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STAR CHART NORTHERN HEMISPHERE

A clear is a thing of beauty and wonder. Thousands of scattered twinkle in the darkness. What are the stars? Over the past century or so have by observation and calculation established the true nature of these gleaming specks. Now we know that stars are basically enormous balls of very hot gas, mainly hydrogen, with some helium and small amounts of a few other things. Inside the huge quantities of energy are generated by a nuclear process called fusion. Planets, in contrast are balls of rock, metal and gas with no internal nuclear energy source. Earth is a planet, while the sun is a star.

Stars come in different brightnesses, sizes and colours. Look out at the sky tonight and you will see how stars vary in brightness. Some are bright because they are relatively close to us, while others are bright because they are thousands of times brighter than our own nearby Sun. Find the easily-spotted of the hunter. There you will see the red star Betelgeuse in his shoulder, the bluish white Rigel in his foot. To bring order to star catalogues, astronomers classify stars into what are called spectral types. This means stars are listed and placed in an order based on the temperature and brightness of their surfaces and the characteristics of the spectrum of light they shine out. In order of brightest to dimmest star, the sequence runs OBAFGKM. Here is the classification sequence with a rough guide to how common each type is.

• O- blue-white, brightest and hottest (30 000°C or more). About 1 star in every thirty thousand is type O. • B- white, very bright stars. About 1 star in every thousand is type B. • A- bluish white stars. About 1 star in a hundred is type A. • F- yellowish white stars. About 1 star in thirty is type F. • G- yellow stars (about 5500°C). About 1 star in fifteen is type G, eg the Sun. • K- orange stars, not as bright as the Sun. About 1 star in eight is type K. • M- red stars (about 3500°C). About four out of five stars are type M. 2009 ODYSSEY SPACE

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reddish surfaces, cool by stellar standards. In the distant future our Sun is Sun our future distant the In standards. stellar by cool surfaces, reddish

this great show above our heads. Happy star-gazing! Happy heads. our above show great this energy using other fuels, swelling enormously into huge bloated stars with stars bloated huge into enormously swelling fuels, other using energy

but most marvellous of all is to step into the night to look up wonder at wonder up look to night the into step to is all of marvellous most but stars which have run out of hydrogen in their cores and are instead generating instead are and cores their in hydrogen of out run have which stars

Studying the great cosmic drama of stellar life and death is fascinating, is death and life stellar of drama cosmic great the Studying heat and light as a by-product. The red giants are another group. These are These group. another are giants red The by-product. a as light and heat

converting hydrogen into helium in their hot, seething centres and producing and centres seething hot, their in helium into hydrogen converting

that not even light escapes its gravitational grip. gravitational its escapes light even not that Our Sun is a main sequence star. These are stars in their prime of life, steadily life, of prime their in stars are These star. sequence main a is Sun Our

leave behind the strangest object of all; a black hole, matter crushed so tightly so crushed matter hole, black a all; of object strangest the behind leave

corpse is called a neutron star. Larger still stars will explode in a supernova but supernova a in explode will stars still Larger star. neutron a called is corpse groups. The most important group is the ‘main sequence’. ‘main the is group important most The groups.

tiny shrunken remnant composed of strange superdense matter. Such a stellar a Such matter. superdense strange of composed remnant shrunken tiny important diagram in astronomy. It shows that stars are divided into several into divided are stars that shows It astronomy. in diagram important

Debris from the explosion forms a great cloud or . At the centre remains a remains centre the At nebula. or cloud great a forms explosion the from Debris Scientists call this the Hertzsprung-Russell diagram and it is the most the is it and diagram Hertzsprung-Russell the this call Scientists

is a giant star tearing itself to pieces in nature’s most destructive detonation. destructive most nature’s in pieces to itself tearing star giant a is plot a graph of stars’ spectral type against their actual brightnesses. actual their against type spectral stars’ of graph a plot

giant stages terminate in cataclysmic explosions called supernovae. A supernova A supernovae. called explosions cataclysmic in terminate stages giant our Sun is one of the biggest and brightest stars in the . It is possible to possible is It galaxy. the in stars brightest and biggest the of one is Sun our

fate of our Sun. Stars larger than ours have more spectacular ends: their red their ends: spectacular more have ours than larger Stars Sun. our of fate dimmer than our Sun, and only about 3% are significantly brighter. So actually So brighter. significantly are 3% about only and Sun, our than dimmer

balls of dense matter not much bigger than a planet. This will be the ultimate the be will This planet. a than bigger much not matter dense of balls see. It is clear that most stars (about 9 out of 10) are actually smaller and smaller actually are 10) of out 9 (about stars most that clear is It see.

continuing to glow like dying embers until they have slowly cooled to cold black cold to cooled slowly have they until embers dying like glow to continuing than the Sun, also means that most stars in the galaxy are too dim for us to us for dim too are galaxy the in stars most that means also Sun, the than

dwarf. White dwarf stars no longer produce light by nuclear fusion, merely fusion, nuclear by light produce longer no stars dwarf White dwarf. naked eye. The fact that the majority of stars we see in the sky are brighter are sky the in see we stars of majority the that fact The eye. naked

space. The tiny shrunken core, about the size of the Earth, remains as a white a as remains Earth, the of size the about core, shrunken tiny The space. stars to the Sun, 80 are M-type red dwarf stars, too dim be seen with the with seen be dim too stars, dwarf red M-type are 80 Sun, the to stars

the process until eventually all the star’s outer layers have been blown away into away blown been have layers outer star’s the all eventually until process the stars in space, at least in our part of the Milky Way galaxy. Of the 100 closest 100 the Of galaxy. Way Milky the of part our in least at space, in stars

experience huge internal eruptions, blasting off great concentric shells of gas in gas of shells concentric great off blasting eruptions, internal huge experience smaller than our Sun are classed as dwarf stars) seem to be the most common most the be to seem stars) dwarf as classed are Sun our than smaller

These are essentially the cores of dead stars. Red giant stars are believed to believed are stars giant Red stars. dead of cores the essentially are These the Sun, actually small and dim M type stars called red dwarfs (stars physically (stars dwarfs red called stars type M dim and small actually Sun, the

fated to become one of these red giants. A third group are the white dwarfs. white the are group third A giants. red these of one become to fated Although the vast majority of stars we see in the night sky are brighter than brighter are sky night the in see we stars of majority vast the Although

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