Monday, March 11, 2024

Good News and Bad News for Astronomers’ Biggest Dream

The National Science Foundation takes a step (just one) toward an “extremely large telescope.”


One of the two proposals for an “extremely large telescope” could involve construction on Mauna Kea in Hawaii.
Credit...Caleb Jones/Associated Press


By Dennis Overbye
March 8, 2024


The United States should commit $1.6 billion to building an “extremely large telescope” that would vault American astronomy into a new era, according to the National Science Board, which advises the National Science Foundation.

In a statement on Feb. 27, the board gave the foundation until May to decide how to choose between two competing proposals for the telescope. The announcement came as a relief to American astronomers, who have been fretting about losing ground to their European colleagues in the quest to examine the heavens with bigger and better telescopes.

But which of the two telescopes will be built — and the fate of the dreaming and the billions of dollars’ worth of time and technology invested already — remains an open question. Many astronomers had hoped that the foundation, the traditional financier of national observatories, would find a way to invest in both projects.

The two projects are the Giant Magellan Telescope at Las Campanas in Chile and the Thirty Meter Telescope, possibly destined for Mauna Kea on the island of Hawaii, also known as the Big Island. Both would be larger and more powerful than any telescope currently on Earth or in space. Each is expected to cost some $3 billion or more, and less than half the projected cost has been raised so far by the international collaborations backing them.

In an announcement circulating among astronomers, the board said that funding even one telescope at the price point of $1.6 billion would take up most of the N.S.F.’s typical budget for construction.

“Moreover, the priorities of the astronomy and astrophysics community must be considered in the broader context of the high-priority, high-impact projects for the many disciplines that N.S.F. supports,” the board said in its statement last week.

So far, astronomers with a stake in the outcome have been careful to note that Congress, as well as the White House and the science foundation, would eventually all have their say.

“This is a marathon, not a sprint,” said Robert Kirshner, director of the Thirty Meter Telescope International Observatory and a former member of the Giant Magellan team. He added that he was hopeful that both telescopes could go forward.


Michael Turner, an emeritus cosmologist at the University of Chicago and former assistant director for mathematical and physical sciences for the N.S.F., called the recent development “excellent news for U.S. astronomy and saw “a realistic path forward” for an extremely large telescope.

“Before you know it, the telescope will be dazzling us with images of exoplanets and the early universe,” he said. “Should it have happened faster? Of course, but that is history. Full speed ahead, eyes on the future!”

Wendy Freedman, a cosmologist at the University of Chicago who led the Giant Magellan project in its first decade, said in an email: “I am very pleased that the N.S.B. has decided to fund an E.L.T. I think that the worst outcome would have been not to fund any E.L.T. at all; that would have been a tragedy! Realistically (and unfortunately), there is not a budget for two. But an E.L.T. is critical for the future of U.S. astronomy.”

She added, “So I am very relieved.”

Robert Shelton, president of the Giant Magellan collaboration, said: “We respect the National Science Board’s recommendation to the National Science Foundation and remain committed to working closely with the N.S.F. and the astronomical community to ensure the successful realization” of an extremely large telescope, “which will enable cutting-edge research and discoveries for years to come.”

But Richard Ellis, an astrophysicist at University College London who was one of the early leaders of the Thirty Meter Telescope project, told Science, “It’s a tragedy, given the investment made in both telescopes.”

The power of a telescope to see deeper and fainter objects in space is largely determined by the size of its primary mirror. The largest telescopes on Earth are eight to 10 meters in diameter. The Giant Magellan would group seven eight-meter mirrors to make the equivalent of a 25-meter telescope; the seventh and final mirror was cast last year, and workers are ready to pour concrete at the site on Las Campanas.

The Thirty Meter would be composed of 492 hexagonal mirror segments, scaling up the design of the twin 10-meter Keck telescopes being operated on Mauna Kea by the California Institute of Technology and the University of California. (The 100th segment was just cast in California, but protests by Native Hawaiians and other critics have prevented any work on the T.M.T. site on Mauna Kea; the project group has been considering an alternative site in the Canary Islands.) Neither telescope is likely to be ready until the 2030s.

Even as the American-led effort progresses, the European Southern Observatory is building an extremely large telescope — called the Extremely Large Telescope — at the Paranal Observatory in Chile. Its main mirror, composed of 798 hexagonal segments, will be the biggest and most powerful of all — 39 meters in diameter. It will also be the first among the competitors to be completed; European astronomers plan to start using it in 2028. If the effort is successful, it would be the first time in a century that the biggest functioning telescope on Earth is not on American soil.

Both the Giant Magellan and the Thirty Meter telescopes are multinational collaborations headquartered a few miles apart in Pasadena, Calif.

Support from the N.S.F. has been a point of contention between the two groups from their beginnings 20 years ago.

In 2019, the two groups agreed to join forces to create an American E.L.T. program, under the purview of the National Optical-Infrared Research Laboratory in Tucson, Ariz., that would allow American astronomers to utilize both telescopes. Astro 2020, a blue-ribbon panel of the National Academies of Science, endorsed the proposal, calling it the top priority in ground-based astronomy for the decade. The panel recommended that the science foundation chip in $1.6 billion to buy part ownership in one or both of the telescopes.

But the costs of these telescopes has continued to rise, and $1.6 billion doesn’t go as far as it once did. And the wheels of the scientific community and the federal government turn slowly.

“That process takes three to five years,” said Linnea Avallone, chief officer for research facilities at the N.S.F. “We’ve been engaged for just a bit over a year. I don’t think we’re dragging our feet; I don’t think we’re not being aggressive. She added that the foundation was being “very good stewards of the taxpayers’ money.”

Did she see a risk to the United States not funding an Extremely Large Telescope of its own?

“That’s a good question, better answered by astronomers,” Dr. Avallone said.


Dennis Overbye is the cosmic affairs correspondent for The Times, covering physics and astronomy. More about Dennis Overbye


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Why astronomers are worried about 2 major telescopes right now

By Monisha Ravisetti 
SPACE.COM
published  23 hours ago


Scientists may only get to have either the Giant Magellan Telescope or the Thirty Meter Telescope. The problem? Both are already in the works.

An artist's rendering of the US-ELTP Thirty Meter Telescope (TMT) (left) and Giant Magellan Telescope (GMT) (right) with their Laser Guide Stars (LSG) turned on.
 (Image credit: US-ELTP (TIO/NOIRLab/GMTO))

There's a bit of tension right now in the U.S. astronomy community and, perhaps unsurprisingly, it has to do with telescopes — extremely large telescopes, in fact. Here's what's going on.

The National Science Foundation (NSF), a source of public funding that two powerful next-gen observatories have been banking on for financial support, is facing pressure to go forward with only one telescope. This is because last month, the National Science Board — which is basically an advisory committee for the NSF — recommended that it cap its giant telescope budget at $1.6 billion. This is a lot of money, but it's just not enough for both. The board even says the NSF will have until only May of this year to decide which telescope gets the go-ahead.

Yet, both telescopes are already in the middle of construction, both are equally important and both are actually supposed to work together to fulfill a wide-eyed dream for astronomers. Because of how utterly huge they're meant to be, they're expected to one-up even the $10 billion James Webb Space Telescope (JWST) in many ways. That's the gold-mirrored, silvery-shielded trailblazer sitting a million miles from Earth right now, finding deep space gems so quickly it's normalizing us to seeing things humanity once couldn't fathom seeing. Imagine something better.

"To my knowledge, neither telescope today has a path forward without the investment by NSF," John O'Meara, chief scientist at the Keck Observatory, told Space.com. "I've said in other interviews that 'great vision should drive great budget, not vice versa,' and I believe it here."

One of the big scopes is the Giant Magellan Telescope (GMT). It's taking shape as you read this in the clear-skied deserts of Chile, and it's projected to cost something like $2.54 billion as a whole. The other is called The Thirty Meter Telescope (TMT). That one's location is a bit more controversial. It's planned to decorate a mountain in Hawaii called Mauna Kea, but locals have protested the decision because this stunning volcanic peak that boasts low humidity and gentle winds (perfect conditions for astronomy) is extremely meaningful in native Hawaiian culture. It's a fraught situation, as 13 other telescopes already live in the area and some local people say the facilities are impacting the natural environment. In terms of cost, however, the projected amount is just about symmetrical to the GMT's.

"They're expensive," Eric Isaacs, the president of the Carnegie Institution for Science, which has provided a sizable amount of private funding for the GMT, told Space.com "Not so much that the NSF couldn't do it — but they'd have to move things around and decide that's a priority."


An artist's illustration of the Thirty Meter Telescope atop the volcanic peak of Maunakea in Hawaii. (Image credit: Thirty Meter Telescope)

As of now, both telescope crews seem to remain hopeful while waiting for a decision.

"Our international consortium is fully committed to successfully completing the $2.54 billion Giant Magellan Telescope," the GMT team told Space.com.

"We read with great interest the NSB's recommendation to the NSF and are eager to work with the NSF to advance US leadership in astronomy for the next generation of astronomers," a spokesperson for the TMT told Space.com.

Isaacs acknowledges there's some natural competition due to the $1.6 billion announcement, but all in all, emphasizes that the teams have a united front. "We're sticking together," he said. "We were hoping NSF would come up with anything at this point, and they're really waking up to this."
Telescope friends

There's a key reason these telescopes are meant to be companions. Each can find the other's missing pieces; together, they can paint a picture of the universe in its grand totality.

The GMT is going to be on call for the Southern Hemisphere, while the TMT will have the Northern Hemisphere. Both also have complementary expertises. Some things the TMT can do, the GMT won't be as trained on. But the GMT can pick up where the TMT leaves off in other regards. Tag-team vibes. In this way, while holding hands and walking through the cosmos, the telescopes are supposed to be able to execute science our current robotic eyes on the sky simply can't compete with. How could a ground-based telescope view things the spaceborne JWST can't, you wonder? The quick answer is that a telescope on our planet can be bigger than one in space. For now, at least.
The overlapping observing coverage of the US-ELTP provides US astronomers with unfettered all-sky access from the Giant Magellan Telescope in the southern hemisphere and the Thirty Meter Telescope in the northern hemisphere. The timezone separation between the sites would increase the system’s capabilities for time-domain astrophysics. (Image credit: US-ELTP (TIO/NOIRLab/GMTO))

The TMT, which just finished polishing the 100th of its 492 total mirror segments, is planned to have a primary mirror that's (obviously) 30 meters, or 100 feet, in diameter. The GMT will have seven 27.6-foot-wide (8.4 m) mirror segments positioned in a pattern that resembles a six-petaled daisy to form a single 83.3-foot-wide (25.4 m) light-collecting surface. The bigger the mirror, the more light you can get. The more light you can get, the deeper you can see, and the dimmer objects you can pick up.

"TMT will deliver images that are more than 12 times sharper than the Hubble Space Telescope and more than four times sharper than those from JWST," the TMT team said in a release.

"These are the instruments for the next decades," Isaacs said.

Plus, both ground-based observatories can be adapted over time because they're physically on our planet. A bunch of astronauts can't exactly travel a million miles to reach Lagrange Point 2, where the JWST is situated, to tinker with the machine. The Hubble Space Telescope could be serviced back in the day because it sits in low Earth orbit — but even that was enough of a feat to warrant celebration decades later.
Why the U.S. government has a stake in the stars

It's fascinating how the science board's recommendation has sent ripples down into politics, managing to make headlines about the country's tricky status as a leader among the stars.

The worry comes from the fact that these telescopes are supposed to represent a significant leap forward for U.S. astronomy and U.S. astronomers.

Already, the European Southern Observatory's giant telescope project (unironically named the Extremely Large Telescope) is walking steadily to completion; China also has plans for its own enormous bridge to the stars.

"From our view, the most important thing is, let's at least build one," Isaacs said. "If we don't, we're out of the game, and China and the EU [European Union] are going to continue on. But we certainly want to advocate for two at this point, because we think it really keeps us in a leadership position."

In fact, soon after the board presented its $1.6 billion recommendation, Congress released its Fiscal Year 2024 funding bill. In this bill, Congress says it would like the nation to have a "two-observatory footprint" via the U.S. Extremely Large Telescope (USELT) program, though funding levels weren't specified. Interestingly, it does mention that the NSF, in total, will get $9.06 billion to work with. Still, the NSB's number remains the only one scientists have to contend with as of yet for the telescope program.

"I think that number, it sends a message," Isaacs said. "I mean, we have roughly a third of what we need, but we can't build it unless we get NSF involved because it's just going to be hard to raise that kind of money, even from wealthy, private people. It's the same thing with the TMT.

However, it's also worth considering, as Isaacs points out, that $1.6 billion isn't exactly an out-of-the-blue figure. "It wasn't a magic number," he said. "That was the number that was originally in the Astro 2020 report."

Which brings us to the next layer of complexity in the situation.

In short, Astro2020 refers to a super-detailed outline of what the nation's astronomy and astrophysics priorities should be during the 2020s. For this reason, it's also called the Decadal Survey. It's written by the National Academies of Science, Engineering and Medicine — but most importantly for this bit of astronomy drama, Astro2020 specifically advocated for at least one extremely large telescope, and "ideally" two: The GMT and the TMT.

"The Astro2020 report is not a mere suggestion," Isaacs said. "It's a very strong statement."

"The Decadal put forward a bold vision for what tools we need and the mandate that we build and use them responsibly," O'Meara said. "I think we can rise to that challenge and work with congress to fund USELT as a two-telescope project. Otherwise, U.S. leadership is at risk."

The slight contradiction, however, is that the report says the NSF should invest $1.8 billion in the project. This issue stems from the survey being a bit dated. It was released in 2021; since then, costs have risen.

"The next generation of telescope projects have gotten so huge and ambitious, and as a result they require an immense amount of coordination and planning," Dillon Brout, an assistant professor of astronomy and physics at Boston University, told Space.com. "While the announcement is indeed a tough pill to swallow, it's commendable that the NSF has made this decision sooner rather than later."

"It is an investment at a scale NSF is not used to for a facility, both in construction and in eventual operations," O'Meara said. "That said, the science demands these capabilities."

Taxpayer astronomy

There is one aspect of the situation that, when we really sit back and consider it, may feel either humbling or frustrating, depending on your perspective. The NSF's money is public money, aka taxpayer money, aka our money.

The topic has therefore spurred a lot of interesting conversations in this vein. What does this conundrum say about how we fund scientific advancement? What does it say about anyone having an interest in science?

"We must use opportunities when astronomy funding is in the public discourse to reiterate how essential it is to continue to financially support these efforts that will unlock never-before-seen depths of our universe," Brout said. "This is especially true if the United States wants to maintain its position as a world leader in the fields of astronomy, astrophysics and cosmology."

Sometimes, Isaacs says, he'll sit down at a restaurant and wonder how people in the room would react if it were announced that scientists had found an alien.

"I look at the person next to me and say, 'How would you like it if I could tell you there was life on another planet?'" he recalled. "And half of them say, 'Oh, that'd be so cool.' And half of them say 'Why? Why would we spend money on that? We've got to care about our problems on Earth.'"

It's a fair question, and one that's been raised many times in the past. We see a version of it raised when it comes to NASA's modern Artemis moon missions, for instance, and it was absolutely raised during NASA's older Apollo lunar program. And we'll surely see it brought up many more times in the years to come.

But maybe science is worth it. Not just medical science and climate science due to the direct, tangible repercussions they have, but also star science, black hole science and dark energy science. The James Webb Space Telescope has undoubtedly helped humans across the world feel like they're under the same blanket of awe despite tragedy and war, and the first direct image of a black hole, captured a few years ago by the Event Horizon Telescope, was on the front page of every major news outlet for a reason. Space discoveries may not impact our bodies, but they surely impact our perspectives. Beyond that even, a few billion dollars for science advancement is meager compared to the huge sums of public funding allocated for things like defense, which receives many hundreds of billions year after year.

And, though NASA is working on building some relevant instruments for the planned big observatories, private funding right now is leading the charge. For some context, NASA's funding allotment in the FY2024 bill was set at $24.875 billion to "explore the solar system, understand climate change, promote innovation and sustainability in aeronautics, and protect our planet."

"When the opportunity arises to answer the toughest questions the universe can throw at us, astronomy has worked with Congress to fund those tools," O'Meara said. As he underlines, the Rubin Observatory, set to achieve first light in 2025, the Nancy Grace Roman Space Telescope, slated to launch to space in 2027, as well as the Daniel K. Inouye Solar Telescope and the JWST of course, already churning out results, are all examples of "going big because the questions are big."

"We should be doing that with USELT as well," he said.

Private funding has worked for other telescopes, such as with the Keck Observatory, but those projects weren't as big as this one. Keck's cost ran into the millions, not the billions.

— This new authority will decide the fate of astronomy atop Hawaii's contested Maunakea volcano

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"Once NSF says they're in, you're going to get everybody interested. Right now, we have 14 members of the consortium, which is a lot, but we are still looking for a way to make ends meet," Isaacs said.

So, where do we go from here?

Well, it seems like we'll know more in May, when the NSF tells us what they've been discussing behind the scenes. "NSF has to come in, or else it's going to be very hard," Isaacs said. You know, of course, we'll do other things with a lot of other great ideas in astronomy — but this is the big idea."

"I'd say astronomy is in a golden age right now," he remarked. "And, to give up on ground-based astronomy at this point would be the wrong time."

Update 3/10: In Eric Isaacs' third-to-last comment, he was referring to the NSF, not NASA. This article has been updated to reflect that.


STARTS WITH A BANG 

The future of US astronomy just dimmed by half

Ground-based facilities enable the greatest scientific production in all of astronomy. The NSF needs to be ambitious, and it's now or never.


The 25-meter Giant Magellan Telescope is currently under construction, and will be the greatest new ground-based observatory on Earth. The spider arms, seen holding the secondary mirror in place, are specially designed so that their line-of-sight falls directly between the narrow gaps in the GMT mirrors, creating a view of the Universe without sharp corners to its mirrors or diffraction spikes around its stars. As one of the two US Extremely Large Telescopes proposed by astronomers and currently in development, it is an essential part of bringing about a new generation in cutting-edge ground-based astronomy facilities.
Credit: Giant Magellan Telescope/GMTO Corporation

KEY TAKEAWAYS

For decades, the plan for astronomy has included an array of space-based and ground-based facilities to complement one another, covering the full sky with a new generation of extremely large telescopes.

With three observatories planned: the European Extremely Large Telescope, the Giant Magellan Telescope, and the Thirty Meter Telescope, those science goals would be met, ensuring a bright future for astronomy.

In a shocking statement released in late February of 2024, however, the National Science Foundation recommended investing in only one new telescope: not two, as had always been planned. Here's why the investment is worth it.



Ethan Siegel
— MARCH 7, 2024

If you want to push the frontiers of science, you don’t just need brilliant minds with first-rate educations, you also need cutting-edge facilities to support them. 

When it comes to the science of astronomy and astrophysics, the next generation of necessary facilities — in the ground and in space, across all wavelengths of light, and even extending beyond light to particles and gravitational waves — were just recently agreed-upon by the National Academies of Sciences in a decadal report known as Astro2020. With a truly balanced portfolio between: ground-based and space-based endeavors,
small, medium, large, and flagship missions,
various fields of astronomy, from within our Solar System to exoplanets to stars and galaxies to cosmology,
and a series of new and upgraded facilities, including two extremely large telescopes, the next-generation Very Large Array, and upgrades to the IceCube facility for detecting neutrinos at the south pole,
as well as investments in the next generation of scientists,

These recommendations were adopted, across-the-board, by federal agencies such as NASA and the Department of Energy, and were expected to be (but have not been, to date) adopted by the National Science Foundation as well. However, with one penny-pinching and short-sighted resolution, the NSF has decided that instead of building two extremely large telescopes, the United States will only contribute towards one, and even that is only to the tune of a maximum of $1.6 billion, as recommended by the National Science Board. The truth is we need these facilities, as many have argued, and perhaps the best way to understand why is to debunk the most common myths associated with arguing why we don’t.


This artist’s rendering shows a night view of the Extremely Large Telescope in operation on Cerro Armazones in northern Chile. The telescope is shown using lasers to create artificial stars high in the atmosphere. The use of artificial guide stars, which reflect off of the atmosphere’s sodium layer 60 km up, are tremendously useful for the implementation of adaptive optics, and can allow ground-based telescopes to compete with or even outcompete smaller space-based telescopes that are above Earth’s atmosphere entirely across a variety of metrics.Credit: ESO/L. Calçada

1.) All the best astronomy is now done from space. It’s true that our space-based observatories, including Hubble and the JWST, have made and continue to make discoveries that no ground-based facility can match. However, around 90% of all scientific proposals to use those facilities are rejected for one very non-scientific reason: they’re oversubscribed. There are too many scientists with too many good ideas for doing science for most proposals to get accepted. In other words, there are too many things to learn, and too many good science cases, for the expensive space-based observatories to do it all.

Instead, space-based and ground-based facilities work best together: with space-based facilities usually ideal for discovery and ground-based facilities preferred for follow-up and further investigation. 

The five major arenas where ground-based facilities are superior to space-based facilities are:size, as building as large and as heavy as you like is no obstacle to ground-based construction,
reliability, as there are no launch costs or risk of launch failure,
versatility, as each individual ground-based facility provides a unique set of locations and opportunities for observing unique or one-time events,
maintenance, as there’s plenty of ground-based infrastructure (and no space-based infrastructure) for repairing, servicing, and replacing worn-out components on these observatories, and upgradeability, as old instruments are easily swapped out on the ground for newly-built ones, unlike in space, where it can only be done with great investments of money and labor.

The instruments aboard Hubble and JWST will be the same in 10 or 20 years as they are today, while ground-based telescopes only continue to improve with minimal further investment

.
This multi-paneled image shows the details returned by each of the JWST’s instruments in the same pointing/field-of-view during its commissioning in the first half of 2022. For the first time, in late April of 2022, all of the instruments across the full field-of-view were properly and fully calibrated, bringing JWST one step closer to being ready to begin science operations. Although JWST and its instruments give us a truly world-class space-based observatory, this technology is “frozen in,” and cannot have its instruments upgraded the way we can upgrade instruments easily and cheaply on ground-based telescopes.
Credit: NASA/STScI

2.) Philanthropic contributions should be enough to support astronomy. It’s true that both of the proposed US extremely large telescopes, the Giant Magellan Telescope (GMT) and the Thirty Meter Telescope (TMT), have assembled an impressive series of funding partners from across the world, from both private foundations and commitments from other governments and public institutes. GMT, for example, boasts funding from Taiwan, Australia, Brazil, Chile, Israel, South Korea, and the United States, and has already fabricated each and every one of its giant, 8.4-meter diameter primary mirror segments that will compose the eventual 25.4-meter diameter assembled mirror for observing the Universe.

TMT, meanwhile, is supported by India, Japan, and Canada, as well as AURA (the Association of Universities for Research in Astronomy) and the Moore foundation, and the TMT International Observatory has just produced the 100th polished mirror segment of an eventual 492, required to compose the 30-meter diameter primary mirror. This is an enormous amount of support, but public funding — especially for staffing and the maintenance of the observing facilities — is also required. Without the support of the National Science Foundation, ground-based astronomy as we know it, including last generation’s flagship ground-based observatories like:the Keck telescopes,
the Very Large Array, the IceCube Neutrino Observatory, and LIGO, all would have been impossible.


This aerial view shows the main science hub of the LIGO Livingston detector in Louisiana, with a view peering all the way down one of its 4 km long detector arms. Complemented by LIGO Hanford in eastern Washington, these two detectors not only brought us our first gravitational wave detection, but have netted more gravitational wave discoveries than all other efforts combined. Without investments in cutting edge facilities such as this, our ground-based astronomy efforts, from light to gravitational waves to particles like neutrinos, would still be in their infancy.
Credit: Caltech/MIT/LIGO Lab

3.) One US-based giant telescope can do all the science that two can do, it just takes more time. Whenever and wherever you are on Earth, every time you look up at the night sky, you’re only seeing half of what there is to observe. Even if each and every night were clear and cloud-free, and you observed the sky every night throughout the entire year as Earth revolves around the Sun, you wouldn’t manage to cover the whole sky. That’s because from our perspective on planet Earth, every location can only see:the entire half of the celestial hemisphere that corresponds to their latitude (north or south),
and the portion of the opposite celestial hemisphere that extends down to 90° minus their actual latitude.

Furthermore, the best observing always occurs close to overhead, rather than near the horizon, so if you have a telescope in the northern hemisphere, it’s impossible to look at objects with deep southern latitudes, and if you have one in the southern hemisphere, objects too far north will be unobservable. If you’re right at the equator, viewing near either pole will be a challenge as well. Also, for the purposes of “targets of opportunity,” which is what astronomers do when they observe transient objects, you need to be able to view the needed target at the critical moment, which is usually as quickly as possible. For flexibility, you want telescopes at various longitudes, so it’s always night when some powerful telescope can access the skies. Fewer telescopes means more missed opportunities and more missed objects.


This diagram shows the novel 5-mirror optical system of ESO’s Extremely Large Telescope (ELT). Before reaching the science instruments the light is first reflected from the telescope’s giant concave 39-meter segmented primary mirror (M1), it then bounces off two further 4-meter-class mirrors, one convex (M2) and one concave (M3). The final two mirrors (M4 and M5) form a built-in adaptive optics system to allow extremely sharp images to be formed at the final focal plane. The primary mirror consists of 798 segments to form the 39-meter mirror, but the light that matters isn’t the light that’s collected, but rather the light that reaches the instruments.
Credit: ESO

4.) The European Extremely Large Telescope, at 39 meters in diameter, is superior to the smaller US-based ones anyway. It’s difficult to emphasize just how wrongheaded this line of thought is. Here on Earth, there are around 15 optical telescopes of the current flagship class: with primary mirrors between 6.5 meters and 11 meters in diameter. All built during the decades of the 1990s and 2000s, the overwhelming majority of them are located in the three best physical locations on Earth for ground-based optical astronomy. In order, from best to third best, they are:the summit of Mauna Kea in Hawaii, the top of the Chilean Andes mountain range, and the summit of the island of La Palma, in the Canary Islands in Spain.

These are the locations that have the combination of the highest altitudes, stillest, lowest-humidity air, the least amount of turbulence, the lowest chances of cloud cover, and are closest to equatorial latitudes.

You might think that the largest telescopes in the best locations, like the Gran Telescopio Canarias and the Keck 1 and 2 telescopes, would be the most scientifically productive and prolific telescopes year after year, but that simply isn’t true. Every one of the telescopes that are 6.5 meters in diameter or larger at any of the above three mentioned locations are all comparably scientifically productive to one another, with similar numbers of scientific papers, similar scientific impacts, and similar numbers of major discoveries coming from each of them. Having more telescopes allows you to design more specialized instruments for them, enabling a broader array of science, from infrared observing to spectroscopy to coronagraphy to planet imaging and more. The jump from one size class to another is huge; the minor differences between the sizes of telescopes in the same class is far smaller than the differences in instrumentation.



The three largest telescopes in this image, located along the right, are the TMT, ELT, and GMT, and represent a new 30 meter class, from 25.4 to 39 meters in diameter. For comparison, today’s cutting-edge modern day telescopes range from 6.5 to 11.0 meters in diameter, and are represented by the majority of ground-based telescopes shown in the two middle columns. The leap from the current to the next generation will be transformative.
Credit: Cmglee/Wikimedia Commons

5.) Upgradeability is a major factor, as well as an underappreciated factor, in the sustained productivity of a telescope. How long does it take to build an instrument for a telescope, and how expensive does that instrument wind up being? If you look at the last 20 years of astronomy’s history, you’ll find that the biggest determining factor, on both accounts, is the size of the instrument. While the European Extremely Large Telescope (ELT) might have a 39 meter primary mirror and the Giant Magellan Telescope (GMT) may only have a 25 meter primary mirror, the size of the first-generation instruments aboard the ELT are planned to be a whopping thirty times the volume, each, of the first-generation instruments that have been planned and designed for GMT.

Costs scale with size, and although the ELT is promising a completion date of 2028, their instruments have not even reached final design, making that a dubious goal in the eyes of most astronomers who are instrument specialists. Additionally, the more reflections your optical system requires and the more upward-facing mirrors that system possesses, the more light you lose before it ever arrives in the instruments. The ELT has three up-facing mirrors and requires a total of four reflections before light reaches the instruments, whereas the GMT has only one up-facing mirror and requires only one reflection (for two instruments; two other instruments need a second reflection) before light reaches the instruments.

The ELT might be the “Cadillac” of 30-meter class telescopes, but for a wide variety of applications — including coronagraphy, planet imaging, and building the second generation of instruments down the road — the “Honda” that is the GMT or the “Subaru” that is the TMT will be the superior choice.


The Giant Magellan Telescope is already well under construction, and should reach completion by the decade’s end. At 25 meters in diameter, it will be either the largest or second-largest telescope in the world upon completion, depending only on whether the 39 meter diameter E-ELT is completed first.
Credit: Giant Magellan Telescope – GMTO Corporation

6.) The tensions between astronomers and native Hawaiians means that the Thirty Meter Telescope (TMT) can never happen anyway. This might have been a defensible position five years ago, but changes in TMT leadership, the government in Hawaii, and the stewardship plan and process for Mauna Kea have paved a path forward that is incredibly encouraging. The total number of telescopes on Mauna Kea is presently being reduced but not eliminated, and a scientifically productive future for astronomy is currently being planned and negotiated right now. While it is still being decided which telescopes will remain, which old ones will be decommissioned, and which new ones will be built, there is a future for TMT regardless of what decisions are made.


If there is a suitable site atop Mauna Kea where all parties agree the TMT should be built, then that will be the location of the northern hemisphere’s premiere and only 30 meter-class telescope. If not, La Palma in Spain has offered to provide the land and host the TMT as a backup location, which would then be where the northern hemisphere’s premiere and only 30 meter-class telescope would be located. There are options for where it can be built and — realistically — where it can serve the needs of the astronomical community for the next 30 to 50 years. There is a path forward for both astronomy and native Hawaiians to work fruitfully together on Mauna Kea, and for the TMT to exist as either part of that collaboration or as external to that endeavor.
This aerial view shows the summit of Mauna Kea with a series of astronomical observatories and roads connecting them to one another and to the Mauna Kea access road. These observatories, on one of the most sacred locations in Hawaiian society and culture, should not continue to exist as a legacy of an unethical past, but can only continue to exist with the consent of the native population.Credit: Richard Wainscoat/International Gemini Observatory/AURA/NSF

7.) Nothing would be lost by deciding not to build one of these telescopes at this point in time. Once you stop investing in something important to your nation, that field almost never recovers in that country. In the late 1980s and early 1990s, particle physicists around the world had set the highest priorities for their field as being a next-generation collider capable of reaching higher energies and greater numbers of collisions than ever before, and the United States was going to lead the way: by building the SSC: the Superconducting Super-Collider. It’s now around 30 years since that project was killed, and if you look at the priorities of the United States particle physics community today, you’ll see that the United States is playing only a complementary, supporting role when it comes to cutting-edge particle physics. There are no particle colliders or particle accelerators at the frontiers in this country any more.

If we abdicate leadership in astronomy and astrophysics today, and abandon the commitment to cutting-edge ground-based facilities that quite literally have brought us an understanding of the Universe, from the nature of galaxies to cosmic expansion to the Big Bang to the discoveries of dark matter and dark energy, we would be choosing to sunset our status as the scientific leader in the world of astronomy and astrophysics. Deciding to only build one extremely large telescope would signal to one of those two collaborations — either the GMT or the TMT — that all of the efforts, money, and time put into that project, including the millions of worker-hours and the commitments and investments of hundreds of millions of dollars, were wasted, because the United States itself, through the National Science Foundation, is unreliable as a funding partner.
The Thirty Meter Telescope is shown at a very low elevation angle in this digital rendering. The segmented primary mirror reflects the convex secondary mirror. The tertiary mirror in the center of the primary mirror is oriented to send light to the Wide Field Optical Spectrograph, the gray structure located on the right side of the image: one of the observatory’s main instruments. The left and right instrument platforms are seen and the dark blue adaptive optics enclosure is seen on the upper left on the instrument support structure.Credit: TMT International Observatory

8.) This decision will save money, in both the long and short runs, for the country. Financial austerity, when it comes to being truly fiscally responsible, should absolutely never be applied to basic research the way it is to other areas of government spending. The entirety of the National Science Foundation’s budget has never once totaled more than 0.05% of Gross Domestic Product or more than $10 billion in any fiscal year, and yet has spawned multiple companies whose net worth exceeds $100 billion. According to:the Center for American Progress,
the National Institute of Standards and Technology,
and even the National Science Foundation itself,

every dollar invested in science through the NSF, NASA, and DARPA, generates more than 100% of that investment in American economic activity: a positive return-on-investment. That means that not investing those dollars in basic research hurts the American economy by a greater amount than the cost of making the investment. As the former direction of the NSF, France Córdova, wrote in 2018:

“Scientific breakthroughs start with a question, a big idea, about the nature of things that often leads to a fundamental shift in thinking. The ability to pursue and investigate that question, and to innovate along the way, is what enables the discoveries that ultimately transform the world.”

If we don’t invest in asking and answering those questions, that’s the same as choosing to remain exactly where we are instead of furthering our path down the roads of progress
.
The various plans and initiatives from the Astro2020 decadal survey touch on a wide variety of initiatives and pathways, ensuring a successful long-term and short-term future for astronomy and astrophysics if we choose to follow this roadmap. If we choose instead to abandon it, that progress will not occur in the United States.
Credit: National Academies/Astro2020 decadal survey

The reality is that, when political whims supersede the actual facts about investing our dollars into something worthwhile — even if making that investment would be a victory for our nation all-around — it’s a signpost of an empire not only in decline, but in the process of crumbling. There are many among us, maybe even the majority of us, who are simply not ready to accept that fate for our nation and for the fate of science within our nation, and the act of looking to the Universe itself for answers about the biggest questions of all is perhaps the most ambitious act of fundamental research we can engage in.

Questions such as:are we alone in the Universe, if there are inhabited worlds out there, what are they like, where did our solar system and planet come from, how did life arise on Earth, where did the Milky Way and the entire Universe come from, and what is the cosmic story that allowed us to come into existence, are not just questions for a privileged set of a few thousand researchers to investigate, but questions fundamental to all of humanity whose answers lie within our reach, if only we dare to look beyond the few fractions-of-a-percent of the cost of investing in finding out those answers. The scientists laid out the case for the path forward for the fields of astronomy and astrophysics in 2021 for the next decade, and all the major federal agencies except for the National Science Foundation have adopted what they recommended. If we want a future where the United States of America remains on the cutting edge of science, we’ll change course and make the investment we need to bring about a better tomorrow. And if not, we’ll meet with the same fate as every country that’s chosen cowardice when it comes to making those critical investments: stagnation and decline.

The secret history of water on Mars: What ancient climate change tells us about the future on Earth

Mars’ atmosphere was once thick and wet, with raindrops that were so tiny they couldn’t even penetrate the soil


By RAE HODGE
Staff Reporter
SALON
PUBLISHED MARCH 6, 2024 

Mars Dust Storm
 (Getty Images/MARK GARLICK/SCIENCE PHOTO LIBRARY)

If you suddenly found yourself standing on the surface of Mars, it would feel like you’d been transported into a dusty space western. The arid soil lays a rocky palette of red powder across the horizon, where you’d see sprawling canyons and old volcanoes with edges whipped sharp by unforgiving wind storms. But, 4.5 billion years ago, this barren wasteland was home to a rich system of groundwater, vast oceans and galloping rivers. And in the the past month, a growing tide of scientific research has begun uncovering a hidden history of Mars’ once-rushing waters.

Evidence of an ancient planet-wide groundwater system, previously only theorized, was discovered in 2019. But only recently, in early February, a NASA spacecraft brought back exciting images of Mars’ surface which contained evidence the planet teemed with flowing water across an ancient spread of now-dry lake beds, channels, valleys and gullies. The same week, the European Space Agency’s Mars Express discovered ice buried under the equator, hinting at massive groundwater aquifers.

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Unlocking the secret of how those aquifers recharge (or refill) is the next step in exploring a possible human future on Mars. Last November, a team of Chinese scientists found a way to create oxygen out of the water found on Mars. Now, researchers at the University of Texas at Austin have combined a number of methods — from new computer models to simple back-of-the-envelope calculations — to uncover something curious about how that ice came to be in the first place. Despite a climate full of surging rainstorms, the scientists said, early Martian soil simply didn’t absorb much of it. The groundwater systems refilled themselves, but we have no idea how.

“Understanding groundwater flow can help inform where to find water today,” said lead study author Eric Hiatt, in a university release. “Whether you’re looking for signs of ancient life, trying to sustain human explorers, or making rocket fuel to get back home to Earth, it’s essential to know where the water would most likely be.”

"Understanding groundwater flow can help inform where to find water today."

The new findings, published in the journal Icarus, raise even more questions about how water systems work on Mars compared to those which exist on Earth today. And, because these groundwater systems likely fed Mars’ ancient network of lakes, finding out how long it took those lakes to fill up and overflow onto the surface could help us figure out whether, and where, life on Mars may have existed in the past.

“The fact that the groundwater isn’t as big of a process could mean that other things are,” Hiatt said. “It might magnify the importance of runoff, or it could mean that it just didn’t rain as much on Mars. But it’s just fundamentally different from how we think about [water] on Earth.”

Much of the groundwater mystery centers on one of Mars’ most notable features, called “the great dichotomy.” The term describes the stark difference in land height between two of the planet’s regions — the northern lowlands and the southern highlands. This contrast in elevation is where we can see how groundwater aquifers surged up to the surface, creating markers and leaving a trail of evidence for scientists to follow today.

Researchers said most of the liquid water that existed on Mars billions of years ago resided in a vast ocean in the northern lowlands. But when Hiatt’s team used their new combination of computer modeling techniques to analyze the great dichotomy, they were able to estimate how much groundwater recharge occurred in the Martian southern highlands.

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The mystery deepened when researchers found the groundwater aquifers in the southern highlands on Mars only recharged about 0.03 millimeters (0.001 inches) per year. The Trinity and Edwards-Trinity Plateau aquifers — which provide water for the city of San Antonio — range between 2.5 to 50 millimeters (0.1 inches to 2 inches) per year. That’s 80 to 1600 times more annual recharge than Martian groundwater.

“While other studies have simulated groundwater flow on Mars using similar techniques, this research by [Hiatt] published in [Icarus] is the first to incorporate the influence of the oceans that existed on Mars more than three billion years ago,” in the Hellas, Argyre, and Borealis basins, the university said in a tweet.

Even as the sharp differences between Mars and Earth’s water systems emerge in the team’s latest findings, research like this could also help us understand how to survive water and climate changes on our own planet. The technology we’re using to find water on Mars now, for instance, can also double in value for our own planet’s inhabitants. Using it to find leaks in public water systems has already proven to be a more effective and inexpensive than traditional methods.

"When we think about what Mars looked like 3.5 billion years ago, we probably should be thinking about an environment that in some ways looks a lot like Earth," said University of Texas Associate Professor Tim Goudge in a 2021 interview.

Mars’ atmosphere was thick and wet, with four times more pressure than Earth’s today and resulting raindrops that were so tiny they looked more like a dense fog and couldn’t even penetrate the soil. As that pressure waned, though, rainfall came down hard on the Red Planet’s surface, carving grooves and valleys. Just as floods on Earth carved out the Grand Canyon, catastrophic floods accounted for a quarter of Mars’ surface erosion, according to UTA researchers.

Then things changed. Mars lost its magnetic field, and with it the vast oceans which contained more water than contained in the Earth’s Artic Ocean today. A new theory from the University of Chicago emerged on Feb. 14 after a duo of scientists examined sediment and erosion evidence on Mars and noticed a pattern in the planet’s history.

“Like Earth, which has over the past billion years experienced periods of global glaciations and hyperthermals, the climate history of early Mars may have been intermittent,” the study authors write in Nature Geosciences.

“We suggest that Mars did not undergo a single wet-to-dry transition, but rather experienced seven major climate transitions, with the planet intermittently under climates warm enough to support surface liquid water even after 3.0 billion years ago (Ga). However, there is evidence for long dry spells, with some locations fully dry after 3.6 Ga.”

The study also looks into the reasons driving these climate shifts — testing hypotheses about volcanic eruptions and changes in the planet’s axial tilt. This new wave of Martian water research is quickly expanding our base of knowledge about alien climates, and understanding how a procession of climate changes could dramatically shape Mars could give us key insight into the challenges Earth may face as it encounters its own climate upheaval.

Critically, though, the more we can figure out about the mystery of Martian water, the sooner we can figure out how human life on a new planet could work — and how, if ever, it worked in the past.


Read more

about water and life on Mars

A simple algorithm could reveal the ghosts of alien life in Mars dirt, study finds


By RAE HODGE
is a science reporter for Salon. Her data-driven, investigative coverage spans more than a decade, including prior roles with CNET, the AP, NPR, the BBC and others. She can be found on Mastodon at @raehodge@newsie.social.


Space photo of the week: Can you spot the hidden robot on the slopes of Mars?


By Jamie Carter published about 21 hours ago

NASA's Mars Curiosity rover hides in plain sight in this aerial photo of the treacherous Martian landscape.

NASA's Curiosity Mars rover appears as a dark speck in this image captured from directly overhead by the agency's Mars Reconnaissance Orbiter, or MRO. 
(Image credit: NASA/JPL-Caltech/University of Arizona)

What it is: NASA's Curiosity Mars rover

When it was published: Feb. 29, 2024

Why it's so special: Can you spot the hidden robot on Mars?

In this photo, NASA's Curiosity rover, which has been exploring the surface of Mars since 2012, appears as a tiny, dark speck. The rover is seen on the steep slopes of Upper Gediz Vallis in a vast landscape scarred by dark and light bands.

Curiosity's current location is a massive achievement for the engineers at NASA's Jet Propulsion Laboratory, who built and now remotely operate the rover from 203 million miles (326 million kilometers) away. Curiosity spent three years gradually climbing Gediz Vallis Ridge; after three failed attempts, it finally succeeded in August 2023, according to NASA.

The space agency thinks water flowed in this region 3 billion years ago, and carried mud and boulders with it to create the ridge. Early last year, Curiosity found evidence of water and waves on Mars.

This image was taken on Dec. 29, the 4,051st Martian day, or sol, of the rover's mission, and NASA published the photo Feb. 29. The view from space was captured directly overhead by the High-Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter, which has been orbiting the Red Planet since March 2006. According to NASA, the camera is capable of viewing objects as small as a dinner table on Mars' surface.

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In addition to the Curiosity rover, NASA has its Perseverance rover on the surface of Mars. Also in orbit, alongside the Mars Reconnaissance Orbiter, are NASA's Odyssey and MAVEN (Mars Atmosphere and Volatile Evolution) spacecraft. A tiny remote-controlled helicopter named Ingenuity, which accompanied the Perseverance rover on its Martian journey for the last three years, recently sustained irreparable damage on its final, 72nd flight.

 

Scientists Uncover Secret Driver of Climate Change

Global Warming Climate Change Model

Scientists have discovered that viruses infecting microbes significantly impact climate change by affecting methane cycling. This study, analyzing DNA from various environments, shows that the environmental impact of viruses varies by habitat. The research underscores the complex relationship between viruses, microbes, and methane emissions, suggesting the need for further exploration into viral roles in climate dynamics.

Study reveals microorganisms, once infected, harbor novel genes for methane generation.

A recent study reveals that viruses that infect microbes contribute to climate change by playing a key role in cycling methane, a potent greenhouse gas, through the environment.

By analyzing nearly 1,000 sets of metagenomic DNA data from 15 different habitats, ranging from various lakes to the inside of a cow’s stomach, researchers found that microbial viruses carry special genetic elements for controlling methane processes, called auxiliary metabolic genes (AMGs). Depending on where the organisms dwell, the number of these genes can vary, suggesting that viruses’ potential impact on the environment also varies based on their habitat.

This discovery adds a vital piece to better understanding how methane interacts and moves within different ecosystems, said ZhiPing Zhong, lead author of the study and a research associate at the Byrd Polar and Climate Research Center at The Ohio State University.

“It’s important to understand how microorganisms drive methane processes,” said Zhong, also a microbiologist whose research examines how microbes evolve in diverse environments. “Microbial contributions to methane metabolic processes have been studied for decades, but research into the viral field is still largely under-investigated and we want to learn more.”

The study was published in the journal Nature Communications.

The Role of Viruses in Greenhouse Gas Emissions

Viruses have helped foster all of Earth’s ecological, biogeochemical, and evolutionary processes, but it’s only relatively recently that scientists have begun exploring their ties to climate change. For example, methane is the second-biggest driver of greenhouse gas emissions after carbon dioxide, but is largely produced by unicellular organisms called archaea.

“Viruses are the most abundant biological entity on earth,” said Matthew Sullivan, co-author of the study and a professor of microbiology at the Center of Microbiome Science at Ohio State. “Here, we expanded what we know about their impacts by adding methane cycling genes to the long list of virus-encoded metabolic genes. Our team sought to answer how much of the ‘microbial metabolism’ viruses are actually manipulating during infection.”

Though the vital role microbes play in accelerating atmospheric warming is now well-recognized, little is known about how methane metabolism-related genes encoded by the viruses that infect these microbes influence their methane production, said Zhong. Solving this mystery is what led Zhong and his colleagues to spend nearly a decade collecting and analyzing microbial and viral DNA samples from unique microbial reservoirs.

One of the most important places the team chose to study is Vrana Lake, part of a protected nature reserve in Croatia. Inside the methane-rich lake sediment, researchers found an abundance of microbial genes that affect methane production and oxidation. Additionally, they discovered diverse viral communities and uncovered 13 types of AMGs that help regulate the metabolisms of their host. Despite this, there isn’t any evidence that these viruses directly encode methane metabolism genes themselves, suggesting that viruses’ potential impact on the methane cycling varies by their habitat, said Zhong.

Livestock and Environmental Impacts

Overall, the study revealed that a higher number of methane metabolism AMGs are more likely to be found inside host-associated environments like the inside of a cow’s stomach, whereas fewer of these genes were found in environmental habitats, such as in lake sediment. Since cows and other livestock are also responsible for generating about 40% of global methane emissions, their work suggests the complex relationship between viruses, living beings, and the environment as a whole may be more intricately tied together than scientists once thought.

“These findings suggest that global impacts from viruses are underestimated, and deserve more attention,” said Zhong.

Though it’s unclear whether human activities might have affected the evolution of these viruses, the team expects new insights gleaned from this work will raise awareness about the power of infectious agents to inhabit all life on Earth. Still, to keep learning more about these viruses’ inner mechanisms, further experiments will be needed to understand more about their contributions to Earth’s methane cycle, said Zhong, especially as scientists work toward ways to mitigate microbially driven methane emission.

“This work is a beginning step for grasping the viral impacts of climate change,” he said. ‘We still have lots more to learn.”

Reference: “Viral potential to modulate microbial methane metabolism varies by habitat” by Zhi-Ping Zhong, Jingjie Du, Stephan Köstlbacher, Petra Pjevac, Sandi Orlić and Matthew B. Sullivan, 29 February 2024, Nature Communications.
DOI: 10.1038/s41467-024-46109-x

This work was supported by the National Science Foundation, the Croatian Science Foundation, the Gordon and Betty Moore Foundation, the Heising-Simons Foundation, the European Union, and the U.S. Department of Energy. Co-authors include Jingjie Du of Ohio State, as well as Stephan Kostlbacher and Petra Pjevac from the University of Vienna, and Sandi Orlić from the Ruđer Bošković Institute.

Can Volcanic Super Eruptions Lead to Major Cooling? Study Suggests No

NASA
Goddard Digital Team
MAR 01, 2024

New research suggests that sunlight-blocking particles from an extreme eruption would not cool surface temperatures on Earth as severely as previously estimated.

Some 74,000 years ago, the Toba volcano in Indonesia exploded with a force 1,000 times more powerful than the 1980 eruption of Mount St. Helens. The mystery is what happened after that – namely, to what degree that extreme explosion might have cooled global temperatures.

Crew aboard the International Space Station photographed the eruption of Mount Etna in Sicily in October 2002. Ashfall was reported more than 350 miles away. When it comes to explosive power, however, no eruption in modern times can compare with a super eruption – which hasn’t occurred for tens of thousands of years.

When it comes to the most powerful volcanoes, researchers have long speculated how post-eruption global cooling – sometimes called volcanic winter – could potentially pose a threat to humanity. Previous studies agreed that some planet-wide cooling would occur but diverged on how much. Estimates have ranged from 3.6 to 14 degrees Fahrenheit (2 to 8 degrees Celsius).

In a new study in the Journal of Climate, a team from NASA’s Goddard Institute for Space Studies (GISS) and Columbia University in New York used advanced computer modeling to simulate super-eruptions like the Toba event. They found that post-eruption cooling would probably not exceed 2.7 degrees Fahrenheit (1.5 degrees Celsius) for even the most powerful blasts.

“The relatively modest temperature changes we found most compatible with the evidence could explain why no single super-eruption has produced firm evidence of global-scale catastrophe for humans or ecosystems,” said lead author Zachary McGraw, a researcher at NASA GISS and Columbia University.

To qualify as a super eruption, a volcano must release more than 240 cubic miles (1,000 cubic kilometers) of magma. These eruptions are extremely powerful – and rare. The most recent super-eruption occurred more than 22,000 years ago in New Zealand. The best-known example may be the eruption that blasted Yellowstone Crater in Wyoming about 2 million years ago.

Small Particles, Big Questions

McGraw and colleagues set out to understand what was driving the divergence in model temperature estimates because “models are the main tool for understanding climate shifts that happened too long ago to leave clear records of their severity.” They settled on a variable that can be difficult to pin down: the size of microscopic sulfur particles injected miles high into the atmosphere.

In the stratosphere (about 6 to 30 miles in altitude), sulfur dioxide gas from volcanoes undergoes chemical reactions to condense into liquid sulfate particles. These particles can influence surface temperature on Earth in two counteracting ways: by reflecting incoming sunlight (causing cooling) or by trapping outgoing heat energy (a kind of greenhouse warming effect).

Over the years, this cooling phenomenon has also spurred questions about how humans might turn back global warming – a concept called geoengineering – by intentionally injecting aerosol particles into the stratosphere to promote a cooling effect.

The researchers showed to what extent the diameter of the volcanic aerosol particles influenced post-eruption temperatures. The smaller and denser the particles, the greater their ability to block sunlight. But estimating the size of particles is challenging because previous super eruptions have not left reliable physical evidence. In the atmosphere, the size of the particles changes as they coagulate and condense. Even when particles fall back to Earth and are preserved in ice cores, they don’t leave a clear-cut physical record because of mixing and compaction.

By simulating super-eruptions over a range of particle sizes, the researchers found that super-eruptions may be incapable of altering global temperatures dramatically more than the largest eruptions of modern times. For instance, the 1991 eruption of Mount Pinatubo in the Philippines caused about a half-degree drop in global temperatures for two years.

Luis Millán, an atmospheric scientist at NASA’s Jet Propulsion Laboratory in Southern California who was not involved in the study, said that the mysteries of super-eruption cooling invite more research. He said the way forward is to conduct a comprehensive comparison of models, as well as more laboratory and model studies on the factors determining volcanic aerosol particle sizes.

Given the ongoing uncertainties, Millán added, “To me, this is another example of why geoengineering via stratospheric aerosol injection is a long, long way from being a viable option.”

The study, titled “Severe Global Cooling After Volcanic Super-Eruptions? The Answer Hinges on Unknown Aerosol Size,” was published in the Journal of Climate.

By Sally Younger
Earth Science News Team
NASA’s Jet Propulsion Laboratory, Pasadena, Calif.
sally.m.younger@jpl.nasa.gov