Category Archives: astronomy

teaching a master about planetary exploration

I’ve often wondered what it would be like for one of the astronomers of the past to come alive today. What would it be like for them to see what we’ve been doing in physics, space and planetary exploration, biology, chemistry, and so on? It’s a great storytelling hook: bring somebody like Galileo, for example, to a modern time and let them marvel at what we’ve done.

In Galileo’s case, he’d likely understand planetary exploration pretty well. People have been looking at the planets for several thousand years and he took advantage of that. Yet, I think you could say that the true exploration of the solar system began with him. He pointed his homemade telescope at Jupiter in early 1610 and found the four largest moons, which astronomers later gratefully named “the Galileans” in his honor. That set off a mad dash of Earth-based observations that continues to this day. And, I bet he’d be enthused that a Jupiter exploration spacecraft was named for him: Galileo.

A artist's concept of our solar system worlds as seen through our planetary exploration tools. Courtesy NASA.
Our understanding of the solar system has grown greatly in the days since Galileo’s first observations.
Courtesy NASA.

Planetary Exploration: What’s First?

So, what would Galileo think of the most recent planetary exploration efforts? Imagine that we could sit down with him for an afternoon and bring him up to speed. Where would we start? Probably the best approach is to take it in a linear timeline. That would give him the depth and breadth of humanity’s efforts at learning about the solar system in situ.

Planetary scientists began their spacecraft explorations in the early 1960s, with spacecraft sent to the Moon and Mars. After that came Venus and Mercury. Oh, and the Sun, let’s not forget that.

In the 1970s, they added Jupiter, Saturn, Uranus, and Neptune to the list of targets. Pluto didn’t get a visit until nearly five years ago, in 2015. And,the rest of the solar system objects (such as asteroids and comets), have been explored only beginning in the mid 1980s (with four spacecraft sent to Comet Halley). I’m sure I’m forgetting something, but this is the general trend of solar system exploration: select the targets and make spacecraft to explore them.

So, I can imagine telling Galileo, “Well, sir, we’ve looked at nearly everything now. You’re best remembered for those Galilean satellites you found, so we’ve sent several spacecraft out to explore Jupiter and its moons. In fact, we’re thinking of sending more spacecraft to explore Europa.”

And, then, he nods sagely in agreement. With a quirky smile and a glint in his eye, he raises his arms to the heavens and asks, “What about exoplanets? I’ve read about those? What are you doing about them?”

And, I say, “We’re still at the stage of merely detecting them from a distance. But soon, very soon, we should be able to point very complex instruments at them and learn much more about those distant worlds.”

He nods again. “Of course. Now, tell me more about the most-explored world!”

Would that Be Mars?

Of course, Earth is the world we know best. And, we explore it with spacecraft continually. There’s still much to learn about our home planet. But, our imaginary Galileo isn’t interested in that. He wants to know more about other planets. So, I choose Mars. “You know of Mars, the Red Planet, right?”

He nods, favors me with a gentle smile, and opens his hand to encourage me to tell him more. “Sì, per favore continua.”

I smile because I know he’s gonna LOVE the tale of Mars exploration.

“Well, we’ve sent dozens of spacecraft to explore Mars—about eighty, in fact. Not all of them made it safely, but the ones that have told us wondrous tales of the Red Planet,” I start out by saying.

I go on to tell him about my favorite spacecraft (of the moment): Mars Curiosity. “It’s a roving machine that landed on Mars in the year 2012. It has wheels and follows commands sent to it from Earth to roll around and study the rocks and sand that are on the surface. Curiosity is a rugged explorer and has taught us much.”

As I talk, I wonder if he’s understanding half of what I say. But, the alert, lively look in his eyes tells me that this whole story has piqued his curiosity. He nods in understanding, and bids me to go on.

Curiosity’s Summer of Planetary Exploration

When Curiosity landed on Mars, it settled down near a peak called Mount Sharp. It’s centered in Gale Crater, an impact feature that appears to also have been inundated with water sometime in the past. Curiosity has explored clay-rich regions and will soon begin to explore sendimentary rocks on the slopes of Mount Sharp. Every layer of rock will reveal some clue to Mars’s water-rich past.

To get to its target, Curiosity will have to steer around a sandy stretch of landscape. Controllers don’t want it to get stuck in the sand as one of its predecessors, the Spirit rover did. So, it has to move about a mile (about a kilometer and a half) around the sand pit. Once Curiosity arrives on the slope of Mount Sharp, then it will resume its study of topsoil and rocky layers.

“But, why study the rocks?” asks Galileo. I smile at him. It could be that he’s not completely aware of the relationship between rocks, water, and the possibility of life. So, I take a deep breath and explain more.

“Signore Galileo, rocks tell a tale of conditions on the planet. Here on Earth, some rocks erupt from volcanoes and flow onto the landscape. Other rocks form as layers of dirt and sand pile up on each other. The wind may deposit them. Or, water may move them into layers. Rocks that have been in contact with water have special characteristics and chemical elements. The same types of rock have formed on Mars. We look for sedimentary rocks, for example, in order to understand where and when the water existed on this planet. And, of course, life requires water. So, if Mars once had a lot of water, perhaps it supported life.”

Why Explore a Planet?

Galileo considers this for a while. In fact, he stays deep in thought for a long, long time. Then, he asks many questions about how the spacecraft does this. I tell him about Curiosity’s instruments and how they work. I mention that teams of scientists and technicians control the spacecraft and tell it what to do. Of course, I also tell him about the long distance between us and Mars. Finally, he asks, “What will you do with all this knowledge of Mars?”

A good question.

“Signore, among other things, we hope one day to GO to Mars,” I say, hoping that he understands the need for humans to explore. “To have people stand on its surface and explore it first-hand is a big step for all of us. These spacecraft we send are like the first explorers of your own time who sailed the seas of Earth to find new lands. In this case, however, we want to approach Mars with respect, and if it has life, we need to know what that life consists of. If it has no life, or if we decide to live there, we need to know about its characteristics. Spacecraft such as Curiosity send back valuable data so that we can plan future missions for more robotic missions, and eventually, for humans.”

The Future Through the Past

The first peek through a telescope that Galileo Galilei took may have been a baby step, but it provided humanity with a leap to the planets. What if Galileo had never looked through a telescope? Chances are that somebody else would have, eventually. The telescope existed in his time, and it only needed one person to use it for planetary exploration. So, somebody else would get the credit for first astronomy use of a scope. But, the story might not be as crucial to science as Galileo’s contributions came to be.

If Galileo lived today, I have no doubt he’d be heading up spacecraft missions, directing people to do everything they could to explore distant worlds. That’s because he was a curious person, just as we are today. His questions started revolutions of thought and science. Galileo’s influence may have begun in the past, but it pointed the way to a future of planetary exploration. The smallest acts reverberate throughout time. And so, we have Galileo peeking through a scope at distant worlds, and with that act, he inspired the exploration of places such as Mars.

distant Quasars: Action in the Early Universe

We live in a time when our telescopes can look back to almost the beginning of the universe. That includes the most distant reaches of the cosmos, and, of course, everything in between. Even though astronomers have a good idea of the different categories of objects in the universe, they’re still learning about the details. Take quasars, for example. They exist throughout the universe and appear to have been most active earlier in cosmic history. Understanding them has taken decades, and there is still a LOT to learn about these distant cosmic objects.

An artist's conception of the quasar Poiua'ena. Courtesy W.M. Keck Observatory. Quasars like this raise questions about the early universe.
An artist’s conception of the quasar Poniua’ena. Quasars like this raise questions about the early universe.Courtesy W.M. Keck Observatory.

The name “quasar” comes from the term “quasi-stellar object”. They caught astronomers’ attention back in the 1950s. That’s when the first ones were detected as strong radio-frequency emitters. Images taken later on showed dim, star-like objects that were the sources of the strong radio emissions. Yet, spectroscopic studies of the light emitted showed that these dim things lay at huge distances from Earth. What could be that strong in radio, show up as a dim star, and be so far away? It was a challenge for astronomers to explain them.

Today, we know quite a bit more about quasars. Their activity comes from the gobbling action of central supermassive black hole embedded in massive galaxies. Yes, black holes are the “engines” of quasars. Astronomers estimate that 50,000 exist and more will be discovered as they scan the sky.

Distance is Important

Recently, astronomers using the Gemini Telescope on Mauna Kea in Hawai’i found Poniua’ena, in a sky survey. Then, they followed up with spectroscopic studies using the Keck telescope. Poniua’ena is a Hawai’ian name. It means “unseen spinning source of creation, surrounded with brilliance.” (The catalog number is J1007+2115.) And, yes, it’s incredibly brilliant and, at just over 13 billion light-years, is nearly as far away as ULAS J1342+0928.

The most known distant quasar, called ULAS J1342+0928 is the current record-holder, at just over 13 billion light-years. The universe itself currently is somewhere around 13.7 billion years old. ULAS (for short) was born during a time when the first stars and galaxies were coalescing (the so-called “epoch of reionization” (EOR). So, that makes this quasar and Poniua’ena very old. They formed when the universe was very young. And, early quasars raise questions about their black holes. How could they grow so large so quickly to create quasars only a few hundred million years after the universe was born?

Quasars and the Epoch of Reionization

The EOR is, itself a fascinating challenge to study. Its distant, its objects are mostly dim, and astronomers are still watching for its earliest “ignition”. The birth of stars and galaxies started during the EOR, and about 400 million years into this period of cosmic history, the first black holes “seeds” may have begun to form. Interestingly, black holes are the central engines for quasars, but they are far more massive than the tiny ones that existed “way back when”.

Like other quasars, ULAS J1342+0928 and Poniua’ena get their power from the black holes at the hearts of their host galaxies. For ULAS, the black hole has about 800 million times the mass of the Sun. Poniua’ena’s is 1.5 billion solar masses.

Activities in the superheated region around the black holes (including jets) are what make the quasars look so bright. As material spins down into the black hole, it gets heated by friction, and also by the action of powerful magnetic fields. That heating produces radiation in the form of light across the electromagnetic spectrum. Some material escapes through powerful jets that stream from the region of the black hole. That, too, emits radiation. It’s a busy, hot, and lethal environment.

Looking for Quasars

So, are there other quasars just as distant as ULAS J1342+0928? and Poniua’ena? That’s the question astronomers want to answer as they survey the sky with various instruments that can detect the light and other radiation emanating from quasars. Since quasars appear early in cosmic time, they play some role in the history and evolution of the universe. The exact nature of that role remains to be understood. To even being to figure it out, astronomers have to do wide-area sky surveys to find these quasars, which is like searching for the proverbial needle in a haystack.

Forming Quasars

Obviously, to get to be a quasar, a massive galaxy needs a supermassive black hole at its heart. Early on in its formation, the galaxy may have a fairly small black hole in the core. But, to shine brightly across billions of light-years, the black hole has to become more massive. Since it grows by gathering more and mass into itself, eventually it becomes a supermassive black hole that powers the quasar. But, that raises an interesting conundrum.

Making a supermassive black hole takes a long time. And, for a quasar to exist when the first stars were forming after the birth of the universe, that means its supermassive black hole “engine” had to grow fairly fast. So, one big question about these early, distant quasars is: how did the universe produce such massive quasar engines so quickly?

Quasar Poniua’ena’s Early Existence

For Poniua’ena, that means its black hole had to start as a fairly massive black hole “seed” a hundred million years after the Big Bang occurred. That’s sort of like expecting a newborn baby to write the complete works of Shakespeare or formulate a new language only a few months after it is born. The existence of such massive black holes in the hearts of galaxies so soon after the universe was born challenges current theories about how they form.

The discovery and study of very distant quasars such as Poniua‘ena and ULAS J1342+0928 shed insight into the early universe. Both they and their massive galaxy hosts formed deep in the Epoch of Reionization. How and why did they form so early? What processes are at work to enable such massive objects to exist so early? Are there earlier quasars than these? The answers to all these questions will (if you’ll pardon the pun) shed light on the earliest events that we can possibly observe in our universe.