Category Archives: astronomy

Hot Times in NGC 1569

NGC 1569
NGC 1569

We usually think of space as this serene place where stars shine and planets bob around and galaxies are out there. Except, of course, it’s not quite true. Depends on where you’re looking to and from. Take the the nearby dwarf galaxy NGC 1569 as an example. It’s a close (meaning it’s about 7 million light-years away) starburst galaxy — a hotbed of vigorous star birth that blows huge bubbles of gas. The galaxy’s “star factories” are also manufacturing brilliant blue star clusters.

As it turns out, NGC 1569 had a sudden onset of star birth about 25 million years ago. Lots of new stars were born and then things quieted down a bit about the time the very earliest human ancestors appeared on Earth.

This new image from the Hubble Space Telescope shows the bubble structures being sculpted by galactic super-winds and outflows. These are the result of supernova explosions that are themselves linked to massive episode of star birth. That makes sense when you think about it: the stars are born, and then some millions of years later they start to die. If they’re massive stars, they live short lives (well, short compared to longer-lived stars like the Sun) and die spectacularly as supernovae.

This whole episode of star formation and star death, intertwined in a single spectacular image, brings us to one of the still unresolved mysteries in astronomy: how and when galaxies formed and how they evolved. Most of today’s galaxies (including the Milky Way) seem to have formed quickly very early on in the history of the universe. Galactic births very likely involved one or more galaxy collisions and/or episodes of strongly enhanced star formation activity (the so-called starbursts).

While any galaxies that are actually forming are too far away for detailed studies of their stellar populations even with Hubble, their local counterparts, nearby starburst and colliding galaxies, are far easier targets. NGC 1569 is a particularly suitable example, being one of the closest starburst galaxies. It harbors two very prominent young, massive clusters plus a large number of smaller star clusters. The two young massive clusters match the globular star clusters we find in our own Milky Way galaxy, while the smaller ones are comparable with the less massive open clusters around us.

The majority of clusters in NGC 1569 seem to have been produced in an energetic starburst that started around 25 million years ago and lasted for about 20 million years. The bubble-like structures that resulted are made of hydrogen gas. It glows when hit by the fierce winds and radiation from hot young stars and is racked by supernovae shocks. The first supernovae blew up when the most massive stars reached the end of their lifetimes roughly 20-25 million years ago. The environment in NGC 1569 is still turbulent and the supernovae may not only deliver the gaseous raw material needed for the formation of further stars and star clusters, but also actually trigger their birth in the tortured swirls of gas.

So, in one image you get starbirth, stardeath, galaxy evolution, and something a little more: another great image to learn from, thanks to the Hubble Space Telescope.

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!