Showing posts with label galaxies. Show all posts
Showing posts with label galaxies. Show all posts

Tuesday, November 30, 2010

A Sandbar Made of Galaxies

"Astronomers Probe 'Sandbar' Between Islands of Galaxies"
Adam Hadhazy, Mission News, Spitzer, NASA (November 24, 2010)

"Astronomers have caught sight of an unusual galaxy that has illuminated new details about a celestial 'sandbar' connecting two massive islands of galaxies. The research was conducted in part with NASA's Spitzer Space Telescope.

"These 'sandbars,' or filaments, are known to span vast distances between galaxy clusters and form a lattice-like structure known as the cosmic web. Though immense, these filaments are difficult to see and study in detail. Two years ago, Spitzer's infrared eyes revealed that one such intergalactic filament containing star-forming galaxies ran between the galaxy clusters called Abell 1763 and Abell 1770.

"Now these observations have been bolstered by the discovery, inside this same filament, of a galaxy that has a rare boomerang shape and unusual light emissions. Hot gas is sweeping the wandering galaxy into this shape as it passes through the filament, presenting a new way to gauge the filament's particle density. Researchers hope that other such galaxies with oddly curved profiles could serve as signposts for the faint threads, which in turn signify regions ripe for forming stars...."

Since this 'bent' galaxy is about 11,000,000 light years away, we're not sending a probe there. Not any time soon. And what astronomers and cosmologists learn about it isn't likely to affect the next Super Bowl, or help anyone win the lottery.

Still, the Lemming thinks this sort of thing is interesting.

As for why studying this cosmic sandbar is important:

"...Knowing how much material these filaments contain and how they interact with galaxy clusters will be very important for understanding the overall evolution of the universe, Edwards said...."

Sort-of-related posts:
A tip of the hat to NASA, on Twitter, for the heads-up on this page.

Wednesday, November 10, 2010

Whacking Great Radiation Bubbles Blown From Milky Way's Center

"Huge Bubbles Found at Milky Way's Heart Could Signal a Black Hole Eruption"
Mike Wall, Space.com (November 9, 2010)

"Scientists have detected two gigantic bubbles of high-energy radiation spilling out from the Milky Way's center that may have erupted from a supermassive black hole.

"The mysterious structures each span 25,000 light-years across, meaning that together they cover more than half the area of the visible sky, and are emitting gamma rays, the highest-energy wavelength of light.

"The bulbous features may be evidence of a burst of star formation a few million years ago, researchers said. Or they may have been produced when a supermassive black hole in the center of our galaxy gobbled up a bunch of gas and dust.

"The newly discovered structures remain an enigma for now, scientists said. [New photo of gamma-ray bubbles]

" 'We don't fully understand their nature or origin,' said study leader Doug Finkbeiner of the Harvard-Smithsonian Center for Astrophysics...."

The article gives a brief overview of how astronomers looked for these oversize bubbles - and why.

We're not completely in the dark about what these things are - or what caused them. In general terms, at least. Specifics? That's going to take a lot more work. What we do know is that there was an enormous amount of energy involved in making the bubbles. And their appearance should narrow down possibilities for what started them:

"...Researchers aren't yet sure what created the bubbles. But the structures appear to have sharp, well-defined edges, suggesting they were formed by a large, rapid and relatively recent release of energy.

"Two leading candidate causes, according to Finkbeiner, are a surge of star formation several million years ago and a burst of activity by the Milky Way's central black hole, which is as massive as four million suns...."


(from Space.com, used w/o permission)
"These newly discovered gamma-ray bubbles extend 50,000 light-years, roughly half of the Milky Way's width, as shown in this illustration. Hints of the bubbles' edges were first observed in X-rays (blue) by ROSAT, a Germany-led mission operating in the 1990s. The gamma rays mapped by Fermi (magenta) extend much farther from the galaxy's plane. Credit: NASA's Goddard Space Flight Center...."

The Lemming's very interested in this sort of thing. Your experience may vary. That picture is a half-scale thumbnail of the one on the Space.com website. They've got two more: one showing a full-sky projection that gives an idea of what these twin bubbles 'look' like in the extremely high-frequency wavelengths the astronomers were studying.

One thing this almost certainly doesn't mean is that the Milky Way galaxy is exploding, and we're all doomed. Quite a few galaxies of the sort we live in have activity something like this happening in their core. We've known about the Milky Way's central black hole for some time, by the way. That was quite a discovery.

It's just as well that our star is in a more-or-less circular orbit around the Milky Way's core, and stays pretty much in the plane of the galaxy. As it is, we've got great seats for this show.

Or, rather, our robot observatories in space do. Very high-frequency 'light' like what these bubbles are emitting doesn't travel well through Earth's atmosphere. Which is just as well for us.

Related posts:

Tuesday, September 7, 2010

A Galactic 'Supervolcano' - No Kidding

"Galactic 'Supervolcano' Seen Erupting With X-Rays"
Space.com (September 6, 2010)

"A galactic 'supervolcano' in the massive galaxy M87 is erupting, blasting gas outwards. The cosmic volcano — driven by a giant black hole in M87's center — is preventing hundreds of millions of new stars from forming.

"An image, taken by NASA's Chandra X-ray Observatory and the National Radio Astronomy Observatory's Very Large Array, captures the drama in action.

" 'Our results show in great detail that supermassive black holes have a surprisingly good control over the evolution of the galaxies in which they live,' said Norbert Werner of the SLAC National Accelerator Laboratory in Melo Park, Calif., who led one of two studies of M87's black hole and its effects. 'The black hole's reach extends ever farther into the entire cluster, similar to how one small volcano can affect practically an entire hemisphere on Earth.'..."

That "supervolcano" remark isn't empty hyperbole. Although the space in and around a galaxy is pretty close to being a vacuum, there's a sort of 'atmosphere' of particles, atoms, and molecules. And x-rays from M87's black hole affect that ultra-thin gas in ways that are similar to the ways plumes from volcanoes affect our atmosphere.

On a much larger, and slower, scale of course.

Saturday, January 9, 2010

Early Returns From Galactic Census: Not As Many Planets as Expected

"Plenty of Solar Systems Like Ours Expected "
Space.com (January 5, 2010)

"There's good news and bad news.

"The bad news is that solar systems like ours are in the minority in the Milky Way. The good news is that's still an awful lot of potential twins out there.

"Combining the results of a search for extrasolar planets in our galaxy and a method for calculating the likelihood that extrasolar planets exist, only about 15 percent of the stars in the Milky Way likely host systems of planets like our own, one astronomer said here today at the 215th meeting of the American Astronomical Society.

" 'Now we know our place in the universe,' said Ohio State University astronomer Scott Gaudi. 'Solar systems like our own are not rare, but we're not in the majority, either.'

"The speculation came partially from an exoplanet-hunting effort called the Microlensing Follow-up Network (MicroFUN). MicroFUN uses a method called gravitational microlensing, which occurs when one star crosses in front of another from the perspective of Earth...."

If 'only' 15 % of the Milky Way galaxy's 200,000,000,000 to 400,000,000,000 stars have planets, that's 30,000,000,000 to 60,000,000,000 stars with planets sharing the galaxy with us.

That's a whole lot of zeroes.

And, as the Space.com article discusses, astronomer Gaudi's speculation and others are just that: speculations.

But, with hundreds of planets already spotted around other stars, they're informed speculations.

The phrase "like ours" isn't all that well defined. It could mean a star with a handful of rock planets orbiting nearby, with a few gas giants on longer orbits. Or, something else.

One point I found interesting was that there's a possibility that our Solar system has more than the average number of planets.
Related posts, at

Tuesday, December 29, 2009

Our Sun and The Fluff

"Fluffy Mystery at Edge of Solar System Solved"
Space.com (December 23, 2009)

"Our solar system is passing through a cloud of interstellar material that shouldn't be there, astronomers say. And now the decades-old Voyager spacecraft have helped solved the mystery.

"The cloud is called the 'Local Fluff.' It's about 30 light-years wide and holds a wispy mix of hydrogen and helium atoms, according to a NASA statement released today. Stars that exploded nearby, about 10 million years ago, should have crushed the Fluff or blown it away.

"So what's holding the Fluff in place?

" 'Using data from Voyager, we have discovered a strong magnetic field just outside the solar system,' explained Merav Opher, a NASA Heliophysics Guest Investigator from George Mason University. 'This magnetic field holds the interstellar cloud together ["The Fluff"] and solves the long-standing puzzle of how it can exist at all.'..."

The Voyager spacecraft aren't in The Fluff yet, but they're close enough to pick up its magnetic field.

So now astronomers have a really good idea what's holding The Fluff together. Next, I figure they'll be trying to discover what's generating the magnetic field.

More, about The Fluff:

Monday, December 21, 2009

Lemming Tracks: Dark Matter, Dark Stars, and Keeping Up

"Mystery Swirls Around 'Dark Stars' "
Space.com (December 21, 2009)

"When the very first stars lit up, they may have been fueled by the dark matter that has long eluded scientists.

"These 'dark stars,' first born nearly 13 billion years ago, might still exist today. Although they would not shed any visible light, astronomers might detect these invisible giants — some 400 to 200,000 times wider than our sun and 500 to 1,000 times more massive — because they should spew gamma rays, neutrinos and antimatter and be linked with clouds of cold, molecular hydrogen gas that normally would not harbor such energetic particles.

"If scientists find these stars, they could aid the search to discover and identify dark matter. They could also help solve the mystery of why black holes formed much faster than expected.

"Scientists think unseen, as-yet unidentified dark matter makes up about 95 percent of all matter in the universe. They know it exists because galaxies rotate faster than can be explained by the visible matter within them...."

This is a quibble, but that last paragraph isn't, quite, accurate - as far as I can tell. It's a fact: The visible parts of galaxies spin too fast, assuming that the stuff we see is all that's in the galaxies - and that gravity is all that's pulling the visible matter toward the center of the galaxy.

Dark matter is a pretty good working model to explain the odd behavior of stars and gas clouds in galaxies. And, it may actually exist.

Or, although this is getting more and more unlikely, dark matter may join phlogiston as a reasonable explanation for otherwise-unexplained phenomena - which turned out to be wrong.

The Space.com article discusses the possibility that the first stars were powered by the conversion of dark matter into energy. At this point, it looks like these "dark stars" wouldn't have radiated visible light - but would have emitted gamma rays, as the 2nd paragraph said.

Articles of this sort often use the phrase "dark matter" without trying to explain what it is. Can't say that I blame the writers and editors for that. It's easier to say what it isn't, than what it is.

Dark matter isn't ordinary stuff that's not illuminated. In other words, a rubber ball doesn't become "dark matter" when you put it in a drawer.

Princton's WordNet defines dark matter this way: Dark matter is "a hypothetical form of matter that is believed to make up 90 percent of the universe; it is invisible (does not absorb or emit light) and does not collide with atomic particles but exerts gravitational force".

Then there's dark energy - but that's another topic.

Dark Matter, Dark Stars, Stuff That's Billions of Years Old: So What?

I'll admit that it's hard to see how pushing the envelope of knowledge about dark matter will make a difference in whether or not the New Orleans Saints make it to the Super Bowl this year.

Or keep the sidewalks shoveled this winter.

On the other hand, right now I'm using practical applications of wave and particle physics to write this blog.

Whether or not there turns out to be a practical application to research in physics and cosmology - and, eventually, I'm pretty sure there will be - I think there's value in the knowledge itself. It helps that I'm one of those people who is interested in the universe and how it works.

And, I'm glad there are resources like Space.com, where I can try to keep up with what's known, what scientists are discovering about how much they don't know, and observations that conform (or refute) established models to explain why things happen.

Sunday, December 13, 2009

Gamma Ray Flare in Pegasus

"Brightest Gamma-Ray Flare in Universe Spotted"
Space.com (December 11, 2009)

"A distant galaxy with a giant black hole in its center has been acting up recently, emitting extremely bright flashes of gamma ray light.

"The flares began Sept. 15, making the galaxy currently the brightest source of gamma rays in the sky and boosting its own brightness to more than 10 times its regular luminosity over the summer. NASA's Fermi Gamma-ray Space Telescope has been observing the phenomenon to learn more about how such active galaxies work. Astronomers think this galaxy, identified as 3C 454.3, is what's called a blazar.

"Blazars, like many active galaxies, emit oppositely directed jets of particles traveling near the speed of light when matter falls toward their central supermassive black holes. What makes a blazar so bright in gamma rays is its orientation in space. One of the jets happens to be aimed straight at us, so it is easy to spot when viewed from Earth...."

Astronomers and astrophysicists still don't know what happened in 3C 454.3's jet to make it flare up, but right now it's the brightest persistent gamma-ray source in Earth's sky. Happily, the jet of high-energy particles that's pointed at us is a nice, safe 7,200,000,000 or so light-years away from us. Right now, even at that distance, it's outshining the Vela pulsar, whose jet is also pointed at us, and is a comparatively close 1,000 light-years away.


(from Fermi/NASA, used w/o permission)

Whatever's boosting gamma ray output in 3C 454.3 is increasing its brightness in radio and visible wavelengths, too: just not as much.

I'll grant that all of this doesn't have much to do with who's likely to win the next soccer cup, or (probably) what the weather will be like tomorrow.

On the other hand, I'm interested in this sort of thing for two reasons.

First, it's knowledge; knowledge is power; and "I like power." (Cobra Bubbles, "Stitch! The Movie" (2003))

And, although there's no guarantee that this particular avenue of exploration will pan out - immediately, anyway - I suspect that studying how apparently-unreasonable amounts of energy gets generated and directed could lead to quite practical applications. Like squeezing more energy out of matter than nuclear reactions manage.

We don't need that sort of power, yet. But, if people want to travel around at what we regard as a reasonable rate, we'll need power sources that aren't off-the-shelf technology today.

"...Alcubierre's intriguing equations suggest that we'll be able to travel faster than the speed of light: as soon as we figure out how to build machines that can warp space-time on a fairly large scale...." (May 29, 2009)

Actually, that'll probably take more power than any source we know of, theoretical or otherwise.

Friday, October 16, 2009

High-Energy Emissions From the Edge of the Solar System

"Mystery Emissions Spotted at Edge of Solar System "
Space.com (October 15, 2009)

"In the murky boundary between our solar system and the rest of the galaxy, scientists have spotted a bright band of surprising high-energy emissions.

"The results come from the first all-sky map created by NASA's new Interstellar Boundary Explorer (IBEX) spacecraft, which launched in October 2008. While orbiting Earth, IBEX monitors incoming neutral atoms that originate billions of miles away at the solar system's edge to learn about the interaction between the sun and the cold expanse of space.

" 'The IBEX results are truly remarkable, with emissions not resembling any of the current theories or models of this never-before-seen region,' said David McComas, IBEX principal investigator at the Southwest Research Institute in Texas. 'We expected to see small, gradual spatial variations at the interstellar boundary, some 10 billion miles away. However, IBEX is showing us a very narrow ribbon that is two to three times brighter than anything else in the sky.'..."

As I've mentioned before, it's pretty exciting when data comes in - and it's nowhere close to what the existing models predicted.

In this case, the strip of high-energy stuff seems to be lined up with this galaxy's magnetic field - so there's a really good chance that there's an unexpected interaction between the solar wind and the galactic environment.

The article has a couple of images from IBEX, and a diagram that shows one of the less-unlikely tentative explanations:

"
(from Adler Planetarium/Southwest Research Institute (SwRI), via Space.com, used w/o permission

Thursday, August 6, 2009

Like, Far Out! Offbeat Galaxies

"Speeding Stars Confirm Bizarre Nature of Faraway Galaxies"
Space.com (August 5, 2009)

"Stars in a distant galaxy move at stunning speeds — greater than 1 million mph, astronomers have revealed.

"These hyperactive stars move at about twice the speed of our sun through the Milky Way, because their host galaxy is very massive, yet strangely compact. The scene, which has theorists baffled, is 11 billion light-years away. It is the first time motions of individual stars have been measured in a galaxy so distant.

"While the stars' swiftness is notable, stars in other galaxies have been observed to travel at similarly high speeds. In those situations, it was usually because they were interlopers from outside, or circling close to a black hole.

"But in this case, the stars' high velocities help astronomers confirm that the galaxy they belong to really is as massive as earlier data suggested.

"Bizarre, indeed

"The compact nature of this and similar galaxies in the faraway early universe is puzzling to scientists, who don't yet understand why some young, massive galaxies are about five times smaller than their counterparts today...."

The article is a pretty good overview of an intriguing situation in astronomy, physics, and cosmology. Until the latest set of observations were made, there was a somewhat comfortable amount of uncertainty about exactly how massive these galaxies were and how far they are from us. It was possible to assume that the masses were lower than assumed, and the distances less.

That set of assumptions allowed existing theories of how galaxies - and the universe - developed to stand.

That was then, this is now.

"...'It's a bit of a puzzle,' [study leader and Yale University astronomer Pieter] van Dokkum told SPACE.com. 'We think these galaxies must grow through collisions with other galaxies. The weird thing is that these mergers must lead to galaxies that are larger in size but not much more massive. We need a mechanism that grows them in size but not in mass.'..."

I've written before, how it's nice when data confirms an existing theory: but exciting and rewarding when data doesn't fit the mathematical models. (March 23, 2009)

The trick is to come up with a revised, or new, theory - a new mathematical model - and see if that matches the real world.

"How Strange, Small Galaxies Lost Their Stars"
Space.com (August 4, 2009)

"Close encounters of the galactic kind may explain the existence of an unusual type of dwarf galaxy, a new study suggests.

"So-called dwarf spheroidal galaxies are small and very faint, containing few stars relative to their total mass.

"These star-deprived galaxies appear to be made mostly of dark matter — an elusive form of matter detectable only by its gravitational influence. Dark matter outweighs normal matter by a factor of five to one in the universe as a whole.

"Astronomers have found it difficult to explain the origin of dwarf spheroidal galaxies...."

Again: observed data and current mathematical models don't quite agree. I'm enough of an old fogy to think that it's the theories that need to be changed.

This article is a look - quick, but pretty good - of another bit of the cosmological puzzle that researchers are working on today.

Some words about dark matter:

"Dark matter" and "dark energy" are phrases that come up now and then in articles about what astronomers, physicists, and cosmologists are thinking these days. Some of those articles seem to have been written - or edited - by someone who learned science by watching the Star Wars movies.

I like the Star Wars movies, by the way: but they're to physics and astronomy what the Terminator movies are to robotics: 'Any resemblance to real science or technology, off-the-shelf or in development, is purely coincidental.'

Where was I? Dark matter and energy, right.

Turns out, "dark matter" isn't just a way for an astronomer to say, "I can't see it." Dark matter and dark energy are pretty good ways of explaining some observed phenomena. If they exist, they're very odd stuff. Dark matter isn't unlit stuff of the sort that the sun and planets are made of; it isn't antimatter; and it's not black holes. As for what it is - that's a matter of some debate.

I found a fairly clear discussion of dark matter and dark energy on the NASA website.

Right now, some enthusiasts notwithstanding, dark matter and dark energy are convenient mathematical models. The models may describe something that's real, or not.

This wouldn't be the first time that additional research showed that a part of the universe 'discovered' by a theory wasn't really there. I remember phlogiston. That doesn't mean that chemistry and physics are a fraud: Just that we don't know everything there is to know. There may be better models than what we have today, which more accurately reflect the underlying reality.

More-or-less-related posts: Background:

Tuesday, June 9, 2009

Colliding Galaxies Leave Debris

"Galactic Collisions Leave Cosmic Skid Marks "
Space.com (June 9, 2009)

"Cosmic debris stripped away from the wreck of colliding galaxies has been found by the Subaru telescope atop Mauna Kea, Hawaii.

"The debris fields could shed light on galaxy formation and starburst activity in the early universe by allowing astronomers to retrace the paths of the colliding galaxies before they merged.

" 'This is equivalent to finally being able to trace the skid marks on the road when investigating a car wreck,' said team member Nick Scoville of the California Institute of Technology...."

The article tells a bit about why finding new debris from a galactic collision is important to better understanding of what happened. The debris field is connected to "the Antenna" galaxies, a pair that's about 65,000,000 light years away. The field is big: several times the size of the Milky Way Galaxy.

As is usual with cosmological studies, the results won't have much effect on the price of gasoline or who wins the next World Series. But, I find humanity's continuing efforts to understand the universe a story that's worth following.

Tuesday, September 23, 2008

Re-Thinking This Galaxy's Habitable Zone

This won't make a bit of difference in how your coffee tastes, or whether the Mets will win the pennant.

But I thought it was interesting.

"Sun May Be Galactic Hitchhiker"
Space.com (September 22, 2008)

There have been assumptions about how stars orbit in the Milky Way galaxy, and what areas of the galaxy would be more - or less - favorable for life to exist. Those assumptions were reasonable, based on data that astronomers had, and mathematical models that they'd developed.

Now, there's a new model that may be a better fit with the real world. And, it shows that circular orbits in this galaxy shouldn't be that unusual - and that the orbits can shrink or grow and stay circular.

Which means that stars, including our sun, don't necessarily stay near where they were formed. It also means that the idea of "habitable zones" in the galaxy needs to be re-thought, since stars shift around more than we thought.
Related posts, at

Tuesday, June 3, 2008

"You Are Here" on a Galactic Scale - a Desktop Sculpture

"Beyond our solar system"
Living World (commercial site)

"A 3D model of the Milky Way,
with the Solar System positioned
in the exact center of the glass cube.
Small lot production....
"

For just 80,000 Japanese Yen. I think that's around $763USD.

There's a photo of this desktop sculpture.

It's the sort of thing I'd love to have - and couldn't justify buying.

Thursday, February 7, 2008

You are Here:
Map of Our Corner of the Universe

"The Universe within 1 billion Light Years The Neighbouring Superclusters"

Our galaxy doesn't show up at this scale. It's toward the edge of the Virgo cluster, about halfway between the Centaurus and Perseus-Pisces Superclusters.

I've been a little overwhelmed by personal events lately. Thinking about the 3 million or so large galaxies and roughly 500 million billion stars there helped me put my experiences in perspective: Worrying about family transitions and finances tends to fade when contemplating the vast scale and awesome structures of creation.

Thursday, November 22, 2007

Galaxies and Grocery Lists: Keeping Life in Perspective

One thing I like about astronomy is the way it puts things like international affairs and grocery lists in perspective.

These photos from the Hubble space telescope might help you put concerns in perspective: Now, because I feel like putting it here:

Vastness (excerpt)
Alfred, Lord Tennyson

Many a hearth upon our dark globe sighs after many a vanish'd face,
Many a planet by many a sun may roll with the dust of a vanish'd race.

Raving politics, never at rest—as this poor earth's pale history runs,—
What is it all but a trouble of ants in the gleam of a million million of suns?...

Related posts, at
Unique, innovative candles

Visit us online:
Spiral Light CandleFind a Retailer
Spiral Light Candle online store

Pinterest: From the Man Behind the Lemming

Top 10 Most-Viewed Posts

Today's News! Some of it, anyway

Actually, some of yesterday's news may be here. Or maybe last week's.
The software and science stuff might still be interesting, though. Or not.
The Lemming thinks it's interesting: Your experience may vary.
("Following" list moved here, after Blogger changed formats)

Who Follows the Lemming?

WebSTAT

Family Blogs - Blog Catalog Blog Directory