 to 5.0 AU. If Thule is lonely today it can only get lonlier tomorrow. The other
residents of this forbidden zone are all in orbits that appear to be
unstable. Jupiter's gravity is gradually sweeping this region clean.
- Sometimes the connection made between a particular group or gap and an orbital
resonance is very loose.
- The Cybele group is reported to be in a 7:4 resonance with jupiter. The core
of this group orbits 3.38 AU from the sun, but the resonance it's assigned to lies at 3.58 AU -- a 6% difference.
- Many reliable sources show a prominent gap at the 7:2 resonance (2.256 AU), but in my own analysis of the MPCORB data there is barely a dip in the
population at this radius.
To finish this problem off, here's a table identifiying the key orbital resonance
features of the asteroid belt.
| |
| Features of the Asteroid Belt Shaped by Orbital Resonance with Jupiter |
| orbital radius (AU) |
feature |
harmonic ratio |
| ~1.91 |
hungaria group |
9:2 |
| 2.06 |
inner edge of main belt |
4:1 |
| 2.06~2.50 |
main belt i |
|
| 2.50 |
gap |
3:1 |
| 2.50~2.70 |
main belt iia |
|
| 2.70 |
gap |
8:3 |
| 2.70~2.82 |
main belt iib |
|
| 2.82 |
gap |
5:2 |
| 2.82~3.03 |
main belt iiia |
|
| 3.03 |
gap |
9:4 |
| 3.03~3.28 |
main belt iiib |
|
| 3.28 |
outer edge of main belt |
2:1 |
| ~3.58 |
cybele group |
4:7 |
| ~3.96 |
hilda group |
3:2 |
| 4.29 |
thule group |
4:3 |
| 4.2~5.0 |
big empty region |
|
| ~5.20 |
trojan group |
1:1 |
| |
- Write something different.
- Write something different.
conceptual
- Kepler's first two laws of planetary motion state that "the path
of each planet about the sun is an ellipse with the sun at one focus" and "each
planet moves so that a line drawn from the sun to the planet sweeps out
equal areas in equal periods of time." Explain in one paragraph
how these two laws together agree with the more fundamental laws of …
- conservation of angular momentum and
- conservation of energy.
numerical
- In 1984 Marc Davis, Piet Hut, and Richard A. Muller presented the following
highly speculative hypothesis in a letter to
the British science journal Nature.
A 26-Myr periodicity has recently been seen in the fossil record of
extinction in the geological past. At least two of these extinctions
are known to be associated with the impact on the Earth of a comet
or asteroid with a diameter of a few kilometres. We propose that
the periodic events are triggered by an unseen companion to the Sun,
travelling in a moderately eccentric orbit, which at its closest
approach (perihelion) passes through the "Oort cloud" of
comets which surrounds the Sun. During each passage this unseen solar
companion perturbs the orbits of these comets, sending a large number
of them (over 1 × 109) into paths which
reach the inner Solar System. Several of these hit the Earth, on
average, in the following million years….
This "unseen solar companion" later acquired the name Nemesis,
after the Greek goddess of divine retribution (Νέμεσις).
Determine the average distance from Nemesis to the sun. Give your answer
in …
- astronomical units
and
- light years
and
- compare it to the distance to the nearest star (4.3 light years).
statistical
- de-revolutionibus.txt
Read the following passage from the English translation of De Revolutionibus.
Determine the period of each of the five planets known to Copernicus
in the Sixteenth Century using his measurements. State your answers in
years or days as appropriate. Compare them to the Twenty-first Century
values. Compile your results in a table like the one below.
| planet |
period (copernicus) |
period (contemporary) |
per cent deviation |
| saturn |
|
29.4580 years |
|
| jupiter |
|
11.8625 years |
|
| mars |
|
686.980 days |
|
| venus |
|
224.701 days |
|
| mercury |
|
87.9708 days |
|
| |
|
average deviation → |
|
- The asteroids in the following table are reported to be in resonant
orbits with a planet. Determine
- the ratio of the number of periods of the asteroid to the number
of periods of the planet,
- the most likely ideal ratio that relates them, and
- the per cent deviation between the observed and ideal ratios.
| asteroid |
planet |
nasteroid : nplanet |
deviation |
| name |
r (AU) |
name |
r (AU) |
observed |
ideal |
(%) |
| 1685 |
toro |
1.367 |
venus |
0.723 |
|
|
|
| 1685 |
toro |
1.367 |
earth |
1.000 |
|
|
|
| 1221 |
amor |
1.920 |
earth |
1.000 |
|
|
|
| 3753 |
cruithne |
0.998 |
earth |
1.000 |
|
|
|
| 87 |
alinda |
2.485 |
jupiter |
5.204 |
|
|
|
| 8 |
flora |
2.201 |
jupiter |
5.204 |
|
|
|
| |
pluto |
39.482 |
neptune |
30.047 |
|
|
|
- Write some sort of resonant orbit problem to go with this nice illustration.
| |
janus |
mimas |
enceladus |
tethys |
dione |
rhea |
titan |
| 1.120 rs ringlet |
|
|
|
|
|
|
|
| 1.190 rs ringlet |
|
|
|
|
|
|
|
guerin division d-c ring interface |
|
|
|
|
|
|
|
| titan ringlet |
|
|
|
|
|
|
|
maxwell ringlet? maxwell division? lyot division? french division? |
|
|
|
|
|
|
|
| 1.470 rs ringlet |
|
|
|
|
|
|
|
| 1.495 rs ringlet |
|
|
|
|
|
|
|
bond-dawes gap c-b ring interface |
|
|
|
|
|
|
|
| huygens ringlet |
|
|
|
|
|
|
|
| end of b ring |
|
|
|
|
|
|
|
| cassini division |
|
2:1 |
3:1 |
4:1 |
5:1 |
9:1 |
|
| start of a ring |
|
|
|
|
|
|
|
encke gap? encke minima? |
|
5:3 |
|
|
|
|
|
| keeler gap |
|
|
|
|
|
|
|
| outer edge of a ring |
7:6 |
|
|
|
|
|
|
| f ring |
|
|
|
|
|
|
|
| start of g ring |
|
|
|
|
|
|
|
| end of g ring |
|
|
|
|
|
|
|
Resources
- general
- bruno
- copernicus
- galileo
- kepler
- tycho
- nemesis
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