Author: Fraser Cain

It’s time for another pretty picture. This time you’re looking at an image of the Rho Ophiuchi dark cloud, captured by NASA’s Spitzer Space Telescope. It’s one of the closest star-forming regions to the Earth, located a mere 407 light-years away.

The nebula is mostly a large cloud of molecular hydrogen. This is the main material that all stars form from. Some gravitational event caused a cloud of this hydrogen to collapse down, condensing into vast regions of star formation.

According to recent X-ray and infrared studies, there are more than 300 newly forming stars in the central nursery. And their average age is only 300,000 years old; much younger than our own Sun’s billions of years.

The colours look nice, but that’s not what you’d actually see if you could travel to “Rho Oph”. Its colours were chosen by astronomers to clearly highlight the various temperatures and evolutionary stages of the various stars. The young stars are surrounded by disks of gas and dust, and show up as red in the image.

The extended white nebula in the centre right of the image is glowing bright in infrared radiation because of the dust there has been heated by bright young stars. The rest of the stars forming are concentrated into the filament of cold, dense gas that shows up as a dark cloud in the lower centre and left side of the image.

Original Source: Spitzer News Release

 

Because stars are just points of light in the sky, it’s very difficult to know how far away they are. Astronomers use several techniques to measure distance, but they’ve got a new one now. By measuring echos of light bouncing off a distant nebula, researchers have fine-tuned their accuracy to an amazing level of precision.

Astronomers used ESO’s New Technology Telescope at La Silla to perform detailed observations of a star called RS Pup. It’s a member of a group of pulsating stars known as Cepheid variables. RS Pup changes in brightness by a factor of 5 every 41.4 days. It’s 10 times more massive than the Sun, 200 times larger and puts out 15,000 times more light.

You can look through these books and instructional materials from Amazon.com for more information about stars.

Because Cepheids pulse at a rate in proportion with their size, astronomers can measure how far they are by how often they pulsate.

But this only tells you how far they are relative to one another. So astronomers use a different technique called parallax to measure distance as well. If you want more info on this, check an episode of Astronomy Cast where we measure different techniques to measure distance in the Universe.

Now astronomers have come up with a second technique to measure distance to a star like RS Pup; to confirm that the Cepheid variable technique is correct.

They did this by watching how light moves through the nebula of material shed by RS Pup in the past. Since light is going 300,000 km/s, it takes time to pass by various blobs of gas and dust in the nebula.

The researchers calculated the light curve from an event on the star, and then watched as that same curve passed different parts of the nebula. It was then a relatively straightforward calculation to determine how far away RS Pup is.

To really appreciate what’s happening, check out the video, where you can see pulses of light move through the nebula. I’ll warn you, it’s a 3.4 MB download.

According to their calculations, the star is 6,500 light-years away, give or take about 90 light years. It’s the most accurate distance to a Cepheid ever captured, with a 1% level of precision.

Original Source: ESO News Release