Guide to the Cosmos

December 16, 2010 

 

Newsletter: More Stars, Big and Small, for the Holidays

 

Just in time for the holiday season, astronomers have announced the discovery of new stars—trillions of little red elves and one giant Santa.

 

The new Santa is over 250 times more massive than our Sun, and ten million times brighter. R136a1 lies in the Large Magellanic Cloud, a satellite galaxy of our Milky Way, and has over twice the mass of the prior record holder. Unlike humans, stars are born heavy, this one at over 300 solar masses, progressively shed weight throughout their lives. The real heavyweights die in spectacular explosions called supernovae. In the illustration below from the European Space Agency, the yellow star represents our Sun and R136a1 is the mammoth blue star. That’s one super-sized HO, HO, HO.

 

 

At the opposite end of the stellar spectrum are red dwarfs; one is illustrated above. Red dwarfs are just barely massive enough to sustain nature’s ultimate fire—nuclear fusion, the process that powers all stars. These stars often have only one-tenth of our Sun’s mass and emit thousands of times less energy. Because they are so dim, counting them is a real challenge. New results from Yale indicate that red dwarfs are far more common in elliptical galaxies than in spiral galaxies like ours—perhaps 30 times more common. This means prior estimates, which were based on the numbers seen in the Milky Way, were far too low. While these data are not yet confirmed, adding so many more red dwarfs would triple the total number of stars in the observable universe (to 30,000 billion, billion). The number of stars “dwarfs” the number of grains of sand on all the beaches on Earth (“only” 10 billion, billion).

 

Some astrobiologists believe the vast number of red dwarf stars may harbor a vast number of habitable planets. In fact, the exoplanet (a planet outside our solar system) that seems most likely to be habitable orbits the red dwarf star Gilese 581, 20 light-years from Earth. Exoplanet “g” is in the habitable zone (where water can be liquid) and has a nearly circular orbit; it’s “year” is 37 of our days, and it orbits 7 times closer to its star than does Earth. At that close range, “g” is likely to be tidally locked, meaning that one side of the planet always faces its star while the other side is in perpetual darkness (our Moon is tidally locked relative to Earth). This may result in one side of the planet being too hot for life while the other is too cold, although there may be a sweet spot in the Twilight Zone. Red dwarfs also have occasional dramatic changes in energy output, further challenging nearby life.

 

Much to ponder as we anticipate more exciting discoveries in 2011.

 

With all the new stars to add to your holiday cheer,

we wish you the very best for a great New Year!

 

Regards,
Robert
www.guidetothecosmos.com

 

 

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