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The five most amazing ESO images for 2014 ... so far

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April 30, 2014

A look at some of the most impressive images from the European Southern Observatory, captu...

A look at some of the most impressive images from the European Southern Observatory, captured over the past four months (Image: ESO)

Image Gallery (6 images)

Though we’re only a third of the way through the year, the European Southern Observatory (ESO) has already produced some spectacular new images of what’s out there in the Universe. From a rare yellow hypergiant star to a celestial trick of the light, we take a look at five of the most impressive ESO snaps of the year so far.

A celestial diamond ring

Planetary nebula Abell 33 pictured with a foreground star (Image: ESO)

Taken by the Very Large Telescope (VLT) in Chile, this image is one of the more spectacular released by the ESO so far this year. The "diamond ring" appearance is the result of a chance alignment of an aging star blowing off its outer rings (known as a planetary nebula), and a separate star in the foreground.

The nebula, formed from a star known as Abell 33, is located some 2,500 light-years away and is remarkably symmetrical for an object of its type. The aligned star, which lies between the VLT and the nebula, is known by the catchy name of HD 83535.

A rare yellow hypergiant

The yellow hypergiant HR 5171 was identified as a double star by ESO’s Very Large Telescop...

In March, the ESO’s VLT Interferometer discovered the largest known yellow star. Coming in some 50 percent larger than the well-known red supergiant Betelgeuse, the star is more than 1,300 times the diameter of the Sun, and more than one million times brighter. Not only is the star truly gigantic, but it is also extremely rare, with only a dozen found in our galaxy.

The star, known as HR 5171 A, is located almost 12,000 light-years away, and is actually part of a double star system (known as binary stars), with the second star so close to the yellow giant that the two objects are actually touching.

The object has been under observation for decades, and is thought to be changing at a rapid pace, greatly expanding in size as it cools.

A galactic serial killer

MPG/ESO 2.2-meter telescope image showing galaxies NGC 1316 (center) and NGC 1317 (right) ...

This image, taken by the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile, shows two galaxies – the smaller NGC 1316 seen on the right, and the much larger and more interesting NGC 1317 on the left.

During its lifespan the larger object has consumed a number of galaxies, including a dust-rich spiral galaxy some three billion years ago. The unusual dust lanes, globular star clusters and faint tidal tails in the structure of NGC 1317 are telltale signs of its turbulent past.

At the center of the galaxy lies a supermassive black hole, providing fuel for the engulfing of neighboring galaxies, and making it the brightest source of radio emissions in the constellation of Furnax, and the fourth brightest in the entire sky.

A red hot nebula

The Gum 41 nebula as taken by the Wide Field Imager on the MPG/ESo 2.2-meter telescope at ...

Located some 7,300 light-years away in the constellation of Centaurus, the Gum 41 nebula shines with a radioactive red hue. The picture here is a product of the ESO’s La Silla Observatory, and shows a region rich in star formation. Like many such regions in the constellation of Centaurus, the nebula is filled with young stars that ignite the hydrogen surrounding them, creating the characteristic colored glow.

Despite the object appearing bright and thick from a distance, it is actually barely perceptible to the human eye. To capture it in such vivid detail, the team at the La Sillla Observatory took advantage of the Wide Field Imager (WFI) on the MPG/ESO 2.2-meter telescope, using a combination of blue, green and red filters in addition to a filter designed specifically to pick up the red glow of the hydrogen.

A new look at the Lagoon Nebula

The Lagoon Nebula as pictured by the ESO's VLT Survey Telescope (Image: ESO/VPHAS+ team)

The VLT Survey Telescope (VST) at the ESO’s Paranal Observatory in Chile has captured this new, highly detailed visible light image of the distant Lagoon Nebula.

The nebula, which is also known as Messier 8, is located some 5,000 light-years away in the constellation of Sagittarius. The cloud itself is a full 100 light-years across, and is made up of gigantic star-forming clouds of dust and gas.

The new image measures 16,000 pixels across and is part of the VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+), which aims to address key astronomical issues such as the nature of dark energy and the structure of the Milky Way.

A fully zoomable version of the image is available on the ESO website.

Source: ESO

About the Author
Chris Wood Chris recently graduated from the University of Exeter with a degree in Politics and Ancient History. Based in the U.K., he has an enthusiasm for technology of all kinds, specializing in mobile tech and games. In his spare time you might find him running, playing music, following NFL (Pats fan) or fueling his ever growing Swiss watch obsession.   All articles by Chris Wood
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2 Comments

Chris, if you're going to write about science, please don't use such loose or misleading language as you sometimes do here.

Take for example your story above about the Gum 41 nebula.

Your heading "A red hot nebula" is incorrect because when we say that something is "red hot" (as in a heated fire poker or blacksmith's horseshoe) we mean that its blackbody emission includes a reddish, visible light component. That happens at a MUCH (about 15 times) lower temperature than the Hydrogen plasma in an astronomical emission nebula like Gum 41.

Then to say that the "nebula shines with a radioactive red hue" is misleading, because radioactive decay has nothing to do with emission from this kind of nebula. I know that describing a strong colour as "radioactive" happens in the fashion industry. It works in that context; but in the context of a giant cloud of space gas, it is only confusing, because some other types of nebulae (young supernova remnants) genuinely are powered in part by radioactive decays.

Finally, "the nebula is filled with young stars that ignite the hydrogen surrounding them" is misleading because "ignition" equates to "starting combustion" (with oxygen) in most people's minds. It is also used to indicate the onset of nuclear fusion in stars. Neither of those processes is what happens to make a hydrogen nebula shine. Perhaps you confused "ignite" with "ionize", which is the correct term.

Readout Noise
1st May, 2014 @ 06:24 am PDT

If the universe is expanding, i.e., all objects moving away from each other, then how can galaxies collide?

Don Duncan
1st May, 2014 @ 02:21 pm PDT
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