Probing the Nearby Space Between Stars

The Value of Long-Term Observations of Space

space
Both HST and our old friends the Voyagers are giving new looks at interstellar space,. STScI/NASA

Space has an infinite number of stories, and they get told many different ways. It’s been a while since I’ve attended a press conference where Voyager observation results have been discussed. So, it was with great interest I went to a talk this morning describing how these venerable spacecraft are helping astronomers probe the makeup of interstellar clouds beyond our solar system.

The presentation was doubly interesting because it also talked about a result that began astronomers on the path of discovery in the clouds of the local instellar medium. I first heard about in 1996 when I was at CU as a graduate student. The first study was made by dissecting starlight streaming through the so-called Local Interstellar Cloud. The work was done by Dr. Jeffrey Linsky and colleagues, using the Goddard High Resolution Spectrograph on Hubble Space Telescope. Those observations allowed Linsky to “illuminate the cloud” and use the starlight streaming through to figure out its rough extent. He’s continued to work on the problem, and in recent years, people have turned to starlight to understand more about the chemical makeup and structure in the cloud.

So, fast forward to today, where a student researcher described using data from Voyagers 1 and 2, plus the Hubble Space Telescope, to further probe the cloud.

The Voyager Contribution

While today’s story included HST data, the tale really began in 1977. That’s when the Voyager 1 and 2 spacecraft left Earth on a jaunt past several outer solar system planets on their way out of the solar neighborhood. They are now on a one-way road trip to the stars, and are sampling the interstellar medium as they go. The ISM, as it’s called for short, is filled with gases and elements ejected from long-gone stars, as well as clouds of hydrogen gas. As they go along, their instruments are studying the ISM and sending data back to Earth.

HST Gets into the Act

The Hubble Space Telescope, which came along well after the Voyagers had finished their planetary missions, has been measuring the ISM along a line of sight that includes the paths that both Voyagers are following. This is the work that Linsky has been doing. HST has been finding evidence for multiple clouds of hydrogen along the path, clouds that also contain other elements from stars. All this data from all the probes is giving us a new and more nuanced look at the ISM, and the solar system’s

A student who was likely a small child when Linsky was doing his first observations told us today that her team’s work will synthesize the data from the Voyagers — which are our “on the spot” reporters. Along with the Hubble data (which is giving us the long view of the starlight passing through the clouds), the observations give us a much better “view” of the interstellar medium both from Earth orbit and “in situ“.

The good news is that the Voyagers are still working and should be able to give us maybe 10 years of data as they probe the clouds of gas and dust beyond the solar system. And, as long as HST is orbiting and working, we’ll probably hear a lot more about our neighborhood in the galaxy.

For example, Hubble found that Voyager 2 will move out of the interstellar cloud that surrounds the solar system in perhaps 2,000 years. After that, astronomers think that the spacecraft will spend 90,000 years in a second cloud before passing into a third interstellar cloud.

The Sun’s Progress

Based on the HST data, it also seems that the Sun is passing through clumpier material in nearby space. This which may affect the heliosphere, which is the large bubble containing our solar system that is produced by solar wind. At its boundary, called the heliopause, the solar wind pushes outward against the interstellar medium. Hubble and Voyager 1 made measurements of the interstellar environment beyond this boundary, where the wind comes from stars other than our sun.

The heliosphere gets compressed when the Sun moves through dense material, but it expands back out when the star passes through low-density matter. So, HST gives good insight into that, while the Voyagers are still our outermost scouts probing the space beyond the heliosphere.

I love stories that demonstrate the value of long-term studies. It’s one thing to look at the sky quickly and see an object and its events. But, if you really want to know what’s happening over time, the work of generations of astronomers and their instruments is the way to go!

(Note: this story came from a press conference and press release by STScI and the AAS.)

11.5 Weeks to Black Holes in the Distant Universe

X-rays From Black Holes Reveal Growth Over Time

black holes
This image contains the highest concentration of black holes ever seen, equivalent to 5,000 over the area of the full Moon. CXC.

What do you think you could find if you pointed an extremely sensitive x-ray telescope toward a distant part of the sky for nearly three weeks? That’s the challenge that Chandra X-ray Telescope scientists took on. The result is the image on the left.

This highly detailed view was produced by the observatory and gives astronomers the best look yet at the growth of black holes over billions of years beginning soon after the Big Bang.

This is the deepest x-ray image ever obtained. It comes from what is known as the Chandra Deep Field-South study. The central region of the image contains the highest concentration of supermassive black holes ever seen. The observations, which began in 1999 and continued into 2016, totaled more than 7 million seconds of telescope time. What those 11.5 weeks of total time covers an astonishing depth of study that stretches back through 12.5 billion years of time.

Using X-rays to Trace Black Holes

The image explores the earliest days of black holes in the universe. About 70% of the objects in the new image are supermassive black holes and it’s so rich that it allows scientists to see change over time.

How can black holes emit x-rays? Gas falling towards these black holes becomes much hotter as it approaches the event horizon/ That superheating results in bright x-ray emission. And, tracing those emissions is what gives astronomers new insights about the types and sizes of black holes nurtured by the early cosmos and their rates of growth.

How Does the Black Hole Garden Grow?

The growth of black holes in the early universe is a huge topic of scientific interest. Deep x-ray studies give astronomers a good idea about their evolution back “in the day”. It turns out that black holes grew mostly in bursts rather than slowly gobbling up material over time to get bigger in the epoch just after the Big Bang.

The x-ray emissions from these massive objects also help astronomers understand something about the “seeds” they grew from. It turns out that they may have started out with masses about 10,000 to 100,000 times that of the Sun, rahter than as really small black holes of just a few hundreds of solar masses. Moreover, they appear to have grown very rapidly to more than a billion solar masses very early on.

Black Holes as Far as They Can “See”

The researchers also detected x-rays from massive galaxies at distances up to about 12.5 billion light-years from Earth. Most of the x-ray emission from these distant galaxies likely comes from large collections of stellar-mass black holes within them. They formed from the collapse of massive stars and typically weigh a few to few dozen times the mass of the Sun.

How They Observed The X-Ray Deep Field

The team combined Chandra x-ray data with very deep Hubble Space Telescope data over the same patch of sky. They studied x-ray emission from more than 2,000 galaxies identified by Hubble that are located between about 12 and 13 billion light-years from Earth.

What’s Next?

Chandra and future x-ray observatories will be needed to provide a definite solution to the mystery of just how supermassive black holes grew to reach their current massive states. Now that the deep field has shown the way, astronomers will take much larger samples of distant galaxies using the James Webb Space Telescope. That will give even more targets for x-ray sensitive observatories to observe further out in space and back in time.