By Jayant V. Narlikar

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A G ... , " .. o .. "" c" . ·.. n - .. : o .. , '. -, - -- "-? +5 • " 0" " . l":_r, 3! &> ~ + 10 o . 0' BO - 0 ·2 , 85 AD 0 -0 FO GO 0 ·6 KO tAO M 'S 1-6 Spectral type/Colour ind e x A typical H-R diagram. The Sun's position is shown by S. The absolute magnitude and spectral typelcolour index indicate [he star's luminosity and surface temperature respectively. bottom right hand corner (cool and faint stars). This band is called the 'main sequence' . As we shall see, a star spends most of its life on the main sequence .

While the rnaioritv of astronomers accept this 'relic' inrerp reta60 Penzias and Wilson in front of their microwave antenna that led to the discovery of the all-pervading microwave radiation. non of the radiation, there are still some outstanding difficulties WIIh this scenario . For example, II is a mystery that the microwave background IS found to be so smooth. If it is a relic of the early epochs why does II not carry clear imprints of the events that led to 61 the formation of galaxies? And so, the question as to whether the Universe originated in a big bang has been answered in the affirmative by the majority but not by all astronomers.

1M ...... ..... tf $0 1I1t1/_ . eI. Known as Hubble's law, this conclusion dramatically changed our view of the Universe. It led to the idea that the Universe is 'expanding'; the galaxies are moving away from one another much like the dots on a balloon that is inflated. And , of course, there is nothing special about our Galaxy. If we were to look at the Universe from another galaxy, we would notice the same thing : other galaxies would be seen moving away from our new vantage point. 28 ) How far does this expansion extend?

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