Get A Journey through the Universe: Gresham Lectures on PDF

By Ian Morison

ISBN-10: 1107073464

ISBN-13: 9781107073463

Delivering an in-depth realizing either for normal readers and astronomy fanatics, this hugely finished publication presents an up to date survey of our wisdom of the Universe past Earth. The ebook explores our sun process, its planets and different our bodies; examines the solar and the way it and different stars evolve via their lifetimes; discusses the quest for planets past our sunlight procedure and the way we would observe existence on them; and highlights attention-grabbing gadgets came across inside our galaxy, the Milky method. It additionally seems at our present figuring out of the foundation and evolution of the Universe, in addition to many different fascinating subject matters, corresponding to time, black holes and Einstein's theories, darkish subject, darkish power and the Cosmic Microwave history. The ebook is uniquely supported via video lectures given through the writer, to be had on-line. it is also the very most recent astronomical observations, resembling these made through the Planck and Kepler spacecraft.

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Additional info for A Journey through the Universe: Gresham Lectures on Astronomy

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000055% of the atmosphere! In contrast, consider Jupiter: its escape velocity is 60 km/s and it has a surface temperature of only 100 K. In the Jovian atmosphere, the speed of the hydrogen molecules is only about 1 km/s, 60 times less than the escape velocity, and so Jupiter has been able to keep the hydrogen as the largest constituent in its atmosphere. In summary Mercury, the Moon and all satellites except for Titan and Triton have effectively no atmospheres, though Mercury has an extremely thin ‘transient’ atmosphere of hydrogen and helium temporarily captured from the solar wind.

Sunspots are intimately linked to this differential rotation and how it affects the Sun’s magnetic field. The Sun’s field must be created by the movement of charged particles and its cause almost certainly lies in the convective zone, but no really good model yet exists. Imagine that at one particular moment the Sun has a uniform bipolar field just like that shown by iron filings under the influence of a bar magnet. Looking at the Sun’s face we could imagine a field line directly down the centre of the Sun’s disc that lies just below the photosphere.

The umbra has a typical temperature 1,000 K less than its surroundings. Around the outside of a sunspot group may be seen an area that is brighter than the normal surface. This is called a ‘plage’ – the French word for a beach. ) The passage of sunspots across the Sun’s surface has been used to measure its rotation period. It has been found that at the equator the period is ~28 days, but this increases with increasing latitude and is ~35 days near the Sun’s poles, an effect called differential rotation.

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A Journey through the Universe: Gresham Lectures on Astronomy by Ian Morison


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