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Mystery Blob Detected 12.9 Billion Light Years Away

Take a good look, this is one of the most mysterious, massive objects ever discovered in the cosmos. We don’t really know what it is, but this thing is huge, spanning 55,000 light years across (the approximate radius of our Milky Way). What makes this all the more intriguing is the fact that this object formed only 800 million years after the Big Bang and it is 10 times more massive than the next biggest object observed in the early Universe. But what is it?
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Astroengine Live Show #17: Not-So-Brown Dwarf

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In today’s show, I’ll be giving brown dwarfs some airtime. They may be considered to be “failed stars”, but are they? Also, I’ll be giving a rundown of the week’s space news with some surprises thrown in. Be sure to tune in at 4pm PST/7pm EST!

Get Involved!

Have any articles or stories you want to contribute? Have an opinion on anything in the world of space? Follow me on Twitter to send me live input when I’m on the air, or email me on astro@wprtradio.com and I’ll be sure to give it a mention. Eventually, I hope to have telephone call-ins, but for now, email will do.

Listen to Astroengine Live using the Paranormal Radio player. Or, pick up the podcast feed to activate your favourite audio software.

Could Active-SETI Learn From… Twitter?

The Search for Extraterrestrial Intelligence (SETI) has been an ongoing endeavour for the last 50 years. Detecting radio communications from an alien civilization would be the most profound event in mankind’s history; its effect would change the way we view our origin and our place in the Universe. It could mean that far from “being alone” we could be existing in a cosmic ecosystem, where life is more common than not and advanced extraterrestrial civilizations are no longer science fiction. A positive SETI signal would affect us globally; science, religion, society, daily life would alter radically.

Unfortunately, SETI is currently drawing up blanks. Apart from one or two inconclusive signs, it looks like we live in a dead part of the galaxy. Life As We Know It™ is an Earth-only affair. Who knows, we might be searching for another five decades and still be no closer to answering the question “are we alone?”

Not to be too downhearted, scientists have been trying to make our presence felt by reversing SETI; we’ve been Messaging Extraterrestrial Intelligence (METI, a.k.a. “Active-SETI”) ever since we attached a plaque depicting the human form and a handy galactic map to Earth to the side of the Pioneer probes in the 1970s. Now we send a variety of radio signals to the stars in the hope of attracting ET’s attention.

But what signal do we send? Do we send a message with only good stuff from Earth? Or should we send a more gritty message, detailing our flaws as well as achievements? What actually makes a “good” METI signal in the first place?

Perhaps SETI could take some advice from the evolving social media scene, after all, when done right, there’s no more efficient way of conveying a clear message via 140 characters or less…
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Brown Dwarfs: “Over-Achieving Jupiters” not “Failed Stars”

Why is the term “failed star” synonymous with brown dwarfs? On the one hand, brown dwarfs lack the mass to sustain nuclear fusion in their cores. On the other hand, who said brown dwarfs were trying to be stars? Who ever said that becoming a star was the pinnacle of stellar living? Perhaps brown dwarfs are perfectly happy the way they are. In a world of equality and political correctness, brown dwarfs could be viewed as “over-achieving Jupiters”, or gas supergiants…
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An Explanation For Solar Sigmoids

Hinode X-ray observation of a solar sigmoid (David McKenzie/Montana State University)

Sigmoids in the solar corona have been studied for many years, but little explanation of their formation or why they are often the seed of powerful solar flares have been forthcoming. Using high-resolution X-ray images from the Japanese-led solar mission Hinode (originally Solar-B), solar physicists have known that these very hot S-shaped structures are composed of many highly stressed magnetic flux tubes filled with energized plasma (also known as ‘fibrils’), but until now, little was known about the formation and flare eruption processes that occur in sigmoids.

Now, a team of solar physicists from the University of St Andrews believe they have found an answer using powerful magnetohydrodynamic (MHD) computer models, aiding our understanding of coronal dynamics and getting us one step closer to forecasting space weather…

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Are Brown Dwarfs More Common Than We Thought?

In 2007, a very rare event was observed from Earth by several observers. An object passed in front of a star located near the centre of the Milky Way, magnifying its light. Gravitational lensing is not uncommon in itself (the phenomenon was predicted by Einstein in 1915), but if we consider what facilitated this rare “microlensing” event, things become rather interesting.
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Astroengine 3.0

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Now we’re cookin’… Welcome to the new-look Astroengine.com!

As you may have noticed I’ve been a little patchy with blog posts of late and now you can see why. I decided to migrate the entire Astroengine installation to a brand new server after the site suffered some serious downtime after a recent article (“Where is Planet X? Where is Nemesis?“) was slammed by Digg traffic. Now we are on a sparkling new server with a brand new design. I told you this year was going to be a big year for Astroengine, this officially marks the beginning of a new era…

After asking readers about suggestions for a new direction in design, it was Darnell Clayton (Colony Worlds) who came up with the winning suggestion. He pointed me in the direction of the designs by Elegant Themes and once I saw a design called StudioBlue, I was hooked. A few modifications later and I arrived at what you see here, Astroengine 3.0. It has a fresher, more magazine/blog vibe, so I hope you like it.

With all the technical stuff calming down, I can now get back to what I’m here for. Expect a tonne of space science articles over the coming months – 2009 is going to be a big year.

Thank you for your support (and patience!).

Cheers, Ian

A Change Is Coming…

Apologies for the break in Astroengine transmission, a change is brewing.

I’m currently migrating my WordPress installation over to a brand new server. This is primarily due to the huge increase in traffic Astroengine has been experiencing in recent months. All great news, but something had to give and it was my shared hosting account that eventually broke.

To celebrate the new server and faster delivery of content, I’ve also been working on a redesign. Expect a big change sometime between now and whenever I finish uploading the thousands of files to their new home (hopefully within the next day).

Thank you for your continuing loyal support.

A new era for Astroengine.com awaits…

Cheers, Ian

In the Cosmos/Iridium Collision, Which Satellite Won?

When two satellites collide at 790 km above the Earth’s surface, who really cares which satellite “won”? It’s going to be a mess; chunks of metal and shards of solar panels exploding to life after their once-solid satellite structures impacted at a velocity of 11 km/s (that’s kilometres per second). Both satellites are losers, twisted, shattered remains of their former selves, cluttering Earth-orbit, causing all kinds of stress for other vehicles flying around in orbit.

However, when the Iridium communications satellite was hit by the defunct Russian Cosmos 2251 on February 10th, it turns out there was a “winner” in the satellite demolition derby (although I am using the word “winner” very loosely)…
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