Holy Cow We’re Small! Biggest Stars to Biggest Galaxies

April 16th, 2009 | Posted by paul in Uncategorized - (Comments Off on Holy Cow We’re Small! Biggest Stars to Biggest Galaxies)

This is a great visual scale of just how big the biggest stars and galaxies are. Impressive.

Click on image for original size.

BiggestStars

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3 Trillion Suns!

January 7th, 2009 | Posted by paul in Uncategorized - (Comments Off on 3 Trillion Suns!)

galaxy1

That’s the new upper estimate of the number of stars in our galaxy, according to the report in Science News..  Scientist Mark Reid and a team of astronomers at of the Harvard-Smithsonian Center for Astrophysics, used the Very Long Baseline Array to look at star-forming regions across the galaxy. What they observed is that these stellar nurseries are moving in an elliptical orbit, rather than a circular one, and moving more than 100,000 miles per hour faster than previously believed. This extra velocity can only be explained by much larger overall galactic mass, which Reid estimates is at least 50% larger than previous estimates of galactic size.  These estimates pegged the Milky Way’s stellar population at around 400 billion stars, but now that figure has been revised upward to between 1.8 and 3 trillion!

It’s here that I like to wax mathematical with my own (rough) estimate of Drakes Equation.

Lets assume 3 trillion suns is the more accurate figure.  Based on the growing evidence of an abundance of habitable planets, as evidence by the ever widening range of exoplanets being discovered, it’s not too much of a stretch to assume that there is at least one rocky, Earth-like planet for every 10 G-type stars (ones like our sun)  By earth-like I mean that it is rocky and not gaseous, and it’s size is somewhere between 4000 and 16000 miles in diameter (the Earth is 8000 miles).  However scientist are beginning to believe that both K and F type stars are also long lived enough that planets at an appropriate distance could also be habitable.  In this case habitable is defined as having the right conditions for liquid water.  Also, scientists now believeit is possible for habitable planets to form around binary star systems as well.  Finally there is what is called a habitable zone around the galaxy, which is in my opinion too conservative, and is not supported by the majority of scientists.  If we put this all together, G-type, plus a smaller number of K and M type stars gives us about 8% of the total stars capable of supporting habitable planets.  If we cut out most (but not all) of the multiple star systems, and eliminate all the stars closer than 20,000 light-years to the galactic core (just to be conservative), we’re left with about 4% of the stars in our galaxy that our friendly to life-supporting planets should they exist.  And if 1 out of 10 of those stars actually have an earth-like planet, with 3 trillion total stars, leaves us with about 12 billion Earth-like planets in our galaxy capable of supporting liquid water and in turn carbon-based life as we know it. And I believe this to be a conservative estimate, but we’d really know until the Kepler data comes in.

At this point Drake’s Equation become very murky, as our understanding of the formation and likelihood of life forming, given the right conditions, is almost unknown.  What we do know is that many of the major chemical precursors for life have already been identified in space, including water, alcohol, ammonia, carbon monoxide, carbon dioxide, and acetic acid, which gives vinegar its piquant flavor.

Either way what these numbers tell us, is that there could be upwards of 12 billion stars with habitable planets around them.  That or these planets could be terraformed to support life by a life-bearing space civilization.  The ideas of billions of living worlds in our very own galaxy is a prospect worthy of investigation, which is why the search for earth-like planets has become the most important objective of space science both at NASA and abroad.

To get a scifi perspective, Star Trek talks of thousands of inhabited worlds, Star Wars of millions, and our very own Milky Way could be home to billions.

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Virtual Observatory

May 20th, 2003 | Posted by paul in Uncategorized - (0 Comments)

astronavIn today’s New York Times (no link as it disappears within a week), the article talks about the ambitious project underway to digitize and unify all the observable data and images into a single coherent user interface of the observed cosmos. In time, I have no doubt we will all have access to the same thing astronomers do. Reminds me of that scene with Picard and Data in Star Trek: Generations, in the Astronavigation room:

The telescope that Dr. Szalay and his colleagues have constructed is not built of glass and metal. It is a virtual observatory, consisting of terabytes of data collected by dozens of telescopes on Earth and in space, and the software necessary to mine these data for scientific gems.

Like much of the rest of science, astronomy has been the beneficiary — and victim — of Moore’s Law, which states that the capacity of computers and other silicon-based devices like charge-coupled devices, or C.C.D.’s, doubles every 18 months. (The C.C.D has largely replaced photographic film in astronomical cameras.)

Projects like the National Virtual Observatory, which was created in response to the tsunami of data that is threatening to drown astronomers, is creating a new branch of science, Dr. Szalay believes.

Science, he points out, was “originally empirical, like Leonardo making wonderful drawings of nature.” He continued: “Next came the theorists who tried to write down the equations that explained the observed behaviors, like Kepler or Einstein. Then, when we got to complex enough systems like the clustering of a million galaxies, there came computer simulations, the computational branch of science. Now we are getting into the data exploration part of science, which is kind of a little bit of them all.”

Because its primary tools are computers rather than giant, multimillion telescopes, this new form of astronomy has the potential to democratize science.

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