Category Archives: astronomy news

A Rose From Space

This Spitzer Space Telescope image was obtained with an infrared array camera sensitive to invisible infrared light at wavelengths that are about ten times longer than visible light. In this four-color composite, emission at 3.6 microns is depicted in blue, 4.5 microns in green, 5.8 microns in orange, and 8.0 microns in red. The image covers a region that is about one quarter the size of the full moon.
This Spitzer Space Telescope image of a stellar nursery was obtained with an infrared array camera sensitive to invisible infrared light at wavelengths that are about ten times longer than visible light. In this four-color composite, emission at 3.6 microns is depicted in blue, 4.5 microns in green, 5.8 microns in orange, and 8.0 microns in red. The image covers a region that is about one quarter the size of the full moon.

This is kind of cool. The folks at Spitzer Space Telescope have caught onto the “positive PR spin” thing pretty well and have issued a lovely picture of a rosebud-shaped stellar nursery called NGC 7129. Smack in the middle of the bud is a cluster of newborn stars, and all of this loveliness lies about 3,300 light-years away in the constellation Cepheus. There are about 130 young stars here, all formed from a huge cloud of gas and dust.

Here’s what the Spitzer folks have to say about their discovery:

    “As in any nursery, mayhem reigns. Within the astronomically brief period of a million years, the stars have managed to blow a large, irregular bubble in the molecular cloud that once enveloped them like a cocoon. The rosy pink hue is produced by glowing dust grains on the surface of the bubble being heated by the intense light from the embedded young stars. Upon absorbing ultraviolet and visible-light photons produced by the stars, the surrounding dust grains are heated and re-emit the energy at the longer infrared wavelengths observed by Spitzer. The reddish colors trace the distribution of molecular material thought to be rich in hydrocarbons.

    The cold molecular cloud outside the bubble is mostly invisible in these images. However, three very young stars near the center of the image are sending jets of supersonic gas into the cloud. The impact of these jets heats molecules of carbon monoxide in the cloud, producing the intricate green nebulosity that forms the stem of the rosebud.

    Not all stars are formed in clusters. Away from the main nebula and its young cluster are two smaller nebulae, to the left and bottom of the central “rosebud,” each containing a stellar nursery with only a few young stars.

    Astronomers believe that our own Sun may have formed billions of years ago in a cluster similar to NGC 7129. Once the radiation from new cluster stars destroys the surrounding placental material, the stars begin to slowly drift apart. “

Happy Valentine’s Day!

Showing off What Hubble Does Best

HST on orbit
HST on orbit

I just finished work on a planetarium show about Hubble Space Telescope discoveries. I’ve written other shows about HST before, and this is sort of the “latest and greatest” one, and one where I really don’t know the ending. We’ve all been talking about the last HST servicing mission being cancelled, thus sentencing HST to its fate a few years earlier than everybody expected. Now it appears that Congress really does have the last say about this, and several folks have called for a re-investigation of the decision. So, the story’s not over yet. And, up there in orbit around Earth, HST continues on its merry way, sending back great images and science data (not mutually exclusive) for all of us to study and enjoy.

Well, rather than focus on the political aspects of HST’s “human side,” I spend all my time in this planetarium show talking about the great science it has done. It’s not an easy task. There’s a LOT to talk about, and a lot more to come. In fact, the most difficult thing about an HST planetarium show is choosing what NOT to show. There’s only so much time in the program, and in most planetaria, there are only so many slides one can cycle through in the course of a show. Sure we can throw in some video, for those who HAVE video projection capability, but for those who don’t, we’re kind of limited by the slides. I’ve chosen nearly 200 really great images and told a story of cosmic exploration using them as illustration. As I spend time looking at the sights that HST has seen for us, I’m impressed again with just how marvelous this machine has been. And what a wonderful time the astronomers who use it must be having when they open their data sets. Are they like kids opening presents? I like to think so. Or at least HOPE so.

The Eskimo Nebula (planetary nebula)
The Eskimo Nebula (planetary nebula)

One of the images I’ll be using in the show is a study of a planetary nebula that lies about 5,000 light-years away from Earth. It’s called “The Eskimo” Nebula because it looks like an intricate furry hood that an Eskimo might wear. The “parka” is really a disk of material surrounding a dying, Sun-like star. Inside the cloud is a ring of comet-shaped objects, with their tails streaming away from the central, dying star. The “face” consists of a bubble of material being blown into space by the central star’s intense “wind” of high-speed material. The story behind this apparition is fascinating. The star that formed this cloud began to lost much of its mass to space about 10,000 years ago. Before that time it had gone through what’s called the “red giant” phase, breathing out a ring of dense material that collected around the star. That ring is actually moving out from the star at about 115,000 kilometers per hour. Hot on its heels (so to speak) are high-velocity stellar winds, moving out from the star at 1.5 million kilometer per hour. They are shoving material above and below the star, creating elongated bubbles. Each bubble is about one light-year long and about half a light-year wide.

This is just one of a dozen or so planetary nebulae I’m presenting in my show, and while I can’t talk about them in excruciating detail, I can at least show people just what our Sun might look like in 5 or 6 billion years when it starts down the path toward planetary nebula-hood. Fun stuff!