Category Archives: hubble space telescope

Across the Light-years from Andromeda

Revisiting the Past

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Light Years from Andromeda, 2009

This week Mark and I are releasing a fulldome show version of the very first Loch Ness Productions planetarium show I ever wrote, called Light Years from Andromeda. It tells one of the most important stories in astronomy and cosmology — that of cosmic distance, and humanity’s quest to understand the universe. It is, as we say on the show’s Web page touting the show, “a journey of epic proportions across space and time.”

It seems particularly appropriate to talk about it today, with the release of a new, more precise value for the Hubble Constant. That constant is one of the numbers astronomers use to determine the expansion rate of the universe.  Knowing that expansion rate helps us also determine other factors like the size of the universe and just how old the universe really is. But, the root of all this knowledge is cosmic distance.

Distance in the universe is important to understand, and it is measured by using “standard candles” in the darkness. The standard candles are usually specific types of supernova explosions and, in particular,  a type of pulsating star called a Cepheid variable.  These pulsate with a regular rhythm and they are found in every galaxy we’ve seen so far. You can use the observations of those candles to derive distances across the cosmos.

In Light Years from Andromeda, we focus on a distance that most people have heard of, even if they aren’t up on the latest in cosmology: the light-year. It’s the distance that light travels in a year at a speed of roughly 300,000 kilometers per second. We wanted to bring that figure into some kind of reality for people, so I decided to take them out to the Andromeda Galaxy, which lies some 2.5 million light-years away.  We begin the show there, some 2.5 million years ago, and we bring people back home to the Milky Way, across all that time and space at the speed of light. Along the way we discuss human history set against that travel time. And, when we arrive at Earth, we learn about light-speed and the way that we can use light to measure cosmic distances.  It’s really a simple concept and a simple story to tell. And, it’s been very satisfying to see the show come to life in the new fulldome medium, where we really CAN fly from one galaxy to another and take in the breathtaking beauty of the cosmos.  And, to have it come out now, when the precision of the Hubble Constant is even better than before — well, it just sends chills up my spine. These are the times that make my day as a science writer!

(Check out the trailer for the show below.)

Light Years from Andromeda trailer

Arp Goodness!

More Great Views during 100 Hours of Astronomy

Remember that contest to select HST’s next imaging target?  Well, the image has been taken and posted to celebrate 100 Hours of Astronomy and IYA.  HST imaged the winner — Arp 274, set of galaxies jsut beginning to interact with each other.  HST’s view, which was taken on April 1-2 (just the last two days!) is here. It’s a stunner!

Arp 274 in all its glory -- as seen by HST.  (Click to embiggen.)
Arp 274 in all its glory, as seen by HST. This is a set of galaxies about to begin interacting. They're blooming with star-formation sites. When galaxies interact and merge, the actions often spur gas clouds to form new stars in huge "star bursts". (Click to embiggen.)

Arp 274, also known as NGC 5679, is really a system of three galaxies. They’re probably at different distances from us and each other, but from our point of view here on Earth, they appear to be overlapping.  You can make out spiral shapes in two of the galaxies, although upon closer examination, there’s some distortion going on due to the merger activity. As we might expect from galaxies that are undergoing (or have undergone) a merger, there’s a lot of star formation going on. It’s triggered by the interaction of the galaxies as shock waves slam star-forming regions and jump-starting the stellar birth process. The starbirth regions are strong along the arms of the spirals and in the small blobby-looking galaxy to the left. .

The largest component is located in the middle of the three. It appears as a spiral galaxy, which may be barred. The entire system resides at about 400 million light-years away from Earth in the constellation Virgo.

Astronomers used Hubble’s Wide Field Planetary Camera 2 to image this striking galaxy triplet. Blue, visible, and infrared filters were combined with a filter that isolates hydrogen emission. The colors in this image reflect the intrinsic color of the different stellar populations that make up the galaxies. Yellowish older stars can be seen in the central bulge of each galaxy. A bright central cluster of stars pinpoint each nucleus. Younger blue stars trace the spiral arms, along with pinkish nebulae that are illuminated by new star formation. Interstellar dust is silhouetted against the starry population. The pair of foreground stars at the far righth are inside our own Milky Way Galaxy.