20 Million Observations by Amateur Astronomers!

[/caption]Early into the celebration of its centennial year, observers of the American Association of Variable Star Observers (AAVSO) passed another milestone over the weekend, when an amateur astronomer from Belgium contributed the 20 millionth observation of a variable star on February 19, 2011.

Amateur astronomers have been recording changes in the brightness of stars for centuries. The world’s largest database is run by the AAVSO. Started in 1911, it is one of the oldest, continuously operating citizen science projects in the world.

“The long-term study of stellar brightness variation is critical to understanding how stars work and the impact they have on their surroundings. The noble efforts of the engaged AAVSO volunteers play an important role in astronomy and help expand human knowledge,” said Dr. Kevin Marvel, Executive Officer of the American Astronomical Society.

The AAVSO currently receives variable star brightness estimates from about 1,000 amateur astronomers per year. Some variable stars are bright enough to be seen with the unaided eye while others require high-tech equipment. The AAVSO also has a network of robotic telescopes available to members free of charge.

“Because some variable stars are unpredictable and/or change their brightness over long time scales, it is not practical for professional astronomers to watch them every night. Thus, amateurs were recruited to keep tabs on these stars on behalf of professionals,” Dr. Arne Henden, Director of the AAVSO, said.

The 20 millionth observation was made by Dr. Franz-Josef “Josch” Hambsch of Belgium. The observation was of GV Andromeda, member of a class of older, pulsating stars smaller than our Sun. “I like these stars because you can see their entire variation cycle in one night. There have not been many recent observations made of this particular star, so that is why I am monitoring it,” Hambsch said. Hambsch is also a member of the Belgian variable star organization, Vereniging Voor Sterrenkunde, Werkgroep Veranderlijke Sterren (VVS, WVS).

Actual light curve of GV And created from Josch Hambsh's data. One of these points is the 20 millionth observation! Courtesy AAVSO.

The process of estimating a star’s brightness can range from less than a minute to many hours per estimate, but typically takes about five minutes. At that rate, observers have invested the equivalent of about 1.67 million hours of time in collecting observations for the database. Assuming a current median salary of US$33,000, this would be the roughly equivalent to 27.5 million dollars worth of donated time if all the observations were reported today.

“The reality is these observations are invaluable. The database spans many generations and includes data that cannot be reproduced elsewhere. If an astronomer wants to know the history of a particular star, they come to the AAVSO,” Henden said.

The AAVSO’s mission is to coordinate, collect, and distribute variable star data to support scientific research and education. The AAVSO International Database is openly available to the public through their web site (www.aavso.org), where it is queried hundreds of times per day.

Mike Simonsen

Mike Simonsen is one of the world's leading variable star observers. He works for the American Association of Variable Star Observers as Membership Director and heads the organization's Cataclysmic Variable Section, Chart Team, Mentor Program, Speakers Bureau and Writers Bureau. He writes the astronomy and variable star blog, Simostronomy and is a cast member of the Slacker Astronomy podcast. An animated and enthusiastic speaker, Mike has given dozens of talks on stellar astronomy and variable star science for astronomy clubs, star parties, planetariums and university groups throughout the United States. He is author or co-author of dozens peer-reviewed papers on cataclysmic variable stars. Mike's observatory houses two 12" LX200 telescopes, one for visual use and one for CCD observations, or as Mike likes to joke, "One for each eye!" He is now amassing both visual and CCD observations from home and robotic telescopes.

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