AstroInformatics II: From public outreach to public engagement

ResearchBlogging.org
Outreach and education are two areas that stand to gain from developments in semantic astronomy and an increased scientific presence on the web. Big changes have already taken place, driven by a community eager to connect and communicate about the research we do every day. As part of a panel at the AstroInformatics 2010 conference last week, I gave a talk on aspects of science communication and education that are benefiting from the semantic web.

The internet these days is a cacophony of conversations, opinions, visual information (and porn). Many scientists and science enthusiasts write about the stuff that inspires or excites them in blogs, like I do here, which allow them to connect to people they would never have encountered, let alone talked with, in real life. This has led to some great scientific content generated entirely by the science community itself, without intermediate brokerage by communication or media professionals. But in this symphony of chaos, how do we increase the signal to noise? How do we ensure that the best content is heard?

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Shape matters in black hole growth

Fig. 1 (from Schawinski et al., 2010)

ResearchBlogging.org

Active galaxies have gone by many names: active galactic nuclei, quasars, QSOs, Seyfert galaxies, radio galaxies. Astronomers used to think these were all distinct types of objects, unified by the observation of large amounts of energy emerging from a compact region at the centre of the galaxy. These days, despite a great variety in observational characteristics, active galaxies’ engines are generally thought to be driven by a single mechanism, the accretion of material onto a supermassive central black hole.

In a paper published to the Arxiv last week, Kevin Schawinski and collaborators have used Galaxy Zoo classifications of local Universe galaxies to show that active elliptical galaxies are markedly different from those with a more disk-like or spiral shapes, adding morphology as an additional factor to consider in our model of active galaxies.

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The Zooniverse

zooniverse

Today saw the launch of the Zooniverse, home for the growing number of Zoo projects that have spawned from the success of Galaxy Zoo. The site contains info on all the projects, how to join, where to go for more info, and how to get new projects into the Zoo.

The Zooniverse project is run and maintained by the Citizen Science Alliance, whose new website also launched today.

Congrats to Chris, Arfon, Pamela and all the other Zookeepers for a great job on all these projects! Extra points for getting a Mighty Boosh reference into an astronomy project.

.Astronomy Day 1: Citizen Science

Merge galaxies with the new Galaxy Zoo merger project

Merge galaxies with the new Galaxy Zoo merger project

Day 1 of .Astronomy is behind us and I think everyone is pleased with how it went. As organiser I was  particularly happy that there weren’t any technical glitches, and the Unconference sessions sorted themselves out very nicely. The theme of the day was Citizen Science. Several projects have shown how keen non-professionals are to be involved in science, and how scientists themselves can benefit from the citizens’ active participation.

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IAU: The singular future of astronomy

The Hubble Deep Field

The Hubble Deep Field

For many centuries, astronomy has been a powerful inspirational force driving people to look further, build bigger, go deeper. Indeed, other physical sciences, mathematics and engineering have benefited greatly, and continue to benefit, from astronomical research. At the IAU general assembly I heard many speakers comment on the “Golden Age” of astronomy we currently finding ourselves in. But as one speaker argued, when was astronomy not in a Golden Age? An entire 4-day session at the GA was devoted to the topic “Accelerating the rate of astronomical discovery”, which had some fascinating talks about the way astronomical discoveries are made and how technological changes underpin progress in astronomy.

An important theme running through many talks in the session was the power of the individual in astronomy. The balance between the individual and the crowd has always been a delicate one. Many early scientists faced disbelief or even wrath from peers and society for their discoveries, from Copernicus‘ “heretic” claims of a heliocentric universe to the initial rejection of Saha‘s equation of ionisation equilibrium by the 1920′s scientific establishment. Several talks were love stories to the mavericks whose doggedness, eccentricity and creativity changed the face of astronomy, culminating in Dame Jocelyn Bell-Burnell‘s wonderful own account of her discovery of the first pulsars in the 1960s.

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