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July 17 2009 00:40 UTC | Views: 1159 | Comments: 1 Posted by: MarciaB in Astro 101
Anyone can help with astronomy research... really! You do not need a telescope or binoculars, or even clear skies, to participate in a number of research programs that rely on all of us "regular folk" around the globe to help. Here are just 3 of these programs - know of others? Let us know and we'll spread the word!
Galaxy Zoo  The
Galaxy Zoo project started in 2007. You can help classify
about a
quarter of a million galaxies that were imaged using the the
Sloan
Digital Sky Survey system. This will help scientists
to understand
how these galaxies - and our Milky Way - were formed. Believe
it
or not, your brain is better than even the fastest computer when
looking at an image and deciding some characteristics of the galaxy
displayed. Galaxy Zoo 2 is now taking the original project
research to a new level and trying to answer even more questions about
galaxies. Goals like: identifying galaxies that are a cross between
spirals and ellipticals, better categorizing the shapes of elliptical
galaxies, drawing attention to the many spiral galaxies that have bars
across their centers (like the Milky Way) and trying to learn how these
bars formed, and more!
How many galaxies
have two, three, or
more
arms? How tightly wound are the spiral arms? What shape is the bulge in
a galaxy - if there is one? How many "irregular" galaxies are there?
The primary goal of Galaxy Zoo 2 is to construct a database of detailed
shape information for the largest sample of galaxies ever assembled.
But that takes lots of eyes looking at lots of galaxies.
So
far, over 200,000 people have helped (including several AFM members).
Helping is easy.
Go to the Galaxy
Zoo website,
and read the tutorial under "How to Take Part." Then register
and
start classifying! To try it out (but not have your work
counted), you can Classify Galaxies as an unregistered guest by
clicking here.
Stardust@HomeThe
Stardust spacecraft was launched to collect particles of interstellar
dust from comet Wild 2 in January of 2004. On January 15,
2006,
the Stardust spacecraft's sample return capsule safely returned to
earth, and contained these particles trapped in aerogel. This
interstellar dust originated in distant stars, light-years away, and
are the first such particles ever collected in space! But, scientists
can only study the particles once they are found within the
aerogel. This is not easy. For every thousand of particles of
varying sizes collected from the comet, scientists estimate that only
around 45 tiny (about a micron, or a millionth of a meter)
interstellar dust particles were trapped. The aerogel
collector is
1,000 square centimeters in size, and is interspersed with flaws,
cracks, and an uneven surface. Think of how the surface of
old
Jello looks. Scientists used an automated scanning microscope
to
collect images of the entire Stardust interstellar collector and
created stacks of images called "focus movies."
All in all there are
about a million such focus movies for people like us to look
at,
and try to spot these tiny particles using a special Virtual Microscope
(VM) that works in a web browser. If you happen to discover a particle,
you will appear as a co-author on any scientific paper by the
Stardust@home collaboration announcing the discovery of the particle...
and you will be able to name the particle! Using the Virtual
Microscope is easy; spotting particles isn't too difficult either.
You can look back at old movies you have flagged as
containing a
particle and see how many other volunteers also saw the same thing.
There is a tutorial and a quiz, so you can be
confident of your skills before you start.
Citizen
SkyCitizen scientists are volunteers, with or without any training, who
work with trained researchers to answer real-world questions.
And, no equipment is needed for this project so you
and I can easily be citizen scientists! Over the
next 3 years volunteers and experts will observe and
analyze epsilon Aurigae... a bright, eclipsing binary
variable star located in the constellation Auriga, the charioteer.
 The problem: Nobody knows why this
star changes in brightness every 27 years, and
is eclipsed for 2 years! What can eclipse it for that long?
Scientists aren't certain so they are asking for our help. The next
eclipse begins August 2009 and will last until May 2011. The
American Association of Variable Star Observers ( AAVSO)
sponsored this 'citizen science' project to get as many observers as
possible to watch and measure these changes while it eclipses. The star
is too bright to make accurate measurements using a telescope; visual
observation is better -- so truly anyone can help.
It's not difficult to do; you compare epsilon Aurigae to
neighboring stars to estimate its brightness (is it "as bright as" a
given star nearby with a known brightness? if so, that's the brightness
you record). With thousands of people around the world making
and reporting observations, the scientists can perform statistical
analyses to try to determine what's causing the eclipses. Sound
interesting? Read the 10
star Tutorial (the PDFon that page gives loads of
information) and sign up like me!
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