History of Astronomy Evening Classes Week Four Presented by Oisín Creaner.

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Presentation transcript:

History of Astronomy Evening Classes Week Four Presented by Oisín Creaner

The History of Astronomy 3200 BC to Present. 1.Prehistorical Astronomy 2.Greek and Arab Astronomy 1.Renaissance to Instruments 1.Modern Astrophysics

Newgrange Passage Tomb, Co Meath Built 3200BC Light Box Aligned On Winter Solstice Newgrange Image Jimmy Harris

(1)Greeks were great theorists, but poor observers or experimenters. (2)Greeks used Babylonian records & Greek geometry. (3)Ionians (c 600 BC) - first Greek cosmology. Impersonal laws replace mythology. GREEK ASTRONOMY (650 BC AD).

Pythagoras

Aristarchus ( BC) - How to measure the relative distances between the Earth, Sun and Moon

(4)Pythagoreans (c 600 BC) - saw numbers as the basis of reality + wrote of a spherical earth. GREEK ASTRONOMY (650 BC AD).

Aristotle & Plato (5)Aristotle (fl 350 BC)- Round earth at the centre of the cosmos. Aristotle's cosmology is rooted in common sense & rationality.

Aristotle’s Cosmology Earth is at Rest Earth is Round Earth is the Centre of the cosmos

(6) Celestial Sphere's motions are predictable, what about the 7 planets? Plato (fl 400 BC) challenged geometricians to describe planetary motion in lawful terms. This became Astronomy's project for next 2000 years. GREEK ASTRONOMY (650 BC AD).

(7) The most elaborate Greek astronomer. The "Almagest“ (c 145 AD) gave mathematical model of planet's motions that could be calculated for any date, past or future. Ptolemy of Alexandria

Arab Medieval Astronomy Early formal catalogues Names of brigtest stars Refined Greek Models Doubts about Ptolemy Advanced Mathematics Calculated movement

Arab Medieval Astronomy

History of Astronomy Evening Classes Week Four Presented by Oisín Creaner

Nicholas Copernicus

Tycho Brahe (14 December 1546 – 24 October 1601)

Johannes Kepler

Galileo Galilei

Isaac Newton( )

When white light is passed through a prism it is split up into its component colours.

William Herschel

Otto Struve Used parallax measurements to determine distance to nearby stars.

Robert Bunsen ( ) Gustav Kirchoff ( ) Elements are identified in sunlight

The Spectroscope

Frauenhofer Lines Angelo Secchi’s Stellar Spectra Classification

Sirius Type Stars Sun-like stars Red-Giant Variables Red-dwarfs

Christian Doppler

Crab Nebula (M1) Original SN1054 Lord Rosse Observed 1848 Messier Catalogue Long observation

John Herschel ( ) Pioneer of Astrophotography

Herman von Helmholtz Suggested that gravitational contraction was the source of the Sun’s energy.

Edwin Hubble “The spiral nebulae are receeding at speeds proportional to their distances”

Hans Bethe Worked out that sunlight comes from hydrogen fusion (1939).

Post WW 2 The observable spectrum is broadened

Thank You Useful websites