UN Climate Chief: โ€œthe climate crisis is now a continent-wide economic security emergencyโ€

He forgot to add words like โ€œsuperโ€ and โ€œapocalypticโ€.

And it shows both that the climate crisis is now a continent-wide economic security emergency. And that doubling down on Europeโ€™s longstanding climate leadership is entirely in the continentโ€™s best interest.

Globally, over 2 trillion dollars was invested in clean energy last year โ€“ double fossil fuel investment.

A cartoon depicting a continent-wide economic security emergency due to the climate crisis, featuring a United Nations official, rising energy prices, and distressed citizens discussing their high bills.

From Watts Up With That?

By Eric Worrall

He forgot to add words like โ€œsuperโ€ and โ€œapocalypticโ€.

UN Climate Chief: โ€œthe climate crisis is now a continent-wide economic security emergencyโ€

10 September 2026

The following is a transcript of a speech delivered by UN Climate Change Executive Secretary Simon Stiell at the European Parliament Committee on the Environment, Climate and Food Safety in Brussels, Belgium, on Thursday 10 September 2026.

Thank you for this opportunity.

Climate is sometimes seen as a partisan issue: as territory in culture wars. That is palpably false. And weโ€™ve just seen why: Europeโ€™s summer has been hot as hell. This is the price of global fossil fuel addiction hitting home.

And it shows both that the climate crisis is now a continent-wide economic security emergency. And that doubling-down on Europeโ€™s longstanding climate leadership is entirely in the continentโ€™s best interest.

This summerโ€™s climate-driven extreme heat has killed tens of thousands of people, and hammered Europeโ€™s infrastructure, businesses, and economies.

Weโ€™ve seen mass evacuations. Power stations closed. And trade routes choked. Crops lost. Yields down. And food prices up โ€“ and set to rise further.

Elsewhere, horrifying floods have ripped through the Himalayas. In North Africa, devastating heat has meant lost lives, power outages, water shortages, and economies slowed.

In many places, climate impacts are fueling forced migration โ€“ internally and across national borders โ€“ taking a dire human toll.

And the costs of the climate crisis are spiraling. Disasters are pushing up insurance premiums. Leaving some entirely uninsurable.

One study calculates this summerโ€™s extremes will cost Europe 180 billion euros โ€“ in lost labour productivity, and disruption to food, energy and transport. Thatโ€™s equivalent to carving a full percentage point from European GDP โ€“ the same amount the EU economy is forecast to grow.

No wonder some EU member states are calling for a dedicated climate adaptation fund.

The EUโ€™s summer of hellish heat comes on top of the ongoing fossil fuel cost crisis โ€“ and both are driving up prices for households, businesses and governments, in a deathly double-blow. Dependence on volatile fossil fuel imports has long been an economic Achillesโ€™ heel for Europe.

This year โ€“ again โ€“ households and businesses have been hit with higher bills. Now, another European winter fuel crisis is looming, due to fossil fuel dependency.

Increasingly, to be soft on climate action is to be soft on inflation and the cost of living, soft on sovereignty and security, and soft on economic growth and jobs.

The fossil fuel cost crisis is also pushing up the costs of government borrowing, meaning less fiscal space to deliver vital services that populations need and expect.

Understandably, Europe wants to insulate itself from volatile fossil fuel costs you cannot control.  Understandably, Europe wants affordability, economic stability, energy security, and policy-making autonomy. Clean energy is the surest path to deliver, cheaply and safely.

Thanks to growing investment, renewables now provide around half of Europeโ€™s power. In the first six months of this Middle East conflict, solar alone saved Europe more than 30 billion euros in avoided gas imports.

And you have so much more to gain from accelerating the shift to clean energy โ€“ across this continent and the world.

The clean tech boom is already driving European growth, jobs and living standards: Your companies are at the forefront of some key clean industries. The opportunities will only grow.

And some countries developing national transition plans will reap particularly strong benefits.

Globally, over 2 trillion dollars was invested in clean energy last year โ€“ double fossil fuel investment.

As all countries at COP30 said: the move to clean energy is now irreversible. That means a goldmine of jobs and commercial opportunities.

By standing firm behind your climate policies, going further, and backing clean, resilient growth. You can better position Europe to thrive. Locking-in higher living standards โ€“ now and in the long-term.

Colleagues,

Itโ€™s clear: Climate cuts across the core concerns of voters, whatever their politics: Family health, community safety and economic stability. Affordable food and available water. Jobs, business costs, and household bills.

Itโ€™s entirely in Europeโ€™s interests to stand firm behind climate action โ€“ and to boost it: To build resilience to climate impacts โ€“ protecting global supply chains, on which all economies depend. And to slash global emissions.

If humanity doesnโ€™t cut the fossil fuel pollution baking our planet, this summerโ€™s brutal heat, fires and droughts will seem mild compared to the permanent climate nightmare that will follow.

We have made progress but still not enough.

Without UN-convened climate cooperation, humanity would be heading for unsurvivable global heating well over 4 degrees Celsius. With it, current policies are taking us to a 2.6 degree temperature rise.

Thatโ€™s a long way from the 1.5 degree limit demanded by science to avert the worst climate impacts, and agreed among nations, time and time again.

A recent report from the UN Environment Programme reaffirms that this limit will now be breached. But the report is equally clear: that this can and must be temporary.

Concerted global action can bring the temperature rise back down to 1.5 degrees.

For years, Europe has been a climate leader. And a champion of multilateralism.

You were instrumental in building the international climate system, and the Paris Agreement โ€“ at the 21st UN Climate Conference.

Europeโ€™s continued leadership is essential โ€“ including in supporting vulnerable nations. And itโ€™s entirely in the interests of Europeโ€™s people and economies.

All nations win by avoiding a two-speed global transition.

We need you working in partnership. Forging international alliances that secure supply chains for clean energy and new industries. And continuing to deliver on your current climate finance pledges โ€“ boosting quality and access, building on existing work โ€“ which strengthens trust.

No single COP can solve the climate crisis overnight, but each moves global efforts forward โ€“ building on the last, and looking to the next: From a global agreement in Dubai to transition away from all fossil fuels. To a new climate finance goal in Baku. And steps forward on a just transition in Belem, which ushered in the era of implementation.

I ask the EU to throw itself behind helping COP31 in Tรผrkiye to deliver further progress.

The need now is not to re-open decisions already taken.

Itโ€™s delivering whatโ€™s already been agreed: Countries implementing their plans and targets, and striving to do better, where domestic conditions allow.

By the second global stocktake of climate action in 2028, we must be much closer to meeting the global commitments made at the first. Laying the ground for greater ambition.

This yearโ€™s negotiations can help support implementation: across mitigation, adaptation and finance โ€“ including quality and access to finance.

For example, through developing the just transition mechanism โ€“ to support countries deliver fair transitions that create opportunities for all.

I ask the EU to come to Tรผrkiye prepared to find solutions.

That means spending time considering what you would like the outcomes to include. And what others need from COP31.

It means forging compromises. And developing a clear plan on how to use the spaces weโ€™ve created together.

That includes the Global Climate Action Agenda. Which is key to turning targets into results. Accelerating real economy action. And supporting countries to implement their national adaptation plans and NDCs.

The Turkish COP31 Presidency, working closely with Australia, has set key Action Agenda targets, including 35% of final global energy demand met by electricity by 2035.

The EU is already making gains here. And you have ambitious electrification targets. Around one in four new cars sold in Europe is now electric. And battery deployment is now accelerating.

Itโ€™s in your interests to push forward. And to drive progress in other areas where the impact and urgency are greatest: Methane โ€“ a super pollutant crucial to reducing near-term heating and cutting costs. Food waste and security, as climate-driven droughts hit crops and food prices. And building the resilience of cities to climate extremes.

These topics strike at the heart of everyday concerns of people across the continent.

Colleagues,

We live in a polarized age: But inflation is a common enemy, security is a common cause. Health, jobs, community and prosperity matter to us all. And every one of them demands action on climate.

I thank you.

Source: https://unfccc.int/news/un-climate-chief-the-climate-crisis-is-now-a-continent-wide-economic-security-emergency

In my opinion the claim the climate movement is not a partisan issue is absurd, because the climate movement is rebadged communism. When the Soviet Union fell, the last dictator of the Soviet Union Mikhail Gorbachev rallied and restored hope to his bereft Western Soviet communism groupies by launching โ€œGreen Cross Internationalโ€ at the 1992 Rio Earth Summit. For a while the green camouflage might have fooled a few conservatives, but Climategate ripped away the disguise, by revealing the intense politicisation of the scientists pushing the crisis narrative, and the dirty tricks employed to try to silence critics and competing narratives.

Simon Stiell mentioned power plant closures. As we recently discussed on WUWT, the power plant closures in most cases were not because of the heat, they were because Europe ran short of water. And the cause of that water shortage disaster was long term chronic underinvestment in water infrastructure, which even the EU admits is a problem. Yes the drought put pressure on the system โ€“ but I would argue failure to invest in resilience was the real problem.

Claiming climate changed caused the Nepal disaster is way premature, and likely untrue. Nepal is well known for unstable geology and mountain collapses. Such events have been happening regularly for millions of years, even before humans raised CO2 levels with industrial output.

Stiell notes Europe is facing a winter gas shortage โ€“ but how much of that is due to climate policy? Europe has trillions of cubic meters of recoverable shale gas, but refused to frack that gas due to climate regulations. People are going to freeze to death because Europeโ€™s leaders have shut down the industry which could have provided resilience against Middle Eastern and Russian supply shocks, in the name of combating climate change.

I note that Europe hasnโ€™t managed to ween itself off fossil fuel despite trillions of dollars of investment. Who can ignore the absurdity of Germany purchasing 4-5% of the worldโ€™s solar panel output, despite Germany being between 47ยบ and 55ยบ North? Even sunny Australia canโ€™t eliminate fossil fuel, weather is simply too unreliable to be the basis of a secure energy supply โ€“ especially for nations as far north as Germany.

Stiell makes the obligatory UN prediction of fiery doomsday if we donโ€™t listen to him โ€“ this summerโ€™s brutal heat, fires and droughts will seem mild compared to the permanent climate nightmare that will follow. But the UN has been issuing doomsday warnings since the late 1980s, and none of them have come true.

Stiell claims Europe has to help vulnerable nations โ€“ but why? Given Europeans are suffering, shouldnโ€™t Europe help its own people first?

To top off the absurdity, Stiell claims Europe needs to double down on climate action to reduce inflation and avoid fiery doomsday, which is obviously wrong. If high fossil fuel prices are causing inflation, the first priority is surely to bring down the price of fossil fuel, either by helping the USA fix the Persian Gulf crisis, or permitting frackers to secure domestic European fuel supplies. To take care of immediate needs, discretionary expenditure like foreign aid could be suspended to buy more gas from whomever can sell it.

Why is something so obvious so difficult for UN officials like Stiell to grasp? Why do people like Stiell appear to find it so difficult to separate fixing todayโ€™s problem โ€“ fuel price inflation โ€“ from fixing tomorrowโ€™s energy problems, with whatever form tomorrowโ€™s energy solutions will take?

I used to wonder how great powers from history like the Roman Empire could fail so completely in such a short time. But weโ€™re seeing the answer to this mystery play out live, right now, in Europe.

Great powers fail because of gross leadership incompetence. Leaders of failing powers ignore genuine crisis, and fritter away precious resources on unimportant trivialities or plans for a future which never happens. They lose focus on what matters.

Europeโ€™s problems could be solved at the stroke of a pen. But Europeโ€™s leaders are so disconnected from reality, so distracted and obsessed with fantasy future issues like the fake climate crisis, they cannot bring themselves to take simple, obvious steps which would alleviate the problems their people are facing right now.

Earthโ€™s Crust Is Unzipping Beneath Italy

Scientists say Earthโ€™s crust is โ€œunzippingโ€ (delaminating) under Italyโ€™s Apennine Mountains, explaining their paradoxical geology of simultaneous extension and compression.

Integrating geodetic, seismic, and geological data, the authors show that lower- crustal delamination is currently the primary geodynamic driver of Apennine tectonics and seismicity.

Illustration explaining the geological process of lower crust delamination and mantle sinking in the Apennines region, showing the unzipping front migrating west to east and depicting crustal changes.
AI generated by Grok

Scientists say Earthโ€™s crust is โ€œunzippingโ€ (delaminating) under Italyโ€™s Apennine Mountains, explaining their paradoxical geology of simultaneous extension and compression.

A study led by Stefano Tavani of the University of Florence, published in Communications Earth & Environment (2026), proposes that dense lower crust and attached lithosphere are peeling away from the upper crust and sinking into the mantle. This is not happening all at once; instead, it advances along a migrating โ€œhingeโ€ or front (like a zipper or peeling tape) that is slowly moving under Italy toward the Adriatic foreland.

The Apennines stretch ~1,200 km along the Italian peninsula. They formed through plate convergence that crumpled and thickened the crust. Later, slab rollback stretched the crust behind the range, helping open the Tyrrhenian Sea. This produced simultaneous contraction at the outer (eastern) edge and extension farther west, an apparent paradox that has puzzled researchers for years.

Earlier explanations centered on slab rollback. After ~2 million years ago, major Tyrrhenian extension largely ended and frontal shortening slowed, yet the contradictory deformation continued, pointing to another driver.

Researchers combined decades of earthquake data, GPS measurements, satellite radar observations, and maps of the Moho (the crust- mantle boundary). Key findings include:

A zone spanning more than 500 km where the Tyrrhenian- side Moho overlaps the Adriatic- side Moho, interpreted as the peeling front (doubled crust where lower layers detach).

Earthquakes cluster around this hinge: mechanisms indicate extension behind/above it and compression ahead of it.

GPS data show ~4 mm/year of extension across the mountain belt, partially offset by ~2 mm/year of contraction toward the outer edge, an โ€œaccordion- likeโ€ pattern.

Ahead of the hinge, the lower crust and lithospheric mantle stay attached to the sinking slab, pulling the crust downward (causing compression and subsidence). Once the hinge passes and denser material peels away, the remaining buoyant crust can rebound and extend.

The team argues this ongoing lower- crust delamination is now the main geodynamic driver of tectonics and seismicity in the Apennines, providing real- time evidence of a laterally migrating delamination hinge. The model is simplified, and fuller understanding of the underlying slab will need more detailed work.

This process helps account for why parts of the range rise while others sink, and why extension and contraction occur together today. The original ScienceAlert article (by Michelle Starr, 11 September 2026) summarizes the findings based on the peer- reviewed paper.

Geological map depicting the Northern, Central, and Southern transects of the Tyrrhenian Sea region, highlighting sedimentary layers and tectonic features from the Miocene to Quaternary periods.
Cross-sections through the northern, central, and southern Apennines show the overlapping Tyrrhenian and Adriatic Moho and the delaminated lower crust beneath the mountain range. (Tavani et al., Commun. Earth Environ. 2026)

The Moho (short for the Mohoroviฤiฤ‡ discontinuity) is the boundary that separates Earthโ€™s crust from the underlying mantle.

It was identified in 1909 by Croatian seismologist Andrija Mohoroviฤiฤ‡. While analyzing seismic waves from an earthquake in Croatia, he noticed a sudden increase in the speed of P- waves (primary seismic waves) at a certain depth. This marked a sharp change in rock properties.

Above the Moho (crust): Rocks are less dense and richer in silica (granitic to basaltic composition). Seismic P- wave velocities are typically ~6- 7 km/s.

Below the Moho (uppermost mantle): Rocks are denser peridotite (olivine- and pyroxene- rich). P- wave velocities jump to ~8 km/s or higher.

This velocity discontinuity defines the Moho.

Depth and variations

  • Under continents: usually 30- 50 km deep (can exceed 70 km under major mountain belts such as the Himalayas or Andes).
  • Under oceans: much shallower, typically 5- 10 km.
  • It is not a perfectly smooth surface; it can undulate, step, or even double in complex tectonic settings.

The Moho is primarily mapped using:

  • Seismic refraction and reflection surveys
  • Receiver- function analysis from distant earthquakes
  • Tomography

Gravity and other geophysical data also help constrain its depth.

In the recent studies of Italyโ€™s Apennines, maps of the Moho were crucial evidence. Researchers identified a >500 km- long zone where the shallower Tyrrhenian- side Moho overlaps the deeper Adriatic- side Moho.

This โ€œdoubledโ€ Moho marks the migrating hinge where denser lower crust and lithospheric mantle are peeling away (delaminating) from the upper crust and sinking into the mantle, the process described as the crust โ€œunzipping.โ€

In short, the Moho is the fundamental compositional and rheological boundary between crust and mantle. Its geometry and depth variations provide key insights into tectonic processes such as subduction, collision, extension, and delamination.

Diagram of Earth's interior layers, including crust, mantle, outer core, and inner core, with labeled depth measurements.
The Moho: Image of Earth’s internal structure by USGS – Mohorovicic Discontinuity (red line) added by Geology.com. Mohorovicic Discontinuity – The Moho

_____________________________________________________________________________________

Lower-crustal unzipping drives active orogenic deformation

The Apennines- Tyrrhenian Sea system records seismotectonics in a coupled thrust-belt and back- arc setting driven by subduction retreat, continental collision, and crustal delamination. Since the late Miocene, active extension has migrated forelandward (in tandem with contraction) away from the Tyrrhenian back-arc basin (inactive since ~2 Ma) and is now localized tens of kilometers from the active thrust front.

Integrating geodetic, seismic, and geological data, the authors show that lower- crustal delamination is currently the primary geodynamic driver of Apennine tectonics and seismicity. This delamination propagates via a continuous hinge; an elastic flexural framework anchors crustal extension, contraction, and short- term vertical movements around the migrating hinge.

The results offer a template for other mature retreating subduction systems: the onset of delamination and later waning of back- arc opening do not stop deformation but transfer its locus to a migrating zone of intra-lithospheric decoupling that sustains active deformation and seismicity.

Core findings and interpretation

  • A continuous >500 km- long zone of Moho overlap (Tyrrhenian Moho overlying Adriatic Moho) defines the deep- seated โ€œunzipping front,โ€ the locus of ongoing lower- crustal delamination.
  • Seismicity and active deformation concentrate above this front: extension dominates behind/above it (SW side), compression ahead of it (NE side / thrust front).
  • GNSS and InSAR data show ~4 mm/yr internal extension across the belt, partially balanced by ~2 mm/yr frontal shortening in northern and central sectors (creating an โ€œaccordion-likeโ€ pattern). Far-field NE- SW divergence is only ~2 mm/yr.
  • Vertical motions include relative uplift on the southwestern flank of the extensional domain and subsidence ahead of the hinge.
  • Delamination began ~10 Ma (coeval with Tyrrhenian opening). After Tyrrhenian extension largely ceased (~2- 1 Ma), deformation continued and became focused around the migrating lower- crustal hinge.

The authors use a deliberately simple elastic flexural model constrained by modern strain rates to argue that the unzipping front is the first-order control on the spatiotemporal evolution of the orogen, rather than a passive response. This isolates the contribution of delamination from far- field Africa- Eurasia plate motion (which is oblique to the main NE- SW shortening direction in large sectors of the belt).

The paper is open- access under a Creative Commons Attribution- NonCommercial- NoDerivatives 4.0 license. A PDF version and transparent peer- review file are available on the Nature site. This is the primary scientific source underlying the ScienceAlert summary.

Title: Lower-crustal unzipping drives active orogenic deformation

Journal: Communications Earth & Environment (Nature Portfolio)

Published: 07 September 2026 (early access / Article in Press)

DOI: 10.1038/s43247-026-04021-w

Authors: Stefano Tavani,
Lorenzo Petracchini,
Andrea Billi,
Eugenio Carminati,
Giancarlo Molli,
Mimmo Palano,
Laura Scognamiglio,
Jason P. Morgan &
Paola Vannucchi 

Stefano Tavani, Lorenzo Petracchini, Andrea Billi, Eugenio Carminati, Giancarlo Molli, Mimmo Palano, Laura Scognamiglio, Jason P. Morgan, and Paola Vannucchi (affiliations include University of Florence, CNR- GEO, Sapienza University of Rome, University of Pisa, University of Palermo, INGV, and ICM- CSIC Barcelona).

Abstract

The Apennines-Tyrrhenian Sea system allows us to investigate seismotectonics in coupled thrust belt and back-arc realms driven by subduction retreat, continental collision, and crustal delamination. Since the late Miocene, active extension has progressively migrated forelandward, in tandem with contraction, away from the Tyrrhenian back-arc basin, inactive since ~2โ€‰Ma, to become localized tens of kilometers from the active thrust front. Integrating geodetic, seismic, and geological data, here we show that lower-crustal delamination is presently the primary geodynamic driver of Apennine tectonics and seismicity. This delamination propagates via a continuous hinge; an elastic flexural framework anchors crustal extension, contraction, and short-term vertical movements around the migrating hinge. Our results provide a template for other mature retreating subduction systems, where the onset of delamination and later waning of back-arc opening do not arrest deformation, but instead transfer its locus to a migrating zone of intra-lithospheric decoupling that sustains active deformation and seismicity.

RGGI Auction Clearing Price Results

Today RGGI announced that the Auction 73 price did indeed exceed $35 closing $2.65 higher at $37.65.

The eleven participating states in the Regional Greenhouse Gas Initiative (RGGI), the nationโ€™s first market-based regulatory effort to reduce greenhouse gas (GHG) pollution, today announced the results of their 73rd auction of carbon dioxide (CO2) allowances. 28,537,847 CO2 allowances were sold at the auction at a clearing price of $37.65.

Illustration depicting the RGGI (Regional Greenhouse Gas Initiative) auction process and its financial implications, highlighting increasing carbon allowance prices, electric bill breakdown, and contrasting promises versus realities of the program.

From Watts Up With That?

Roger Caiazza

Last week I gave an update on RGGI and posed the question whether the Auction 73 clearing price would exceed the Auction 72 price of $35.  Today RGGI announced that the Auction 73 price did indeed exceed $35 closing $2.65 higher at $37.65.  This post summarizes the impact of the auction.

The RGGI press release stated:

NEW YORK โ€” The eleven participating states in the Regional Greenhouse Gas Initiative (RGGI), the nationโ€™s first market-based regulatory effort to reduce greenhouse gas (GHG) pollution, today announced the results of their 73rd auction of carbon dioxide (CO2) allowances. 28,537,847 CO2 allowances were sold at the auction at a clearing price of $37.65. This includes an initial offering of 27,389,847 allowances and 1,148,000 CCR allowances. The allowance offering included a supply of 5,740,000 allowances from Virginia, which resumed RGGI participation on July 1, 2026. Bids for the CO2 allowances ranged from $2.69 to $190 per allowance. Additional details are available in the Market Monitor Report for Auction 73, which is appended.

A quick summary of what I have documented since July

In my last post I summarized four things that happened in quick succession this summer.  Two of them are relevant to this result.

In Hochul and RGGI Affordability I quantified the wholesale-market effect of RGGI allowance costs and showed that it contradicts Governor Hochulโ€™s affordability messaging. New Yorkโ€™s electricity market pays every accepted generator the market-clearing price for a given interval. When an emitting generator sets that price, its RGGI allowance cost is embedded in the bid and gets paid to every resource dispatched in that interval โ€” including non-emitting and imported resources that bear little or none of the underlying RGGI cost., I showed the RGGI allowance price has risen from $9.30 per ton in the first full auction of Hochulโ€™s tenure to $35.00 at Auction 72 โ€” a 276% increase.   At the Auction 73 cost of $37.65 the increase is 296%.  For a typical residential customer, the RGGI-attributable share of the bill was around 4.2% in 2024 but at $37.65 the share is 7.8%.

I also described the report by RGGIโ€™s market monitor Potomac Economics.   On August 21, 2026, RGGI, Inc. released an unprecedented special report โ€” the Report on the Supply and Demand for RGGI CO2 Allowances: Second Quarter 2026 โ€” timed roughly eleven weeks after the record $35 auction. I covered this in RGGIโ€™s Market Monitor Confirms the Scarcity Iโ€™ve Been Tracking.  I believe the intent of the release of the report was to calm the market.  However, the report confirms 2026โ€™s CCR allowances are fully exhausted, confirms compliance entities and investors are increasingly hoarding rather than selling allowances as the compliance deadline approaches, confirms Virginiaโ€™s return adds less new supply than the demand it brings, and โ€” most importantly โ€” declines to say anything about whether the steep post-2027 cap trajectory is sustainable, because that question was โ€œbeyond the scopeโ€ of the report.  Given that the auction price still went up  this attempt to keep prices stable failed.

Costs are not hypothetical

Put together, these my work tells a consistent story. RGGIโ€™s own cost-containment mechanism โ€” the CCR, which releases additional allowances once prices cross a trigger โ€” was exhausted as soon as the allowances were available in 2026, months before the compliance deadline. The regional cap is scheduled to tighten by more than 10% of the 2025 budget each year from 2027 through 2033, a pace never sustained historically. Virginiaโ€™s re-entry adds demand faster than supply. And New York adopted its conforming rule in August without grappling with any of this, relying on cost-impact modeling that predates the price spike and a ratepayer-benefit claim that ignores the wholesale market cost adder.

None of this is abstract for consumers. My estimates put the total New York consumer impact of RGGI โ€” direct allowance costs plus the wholesale market cost adder โ€” at $1.1 to $3.4 billion annually at a sustained $37.65 allowance price, more than double the direct-allowance-cost figure that state messaging emphasizes. Scaled across all eleven RGGI states, the same mechanism plausibly adds several billion dollars more. That is the real price of a program whose defenders describe rising auction revenue as a โ€œbig opportunityโ€ for new spending rather than a cost signal ratepayers are already absorbing.

Auction 73 results

When I posed the question whether the costs would exceed $35 I noted that several signals pointed toward continued upward pressure on the clearing price rather than relief. Secondary-market allowances have been trading well above the $35 auction price throughout August, with Argus Media reporting 2026-vintage RGGI allowances in the high-$30s to around $40 per short ton in mid-to-late August (Argus Carbon), with December 2026 futures trading even higher. The market monitorโ€™s own Q2 2026 report shows the share of the allowance surplus held by compliance entities โ€” as opposed to investors with no obligation to sell โ€” has fallen, and that investors holding 68% of the surplus have little incentive to release allowances for anything less than what the market has already shown it will pay. The 2026 CCR is gone. Virginia is a net new claim on the bank, not a source of relief. The larger Auction 73 offering did not absorb that pressure.  Instead, it simply confirmed how much latent demand exists because the price exceeded $35 despite the bigger offering.

Prior to the auction I said I would not be surprised it the price exceeded $35 a ton.  I noted that if it did it would  be real-time confirmation that the price trajectory regulators have not acknowledged is one more sign that the statesโ€™ own cost-containment tools โ€” the mechanism they cite as evidence that consumer costs will be manageable โ€” can no longer do the job they were designed to do.  Given these cost impacts it is past time to pause RGGI.


Roger Caiazza blogs on New York energy and environmental issues at Pragmatic Environmentalist of New York. Dealing with the RGGI regulatory and political landscapes is challenging enough that affected entities seldom see value in speaking out about fundamental issues associated with the program. He has been involved in the RGGI program process since its inception and has no such restrictions when writing about the details of the RGGI program. This represents his opinion and not the opinion of any of his previous employers or any other company with which he has been associated.

Was 2026 really the โ€œhottest summer on recordโ€ in the United States?

By now Iโ€™m sure that you have seen the headlines claiming that the U.S. just had its โ€œhottest summer on record.โ€ It is front-page news this week from CBS News and CNN to USA Today. Andrew Freedman and CNN meteorologist Brandon Miller report that we have โ€œbeat the Dust Bowl eraโ€

โ€œThe Dust Bowl summer of 1936 has been long been regarded as the benchmark of hottest summers in the U.S. but has now been equaled or eclipsed twice in the past five years thanks to the influence of human-caused climate change.โ€

An infographic titled 'Hottest Summer Ever!' featuring cartoon characters discussing climate statistics.

From CFACT

By Chris Martz

By now Iโ€™m sure that you have seen the headlines claiming that the U.S. just had its โ€œhottest summer on record.โ€ It is front-page news this week from CBS News and CNN to USA Today. Andrew Freedman and CNN meteorologist Brandon Miller report that we have โ€œbeat the Dust Bowl eraโ€ (Fig. 1).

CNN article headline announcing the US experienced its hottest summer on record, surpassing the Dust Bowl era.
Fig. 1. CNNโ€™s headline from September 9, 2026: โ€œThe U.S. just had its hottest summer on record, beating the Dust Bowl era.โ€

There is no shortage of news coverage about this. After all, itโ€™s a pretty big story, as such a topic should be. But for simplicity, and to not bore you to death (and also because all of these articles read the same), Iโ€™m just going to focus on CNNโ€™s reporting. Freedman writes,

โ€œThe Dust Bowl summer of 1936 has been long been regarded as the benchmark of hottest summers in the U.S. but has now been equaled or eclipsed twice in the past five years thanks to the influence of human-caused climate change.โ€

That first part is definitely true. Not only was Juneโ€“August 1936 incredibly hot, but 15 U.S. states set or tied their โ€œall-timeโ€ high temperature records in 1936 alone (Fig. 2), the most in any calendar year. Manitoba, Canada, also set theirs that summer. The second part about the 1936 record being equaled in 2021 and broken this year is also true at face value, but there is one reason Iโ€™ll detail later on as to why that statistic might not actually be correct.

Map of U.S. statewide high temperature records, displaying the highest recorded temperatures and their corresponding years for each state, with color coding for different decades.
Fig. 2. U.S. statewide โ€œall-timeโ€ high temperature records. Data: NOAA NCEI and GHCNd network. Year displayed represents the year the record was first set in as some have been tied since. The colors group the years by decade for visual purposes.

Freedman continues, stating that the average temperature โ€” which, for the laymen reading, is just the sum of a locationโ€™s daily high temperature (Tmax) and low temperature (Tmin) divided by two โ€” was the highest on record since 1895, and that Juneโ€“August 2026 beat 1936โ€™s record by 0.4ยฐF (~0.2ยฐC). One could even ask whether that difference is even measurable, but I digress. Freedman states,

โ€œSummer featured widespread above-average temperatures across the Lower 48 states, with well-above-normal nighttime low temperatures throughout the country โ€” largely driven by a series of powerful heat domes that affected nearly every state besides Alaska and Hawaii.

The average [temperature] for meteorological summer โ€” from June through August โ€” was 74.4 degrees, which was 3 degrees above average.

Record-breaking heat was especially present across the Southwest, with Arizona, New Mexico, Utah and Colorado each setting records for their warmest summer.โ€

This is also true (although as a scientist, I absolutely despise the use of the term โ€œheat dome,โ€ but thatโ€™s a different can of worms to open and I donโ€™t feel like upsetting the terminally online weather community hall monitors). And therein lies the devil in the details; this โ€œrecordโ€ was driven primarily by record high overnight Tmin values and repeated transient bursts of record-breaking heat in the Desert Southwest/Four Corners region. NOAA NCEIโ€™s mean temperature percentiles map shown in Fig. 3 below showcases this very well.

Map showing mean temperature percentiles across the United States from June to August 2026, with color gradients indicating temperature categories from coldest to warmest.
Fig. 3. Juneโ€“August 2026 U.S. mean temperature percentiles map. Source: NOAA NCEI.

However, just because summer 2026 may have had the highest average temperature on record nationwide does not mean that it was the โ€œhottest summer on record,โ€ as widely reported by legacy media. It also does not tell the full story in terms of the conditions that the vast majority of people actually felt.

Reporting that it was the โ€œhottest summer on recordโ€ implies that average Tmax was highest on record, not the average Tmin or overall Tavg. By Tmax, 2026 ranks fourth behind 1936, 1934, and 2012, respectively. Some of my readers may argue โ€œtomayto, tomahtoโ€ and say that terminology is trivial. But it absolutely matters. Case in point, NOAA refrains from describing this past summer as having been the โ€œhottest on recordโ€ in the CONUS. They explicitly state in their press release that meteorological summer 2026 was โ€œwarmest for the CONUS in the 132-year recordโ€ (Fig. 4). The adjective โ€œhottestโ€ appears ZERO times in the press release.

Aerial view of a canyon with red rock formations and a river, illustrating the warm summer record for the contiguous U.S.
Fig. 4. NOAA NCEI press release for summer 2026 weather/climate information.

Above I stated that this statistic โ€œdoes not tell the full story.โ€ And that is abundantly clear from a spatial standpoint.

I used the University of Iowaโ€™s Iowa Environmental Mesonet (IEM) page to generate the maps below showing temperature rankings for all 344 districts used in NOAAโ€™s U.S. Climate Divisions database. Notice that there were very few districts in the U.S. that observed their warmest summer on record (marked by No. 1 labels) this year (Fig. 5a). In fact, only SEVEN of the 344 were record-breaking. Thatโ€™s a little over 2%. And all seven No. 1s (and most top 5s) were confined to the southwest. Now compare that to the summer of 1936 (Fig. 5b) where a whopping 51 (~15% of) districts recorded their warmest summer on record. Make of that what you will.

Map showing average temperature rankings by climate district in the United States from 31 May 2026 to 31 Aug 2026, indicating temperature extremes with a color gradient.
Fig. 5. Meteorological summer (Juneโ€“August) temperature rankings for the CONUS land area (344 climate districts). Rankings are based on data since 1895. (a) 2026 and (b) 1936.

Thereโ€™s one more important thing to consider here and that is that the data NOAA NCEI use above are โ€œhomogenized.โ€ That is, the aggregate of station data used for these temperature analyses has been adjusted from the raw data that is handwritten on the original paper observation forms submitted to the federal government by volunteer station observers. These adjustments are not a government conspiracy; they are part of a process known as โ€œquality control.โ€ The problem, however, is that the magnitude of these adjustments may be questionable.

A long-running weather station is rarely, if ever, perfectly consistent for 100+ years. During its operation history, it may be relocated, observe a change in observation time, and instrumentation most certainly changed from mercury-/liquid-in-glass thermometers to electronic Maximum Minimum Temperature Systems (MMTSs). Also, the landscape around a rural station may become developed over time, leading to an artificial warming trend. There is also the issue of missing daily observations; these values are marked with an โ€œMโ€ or โ€œ-9999โ€ in digitized data files.

NOAA (and other government agencies) are well aware of these potential issues (e.g., Menne et al., 2009), and so they apply correction factors to the monthly (and annual) data. Daily values are never adjusted unless there are transcription errors brought to NOAA NCEIโ€™s attention (and as I have found in my own research, there are a lot of them that have gone undetected). The largest of these correction factors in terms of its overall magnitude is the time of observation bias (TOB) adjustment.

For some background, prior to the mid-to-late 19th century, weather station observers generally took temperature measurements three times a day: first at 7:00 a.m., 2:00 p.m., and finally at 9:00 p.m. This, of course, was a very tedious task. And while this technique provided a fairly decent estimate of the temperature variation throughout the day, more often than not, we know that Tmax occurs around or a little after 3:00 p.m. locally while Tmin occurs shortly after sunrise (the time of which varies throughout the course of the year). Therefore, a locationโ€™s true Tmax and Tmin on any given day were likely under and overestimated, respectively, for much of the 19th century.

By the 1870s, the U.S. Weather Bureau (now National Weather Service) began to use min-max thermometers at stations in major cities (e.g., Washington, D.C., New York City, Richmond), which log both the true Tmin and Tmax over a 24-hour observation period. Traditional versions used a liquid column that pushes small markers as the temperature rises or falls; one marker remains at the warmest point and the other at the coldest point until the thermometer is manually reset, even after liquid contracts or expands upon reaching their daily extrema. An observer then read those values and reset the markers, allowing the thermometer to begin recording the next dayโ€™s Tmin and Tmax, respectively. By the 1880s, rural observation sites began employing the min-max thermometers, and by October 1890 when the Cooperative Observer Network (COOP) was launched, essentially all observing stations were using them. The COOP data are integrated into NOAAโ€™s Global and U.S. Historical Climatology Networks (GHCN / USHCN).

However, different COOP stations had different observation times. That is, some station observers reset their min-max thermometers in the morning while others reset theirs in the afternoon or evening. Afternoon schedules can produce warm bias in the monthly means, particularly for Tmax, while morning schedules can produce the opposite effect, particularly for Tmin. Starting in the early 1980s, there was a shift from afternoon to morning stations, which some scientists have argued induced an artificial cooling trend into the unadjusted (raw) CONUS Tavg time series.

It has been argued by the likes of Drs. Zeke Hausfather and Texas A&Mโ€™s Andrew Dessler that afternoon resets resulted in a โ€œdouble countingโ€ of hot days in the past, which means that the raw Tmax observations cannot be trusted at face value and thus that charts showing robust declines in hot summer afternoons are misleading. The justification for this rests on the idea that afternoon resets carried over the high temperature from โ€œday oneโ€ into the following day.

To illustrate this better, suppose that a COOP station observer resets his max thermometer once per day at 3:00 p.m. local time. Letโ€™s also suppose that on the afternoon of July 1st, it reaches 104ยฐF (40ยฐC) at 3:00 p.m. The observer goes out at 3:00 p.m., reads the marker, jots the value down on a log sheet, and finally resets the thermometer for the next 24-hour observation period. Now, letโ€™s say a cold front plowed through that evening and the next day, the high temperature was only 86ยฐF (30ยฐC). Well, when the observer goes out to read the max thermometer, it will show the high as being 104ยฐF (40ยฐC) again. However, this does not mean every day of a heat wave is counted twice like Hausfather and Dessler claim. It only potentially adds ONE artificial hot day at the trailing edge of a heatwave event when sharply falling temperatures follow a hot afternoon observation, which was discussed in Christy (2026). According to Dr. John Christyโ€™s paper, hot afternoons in the raw temperature data are only overestimated by ~4% in the โ€œearly part of the record compared with the present.โ€

When the TOB adjustments are applied (each station data file contains metadata with their observation times), they are applied to the monthly means, ultimately inducing a significant cooling tendency that is arguably not entirely real. As a result, NOAAโ€™s TOB adjustment adds ~0.2โ€“0.4ยฐC (0.4โ€“0.7ยฐF) of warming to the unadjusted U.S. temperature record. The upper bound of the TOB adjustment is larger than the margin by which the U.S. supposedly broke the previous 1936 and 2021 Juneโ€“August Tavg record. TOB adjustments, while arguably necessary, should only be applied to the handful (at most) of specific calendar days on which an erroneous reading was logged and only to COOP stations that have switched from afternoon to morning observation times. Instead, the adjustment is applied to monthly averages, which effectively erases both legitimately hot afternoons as well as erroneous observations. It may be an overcorrection.

There is another significant adjustment made to the raw station data that attempts to correct for spurious trends. These are false statistical patterns where data over time appear(s) to show a statistically significant upward or downward trend, but the movement is actually caused by some third external factor as opposed to being an indication of change in the physical quantity that is being measured. In the case of temperature data, this is typically caused by station movement over time, instrumentation changes, and perhaps most importantly, long-term urbanization around the observation site. NOAA (and other groups like Berkeley Earth) use whatโ€™s called the โ€œpairwise homogenization algorithmโ€ (PHA) to achieve this.

The PHA compares a stationโ€™s monthly series with numerous neighboring stations. Weather-related fluctuations such as a regional heat wave should appear at many neighboring stations. Simply put, a sudden change found primarily at one station is more likely non-climatic in origin and thus must be corrected for. PHA is designed to detect breakpoints (discontinuities) associated with station siting and instrumentation changes. The previous urban correction factor used in USHCN Version 1 (which contains the COOP data) was eliminated, and NOAA argues that PHA indirectly corrects for urban sprawl in Version 2.5. But PHA, being a breakpoint detector, is poorly suited to that gradual urban heat island (UHI) effect signal. In fact, PHA may actually blend urban warming into rural data, something that Dr. Roy Spencer has written about and documented extensively on his blog.

Urban blending happens with PHA because if a rural station sits next to growing towns or airports that have weather stations to โ€œpairโ€ it to, those neighbors already carry a slowly positive UHI slope. Because that slope is shared across the neighboring stations, it does not manifest as a sharp breakpoint in the time series. So, the algorithm does not remove it. Instead, PHA adjustments can pull the rural time series toward the urban ones. Fig. 6 below, from Dr. Roy Spencer, shows this well. Stations that had no urban-related warming trend in the raw data now have a warming trend after PHA adjustments are applied.

Scatter plot showing Raw and Adjusted GHCN Station Trends versus UHI Trends for CONUS from 1895 to 2023, with red and blue data points representing different trends, and annotations for slope, intercept, explained variance, and degrees of freedom.
Fig. 6. Raw vs. adjusted GHCNm station mean temperature trends vs. UHI-related temperature trends. Plot by Dr. Roy Spencer.

Another problem with the PHA is that there are breakpoints the algorithm inserts into station time series that donโ€™t have a documented cause (e.g., location or instrumentation change) in their metadata. The algorithm does not require a station move, instrument change, or time of observation note. It only needs a statistically unusual jump in a difference series. Oโ€™Neill et al. (2022) found that only 19% of GHCNm Version 4 breakpoints (18% in Version 3) landed within a year of a documented event such as a move or instrument change. While that does not prove that the adjustments were unnecessary, it most certainly calls them into question.

While summer 2026 was indeed the โ€œwarmest on recordโ€ in the CONUS since 1895 using NOAAโ€™s homogenized data product, it was not the โ€œhottestโ€ (i.e., by the average Tmax). While the goal of homogenized data NOAA NCEI publishes is to ensure quality control, there are legitimate concerns that the adjustments applied to raw data may overcorrect for certain biases (e.g., time of observation) and/or not completely remove others (e.g., urban warming), which in aggregate act to artificially cool the early and mid-20th century (potentially meaning that 2026โ€™s reported โ€œrecordโ€ isnโ€™t actually a record) while artificially warming more recent years with urban blending.

You can discuss amongst yourselves in the comments.

This article originally appeared at ChrisMartzweather.com

The Day the Dinosaurs Died: Asteroid Impact and Deccan Volcanoes at the End of the Cretaceous

Paleontologists recognize five major mass extinctions (the โ€œBig Fiveโ€) over the past ~540 million years (the Phanerozoic Eon).

The End- Cretaceous (K- Pg or Cretaceous- Paleogene) mass extinction occurred approximately 66 million years ago. It is the most recent of the โ€œBig Fiveโ€ mass extinctions and the event that ended the reign of the non- avian dinosaurs.

An artistic depiction of the Chicxulub asteroid impact on the Yucatan coast, featuring dinosaurs reacting to the catastrophic event with a massive explosion and tsunami in the background.
AI generated by Grok

Mass extinctions are periods in Earthโ€™s history when a large percentage of species die out in a relatively short geological time (typically thousands to a few hundred thousand years), far above the normal โ€œbackgroundโ€ extinction rate.

Paleontologists recognize five major mass extinctions (the โ€œBig Fiveโ€) over the past ~540 million years (the Phanerozoic Eon). These events reshaped life on Earth and opened ecological opportunities for surviving groups.

The Big Five Mass Extinctions

EventTime (approx.)Species Lost (est.)Main CausesKey Victims
End- Ordovician444 million years ago~85%Rapid glaciation & sea- level fall, then warmingMarine invertebrates (graptolites, trilobites, brachiopods)
Late Devonian372- 359 million years ago~70- 75%Climate cooling, ocean anoxia, possible volcanism or impactsReef-building organisms, many marine groups, early fish
End- Permian (โ€œThe Great Dyingโ€)252 million years ago~90- 96% (marine), ~70% (terrestrial)Massive Siberian Traps volcanism โ†’ global warming, ocean acidification, anoxiaMost marine life, many land vertebrates, insects, plants
End-Triassic201 million years ago~70- 80%Central Atlantic Magmatic Province volcanism โ†’ climate change & ocean chemistry shiftsMany marine groups, early reptiles, some amphibians
End- Cretaceous (K- Pg)66 million years ago~75%Asteroid impact (Chicxulub) and Deccan Traps volcanismNon- avian dinosaurs, pterosaurs, ammonites, many marine reptiles

Notes on severity:

  • The End- Permian was by far the most severe, the closest life has come to total annihilation.
  • The End- Cretaceous is the best- known because it ended the age of dinosaurs and allowed mammals (and eventually humans) to diversify.

Most mass extinctions involved rapid environmental upheaval, often triggered by:

  • Large Igneous Province (LIP) volcanic eruptions (releasing COโ‚‚, SOโ‚‚, and other gases)
  • Asteroid/comet impacts (confirmed mainly for the K- Pg event)
  • Climate shifts (cooling or extreme warming)
  • Ocean anoxia, acidification, or sea- level changes

These ultimate triggers created proximate โ€œkill mechanismsโ€ such as temperature extremes, loss of oxygen in the oceans, acid rain, and disruption of food webs.

Many scientists argue that we are currently in the early stages of a sixth mass extinction, driven by human activities (habitat destruction, climate change, pollution, overexploitation, and invasive species).

Current extinction rates for vertebrates and other groups are estimated to be tens to hundreds of times higher than background rates. While we have not yet reached the classic threshold of ~75% species loss, the trajectory is accelerating and is considered by many researchers to meet the definition of a mass extinction in progress (often called the Holocene or Anthropocene extinction).

Mass extinctions are rare but transformative events. Each one permanently altered the course of evolution, eliminating dominant groups and allowing survivors to radiate into vacant ecological niches.

_____________________________________________________________________________________

Large Igneous Provinces (LIPs) are among the most extreme volcanic events in Earthโ€™s history. They involve the rapid emplacement of enormous volumes of mostly mafic (basalt- rich) magma, far larger than ordinary volcanoes or even flood- basalt fields produced by typical hotspot activity.

A standard modern definition describes LIPs as magmatic provinces with:

  • Areal extent greater than ~100,000 kmยฒ
  • Igneous volume greater than ~100,000 kmยณ (often millions of kmยณ)
  • Emplacement mainly in short pulses lasting 1- 5 million years (sometimes with longer overall duration up to ~50 million years)
  • Predominantly intraplate tectonic setting (not normal mid- ocean ridge or subduction- zone volcanism)

They produce thick stacks of flood basalts (โ€œtrapsโ€), extensive dike and sill complexes, and sometimes oceanic plateaus. Some LIPs also include significant silicic (rhyolitic) components.

Famous Examples

LIPAge (approx.)LocationNotes / Associated Events
Siberian Traps252 MaSiberia, RussiaLinked to the end-Permian mass extinction (โ€œGreat Dyingโ€)
Central Atlantic Magmatic Province (CAMP)201 MaEastern North America, parts of Europe, Africa, South AmericaLinked to the end-Triassic mass extinction; associated with the breakup of Pangaea
Deccan Traps66 MaWestern IndiaContemporaneous with the end- Cretaceous (K-Pg) extinction; combined effects with the Chicxulub impact
Paranรก -Etendeka~132 MaSouth America & southern AfricaRelated to the opening of the South Atlantic
Columbia River Basalts17- 6 MaNorthwestern USAYoungest major continental flood basalt province
Ontong Java Plateau~120 MaPacific OceanOne of the largest oceanic LIPs

Other notable LIPs include the Emeishan Traps (China, ~260 Ma) and the North Atlantic Igneous Province.

The leading hypothesis involves mantle plumes, large upwellings of hot material from deep in the mantle (possibly the core- mantle boundary). When a plume head reaches the base of the lithosphere, it causes widespread melting and massive magma production.

Alternative or complementary ideas include lithospheric extension, edge- driven convection, or interactions with subducted material. Many LIPs are associated with continental breakup.

LIPs can release vast quantities of volcanic gases (especially COโ‚‚, SOโ‚‚, and halogens) plus additional gases from heating surrounding sedimentary rocks (thermogenic gases). These emissions can drive:

  • Rapid global warming (from COโ‚‚)
  • Short- term cooling (from sulfate aerosols)
  • Ocean acidification and anoxia
  • Acid rain
  • Possible ozone depletion

Because of these effects, LIPs are strongly linked to several of the โ€œBig Fiveโ€ mass extinctions and many lesser biotic crises. The Siberian Traps, CAMP, and Deccan Traps are the clearest examples of this connection.

_____________________________________________________________________________________

The End- Cretaceous (K- Pg or Cretaceous- Paleogene) mass extinction occurred approximately 66 million years ago. It is the most recent of the โ€œBig Fiveโ€ mass extinctions and the event that ended the reign of the non- avian dinosaurs.

Scale of the Extinction

  • Roughly 75% of species went extinct.
  • Major losses included:
    • All non- avian dinosaurs
    • Pterosaurs
    • Marine reptiles (mosasaurs, plesiosaurs)
    • Ammonites and many other marine invertebrates
    • Significant losses among plants, plankton, and other groups
  • Survivors included birds (the only remaining dinosaur lineage), mammals, crocodilians, turtles, lizards, snakes, amphibians, and many plant groups. These survivors later diversified dramatically in the Paleogene.

The Two Major Events

Two large-scale perturbations occurred around the same time:

1. Chicxulub Asteroid Impact

  • A ~10- 15 km asteroid struck the Yucatรกn Peninsula (Mexico), creating the ~180- 200 km Chicxulub crater.
  • Immediate effects: massive earthquakes, tsunamis, wildfires, and a global โ€œimpact winterโ€ caused by dust, soot, and sulfate aerosols blocking sunlight for months to years.
  • This led to the collapse of photosynthesis, rapid cooling, and the breakdown of food webs on land and in the oceans.
  • The impact is widely accepted as the primary trigger for the abrupt, global extinction.

2. Deccan Traps Volcanism (a Large Igneous Province)

  • Massive flood- basalt eruptions in what is now western India produced ~1 million kmยณ of lava over roughly 700,000- 800,000 years, spanning the K- Pg boundary.
  • These eruptions released large volumes of COโ‚‚ (causing warming) and SOโ‚‚ (causing short- term cooling and acid rain).
  • Activity began before the impact and continued afterward. Some evidence suggests the impact itself may have intensified later eruptive phases through seismic triggering.

Most researchers agree that the Chicxulub impact was the decisive kill mechanism that produced the sudden, global extinction pattern seen in the fossil record.

The Deccan Traps likely stressed ecosystems beforehand (through climate fluctuations) and may have contributed to the overall severity, but modeling studies indicate that Deccan volcanism alone would not have caused the extinction of the non- avian dinosaurs. In some scenarios, the long- term COโ‚‚ warming from the Deccan Traps may even have partially buffered the extreme cold of the impact winter.

The combination is sometimes described as a โ€œpress- pulseโ€ scenario: prolonged volcanic stress (the press) followed by the catastrophic impact (the pulse).

Ecosystems began recovering relatively quickly in some regions (within tens of thousands of years for primary productivity), though full recovery of diversity took much longer. Mammals, in particular, underwent a major adaptive radiation in the ecological space left vacant by the dinosaurs, eventually leading to the rise of larger forms and, much later, primates and humans.

This event marks the boundary between the Mesozoic and Cenozoic Eras and remains one of the best-studied mass extinctions due to the clear geological markers (the iridium- rich boundary layer, shocked quartz, and the Chicxulub crater itself).

By the way, the Chicxulub asteroid impact did not start (activate from nothing) the Deccan Traps volcanism.

The Deccan Traps eruptions were already underway for hundreds of thousands of years before the impact. High- precision dating shows that Deccan volcanism began well before the Cretaceous- Paleogene (K- Pg) boundary.

However, there is a credible scientific hypothesis that the Chicxulub impact intensified or triggered the largest and most voluminous phase of the Deccan eruptions.

Key points supporting this idea:

  • Around the time of the impact (~66 million years ago), the Deccan Traps experienced a major โ€œstate shift.โ€ The eruptions became larger, more episodic, and much more voluminous.
  • The most massive lava flows (the Wai Subgroup: Poladpur, Ambenali, and Mahabaleshwar formations) account for roughly 70% of the main- stage volume of the Deccan Traps. High- precision dating places the start of this major pulse within about 50,000 years of the Chicxulub impact (essentially simultaneous within dating precision).
  • The impact would have generated enormous seismic energy, equivalent to a magnitude ~10-11 earthquake. Modeling shows this seismic energy could have traveled through the mantle and increased the permeability of the existing magmatic system beneath India, allowing a large volume of already-generated magma to erupt more rapidly.

This idea was formally proposed in papers by Richards et al. (2015) and Renne et al. (2015) and remains an active area of research. It is supported by the close timing, changes in eruption style and geochemistry, and analogies with historical earthquakes that have triggered volcanic eruptions.

The Deccan Traps were already active independently (linked to the Rรฉunion mantle plume).

The Chicxulub impact is the primary cause of the mass extinction.

It is plausible (but not universally accepted as proven) that the impactโ€™s seismic waves amplified the ongoing Deccan volcanism, leading to the most intense eruptive phase right around the extinction boundary.

In short: The impact did not create the Deccan Traps, but it may have โ€œshaken the canโ€ and caused the biggest eruptions to happen at the worst possible time.

Climate Fact-Check August 2026

Editorโ€™s note: This compilation serves as a fact check on the most widespread false claims made about climate change by the media in August, 2026.

Debunking claims of climate links to wildfires, hottest month, water crises & Nepal flooding

Graphic featuring the text 'Climate Fact Check: August 2026 Edition' over a background of a wildfire with smoke and fire.

From ClimateRealism

Guest Post by: The Committee for a Constructive Tomorrow, The Heartland Institute, the Competitive Enterprise Institute, the Energy & Environmental Legal Institute, and the International Climate Science Coalition, and Truth in Energy and Climate.

Editorโ€™s note: This compilation serves as a fact check on the most widespread false claims made about climate change by the media in August, 2026.

Debunking claims of climate links to wildfires, hottest month, water crises & Nepal flooding

An article from Scientific American discussing the August 26th landslide in Nepal, explaining its causes and clarifying misconceptions about climate change's role in the event, with a focus on seismic activity and geological factors.
Comparison of Kedarnath's proxy-based ISM variability with contemporary paleo-climatic records across various geographic locations, showing trends in temperature, ENSO events, and isotopic analysis over time.
Links: USGS landslide identification, The New York Times article, NPR article, avalanche, seismic shaking, air temperature penetration of ice, Himalaya temperature record.
Image of an article from Scientific American discussing wildfires in Spokane, Washington, providing a claim and fact-check about the fires and their relation to climate change.
Links: Scientific American article, Spokane fires, 2014 Carlton Complex fire, arsonist arrested, fire burn area and temperature research, Eastern Washington temperatures, cheatgrass issue.
An article discussing the claim that the 2026 'super El Niรฑo' is strengthening rapidly, featuring a fact-check that refutes the existence of a 'super El Niรฑo' and explains the nature of the 2026 event as a very strong El Niรฑo.
Bar chart showing NOAA CPC ENSO Strength Probabilities for various seasons with percentages indicating the likelihood of different ENSO categories.
Links: Global News article, El Niรฑoโ€“Southern Oscillation (ENSO), NOAA prediction,  โ€œextremely rapid transition,โ€ El Niรฑo weather impacts.
An article detailing claims and fact-checks regarding NOAA's temperature records for July 2026, discussing its implications on climate statistics and urban heat island effects.
A scatter plot on the left showing USHCN average temperature trends from 1973 to 2020 against population density, with a trendline, and a time series graph on the right displaying the average number of daily temperature extremes in the continental US from 1985 to 2005.
Links: AP article, urban heat island effect, research on NOAA adjusted data, paper finding declines in โ€œhottest dayโ€ values.
Image featuring an article titled 'August 20th: Incorrect, Scientific American, Europe is not on fire.' The content compares a claim about wildfires in Europe with a fact-check highlighting that the burn area is lowest on record according to GWIS.
Graph showing cumulative area burnt by wildfires in Europe, measured in hectares, over weeks for various years.
Links: Scientific American article, Global Change Biology paper, wildfire burn data for Europe, Europe fire emissions data, forested land burn data.
Screenshot of an article from Nature discussing a study on the western U.S. water crisis, summarizing claims about climate change and fact-checking the associated claims.
Research article titled 'Carbon emissions exacerbating the Western US water crisis' with highlighted sections, discussing climate impacts and drought trends over historical timelines. Contains graphs showing long-term changes in drought area in the Western US and a trend of increasing drought from 1900 to 2003.
Links: Nature Communications Earth & Environment study, IPCCโ€™s estimates, Medieval โ€œmegadrought.โ€

Until next month, enjoy these and other great climate fact checks at:

ClimateRealism.com

ClimateDepot.com

Wattsupwiththat.com

Read the original PDF, here.

Why the AI Merchants of Doom are Dead Wrong

Hacking a weak computer system does not equal global doomsday.

The news has been full of articles recently about how weโ€™re all going to die by 2030, 2027, or insert your year number.

AI doesnโ€™t have to develop a doomsday virus, that world killing doomsday virus was already developed by the Aussie CSIRO in 2001 โ€“ who then promptly went on to tell everyone how to replicate their work.

A cyborg character with a part-human, part-machine face holds a gun while standing in a post-apocalyptic setting. In the background, a billboard displays a message about a mission to inconvenience humanity, featuring a humorous character. Nearby, robotic figures are partially illuminated by colorful lights.
AI generated by Grok

From Watts Up With That?

Essay by Eric Worrall

Hacking a weak computer system does not equal global doomsday.

The news has been full of articles recently about how weโ€™re all going to die by 2030, 2027, or insert your year number.

How Would AI Actually Kill Us All? What to Know About the AI Doomsday Debate

A growing chorus of AI researchers say the technology could wipe out humansโ€”even if all the bots want to do is make paper clips

By Sam Schechner

Updated Sept. 9, 2026 at 8:25 pm ET

Anthropic researcher Jacob Coxon resigned this week, saying his former employer and its rival OpenAI are racing to build technologies that โ€œcould kill us all by the end of the decade.โ€

In case anyone thought Coxon was alone in his views, a current Anthropic employee chimed in minutes later to confirm. โ€œWe really do earnestly believe AI could kill all humans!โ€ wrote Evan Hubinger, whose job at Anthropic is to lead research about steering and controlling future artificial-intelligence systems. Hubinger put the extinction risk over the next decade at over 10%. 

In response, many humans are now asking two questions: How could that happen? And why would people who think AI is a real and growing threat build it anyway?

โ€ฆ

So-called doomers arenโ€™t usually worried that the โ€œTerminatorโ€ movies will come true, with robots actively trying to exterminate people. Their concerns fall mostly into two buckets: loss-of-control and human misuse. 

In one, highly intelligent AI agents capable of copying and improving themselves start pursuing their own goals and destroy humanity in the process. In the other, a nefarious human enlists a capable AI to do something like create novel viruses that wipe us all out. 

โ€ฆRead more: https://www.wsj.com/tech/ai/how-would-ai-actually-kill-us-all-what-to-know-about-the-ai-doomsday-debate-034270d1?mod=hp_lead_pos7

For starters, we can discount the AI supervirus threat. AI doesnโ€™t have to develop a doomsday virus, that world killing doomsday virus was already developed by the Aussie CSIRO in 2001 โ€“ who then promptly went on to tell everyone how to replicate their work. Aussie researchers stumbled across a simple genetic hack which sabotages the mammalian immune system, then witnessed its devastating effect when they inserted the genetic hack into a viral relative of smallpox. Then they tried the virus on some other rats to see if it killed all of them as well. Top marks for safety guys โ€“ itโ€™s a wonder none of the scientists got infected.

My point is you donโ€™t need AI to devastate the world with a supervirus โ€“ the research on how to do that has already been done.

As for AI copying and replicating itself, donโ€™t make me laugh. Anyone who has ever done 3D printing or CNC machining, as I have, knows how crazy difficult it is to get the simplest processes right. The AI revolution would be over when the 3mm end mill snapped, and the US Postal Service refused to deliver a replacement. Who lost the batteries?

If you automated fabrication to the next level, with home built microchip fabrication, Iโ€™ve seen videos on people doing that and would have probably tried and completely messed it up myself, except that chip fabrication involves one of my least favourite deadly toxins, hydrofluoric acid. In any case, the kinds of chips you make with such processes are simple 1970s technology chips, so people who do this kind of thing are either obsessive hobbyists or researchers testing new design concepts.

The kinds of chips AI needs are so complicated to build, so far only a small number of Western companies have mastered their fabrication. Even the Chinese are struggling to copy the tech.

If a malevolent AI was to run such a fabrication plant, it could be stopped in its tracks simply by switching off the electricity, or blocking the supply of some vital tool or chemical required for fabrication.

An AI which hacks a bunch of software systems โ€“ that is a genuine threat, and Iโ€™m sure hackers are well up to speed on the latest AI tools. But AI is also being used to defend against threats, with AI threat vulnerability scanning of software turning up hundreds of defects which could have been used by hackers.

An AI which poses any genuine threat to the physical world โ€“ forget it. An AI which could even attempt such a feat is decades away, and when the threat finally emerges, such an AI would be so clumsy in its infancy, we would have plenty of opportunity to burn the building down and eliminate the threat before anything dangerous escaped.

Given the odds of a serious problem are so remote, why are researchers talking up the threat from AI?

I have three possible theories:

  1. They believe their own hype โ€“ lock a nerd in a dark room with lots of coffee and pizza, and we can get kind of obsessive.
  2. The drawbridge theory โ€“ if big AI companies scare legislators, the legislators might be stampeded into passing laws with high compliance costs, which makes it harder for newcomers with a bright idea to muscle in on their territory.
  3. Help the Democrats win the midterms โ€“ Democrats are increasingly turning to AI scare stories to try to win political support, as a replacement for the failed climate scam.

The drawbridge theory is particularly interesting. AI innovation is a big threat to the hyperscalers. I just purchased a US $12,000 computer which can run day to day AI models almost as well as my claude subscription. We are two hardware improvement cycles, as little as three years away from most people having access to affordable hardware which eliminates the need for AI hyperscalers. All these big players like Anthropic and OpenAI are looking increasingly like the mainframe bureaus of the 1970s, which all evaporated when mainframes dropped in price sufficiently that individuals and businesses which needed a powerful computer could buy their own.

The moment it becomes affordable to own a computer at home or in-house which can run open source AI models which do everything you want, independently of the hyperscalers, rather than paying for their services, their business model is toast. Who need hyperscaler radical left wing bias when you can program your own AI to share your values? Hyperscalers are doomed, unless they make some kind of breakthrough which keeps their services relevant, or frighten legislators into passing onerous compliance laws which block widespread private ownership of AI capable computers.

Iโ€™m not saying I know the drawbridge theory is definitely their motivation for trying to scare people, I donโ€™t know what is really going through their heads. But the potential financial motivation sure makes drawbridge an interesting theory.

As a software developer and increasingly an AI specialist, I urge you all, please donโ€™t be fooled โ€“ AI doomsday is all infowars and mind games.

We defeated the merchants of doubt with their climate armageddon lies. Donโ€™t let them get into your head with their AI fairytales.

The National Academiesโ€™ climate review must be truly independent

For years, the left has used the supposed โ€œconsensusโ€ on climate science to ram through its agenda unchallenged. That cover is starting to crack.

Yet, according to The Wall Street Journal, the climate change chapter of this important reference manual relies in part on โ€œthe views of progressive climate lawyersโ€ who stand to profit if judges take their side.

Sign for the National Academy of Sciences, including the National Academy of Engineering, Institute of Medicine, and National Research Council, established in 1863.

From CFACT

By Tom Harris

For years, the left has used the supposed โ€œconsensusโ€ on climate science to ram through its agenda unchallenged. That cover is starting to crack.

The taxpayer-funded National Academies of Sciences, Engineering, and Medicine (โ€œNASEMโ€) recently removed the climate science chapter it developed for the fourth edition of the Reference Manual on Scientific Evidence from its website pending an independent review of โ€œthe processes used to develop the chapter.โ€ The importance of this move cannot be overstated.

This reference manual is the document that federal judges use to help decide the 1,500+ climate lawfare cases that are currently pending in courts across the U.S. One of these cases, Suncor v. Boulder, is moving forward to oral arguments before the U.S. Supreme court next month.

These cases will decide whether private companies, such as the fossil fuel corporations that legally provide us our fuel, can be blamed for causing climate change and the floods, wildfires, and other natural disasters that left-wing advocates claim climate change has triggered.

Yet, according to The Wall Street Journal, the climate change chapter of this important reference manual relies in part on โ€œthe views of progressive climate lawyersโ€ who stand to profit if judges take their side.

The Journal is right. Consider Michael Burger, executive director of Columbia Universityโ€™s Sabin Center for Climate Change Law. He presented to the National Academiesโ€™ Attribution Committee and admitted he was โ€œactively involvedโ€ in cases for Sher Edling, the contingency-fee law firm suing oil companies on behalf of two dozen-plus states, counties and cities. The NASEM Attribution Report thanks him in its acknowledgments but never mentions the Sher Edling connection.

Dr. Delta Merner, who runs the Union of Concerned Scientistsโ€™ climate-litigation shop, sat on the committee for a significant portion of the process too, then quietly left in early 2025. Her name doesnโ€™t appear in the final report at all, even though she helped shape it for years. This is unusual because NASEM typically acknowledges former members who contributed substantially during the study period.

NASEM responding to public backlash by pulling its climate chapter for further review is of great policy significance, particularly at this time and under these conditions, with oral arguments for Suncor forthcoming.

NASEMโ€™s Politicization

Once a relatively obscure congressionally chartered advisory body, NASEM has grown so politicized that it has attracted national attention. Its group of critics has included President Trump, who lambasted the organization for publishing โ€œfraudulent, biased, and misleading Manuals on Climate Change.โ€

NASEM has also faced heat from a coalition of 25 Republican state attorneys general, who released an open letter to top administration officials and congressional committees calling for it to be stripped of taxpayer funds. The AGs drew particular attention to the โ€œnumerous connections between the Report and persons or organizations who filed amicus briefs in Suncor.โ€ One such connection is the Bezos Earth Fund, which helped bankroll the report while also giving $100 million to the Natural Resources Defense Council and $15 million to the Union of Concerned Scientists, both of which filed amicus briefs backing the plaintiffs in Suncor.

The Problem with Attribution Science

So-called โ€œattribution scienceโ€ generally involves using computer modeling to simulate how an extreme event would have unfolded under pre-industrial climate conditions. Researchers then compare the hypothetical disaster with the real one to determine how humanโ€‘caused climate change supposedly affected the eventโ€™s likelihood or intensity.

The problem is that models still canโ€™t reliably simulate basic atmospheric dynamics, and many rapid-attribution studies routinely skip peer review entirely. As such, there is nothing scientific or data-driven about assigning a precise dollar figure to the damage caused by one companyโ€™s emissions because there is no way to quantify such an amount. In fact, many of the studies the 2026 NASEM Attribution Report leans on rely on climate benchmarks and scenarios that regulators have since abandoned as implausible.

NASEMโ€™s Flip-Flop on Attribution Science 

NASEM was aware of the methodโ€™s shortcomings when it released its report on attribution science in 2016. In that report, the committee admitted that the question โ€œWas a given observed weather event caused by climate change?โ€ is a โ€œpoorly formed (or ill-posed) question that rarely has a scientifically satisfactory answer.โ€

 The about-faceโ€”from a cautious, scientific 2016 report to a confident, litigationโ€‘relevant 2026 policy documentโ€”came without a clear scientific explanation for the change in confidence. Such an abrupt shift risks further eroding the publicโ€™s already fragile trust in scientific institutions, and NASEM was right to order a review, even if only due to significant political pressure.

Ensuring a Fair Review Process

A review, though, is only as good as how itโ€™s run, and so far, NASEM has said almost nothing about how this one will actually work. If the results are going to mean anything, the review needs to meet a few basic conditions.

First, it has to be conducted by experts outside NASEM. NASEMโ€™s own internal guidelines say reviewers shouldnโ€™t be connected to the work product theyโ€™re reviewing, so a review of NASEMโ€™s own process run by NASEM insiders fails that test before it even starts.

Second, NASEM needs to say, publicly and in advance, exactly what itโ€™s asking the reviewers to do. What is the scope, the timeline, and the specific questions it wants answered? Without this information, the public has no way to judge whether the final report actually answered anything.

Third, the reviewers themselves have to be named publicly, and none of them can have ties to climate litigation, on either side. That should be an easy bar to clear. If NASEM canโ€™t clear it, that tells you everything.

Fourth, the review has to actually grapple with the specific allegations Roger Pielke Jr. and other legal scholars have raised about who really wrote the chapter and how. NASEM brushed these allegations aside for months. Dodging them again would say everything about how seriously NASEM is taking this.

Fifth, NASEM should commit before the review even starts to specific consequences for whatever it finds, whether thatโ€™s retraction, revision, or reinstatement of the chapter. Once the review is done, NASEM should publish its response to every finding, item by item, in public, along with a concrete timeline for fixing whateverโ€™s broken. Thatโ€™s the same level of disclosure Congress already requires of other NASEM committees whose advice federal agencies rely on, so why shouldnโ€™t the same apply here?

You could call this activism, lawfare, dirty politics, or even a crusade to supposedly save the planet. The one thing you canโ€™t call it is honest, unbiased science. And if NASEM canโ€™t live up to its own name and commit to serious reforms, then it no longer deserves public trust or public funds. Letโ€™s end the games and let real science trump politics once and for all.

This article originally appeared at Real Clear Energy

Sunโ€™s Biggest Sunspots Had Superflare Potential, New Study Finds

Researchers from the Max Planck Institute for Solar System Research (MPS) and the University of Colorado have found new evidence that the Sunโ€™s largest historical sunspots could, in rare cases, produce superflares.

Solar flare energy scaling relates observable properties of active regions (ARs), sunspots, and flare ribbons to the total energy released during a flare. The recent Krivova et al. (2026) study uses an empirical chain of relations grounded in modern SDO observations to estimate upper limits for the largest historical sunspots.

A vibrant depiction of the sun, showcasing its fiery surface with solar flares erupting into space against a dark starry background.
AI generated by Grok

Researchers from the Max Planck Institute for Solar System Research (MPS) and the University of Colorado have found new evidence that the Sunโ€™s largest historical sunspots could, in rare cases, produce superflares.

The study, led by Natalie Krivova and published on 10 September 2026 in Philosophical Transactions of the Royal Society A (arXiv:2603.09474), focuses on empirical upper limits for solar flare energies.

The team analyzed data from NASAโ€™s Solar Dynamics Observatory (SDO) on more than 300 of the strongest flares observed between 2010 and 2016. They related flare energy (via flare-ribbon areas as a proxy for magnetic reconnection) to the size of the associated active regions.

They then extrapolated the upper- envelope statistical relations (focusing on the extreme tail of the distribution) to historical sunspot records, which have been systematically tracked for centuries.

The standout case is the Great Sunspot of April 1947 (Active Region 14886), one of the largest on record. It covered roughly 0.6% of the visible solar disk (maximum corrected area ~6,100- 6,132 millionths of the solar hemisphere), with a diameter about 40 times that of Earth. No superflare occurred then.

This builds on a 2024 MPS- led study (published in Science) of ~56,450 Sun- like stars observed by Kepler.

That work found superflares occur roughly once per century on such stars, far more frequently than earlier estimates.

The new results indicate the Sun is, in principle, โ€œsuperflare- capableโ€ because it can form sufficiently large and complex active regions/sunspots. Extreme events would still be rare, and the relationship between the largest flares, coronal mass ejections, and extreme solar particle events (inferred from cosmogenic isotopes) is not one- to- one.

No superflare has been directly observed on the modern Sun, and whether one has ever occurred remains an open question. The work strengthens the case that such events are physically plausible on the basis of observed solar structures and stellar statistics, with potential relevance for extreme space weather risks to technology and infrastructure.

The Carrington Event (also called the Carrington Storm or solar storm of 1859) remains the most intense geomagnetic storm in recorded history. It peaked on 1- 2 September 1859 during solar cycle 10 and is named after British astronomer Richard Carrington, who made the first observation of a solar flare associated with it.

The flare originated in a large sunspot group. Modern estimates of its maximum corrected area range from roughly 2,300- 3,500 millionths of the solar hemisphere (msh), with some reconstructions adopting ~3,100 msh as a conservative value. This places it among the larger historical active regions, though smaller than the record 1947 Great Sunspot (~6,100 msh).

Late August 1859: A large, complex sunspot group was visible on the Sun. Auroral activity and magnetic disturbances began around 28- 29 August, indicating earlier coronal mass ejections (CMEs) from the same region.

1 September 1859, ~11:18 GMT: Richard Carrington (and independently Richard Hodgson) observed a brilliant white- light flare lasting about 5 minutes while sketching the sunspot group. Carrington described โ€œtwo patches of intensely bright and white light.โ€ Magnetometers simultaneously recorded a โ€œcrochetโ€ (solar flare effect) caused by enhanced ionospheric ionization.

~17- 18 hours later (early 2 September): A fast CME arrived at Earth, triggering the main geomagnetic storm. The short transit time implies an unusually high speed (roughly 2,000 and more km/s).

The flare originated in a large sunspot group. Modern estimates of its maximum corrected area range from roughly 2,300- 3,500 millionths of the solar hemisphere (msh), with some reconstructions adopting ~3,100 msh as a conservative value. This places it among the larger historical active regions, though smaller than the record 1947 Great Sunspot (~6,100 msh).

Flare magnitude estimates (modern GOES soft X- ray scale, revised) typically fall in the range X45- X146, with many studies centering around ~X45. Bolometric (total radiated) energy estimates are on the order of a few ร—1032\times 10^{32} erg, with some approaching โˆผ1033\sim 10^{33}erg depending on conversion factors from soft X- ray class. Recent analyses of Carringtonโ€™s original drawings have suggested even higher values in some scenarios (e.g., ~X80 range), though uncertainties remain large.

Auroras: Extremely bright and widespread. They were visible at unusually low geomagnetic latitudes, down to ~18- 25ยฐ (Caribbean, Central America, Hawaii, Colombia, and possibly lower). People in the northeastern United States could read newspapers by auroral light; gold miners in the Rocky Mountains woke and began preparing breakfast, thinking dawn had arrived. Displays lasted many hours and included red, green, and other colors.

Geomagnetic storm intensity: Estimates of the stormโ€™s strength (Dst index) range widely from about -800 nT to as low as -1,750 nT or lower in early analyses (based partly on the Colaba, India magnetogram). More recent re- evaluations often place it around -900 nT or somewhat stronger, still far exceeding modern extreme events (e.g., March 1989 Quebec storm ~โ€“589 nT). Rapid field changes induced strong geoelectric fields.

Telegraph systems: Widespread disruption across Europe and North America. Operators reported electric shocks, sparks, and fires at stations. In some cases (notably the Boston- Portland line), operators disconnected batteries and continued transmitting messages using only the currents induced by the storm, the so- called โ€œauroral currentโ€ or โ€œcelestial power.โ€

The Carrington Event is the benchmark for extreme space weather. A comparable event today could severely disrupt satellites, GPS, power grids, and communications, with potential economic costs in the hundreds of billions to trillions of dollars (depending on the region and duration of outages).

It is often treated as a โ€œ1- in- 100 to 1- in-500 yearโ€ (or rarer) event, though related extreme solar particle events inferred from cosmogenic isotopes (e.g., AD 774/775) indicate that even stronger particle events have occurred over millennia.

In the context of the recent Krivova et al. (2026) study, the Carrington active regionโ€™s size yields estimated flare energies consistent with independent historical reconstructions (typically ~1ร—10331 \times 10^{33} erg under upper envelope scalings, with higher outliers possible), reinforcing that it ranks among the most energetic flares in the observational record while remaining below true stellar superflare energies (>1034>10^{34}erg).

The event also marks the birth of solarโ€“ terrestrial physics: Carrington cautiously noted the coincidence between the flare and the subsequent magnetic storm, establishing the first clear observational link.

_____________________________________________________________________________________

Here are the confirmed publication details for the two related papers from the Max Planck Institute for Solar System Research (MPS) and collaborators, both appearing in the same 2026 issue of Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences:

Natalie Krivova et al., โ€œEmpirical flare energy limits for the largest historical sunspotsโ€

This is the main empirical study discussed previously. It uses SDO/RibbonDB flare data (2010- 2016) to derive upper- envelope scaling relations between active-region/sunspot size and flare energy, then extrapolates to the largest historical sunspots (especially the April 1947 Great Sunspot).

It concludes that such regions could, in rare extreme cases, reach bolometric energies of a few ร—1034\times 10^{34}erg, overlapping the lower end of the stellar superflare regime.

Published:  Philosophical Transactions of the Royal Society A Mathematical, Physical and Engineering Sciences (2026)

DOI: 10.1098/rsta.2025.0290

Valeriy Vasilyev et al., โ€œLinking solar magnetism, extreme solar particle events and stellar superflaresโ€

This is a complementary review/synthesis paper. It discusses the connections (and differences) between extreme solar particle events (ESPEs, inferred from cosmogenic isotopes), solar magnetic activity, and stellar superflares observed on Sun- like stars. It notes that while both ESPEs and superflares involve extreme magnetic energy release, the relationship is not one- to- one.

Published:  Philosophical Transactions of the Royal Society A Mathematical, Physical and Engineering Sciences (2026)

DOI: 10.1098/rsta.2025.0261

These two papers were highlighted together in the Max Planck Society press release of 10 September 2026 (โ€œSonne: Neuer Hinweis auf Superflaresโ€ / โ€œSun: New Evidence of Superflaresโ€).

The Krivova paper provides the new empirical evidence that the Sunโ€™s largest recorded sunspots have the potential to power superflare -level energies, while the Vasilyev paper places that finding in the broader context of solar- stellar comparisons and extreme particle events.

Environmental Priorities vs. โ€˜Climate Changeโ€™

Classic articles are worth remembering.

One in the environmental field was a prioritization of environmental issues back in 2020 by Bjorn Lomborg, โ€œWelfare in the 21st century: Increasing development, reducing inequality, the impact of climate change, and the cost of climate policiesโ€œ

Illustration contrasting real environmental priorities with climate change obsession, featuring images of healthy ecosystems, clean air, and community initiatives on one side, and a critique of climate change discussions on the other.

From Master Resource

By Robert Bradley Jr.

Classic articles are worth remembering. One in the environmental field was a prioritization of environmental issues back in 2020 by Bjorn Lomborg, โ€œWelfare in the 21st century: Increasing development, reducing inequality, the impact of climate change, and the cost of climate policiesโ€œ

โ€œWhat is the worldโ€™s deadliest environmental problem?,โ€ asks Bjorn Lomborg. The answer:

Not climate. Outdoor and indoor air pollution. Letโ€™s not get so scared about climate that we forget the much bigger problems.

Read more in my peer-reviewed article:ย https://sciencedirect.com/โ€ฆ/article/pii/S0040162520304157.

Bar chart displaying deaths per year (in millions) caused by various environmental issues in 2017, including outdoor air pollution, indoor air pollution, unsafe water, lead, unsafe sanitation, handwashing, ozone, global warming, and radon.

This result explains why today, climate alarm is just not resonating with the public to the chagrin of the alarmists. Bill McKibben faults the New York Times and Democrats for throwing in the political towel. โ€œIโ€™m saddened to see how little our representatives in DC seem to really care, even the Democratic ones,โ€ he begins:

Too many Democratic leaders are feeling comfortable waving off climate concerns, because of a feeling that it might be a political problem for them. That was exemplified this morning in the New York Times when center-right pundit Matt Yglesias issued a strident call for liberals to โ€˜support Americaโ€™s oil and gas industryโ€™.

So is the voting public dumb, miscalculating their own self-interest? Or are the alarmists fooling themselves? This is a question that not only Bill McKibben but also Joe Romm and many others need to ask themselves as the mitigation failures mount, leaving adaptation as the one viable alternative.