* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Our Place in the Cosmos
International Year of Astronomy wikipedia , lookup
International Ultraviolet Explorer wikipedia , lookup
De revolutionibus orbium coelestium wikipedia , lookup
Lunar theory wikipedia , lookup
Hubble Deep Field wikipedia , lookup
Rare Earth hypothesis wikipedia , lookup
Formation and evolution of the Solar System wikipedia , lookup
Astronomical unit wikipedia , lookup
Theoretical astronomy wikipedia , lookup
Outer space wikipedia , lookup
Shape of the universe wikipedia , lookup
History of Solar System formation and evolution hypotheses wikipedia , lookup
Dark energy wikipedia , lookup
Observational astronomy wikipedia , lookup
Astrobiology wikipedia , lookup
Wilkinson Microwave Anisotropy Probe wikipedia , lookup
Ultimate fate of the universe wikipedia , lookup
Fine-tuned Universe wikipedia , lookup
Future of an expanding universe wikipedia , lookup
Observable universe wikipedia , lookup
History of astronomy wikipedia , lookup
Flatness problem wikipedia , lookup
Expansion of the universe wikipedia , lookup
Cosmic microwave background wikipedia , lookup
Extraterrestrial life wikipedia , lookup
Dialogue Concerning the Two Chief World Systems wikipedia , lookup
Physical cosmology wikipedia , lookup
Chronology of the universe wikipedia , lookup
Ancient Greek astronomy wikipedia , lookup
Non-standard cosmology wikipedia , lookup
Copernican heliocentrism wikipedia , lookup
Our Place in the Cosmos and Introduction to Astrophysics Lecture 2 Historical Milestones in Astronomy The Ancient Greeks By far the most famous early astronomers are the ancient Greeks. Between about 500BC and 100BC, they built a picture of the Universe which dominated for over 1000 years. Thales (624 - 545 BC) Realised that celestial objects were at different distances, that the Earth was spherical, and that the light of the moon was reflected sunlight. Pythagoras (582 - 500 BC) Produced the first geocentric model of the Universe, with everything making perfectly circular orbits around the Earth. Geocentric Model Problem: Retrograde Orbits Plato (428 - 347 BC) Invented the idea of epicycles, later `perfected’ by Ptolemy. Aristarchus of Samos (310-230 BC) He created the first heliocentric cosmology; that is, he was the first to propose that the Earth, and the other planets, went around the Sun. 1,750 years later Copernicus will claim the credit. Aristarchus is also famous for devising a way of measuring the size of the moon in terms of the size of the Earth. Hipparchus later used this to conclude that the moon had about one quarter the radius of the Earth (modern value 0.27) and that its distance was about 60 Earth radii away (modern value 60.4). However, his calculations did not give absolute values; only those relative to the unknown radius of the Earth. Aristarchus also measured the relative distances of the Sun and Moon. He underestimated that badly, but even so realised that the Sun was bigger than the Earth. Eratosthenes (276 - 195 BC) Measured the circumference of the Earth with amazing accuracy. He did so with a particularly powerful piece of observational technology, namely a long stick. Hipparchus (190 - 120 BC) Powerful insights into many aspects of astronomy. Invented the magnitude scale, worked out the size of the moon, developed star and eclipse catalogues. Ptolemy (~85 - 165 AD) Perfected the geocentric model with epicycles. It will go unchallenged for 1300 years. Ptolomey’s revised epicycle mode See also http://astro.unl.edu/naap/ssm/animations /ptolemaic.swf Nicolaus Copernicus (1473-1543) Credited with the heliocentric model of the Solar System. He divided the planets into the `inferior’ ones closer to the Sun than the Earth, and the `superior’ ones outside the Earth’s orbit. Only planets out to Saturn were known at that time. The orbits were all taken as circular. Finally we shall place the Sun himself at the centre of the Universe. All this is suggested by the systematic procession of events and the harmony of the whole Universe, if only we face the facts, as they say, `with both eyes open'. Nicolaus Copernicus Tycho Brahe (1546 - 1601) Almost as famous for his silver nose (he lost the original in a duel) as for his observations. With the support of the King of Denmark, he developed instruments of unprecedented quality, capable of positional accuracies of one arcminute. He is less remembered for his cosmological model, an attempted compromise in which the Sun goes round the Earth but the planets round the Sun. Johannes Kepler (1571-1630) Painstaking studies of Tycho’s observations led him to the nowaccepted conclusion that planets moved not on circles but on ellipses. He went on to formulate his three laws of planetary motion, which we will be studying in a later lecture. Galileo Galilei (1564 -1642) • Didn’t invent the telescope (and might well not have dropped cannonballs off the leaning tower of Pisa either). • But he is considered the inventor of the modern scientific method, with its emphasis on experimental verification of theoretical models. Galileo was the first to properly exploit the telescope for astronomical purposes. Considering that his original telescope had a magnification power of only three, he made amazing new discoveries, including the four large moons of Jupiter, sunspots, and the rings of Saturn. GALILEO NOW His belief in Copernicus’s heliocentric Universe nearly led him to a nasty end. Isaac Newton (1643 - 1727) Widely acknowledged as one of the greatest scientific geniuses of all time. Co-inventor of calculus and founder of the modern theories of dynamics and optics, he also developed a theory of gravity. His theory explains Kepler’s Laws, and shows that the gravity we feel on Earth is the same as the gravity that governs planetary orbits. Despite the development of the telescope, it would be many years before the remaining planets of the solar system were discovered. Uranus was discovered in 1781 by William Herschel. Neptune was first observed in 1846, after its position was predicted by Adams and Leverrier by analysing perturbations to the motion of Uranus... … while Pluto was not discovered until 1930, and its moon Charon only in 1978. Albert Einstein (1879 - 1955) Made numerous vital contributions to physics, the most relevant for astronomy of which is his general theory of relativity (GR) , a new law of gravity which supplanted that of Newton GR unifies space and time into a single entity: space-time GR in words Gravity is caused by the curvature of spacetime; the curvature is induced by the presence of matter “Matter tells space how to curve, space tells matter how to move” (John Wheeler) Light rays are bent when they pass near a large mass, a prediction confirmed by Arthur Eddington in 1919 Edwin Hubble (1889-1953) Discovered in 1929-30 that some nebulae lie outside our Galaxy and that these objects are receding from us at a speed proportional to their distance, the Hubble expansion The expanding Universe Expansion causes redshift Hubble Law Discovery of Cosmic Microwave Background Once Hubble had discovered the expansion of the Universe, cosmological models predicted a Universe of infinite density in the past: the Big Bang cosmology This theory widely accepted once Arno Penzias & Robert Wilson accidentally discovered the Cosmic Microwave Background (CMB) radiation in 1965, a low-temperature (3K) relic of the hot big bang fireball Dark Matter Swiss astronomer Fritz Zwicky was first to suggest in the 1930s that much of the matter in the Universe is in some dark, unseen form Not taken seriously until the 1970s, when evidence from rotation curves of spiral galaxies became compelling Detection of CMB anisotropies Cosmic Background Explorer (COBE) satellite, launched in 1989, made the first detection of anisotropies in the CMB radiation 2006 Nobel Prize in Physics awarded to COBE principal investigators John Mather and George Smoot “for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation" Accelerating Universe Ever since Hubble’s discovery of the expansion of the Universe, it was widely assumed that expansion rate would slow down due to gravitational pull of matter in the Universe In the late 1990s, surveys for distant supernovae showed the surprising result that they were fainter than expected in a matter-dominated Universe Observations indicated that the expansion of the Universe is in fact accelerating, due to presence of a cosmological constant or dark energy “Precision Cosmology” Era COBE (1989) WMAP (2003) Outstanding Questions What are the dark matter and dark energy? Is Einstein’s model of gravity correct? How do galaxies form? Is there other life in the Universe? Seminar 1 Presentation Signup 20% of course marks will come from a 10minute presentation Sign up on Study Direct 3 talks per seminar slot Sign up soon for greatest choice! Topics for Discussion What do you hope to get from this course? What is a scientific model and what must the model be able to do to be useful? How can an incorrect scientific theory still be considered a good scientific theory? What distinguishes a scientific truth from a religious truth? How is astrology different from astronomy? Discussion contd. What two basic kinds of models have been proposed to explain the motions of the planets? What is the Ptolemaic model? What new things did Ptolemy add to his model? In what ways was the Ptolemaic model a good scientific model and in what ways was it not? What is the Copernican model and how did it explain retrograde motion? What important contributions did Tycho Brahe make to astronomy?