Download PDF by Editor Jon White: All About Space Book of the Solar System

By Editor Jon White

ISBN-10: 1909758485

ISBN-13: 9781909758483

All approximately house e-book of the sunlight procedure
The Sun
- realize the important function the celebrity on the center of our sunlight approach playsThe planets
- In-depth courses to all of the planets, from Mercury to NeptuneThe moons
- Take a better examine many of the sun structures finest moonsAmazing illustrations
- discover the lovely attractions on offerAlso inside...
- a whole consultant to the Sun
- sunlight flares
- the outlet within the Sun
- sunlight maximum
- Mercury
- Venus
- Earth
- Mars
- Jupiter
- Saturn
- Uranus
- Neptune
- a glance at Earths moon
- Ganymede
- Europa
- Titan

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Aurorae were visible across the planet, almost down to equatorial latitudes Satellites A variety of orbiting spacecraft were affected, as the storm blocked contact with geostationary weather satellites for several hours. ” Another aspect of the sunspot cycle, meanwhile, gives rise to one of the most iconic diagrams in all of science. By recording not just the number and size of sunspots, but also their latitude on the surface of the Sun, English astronomer Edward Maunder discovered a steady drift in latitude throughout each cycle, with spots first 34 appearing in small numbers at high latitudes in each hemisphere, peaking around mid-latitudes, and dying away as the remaining spots converged on the equator.

Aurorae were visible across the planet, almost down to equatorial latitudes Satellites A variety of orbiting spacecraft were affected, as the storm blocked contact with geostationary weather satellites for several hours. ” Another aspect of the sunspot cycle, meanwhile, gives rise to one of the most iconic diagrams in all of science. By recording not just the number and size of sunspots, but also their latitude on the surface of the Sun, English astronomer Edward Maunder discovered a steady drift in latitude throughout each cycle, with spots first 34 appearing in small numbers at high latitudes in each hemisphere, peaking around mid-latitudes, and dying away as the remaining spots converged on the equator.

Bow shock This boundary where the solar wind meets the magnetosphere is about 1,900 kilometres (1,181 miles) above the surface Solar wind Without a strong magnetic field of its own, Venus’s atmosphere is hit with this electrically charged stream of particles from the Sun The structure of Venus Crust Venus’s crust is mainly made up of silicate rocks Mantle Magnetosphere Venus’s magnetosphere is solely induced by the solar field’s interaction with Venus’s atmosphere 56 Magnetotail The solar wind’s pressure on the magnetosphere creates a taillike structure of plasma flowing away from the planet The mantle is likely rocky and similar in composition to Earth's Core The core is probably molten metal, but how much of it is liquid and how much is solid remains a mystery Venus The greenhouse effect on Venus How Venus’s extreme and inhospitable temperatures are created Incoming sunlight Reflected sunlight Most of the sunlight passing through Earth’s atmosphere makes it through.

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All About Space Book of the Solar System by Editor Jon White


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