About a year and a half ago I ran across a guy in Grand Teton National Park who photographs the night sky using beautiful landscapes as the foregrounds for his “Nightscapes.” I was hooked and wanted to learn how to do that. When I got home to cloudy Ohio I took advantage of the rare clear nights and started learning how to go about it and also learning what it was I was seeing up there. At the time, all I really knew was the Big and Little Dippers, and that the Milky Way was our galaxy and that fuzzy streak you could see in really dark sky places.
My interest in photography has helped me learn about the constellations and other objects in the sky. I’ve shot areas of the sky not knowing what was there, then I’d study the photos and find the constellations by looking at charts. There is so much up there and I find it all fascinating.
On March 5-8 we spent some time in southern Ohio at Lake Hope State Park and also hiking around the various parks in Hocking Hills. It’s very dark out that way and we were fortunate enough to have two very clear nights and a clear early morning. Despite the very bright half-moon in the evenings you could see many things impossible to see in Parma.
I have an app on my iPod called “Star Walk” and I can see what position the stars will be in on any given date and time so I knew the Milky Way would be visible in the southeast a couple hours before sunrise. I woke up one morning around 4:15 AM, looked out the window of our cottage, and could see Cygnus very clearly. So, I packed up my stuff and headed down by the lake and got my best shots to date of the Galactic Center, and a few other nice shots as well.
Specs for the photo: Nikon D600, Nikkor AF-S 24-85mm f/3.5-4.5G ED VR, 20 seconds, f/3.5, ISO 6400. Processed in Lightroom 5.3 for Windows.
Using a whopping nine-gigapixel image from the VISTA infrared survey telescope at ESO’s Paranal Observatory, an international team of astronomers has created a catalogue of more than 84 million stars in the central parts of the Milky Way. This gigantic dataset contains more than ten times more more stars than previous studies and is a major step forward for the understanding of our home galaxy. The image gives viewers an incredible, zoomable view of the central part of our galaxy. It is so large that, if printed with the resolution of a typical book, it would be 9 meters long and 7 meters tall.
“By observing in detail the myriads of stars surrounding the centre of the Milky Way we can learn a lot more about the formation and evolution of not only our galaxy, but also spiral galaxies in general,” explains Roberto Saito (Pontificia Universidad Católica de Chile, Universidad de Valparaíso and The Milky Way Millennium Nucleus, Chile), lead author of the study.
Most spiral galaxies, including our home galaxy the Milky Way, have a large concentration of ancient stars surrounding the centre that astronomers call the bulge. Understanding the formation and evolution of the Milky Way’s bulge is vital for understanding the galaxy as a whole. However, obtaining detailed observations of this region is not an easy task.
“Observations of the bulge of the Milky Way are very hard because it is obscured by dust,” says Dante Minniti (Pontificia Universidad Catolica de Chile, Chile), co-author of the study. “To peer into the heart of the galaxy, we need to observe in infrared light, which is less affected by the dust.”
The large mirror, wide field of view and very sensitive infrared detectors of ESO’s 4.1-meter Visible and Infrared Survey Telescope for Astronomy (VISTA) make it by far the best tool for this job. The team of astronomers is using data from the VISTA Variables in the Via Lactea program (VVV), one of six public surveys carried out with VISTA. The data have been used to create a monumental 108 200 by 81 500 pixel color image containing nearly nine billion pixels. This is one of the biggest astronomical images ever produced. The team has now used these data to compile the largest catalogue of the central concentration of stars in the Milky Way ever created.
To help analyze this huge catalog the brightness of each star is plotted against its color for about 84 million stars to create a color–magnitude diagram. This plot contains more than ten times more stars than any previous study and it is the first time that this has been done for the entire bulge. Color–magnitude diagrams are very valuable tools that are often used by astronomers to study the different physical properties of stars such as their temperatures, masses and ages.
“Each star occupies a particular spot in this diagram at any moment during its lifetime. Where it falls depends on how bright it is and how hot it is. Since the new data gives us a snapshot of all the stars in one go, we can now make a census of all the stars in this part of the Milky Way,” explains Dante Minniti.
The new color–magnitude diagram of the bulge contains a treasure trove of information about the structure and content of the Milky Way. One interesting result revealed in the new data is the large number of faint red dwarf stars. These are prime candidates around which to search for small exoplanets using the transit method.
“One of the other great things about the VVV survey is that it’s one of the ESO VISTA public surveys. This means that we’re making all the data publicly available through the ESO data archive, so we expect many other exciting results to come out of this great resource,” concludes Roberto Saito. For access to much larger versions of these images, visit the ESO Web site.