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!

Two Tales from the World of from Big Astronomy

Astronomy Stories are Cosmic!

Each year about this time, I go stand under a firehose of astronomy information. It’s actually called the American Astronomical Society winter meeting, and it brings together several thousand of the world’s astronomers (not just Americans) to share the latest and greatest in astronomy research.

So, what do we learn at this meeting? Let’s take just take two examples of things I heard about on this first day.

To Pluto…

Pluto mountains
A swatch of mountainous icy terrain on Pluto. Courtesy New Horizons mission.

It began with a Kavli Award talk given by Alan Stern, PI of the New Horizons mission. The view of this distant world as seen by the spacecraft is getting better with each data dump as it sends back mission data across billions of miles as it speeds toward a January 2019 encounter with the Kuiper Belt object 2014 MU69.

Alan’s overview showed that Pluto is an unexpectedly amazing world. For example, the large, heart-shaped Sputnik Planum is distinctly younger than the rest of Pluto’s surface — around only a million years old. This region is, as Alan stated, about the size of Texas and ringed by mountains made of water ice. There is also nitrogen and other ices, but even as cold as it is at Pluto, these ices are about the consistence of cold toothpaste — not something you can build mountains from.  Water ice,  yes — and the flyby data revealed water ice in amounts the team didn’t expect. Yet, there it is, in towering mountains the height of the Rockies in Colorado.

Sputnik Planum is brighter than the rest of the surface of Pluto, and has absolutely NO craters on it — which means that this region is constantly being resurfaced from below. That also implies something is supplying a heat source that melts and softens the ices flowing into the Planum, glacier-like.

The New Horizons team has also found evidence of ice volcanoes on Pluto, something that most of us thought might be there, but with no proof until the mission sent back high-resolution imaqes of intriguing features that do look like volcanic calderas made of ice, and evidence of volatiles (gases) near the vents.

The mission also mapped the Pluto atmosphere, which has distinct haze layers in it; and charted Charon (Pluto’s binary companion), and the smaller moons Nyx, Styx, Kerberos and Hydra. At least two of the smaller moons appear to be smashed-together objects and they spin very rapidly on their axes.

Want to learn more about Pluto? Visit  the New Horizons Web page for more images and info releases.

Astronomy Beyond the Galaxy

astronomy of black holes in galaxy with two black holes
Image of the galaxy SDSS J1126+2944 taken with the Hubble Space Telescope and the Chandra X-ray Observatory. The arrow points to the black hole that lost most of its stars due to gravitational stripping processes.

Now, the second story that intrigued me takes us far out of our own solar system and galaxy.

imagine if you will that you are an astronomer and you’re looking at, oh, say a galaxy called SDSS J1126+2944 using the Hubble Space Telescope and the Chandra X-ray Telescope. Hubble gives you a fine visible-light and near-infrared view of the galaxy, but Chandra reveals something kind of interesting and much more energetic: a pair of black holes at the galaxy’s heart.

One of the black holes is surrounded by stars (as supermassive black holes often are), but the other one is not. In fact, it’s strangely deprived of a stellar “coma”.

Why would that be?

That’s the question that Dr. Julia Comerford of the University of Colorado wants to answer. She’s the one who found the halfway-nekkid black hole, and she described it for us today.

“One black hole is starved of stars, and has 500 times fewer stars associated with it than the other black hole,” she said. “The question is why there’s such a discrepancy.”

One possibility she described is that the galaxy experienced a merger. As the merger went on, the galaxy was subjected to extreme gravitational and tidal forces that stripped away most of the stars from one of the black holes.

The other possibility, however, leads to a rare type of object called an “intermediate” mass black hole. That’s one with a mass of between 100 and 1 million times that of the Sun. Intermediate-mass black holes are predicted to exist at the centers of dwarf galaxies and would have a lower number of associated stars. These intermediate-mass black holes can grow and one day become supermassive black holes. If that’s what happened here, then Comerford has uncovered an object still somewhat rare in the pantheon of galaxy-class black holes.

“Theory predicts that intermediate black holes should exist, but they are difficult to pinpoint because we don’t know exactly where to look,” said Scott Barrows, a postdoctoral researcher at CU-Boulder who co-authored the study. “This unusual galaxy may provide a rare glimpse of one of these intermediate mass black holes.”

If this galaxy does indeed contain an intermediate black hole, it would provide researchers with an opportunity to test the theory that supermassive black holes evolve from these lower-mass ‘seed’ black holes.

There are many more astronomy stories being told at AAS! Stay tuned!

Exploring Science and the Cosmos

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