By Pierre-Yves Bely

Are we on my own within the Universe? was once there whatever sooner than the massive Bang? Are there different universes? What are sunspots? what's a taking pictures celebrity? was once there ever lifestyles on Mars? This publication solutions the attention-grabbing questions that we've got been asking ourselves for centuries. utilizing non-technical language, the authors summarize present astronomical wisdom, taking care to incorporate the real underlying medical ideas. ample colour illustrations, graphs and pictures lend additional weight to their easy but meticulously written motives. an in depth bibliography enables you to pursue or recap at the matters that rouse your specific curiosity. Dip in to find and study interesting proof approximately our sunlight approach and the Universe past!

Show description

Read Online or Download A Question and Answer Guide to Astronomy PDF

Similar astronomy & astrophysics books

The Origin and Evolution of the Solar System, Institute of Physics, 1st Edition

Contents half 1 the final historical past: The constitution of the sunlight method. Observations and theories of big name formation. What may still a conception clarify? half 2 atmosphere the theoretical scene: Theories as much as 1960. half three present theories: a quick survey of contemporary theories. The sunlight, planets and satellites.

The Cambridge Double Star Atlas

This excellent atlas includes the main beautiful and engaging double and a number of stars for viewing with binoculars and telescopes. it's a must-have for stargazers who are looking to discover those interesting items. the 1st smooth megastar atlas dedicated to double and a number of stars, it plots over 2,000 chosen pairs of stars, each one categorised with discoverer, catalog, and/or observatory designations.

Archaeoastronomy in the Old World

This quantity summarises the complaints of a convention which came about on the college of Oxford in September 1981. Held below the auspices of the foreign Astronomical Union and the foreign Union for the historical past and Philosophy of technology, the assembly reviewed examine in previous global Archaeoastronomy.

Jaghmīnī’s Mulakhkhaṣ: An Islamic Introduction to Ptolemaic Astronomy (Sources and Studies in the History of Mathematics and Physical Sciences) (English and Arabic Edition)

This e-book presents the one serious version and English translation of Maḥmūd al-Jaghmīnī’s al-Mulakhkhaṣ fī al-hayʾa al-basīṭa, the main broadly circulated Arabic treatise on Ptolemaic astronomy ever written. Composed within the early thirteenth century, this introductory textbook performed a vital position within the instructing, dissemination, and institutional guide of Islamic astronomy good into the 19th century (and beyond).

Additional info for A Question and Answer Guide to Astronomy

Sample text

Simultaneously, there is further expansion of the outer layers, making the star even larger. When the core’s helium is exhausted, it contracts. This heats it up again, and it now expels its outer atmosphere to Small mass star Medium mass star 18 Stars The planetary nebula, Abell 39, with at its center the star that ejected it. The nebula is an envelope of hydrogen and other trace elements illuminated by the light of the star. Credit: NOAO/AURA/NSF. eta rfs † wa eb. ry N D ite n Pla Wh Mass of the main sequence stars relative to the mass of the Sun ae nov per ants ergi Sup Su form a planetary nebula.

Their Spinning period is typically about 1 s, but some rotate as neutron star S fast as once per millisecond, 100 times faster on ti ia d ra N f Beam o radiation than a power drill. The period can be extremely Beam of stable, constant to within a few seconds over a million years – more accurate than the best atomic clocks on Earth. A pulsar forms when a supernova explodes, leaving a neutron star in place of the original stellar core (Q. 16). The original star revolved slowly on its axis (like our Sun, which rotates once in 27 days), but as it collapsed into an extremely small, compact neutron star, its speed increased – like an ice skater pirouetting (Q.

Above this zone, the density is so low that the layers again become transparent to radiation. This layer, the surface layer of the Sun called the photosphere, is at a temperature of 5800 K. From here, photons escape freely into outer space and it is this last layer that we see when we look at the Sun. The sudden change of opacity makes Corona Chromosphere What causes sunspots? 43 its edge look very sharp, giving the impresChromosphere sion that the Sun has a distinct, crisp surCorona face, but it is actually just gaseous, like the rest of the Sun.

Download PDF sample

Rated 4.63 of 5 – based on 50 votes