Wednesday, 26 September 2012

Bright New Comet on the Way




Bright New Comet on the Way
There’s another comet on the way. And this might be a great one. Called Comet C/2012 S1 (ISON), this comet is about as far away as Jupiter, but it’s expected to buzz the Sun late next year and, if it stays intact, may become as bright as the full Moon.

The comet was discovered by a Russian team of astronomers at the International Scientific Optical Network (ISON). At magnitude +18, the comet is currently beyond the reach of amateur telescopes. But the orbital elements have been calculated, and they show the comet will come amazingly close to the Sun– just 2 million km— on November 28, 2013. In mid-November through December 2013 and into January 2014, the comet may reach negative magnitudes, possible as bright as -11 to -16, which means it will be visible during the day!

Because their composition is not exactly known, each comet is unpredictable. So no one can knows for sure how bright this comet will become, or if it will survive its close encounter with the Sun.  Still, this is promising news. And this comet, unlike many recent bright comets, will be visible at mid-northern latitudes.

Southern stargazers will get their own bright comet next year. Comet Pan-STARRS is expected to become visible without optical aid next March, and come within 45 million km of the Sun on March 9, 2013.

So get your binoculars, telescopes, and cameras ready. Next year should be a good one for bright comets, perhaps the best year since 1996 when Comets Hyakutake and Hale-Bopp graced our skies…

Tuesday, 25 September 2012

Braai Facts: The sun loses 4 million tons of mass per second.



Some facts when you hit that silent moment at a boring braai: 

The sun becomes four million tonnes lighter every second (not minute or hour -  every second).  If there is no reaction. Leave the braai immediately and go home!

It is because  of the fussion taking place in its core. Every second  600 million tonnes of hydrogen are turned into 596  million tonnes of helium. That means that 4 million tonnes goes missing every single second.  That mass is converted into energy, giving us some sunlight.

Why is it not running out of "steam"?  It's total mass is two thousand million  million  million  million tonnes.

Chew on that!

Source:  The Sky at Night. Answers to Questions from Across the Universe -  Patrick Moore and Chris North.