Category Archives: astronomy news

Astronomy Firehose: Day 2 of Exploring the Universe from Florida

 

Astronomy Thought-provokers

The universe is filled with interesting objects that tell some of the most fascinating stories in astronomy. Today, among other topics, we heard about weird x-ray objects and the possibility of searching out civilizations in globular clusters. If anybody in Hollywood needs a writer to cover those ideas for the next galaxy-spanning Sci-Fi epic, I’m your person!

The Andromeda Galaxy’s X-ray Binaries

astronomy news: scientists find x-ray binaries in the Andromeda Galaxy
At approximately 2.5 million light-years away, the Andromeda Galaxy, or M31, is our Milky Way’s largest galactic neighbor. The entire galaxy spans 260,000 light-years across – a distance so large, it took 10 GALEX images stitched together to produce this view of the galaxy next door.
The wisps of blue making up the galaxy’s spiral arms are neighborhoods that harbor hot, young, massive stars. Meanwhile, the central orange-white ball reveals a congregation of cooler, old stars that formed long ago.
Andromeda is so bright and close by that it is one of only three galaxies that can be spotted from Earth with the naked eye. This view is two-color composite, where blue represents far-ultraviolet light, and red is near-ultraviolet light.

So, what happens when an object sends out lots of x-ray radiation? Obviously, it catches the attention of astronomers because it’s very likely telling us that something fascinating is happening. X-rays are generated in very hot, active environments, such as near black holes or in the explosions of massive stars. Our Sun also gives off x-rays, particularly as it generates strong outbursts called flares.

Our galaxy — and many others — has a collection of objects called x-ray binaries. Each one contains a black hole or a neutron star accompanied by a stellar companion. These pairs give off prodigious amounts of x-rays.

Astronomers looked at the nearest spiral galaxy to us — called the Andromeda Galaxy — and 40 of its x-ray binaries. They used the Nuclear Spectroscopic Telescope Array, or NuSTAR, to study them and figure out what role they played in early galaxy formation. Some researchers suspect that these objects could have been responsible for heating up intergalactic gas clouds in the early universe. The idea is to study these x-ray binaries in a “nearby” galaxy and then apply what we learn about them to similar objects that existed when the universe was very young.

In x-ray binaries, material from the companion star can “spill over” and then be captured by the strong gravitational pull of the nearby black hole or neutron star. That material gets heated to incredibly high temperatures, and the result is an intense release of x-rays.

NuSTAR looked at a swath of Andromeda, which revealed the 40 binaries. Now astronomers are working on identifying which ones may have black holes and which are powered by neutron stars. These remnants of stellar evolution and their companion stars may have played a very central part in heating the early universe.

Life in a Crowded Stellar Suburb

astronomers think about planets in globular clusters.
Are there planets orbiting the stars of this globular cluster? If so, could there be a thriving interstellar civilization there? Recent studies at Harvard are exploring those possibilities. Courtesy STScI.

As you probably know, astronomers have been finding planets around other stars for a few decades now. The big question — do they bear life? — is the question that is, so far, unanswered. At least one of those planets has been found in a globular cluster, which is a collection of a million (or more) stars packed into an area of space about 100 light-years across. That led astronomer Rosanne DiStefano of Harvard-Smithsonian Center for Astrophysics to wonder whether more planets might exist in globular clusters. And, since she was engaging in “what if” scenarios, she speculated about what civilizations could exist on those planets.

“A globular cluster might be the first place in which intelligent life is identified in our galaxy,” she said today.

Globular Clusters? Really?

At first glance, globular clusters don’t seem like great places to grow planets. They’re old — they formed about 10 billion years ago. Their stars contain fewer of the heavy elements needed to make planets. Those elements (like iron and silicon) are created in earlier generations of stars. Some scientists have argued that this makes globular cluster stars less likely to host planets. However, DiStefano and Alak Ray (Tata Institute of Fundamental Research, Mumbai) think that view is much too negative.  “It’s premature to say there are no planets in globular clusters,” Ray said.

If you look at a globular cluster, it seems like it would be too crowded to allow planets to exist in stable orbits around their stars. However, it turns out that if a star’s habitable zone is close enough in, a planet could exist in a reasonably stable orbit. And, if it’s an Earth-like planet around an older, cooler star, that zone would be pretty close.

Here’s another thing about those clusters. Since they are old, their most massive stars have died off, leaving behind the older, cooler stars — and a supply of heavier elements that could be useful in planet formation.

So, it does seem possible that habitable planets can form in globular clusters and survive for billions of years. Take the next step and endow them with civilizations, and you have a whole new set of thoughts to consider about the possibilities for life on them, and what globular cluster civilizations would be like.

Such a civilization would enjoy a very different environment than our own. The nearest stellar neighbors would be just a trillion miles away, That would make interstellar communication and exploration quite easy, compared to what we have to do here on Earth to talk to the neighbors.

“We call it the ‘globular cluster opportunity,'” said DiStefano. “Sending a broadcast between the stars wouldn’t take any longer than a letter from the U.S. to Europe in the 18th century.”

“Interstellar travel would take less time too. The Voyager probes are 100 billion miles from Earth, or one-tenth as far as it would take to reach the closest star if we lived in a globular cluster. That means sending an interstellar probe is something a civilization at our technological level could do in a globular cluster,” she said.

The closest globular cluster to Earth is several thousand light-years away, making it difficult to find planets from our vantage point. It’s a big problem in the core of a cluster. That’s because the stars there are really jammed in together. But, it could be possible to detect planets on the outskirts of globular clusters. Astronomers might even spot free-floating planets by using applications of gravitational lensing. That occurs when the planet’s gravity magnifies light from a background star.

A more intriguing idea might be to target globular clusters with SETI search methods, looking for radio or laser broadcasts. That concept has a long history: the late astronomer Frank Drake used the Arecibo radio telescope in 1974 to broadcast the first deliberate message from Earth to the globular cluster Messier 13 (M13).

Okay, so we don’t KNOW if there are planets and civilizations in globulars, yet. But, DiStafano and her colleagues have raised some cool things to think about as we look for exoplanets in our galaxy — and beyond. THAT is one of the great attractions of astronomy!

By the Light of a Wobbly Moon

Mimas Wobbles Due to Ocean or a Weird Core

Meet Mimas, the moon with the wobbly orbit around Saturn that might be hiding a weird core or a subsurface ocean. Courtesy NASA/JPL-Caltech/Space Science Institute

Okay, so this is kind of cool news. Astronomers studying the Saturnian moon Mimas used Cassini images of it to figure out how much it wobbles as it orbits Saturn. Turns out, it jiggles quite a bit, and that has set off a flurry of speculation about what would cause it to do that. Picture a top the shape of a Star Wars Death Star (which is kind of what Mimas looks like) wending its way around Saturn. As it does, its spin is off-kilter. And that means something’s a little odd inside Mimas.

What are the possibilities?  For one, since the wobble is about double what scientists expected it to be, whatever it is that throws the moon off as it spins has to be massive. That could mean an ocean (which would easily affect how the moon spins) or an oddly shaped core. One of the scientists suggested that if it’s the core, then it would have to be nearly football-shaped to do the trick.

How could a core get to be oblong instead of round in a world as old as Mimas? (It dates back to the earliest epochs of the solar system and is about 4 billion years old.)  One school of thought says that the core may have frozen into an oblong shape long ago, thus preserving some hint of its early history.

If Mimas is hiding an ocean beneath its cratered surface, then a little bit of math tells us that a liquid water ocean would be hidden at least 24 kilometers beneath the crust. There also needs to be some mechanism to keep the water liquid. Mimas long ago lost all the heat from its formation and its core is likely cool as well.

So, what would keep things warm enough to sustain liquid?  It turns out that tidal flexing — that is, the squeezing and contracting due to Saturn’s strong gravitational pull that Mimas undergoes as it orbits the planet — could keep things warm enough through friction to do the trick. Mimas undergoes a fairly elongated (think of it as egg-shaped) orbit around Saturn, and so at different times at its orbit it encounters changes in the gravitational pull.  This slight deviation in its orbit causes the point on Mimas’ surface that faces Saturn to vary a bit over time. If you could watch Mimas from Saturn, you’d see that wobble and notice how small areas of the surface limb shift just enough to become visible. This effect is called libration. Our own Moon has the same  motion.

So, which is it: football-shaped core or liquid ocean?  Further analysis leans toward an ocean, since models of an oddly shaped core seem to result in a different-looking Mimas than the one we really have out there. As usual, more data will help tell the story, and the Cassini Solstice mission can be counted on to crank out more images of Mimas as it pursues its wobby path around the Saturn. Stay tuned!