55 billion silly faces

Shamus Young is the most dangerous sort of guy, with lots of ideas and the time and energy to implement them. He first came to my attention several years ago with The Lemon. Later there was The DM of the Rings. Currently he is one of the parties responsible for Chainmail Bikini. His most recent effort is a WordPress plugin, “Wavatars,” which I’ve installed here. If you leave a comment, your name will be accompanied by an eighty-pixel-square avatar determined by your email address. (If you have a Gravatar, as I do, that’s what you will see instead.) On a weblog like mine where comments are infrequent, these are just a cute novelty, but on sites where comment threads get lengthy, these could be useful for keeping the various writers straight.

If you like the idea but want something a little more macabre for your own site, consider MonsterID. (Via Aziz.)

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5 Responses to “55 billion silly faces”

  1. Robin Says:

    I would love to see mine, but I’ll only see my gravatar on this … and your system is not allowing me to change my identity (I thought I might try commenting with another address). But it does seem to be registering the wavatars on old comments. The chain you have on your Dec. 11 post is nicely illustrative.

    –Robin (same old)

  2. Shamus Says:

    Glad you like it! :)

  3. Fredosphere Says:

    Okay, I’ll bite.

  4. Shishberg Says:

    By rights there should be at least one Wavatar in these comments, and I don’t have a Gravatar. :)

  5. JaneC Says:

    Ok, I’ll give it a go.

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A Mosaic of Cassiopeia

 
This mosaic of images from the Wide-Field Infrared Survey Explore, or WISE, in the constellation of Cassiopeia contains a large star-forming nebula within the Milky Way Galaxy, called IC 1805 or the Heart Nebula, a portion of which is seen at the right of the image. IC 1805 is more than 6,000 light-years from Earth. Also visible in this image are two nearby galaxies, Maffei 1 and Maffei 2. In visible light these galaxies are hidden by dust in IC 1805 and were unknown until 1968 when Paolo Maffei found them using infrared observations. Both galaxies contain billions of stars and are located some 10 million light-years away. Maffei 1 is a lenticular galaxy, which has a disk-like structure and a central bulge but no spiral structure or appreciable dust content. Maffei 2 is a spiral galaxy that also has a disk shape, but with a bar-like central bulge and two prominent dusty spiral arms. Image Credit: NASA/JPL-Caltech/UCLA
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