VII Cosmic. VII Cosmic The infinite (apeiron) is inexhaustible The infinite (apeiron) is inexhaustible. Wherever the warrior stands he can stretch.

Slides:



Advertisements
Similar presentations
Chapter 1: Origins of Modern Astronomy
Advertisements

The measure of Cosmological distances Asaf Pe’er Space Telescope Science Institute August 2008.
Summary January The wobble technique assumes that a star will physically be perturbed by the orbit of a planet around it and the resulting motion.
Intro to Astronomy Through the early history of civilization, people made observations about the night sky, sun, and moon. They tried to explain what they.
The Origin of the Universe Massimiliano Galeazzi Miami, 20 November 2002MALS 601.
Astronomy.
History of Astronomy. Our Universe Earth is one of nine planets that orbit the sun The sun is one star in 100 billion stars that make up our galaxy- The.
2.1 History of Astronomy. What is Astronomy?  The branch of science that deals with celestial objects, space, and the physical universe as a whole.
Early Astronomy Chapter 22, Section 1.
VII Kosmisch ¥. Anaxagoras ( ) To every great there exists a greater. Empedokle ( ) The universe is three times as large as the system.
Page 1 FAMOUS ASTRONOMERS. Page 2 ARISTOTLE Proved the Earth is round Worked with Optics Created a "prototype" of the Scientific Method His influence.
Quaestio: Why did the Church try to silence scientific discoveries? Nunc Agenda: Analyze the map of the solar system and try to correctly identify each.
Galaxies and Stars 8.E.4A.1 Obtain and communicate information to model the position of the Sun in the universe, the shapes and composition of galaxies,
Title your notes: Models of the Solar System
1 The Dead Guys. 2 Timeline 3 Ancient Astronomy.
EARTH & SPACE SCIENCE Chapter 27 Planets of the Solar System 27.2 Models of the Solar System.
I. Early History of Astronomy
The Discovery of the Universe BC Aristotle 85 – 165 AD Claudius Ptolemy 1473 – 1543 AD Nicolaus Copernicus AD Tycho Brahe
ASTRONOMY PICTURE OF THE DAY How has our Understanding of the Universe Evolved?
The Scientific Revolution. What is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, a way of thinking,
Astronomy- The Original Science
Astronomy Cosmology.
Astronomy.
Motion of the Moon.
Objective 03/26/12 Identify the units of a calendar. Intro
Astronomy 04 The Solar System
Origins of Modern Astronomy
The Origin of Modern Astronomy
1) What is our galaxy called? Milky Way
Models of the Solar System
Origin of Modern Astronomy
MODELS OF THE SOLAR SYSTEM
Topic F Notes Use Cornell note format.
Astronomers Who Paved the Way
From an Earth-Centered to a Sun-Centered System
The European Renaissance
Astronomy in the Middle Ages to the Modern Era
The Beginnings of Classical Astronomy
Gravity Review By: Josh Fung, Leilani Burke, Logan Wilcox, Kylie Yetenekian, Skyla Park, and Steven Aghakhani.
The Scientific Revolution.
Ch. 22: Astronomers Mr. Litaker 11/10/2018.
BIG BANG THEORY.
Who’s Who in Early Astronomy Part 1
Origins of Modern Astronomy
Astronomy- The Original Science
Periods of Western Astronomy
Astronomy.
Astronomy.
The Copernican Revolution
Introduction to Cosmology
The Scientific Revolution.
Origin of Modern Astronomy
History of Astronomy.
Astronomy Notes The Universe ©Mark Place,
Astronomy Timeline How theory develops and changes over time as new technology allows for more accurate observations.
The Origin of Modern Astronomy
The history of Astronomy!.
Celestial Motion: History and Earth.
Planetary Orbits using Kepler’s Laws
I see, I think, I wonder The Scientific Revolution.
Periods of Western Astronomy
BIG BANG THEORY.
Astronomy It’s out of this world!.
Retrograde Motion, Triangulation & Conclusion Part I
Chapter 2 Sections
The Early History of Astronomy
The Origin of Modern Astronomy
“Earth in Space” Astronomy Part II
Bell Work: What is the center of the Universe?
The Origin of Modern Astronomy
Presentation transcript:

VII Cosmic

The infinite (apeiron) is inexhaustible The infinite (apeiron) is inexhaustible. Wherever the warrior stands he can stretch out his spear. Anaximander of Miletus (611-547) pupil of Thales

Anaxagoras (499-428) To every great there exists a greater. Empedocles (483-425) The universe is three times as large as the system earth moon. Democritus (460-375) Milky way consists of many stars. The universe has no center. Aristotle (384-322) The earth is tiny compared to the universe. The earth is in the center of the universe. When sailing to south always new stars appear: The earth is a sphere.

Aristarchus of Samos (310-230) First proponent of the heliocentric system His hypotheses are that the fixed stars and the sun remain unmoved, that the earth revolves about the sun on the circumference of a circle, the sun lying in the middle of the orbit, and that the sphere of fixed stars, situated about the same center as the sun, is so great that the circle in which he supposes the earth to revolve bears such a proportion to the distance of the fixed stars as the center of the sphere bears to its surface. (reported by Archimedes)

Aristarchus of Samos (310-230) First proponent of the heliocentric system Ratio of distances to moon and sun Angle measured: 87°  cos 87° = 1 : 19 Improved by Kepler: 89°51'  1 : 380

Eratosthenes (276-194) Born in Cyrene (today Schahhat, Libya) 240: third chairman of the Museion Educator of the crown prince Very universal scholar Invented the leap day. Produced the first astronomical map with over 600 stars. Mesolabium, doubling the cube Commited suicide when gone blind. Sieve of Eratosthenes

Determined the circumference of the earth. Alexandria (31°) Well diggers in Syene (= Assuan, 24°) Result: 41000 km improved in 1670: 39800 km correct: 40009 km (measured over the poles)

Titus Lucretuius Carus (95-55) The universe is not bounded in any direction. Otherwise there had to exist a border. But then something had to exist at the other side. Claudius Ptolemaios (85-165) Worked in Alexandria Fair skin, small feet, red birthmark at his chin, black beard ??? Geocentric system Deferent Epicycle

Nicolaus Copernikus (1473-1543) 1510: Foundations of his heliocentric system. 1543: De revolutionibus orbium coelestium

Nicole d‘Oresme (1320-1382) Heliocentric system. The revolution of earth explains the movement of the stars. Jean Buridan (1295-1363) Prof. at Univ. Paris Concept of impetus (inertia) Thought like Oresme. Buridan's donkey Nikolaus Cusanus (1401-1464) Cardinal The universe is endless. It has no centre and looks the same from every position.

William Gilbert (1544-1603) Physicist and physician Invented the word electricity 1651: De mundo nostro sublunari The Gilbert-epoch is a paleomagnetic epoch 4.5-3.3 million years ago with reversed direction of the terrestrial magnetic field.

Thomas Digges (1546-1595) Dark sky paradox 1576: Infinite World "But there can be no movement of infinity and of an infinite body, and therefore no diurnal revolution of that vastest Primum mobile."

Tycho Brahe (1546-1601) 1599 imperial mathematician and astronomer in Prague Refused Copernican circles and epicycles because of his better data. All planets revolve around the sun, but the sun revolves around the earth. Declined to accept crystal spheres. 1600 employed Kepler as his assistant. Johannes Kepler (1572-1630) Accepted the Copernican system. Found the laws of planetary motion, based on Brahe's precise measurements. "The universe is unmeasurably great."

Giordano Bruno (1548-1600) Dominican, accused of heresy. Escaped to Germay, France, England and taught there. Was promised to remain untouched and returned in 1592. The inquisition nevertheless caught and imprisoned and charged him of heresy and burnt him in Rome at the stake. Most important natural philosopher of the renaissance. There are infinitely many inhabited worlds. The universe has no border, it cannot grow nor shrink nor move. It has not been created and cannot cease.

Edmond Halley (1656-1742) 1720 second Astronomer Royal and director of the Greenwich-observatory. Formula for barometric detemination of altitude. Calculated the trajectories of 24 comets, tree of them 1531, 1607, and 1682, were so similar that he recognized them as only one comet: Today called comet Halley with a period of 76 years. Halley pedicted its return for 1759 but did not live to see it. "I have heard urged that if the number of Fixt Stars were more than finite, the whole superficies of their apparent Sphere would be luminous ..."

Thomas Wright (1711-1786) 1750 first explanation of milky way. Nebulae are distant galaxies. Immanuel Kant (1724 - 1804) 1770: Professor of logic und metaphysics 1786-88: Rector of Königsberg university One of the greatest German philosophers founded by his three critiques a new epoch of philosophy. 1754: Tides caused by the moon. Responsible for its bounded rotation. 1755: There are many Welteninseln. Kant's elaboration of the nebular hypothesis founded the scientific cosmogeny.

Astronomer and physician at Bremen Heinrich Olbers (1758-1840) Astronomer and physician at Bremen Olbers' paradox: Why is the sky dark at night? Solid angle covered by a star ~ A/r2 Number of stars in a spherical shell ~ r2Dr Solid angle covered by stars of a shell ~ ADr Stars of infinitely many shells cover the whole sphere. r

Friedrich Wilhelm Bessel (1784-1846) First merchant, then professor of astronomy and director of the observatory at Königsberg, supported by Olbers. 1838 first measuremet of the distance of a fixed star: Angular difference in summer and winter: Parallax 0,5'' = 1/3600 angular diameter of the moon.  11 light years distance. From the ondulatory motion of Sirius he concluded the existence of an unseen companion.

Vesto Slipher (1875-1969) 1912 measured redshift of galaxies. 36 of 41 galaxies move off of us. Edwin Hubble (1889-1953) found, using the 254-cm-reflector on Mount Wilson, Andromeda nebula consists of stars, among them variables with known absolute brightness.  2 mio light years distance. 1929: Expansion of the universe. Hubble-constant: v = Hr. Finite universe with Doppler-redshift Expansion of the universe started 13.7109 years ago. age = 4.31017 s radius: 46.5109 light years

George Gamow (1904-1968) 1949: predicted cosmic background radiation remaining from the big bang. Arno Penzias (*1933) Robert Woodrow Wilson (*1936) 1965: Discovery of cosmic background radiation

2,7 K Maximum at l = 1,1 mm 375 photons / cm3

3 March 1972: Start of Pioneer 10 Directions of 14 pulsars including present frequencies. Binary numbers in units of the length and frequency of the hydrogen molecule. Pioneer 10 left the solar system at 12 June 1983. Last signal received at 22 Jan 2003 from 11 light hours distance. After 2 mio years it will meet Aldebaran (67 light years away). The closest man has ever come to infinity.

Voyager I took this picture 18 September 1977 from 11 million km away. The spacecrafts will probably survive mankind and earth.

The earth at a distance of 6 billion km (Voyager I)

Two things are infinite: The universe and human stupidity. With the universe I am not totally sure.

Radius of the universe = 46.5109 lightyears Volume of the universe = 1080 m3 1080 atoms 1088 photons 1080 m3 / (10-95 m)3  less than 10365 elementary cells

Appendix

n-dimensional Cube Diagonal an Circumference 4a the zero-dimensional interval is the point the one-dimensional interval is the set {x  0  x  a} the two-dimensional interval {(x1, x2)  0  x1  a, 0  x2  a} the three-dimensional interval {(x1, x2, x3)  0  xn  a} the four-dimensional interval {(x1, x2, x3, x4)  0  xn  a} ... Diagonal an Circumference 4a an 2n 2V/a One-dimensional (linear) beings populating the surface (edges) of a square have to go 4a for a full circumnavigation of their world. Two-dimensional (areal) beings populating the surface of a three-dimensional square (cube) have to go 4a for a full circumnavigation of their world. Three-dimensional (spatial) beings populating the surface of a four-dimensional cube have to go 4a for a full circumnavigation of their world. A 4d cube can be imagined as a 3d cube moving or growing or shrinking on the time axis. Each of its six areas gives a cube, just like initial and final state.

n-dimensional Sphere: {(x1,x2,x3,...,xn)  0 Sxn2 r2 } Volume: (n-1)-dimensional Surface: {(x1,x2,x3,...,xn)  Sxn2 = r2 } Area: An = Vn/r Diameter 2r Circumference 2pr One-dimensional (linear) beings populating the surface (periphery) of a circle have to go 2pr for a full circumnavigation of their world. Two-dimensional (areal) beings populating the surface of a three-dimensional circle (sphere) have to go 2pr for a full circumnavigation of their world. Three-dimensional (spatial) beings populating the surface of a four-dimensional sphere have to go 2pr for a full circumnavigation of their world. Universe: r = 46.5 billion light years, so we have to travel c. 300 billion light years.