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Climate scientists must fear sounding like a broken record when discussing new record temperatures yearly. But once again, last year was the hottest one ever recorded, according to a new study by NASA scientists.

Anyone paying close attention to climate news would not be surprised. From June 2023 through August 2024, every consecutive month broke a new monthly temperature record. That is 15 straight months of consistently high temperatures. 

Such a streak directly translates into the year’s overall temperature, but just how bad was it? The Paris Agreement on climate change, signed by 195 countries and the European Union, attempts to limit the global rise in temperatures to 1.5? over a baseline temperature from the middle of last century (1951-1980). 2024 was already 1.28? above it. 

That’s not a great start, but the data gets even more dire for the climate-conscious. Temperatures in 2024 were already 1.47? above a baseline of temperatures from 1850-1900, a time before the industrial revolution, or automobile transportation, had taken off. Gavin Schmidt, director of NASA’s Goddard Institute for Space Studies, says, “That’s halfway to Pliocene-level warmth in just 150 years.”, referring to a geological period where a baseline temperature of just 1.5? above the Earth’s 2024 average resulted in sea levels that were tens of meters higher than total.

Such a sea level rise would devastate population centers home to literally billions of people and have such a dramatic effect on sea and wildlife that it’d be hard to predict the consequences. But it’s not like any of this information is new—it’s just worth reinforcing.

Even with reinforcement, more action is needed to solve the problem. The last ten years have been the warmest on record. While there is some variability between years, the trend in warming temperatures is obvious. Despite that, in 2022 and 2023, there were record releases of carbon dioxide from fossil fuels.

Even 12 years ago, Fraser and Pamela were discussing climate change and what it meant for the planet.

Additional effects could have impacted such a hot year in 2024. A NASA press release mentions everything from El Niño to volcanoes in Tonga to improved sulfur dioxide emissions from cargo ships. All undoubtedly impact the climate, but the contribution of each is difficult to tease out.

NASA’s global temperature assessment is based on data from thousands of weather stations scattered throughout the globe, both on land and sea. The same data was analyzed by other organizations, such as the US’s National Oceanic and Atmospheric Administration, Berkeley Earth, the Hadley Centre, and Copernicus Climate Services. Each used slightly different methodologies and models to determine the Earth’s temperature last year. Still, each showed a trend toward hotter temperatures – which most scientists take as unambiguous proof that the planet is getting hotter.

However, many naysayers still can’t see the forest for the trees, as a nasty cold snap could convince them of the illusion of “global warming” in general. However, the world’s overall temperature shift is getting drastic enough that local areas are literally starting to feel the heat. Schmidt said, “When changes happen in the climate, you see it first in the global mean, then you see it at the continental scale, and then at the regional scale. Now we’re seeing it at the local level.”

The fires currently threatening NASA’s Jet Propulsion Laboratory in Pasadena are just one symptom of the ongoing environmental challenges facing the world. This NASA report is just the most recent in a long line of reports that all point to the same conclusion—the world is getting warmer, and we humans are likely the ones causing it. 

Learn More:
NASA – Temperatures Rising: NASA Confirms 2024 Warmest Year on Record
UT – NASA Confirms that 2023 was the Hottest Year on Record
UT – NASA Confirms That 2023 was the Hottest Summer on Record
UT – Global Temperatures Continue to Rise

Lead Image:
This map of Earth in 2024 shows global surface temperature anomalies, or how much warmer or cooler each region of the planet was compared to the average from 1951 to 1980. Normal temperatures are shown in white, higher-than-normal temperatures in red and orange, and lower-than-normal temperatures in blue. An animated version of this map shows global temperature anomalies changing over time, dating back to 1880. Download this visualization from NASA Goddard’s Scientific Visualization Studio: https://svs.gsfc.nasa.gov/5450.
Credit: NASA’s Scientific Visualization Studio

The post It’s Official, 2024 Was the Hottest Year on Record appeared first on Universe Today.

Carbon-rich cosmic dust comes from different sources and spreads out into space, where it’s necessary for life and for the formation of rocky planets like ours. When astronomers aim their telescopes at objects in the sky, they often have to contend with this cosmic dust that obscures their targets and confounds their observations.

One reason the JWST was built is to see through some of this dust with its infrared vision and unlock new insights into astrophysical processes. In new work, the JWST was tasked with observing the dust itself.

The Wolf–Rayet binary WR 140 is about 5,000 light-years away in the constellation Cygnus. In 2022, researchers published results in Nature Astronomy revealing details about the binary star. The results showed that the stellar winds from both stars regularly collide, producing rings of carbon-rich dust that expand outward from the stars.

“We are used to thinking about events in space taking place slowly, over millions or billions of years. In this system, the observatory is showing that the dust shells are expanding from one year to the next.”

Jennifer Hoffman, co-author, University of Denver

“Massive colliding-wind binaries that host a Wolf–Rayet (WR) star present a potentially important source of dust and chemical enrichment in the interstellar medium,” the authors wrote, noting that the dust’s chemical composition and how it survives are still not understood. “The carbon-rich Wolf–Rayet binary WR 140 presents an ideal astrophysical laboratory for investigating these questions, given its well-defined orbital period and predictable dust-formation episodes every 7.93?years around periastron passage,” the authors explained in their research.

The environment near these stars when they’re close to one another is chaotic, even hostile. The winds from these evolved stars are chemically rich, and when the stronger wind from the WR star collides with the wind from the OB star, the gas is compressed, and dust is produced. Since the dust is only produced at periastron, the dust forms discrete rings. “Galactic colliding-wind WC (Wolf-Rayet stars of the carbon sequence) binaries with resolvable circumstellar dust nebulae, therefore, provide important laboratories to study this dust-formation process, where observations over the past few decades have demonstrated how dust formation is regulated by the orbit of the binary system,” the authors of the 2022 paper explain.

The pair of massive stars, one a Wolf-Rayet and one an OB star, orbit one another and reach periastron every 7.93 years. That’s when the powerful stellar winds from both stars collide. Astronomers think that evolved Wolf-Rayet stars and their colliding winds might be responsible for some of the first carbonaceous dust grains and organic material in the Universe.

The JWST captured the original 2022 images about 5.5 years after the last periastron in 2016. Now, about 14 months after the JWST’s initial look at WR 140, the space telescope has taken another long look at the interacting binary and its concentric rings of expanding carbon-rich dust. The images show how much the rings have expanded in less than two years time.

“The telescope confirmed that these dust shells are real, and its data also showed that the dust shells are moving outward at consistent velocities, revealing visible changes over incredibly short periods of time,” said Emma Lieb, the lead author of the new paper and a doctoral student at the University of Denver in Colorado.

Compare the two mid-infrared images taken by the James Webb Space Telescope of Wolf-Rayet 140, a system of dust shells ejected by two massive stars that are in an elongated orbit. In the top right of the first two images, two triangles are matched up to show how much the rings have moved in 14 months. The dust is moving away from the stars at more than 2,600 km per second, about 1% of the speed of light. The rings of carbon-rich dust are created for a few months every eight years. Image Credit: NASA, ESA, CSA, STScI, E. Lieb (University of Denver), R. Lau (NSF NOIRLab), J. Hoffman (University of Denver)

It’s relatively rare to see astronomical objects exhibit change on short timescales like this. For only 14 months, every eight years, the stellar winds collide and produce the visible carbon-rich dust rings. While WR binaries are known to produce carbon-rich dust, most pairs aren’t this active and their periastrons are much further apart in time.

“We are used to thinking about events in space taking place slowly, over millions or billions of years,” added Jennifer Hoffman, a co-author and a professor at the University of Denver. “In this system, the observatory is showing that the dust shells are expanding from one year to the next.”

“Seeing the real-time movement of these shells between Webb’s observations that were taken only 13 months apart is truly remarkable,” said Olivia Jones, a co-author at the UK Astronomy Technology Centre, Edinburgh. “These new results are giving us a first glimpse of the potential role of such massive binaries as factories of dust in the Universe.”

Astronomers have spotted other WC stars producing dust rings. However, WR 140 exceeds them all. “The extent of these distant circumstellar shells detected around WR 140 exceeds that of all other known dust-forming WC systems by factors of 4 or greater,” the authors of the 2022 paper explain.

The stars follow wide, elongated orbits, and when their winds collide every eight years, they produce carbon-rich dust for several months. The JWST’s powerful MIRI imaged dust rings that date back more than 130 years. Shells older than that have dissipated into interstellar space and are no longer coherent and visible. Some of that material may have already been taken up in star formation.

Thanks to MIRI, the researchers learned that WR 140 will likely generate tens of thousands of dust shells over hundreds of thousands of years.

“Mid-infrared observations are absolutely crucial for this analysis, since the dust in this system is fairly cool. Near-infrared and visible-light observations would only show the shells that are closest to the star,” explained Ryan Lau, a co-author and astronomer at NSF NOIRLab in Tucson, Arizona. Lau led the initial research on this system in 2022. “With these incredible new details, the telescope is also allowing us to study exactly when the stars are forming dust — almost to the day.”

These JWST images don’t show it, but not all of the dust is in the form of rings. Some of it is in clouds larger than our entire Solar System. Some of it floats freely as individual dust particles, each one only one-hundredth the width of a human hair. In all cases, the dust is carbon-rich and moving at the same speed.

One estimate says that the rings are about 1.4 trillion km apart. For comparison, if our Sun were creating these shells, one shell would be about five percent of the distance to Alpha Centauri, our nearest neighbour, before the next shell was created.

Eventually, the creation of carbon-rich dust shells will cease. Most WR stars end their lives as supernovae, with some possibly collapsing directly into black holes.

But that’s in the distant future. In humanity’s direct future, WR 140 will keep producing these carbon-rich dust shells, and the JWST will keep watching this natural laboratory to see how it all happens.

The post The Webb Shows Us Where Cosmic Dust Comes From appeared first on Universe Today.

A huge number of ultracold atoms have been corralled into a grid that could form the basis of the next largest quantum computer

Jupiter’s clouds aren’t what we thought they were. Planetary atmosphere experts have studied them for many years, uncovering new and puzzling mysteries. Recently, several researchers banded together to solve a long-standing mystery about those clouds. It turns out they aren’t made of ammonia ice, which is what everyone has thought for years. Instead, they seem to be largely a mix of smog and ammonium hydrosulfide. That compound forms in the atmosphere as hydrogen sulfide gas passes through ammonia.

Most of us are familiar with the Jovian clouds and know that ammonia and water are involved in their formation. There’s precipitation, meaning that ammonia and other substances “rain out.” Then, they evaporate. Most of the clouds we do see are thought to be mainly ammonia ice, contaminated with other materials that lend color to the clouds. Ammonia is an important “tracer” of activity in Jupiter’s atmosphere and scientists have studied its presence for years. Most of those measurements come from spacecraft instruments and large ground-based telescopes outfitted with special filters and spectroscopes. Even those observations, however, are limited when it comes to determining their positions in the atmosphere. Also, temporal coverage is limited.

Getting observation time to track the presence of ammonia, and there are only so many spacecraft to go around. Plus, the methods for analyzing the observations are complex and time-consuming. What if there was a quick and cost-effective way to get continual observations of the Jovian clouds? Could smaller telescopes used by amateur astronomers be effective enough to chart variations in the amounts of ammonia in and above Jupiter’s clouds over time? If so, that would fill in a huge gap in Jupiter atmospheric observations.

Measuring Those Clouds

The saga of the Jovian clouds began when Dr. Steven Hill, a space weather forecasting expert, tried a fresh approach and made backyard observations of the gas giant’s clouds in 2020-2021 and 2022-2023. He was able to compare images that show absorption in the atmosphere due to ammonia and methane gases. He also determined variations in the amount of ammonia in and above the cloud tops.

With time on big observatory scopes at such a premium, Hill used a 0.28-meter Celestron Schmidt-Cassegrain telescope, outfitted with a ZWO ASI120MM CMOS camera. He used a 647-nm ammonia band filter first. Later on he applied a 619-nm methane band filter. The idea was to detect individual ammonia abundance features. “I always like to push my observations to see what physical measurements I can make with modest, commercial equipment,” said Hill. “The hope is that I can find new ways for amateurs to make useful contributions to professional work. But I certainly did not expect an outcome as productive as this project has been!”

Applying Hill’s Approach to Jupiter’s Clouds

It turns out Hill’s technique is easier and less expensive than the more complex observational and statistical methods scientists use to map clouds. It can be used in professional research to zero in on specific regions of the atmosphere. The approach also gives citizen scientists with backyard-type telescopes a way to track ammonia and cloud-top pressure variations across features in Jupiter’s atmosphere. That includes Jupiter’s cloud bands, its fast-moving small storms, and even the larger features such as the Great Red Spot.

Planetary atmosphere expert Professor Patrick Irwin at the University of Oxford in England, who co-wrote a paper with Hill about the observations, emphasized the advantage of doing such observations. “I am astonished that such a simple method is able to probe so deep in the atmosphere and demonstrate so clearly that the main clouds cannot be pure ammonia ice,” he said. “These results show that an innovative amateur using a modern camera and special filters can open a new window on Jupiter’s atmosphere and contribute to understanding the nature of Jupiter’s long-mysterious clouds and how the atmosphere circulates.”

Insights into Jupiter’s Clouds

Hill’s initial results showed that the clouds he studied lay in a region of Jupiter’s warm atmosphere that doesn’t allow ammonia ice to exist. In their follow-up study, Irwin and his colleagues applied Hill’s method to observations using the Multi Unit Spectroscopic Explorer on the Very Large Telescope in Chile. Doing spectroscopy allows scientists to measure the visible light fingerprints of the gases in the Jovian atmosphere and chart the distribution of ammonia and the height of its clouds. They also simulated how light interacts with those gases and clouds using a computer model.

Projected variations of ammonia abundance in Jupiter’s clouds, as well as cloud-top pressure near the Great Red Spot and the North Equatorial Dark features. These were made following Hill’s methodology. Courtesy Irwin, et al./JGR.

It turns out that the Jovian clouds observed through Hill’s backyard telescope had to be much deeper than previously thought. They lie in an atmospheric region with higher pressures and higher temperatures. That means the region is too warm to allow ammonia to condense. Chemical reactions created by sunlight’s effect on the gases are very active in Jupiter’s atmosphere. In small regions, where convection (heat transport from one region to another) is especially strong, the updrafts may be fast enough to form fresh ammonia ice. Such regions do exist and have been spotted by spacecraft over the years.

Irwin’s team suggests that when moist, ammonia-rich air gets raised upwards, ammonia gets destroyed. It could also be mixed with photochemical products faster than ammonia ice can form. That means the main cloud deck may actually be composed of ammonium hydrosulphide mixed with photochemical, smoggy products. That’s what produces the red and brown colors we see in Jupiter images. And, this method also works for observations of ammonia clouds in Saturn’s atmosphere. Further work should help determine if the same photochemical processes exist there.

For More Information

Citizen Science Reveals Insight into Jupiter
Clouds and Ammonia in the Atmospheres of Jupiter and Saturn Determined From a Band-Depth Analysis of VLT/MUSE Observations
Spatial Variations of Jovian Tropospheric Ammonia via Ground-Based Imaging

The post Jupiter’s Clouds Contain Smoggy Ammonium Hydrosulphide, Not Ammonia Ice appeared first on Universe Today.

There is a gravitational monster at the heart of our galaxy. Known as Sagittarius A*, it is a supermassive black hole with a mass of more than four million Suns. Long-term observations of the stars closely orbiting Sag A* place it at about 4.3 solar masses, give or take 100,000 or so. Observations of light near its horizon by the Event Horizon Telescope pin the mass down to 4.297 solar masses, give or take about 10,000. Those results are astoundingly precise given how difficult the mass is to measure, but suppose we could determine the mass of our galaxy’s black hole to within a single solar mass. That might be possible with gravitational wave astronomy.

Gravitational wave astronomy is still in its infancy. Presently, our gravitational wave observatories are only sensitive enough to detect the mergers of stellar-mass black holes and neutron stars within the Milky Way. We aren’t able to detect the mergers of supermassive black holes, nor the gravitational waves when a star is consumed by a supermassive black hole. But in the not-too-distant future, we will have space-based gravitational observatories such as LISA. They will be orders of magnitude more sensitive than what we currently have. And as a recent study shows, these new observatories should be sensitive enough to give us ultra-precise measurements of a black hole’s mass and rotation.

The idea behind this work is to focus on brown dwarfs. These objects straddle the mass range between planets and stars. Too large to be a planet, but too small to ignite core fusion like a star. Brown dwarfs have masses between 13 and 78 Jupiters and tend to be roughly the size of our Jovian neighbor. They aren’t quite as common as red dwarf stars, but should be fairly common within the center of our galaxy. That means some brown dwarfs should approach very close to Sag A*. Some of them will surely be gravitationally trapped by the black hole, slowly spiraling ever closer to its event horizon and oblivion. These are the ones the article focuses upon.

The gravitational chirp of a black hole merger. Credit: LIGO

Even the largest brown dwarfs have less than a hundredth the mass of the Sun. They are like specks of dust compared to Sag A*. This means the gravitational dance between a brown dwarf and black hole is an example of an extremely large mass-ratio inspiral (XMRI). The gravitational waves produced by this dance would be small perturbations of the black hole, and as such would be critically dependent on the precise mass and spin of the black hole.

To show just how precise those measurements might be, the team looked at the estimated statistics for brown dwarfs near Sag A* as well as the strength of their gravitational signals. They found that within a typical range of mass and orbital eccentricity, an observatory such as LISA should be able to observe about 20 inspiraling brown dwarfs. This would allow us to determine the mass of Sag A* to better than one part in a million and its spin to one part in 10,000. Those estimates are at the best-case end of what is likely, but it shows that as gravitational wave astronomy improves, we are going to make some outstanding observations.

Reference: Vázquez-Aceves, Verónica, Yiren Lin, and Alejandro Torres-Orjuela. “SgrA* spin and mass estimates through the detection of multiple extremely large mass-ratio inspirals.” arXiv preprint arXiv:2412.20738 (2024).

The post Here's How We Could Measure the Mass of SgrA* to Within One Solar Mass appeared first on Universe Today.

Diamond, often celebrated for its unmatched hardness and transparency, has emerged as an exceptional material for high-power electronics and next-generation quantum optics. Diamond can be engineered to be as electrically conductive as a metal, by introducing impurities such as the element boron. Researchers have now discovered another interesting property in diamonds with added boron, known as boron-doped diamonds. Their findings could pave the way for new types of biomedical and quantum optical devices -- faster, more efficient, and capable of processing information in ways that classical technologies cannot.

Diamond, often celebrated for its unmatched hardness and transparency, has emerged as an exceptional material for high-power electronics and next-generation quantum optics. Diamond can be engineered to be as electrically conductive as a metal, by introducing impurities such as the element boron. Researchers have now discovered another interesting property in diamonds with added boron, known as boron-doped diamonds. Their findings could pave the way for new types of biomedical and quantum optical devices -- faster, more efficient, and capable of processing information in ways that classical technologies cannot.

How can we ensure that life-saving drugs or genetic therapies reach their intended target cells without causing harmful side effects? Researchers have taken an important step to answer this question. They have developed a method that, for the first time, enables the precise detection of nanocarriers -- tiny transport vehicles -- throughout the entire mouse body at a single-cell level.

AI applications like ChatGPT are based on artificial neural networks that, in many respects, imitate the nerve cells in our brains. They are trained with vast quantities of data on high-performance computers, gobbling up massive amounts of energy in the process. Spiking neurons, which are much less energy-intensive, could be one solution to this problem. In the past, however, the normal techniques used to train them only worked with significant limitations. A recent study has now presented a possible new answer to this dilemma, potentially paving the way for new AI methods that are much more energy-efficient.

Carbon fiber-reinforced polymers (CFRPs) are used in the aerospace, automotive, and sports equipment industries. However, their recycling remains a major problem. In a recent study, researchers demonstrated a novel direct discharge electrical pulse method for the efficient, effective, and environmentally friendly separation of CFRPs to recover high-quality carbon fibers. This work is expected to pave the way for a more sustainable world.

Engineers have demonstrated a well-known quantum thought experiment in the real world. Their findings deliver a new and more robust way to perform quantum computations and they have important implications for error correction, one of the biggest obstacles standing between them and a working quantum computer.

Engineers have demonstrated a well-known quantum thought experiment in the real world. Their findings deliver a new and more robust way to perform quantum computations and they have important implications for error correction, one of the biggest obstacles standing between them and a working quantum computer.

Scientists are working to produce plant-based cheese with all the characteristics of real cheese, but with better health benefits. To create a cheesy product with the same texture as the real thing, they looked at a variety of physical attributes such as the melting, stretching, and oil-release upon grilling and heating and studied isolates from three proteins and how they interacted with the oil and with the starch matrix of the cheese alternative. Using a blend of sunflower and coconut oil decreased the saturated fat content of the cheese, creating a healthy and sustainable alternative to dairy cheeses and other plant-based cheeses.

Using advanced imaging techniques and precise microfluidics control to stretch out curly DNA into a straight line, new research demonstrates techniques for stretching and immobilizing DNA with minimum thermal fluctuation to enable detailed analysis. A team at Nagoya University experimented with ways to uncurl a DNA molecule using pressure applied to liquid flowing in a channel, with the pressure flow providing shear force that uncurled the DNA molecule. They found that controlling the flow velocity of the liquid helps fine-tune the shear force applied and allows precise adjustments of the stretch ratio of the DNA.

In recent years, more than 60 countries have developed strategies to stimulate the market ramp-up of hydrogen, particularly in the industrial sector. However, in 2023, less than ten percent of the originally announced green hydrogen production was realized, shows a new study. The main reason: hydrogen remains expensive and there is little willingness to pay the cost.

Are humans or machines better at recognizing speech? A new study shows that in noisy conditions, current automatic speech recognition (ASR) systems achieve remarkable accuracy and sometimes even surpass human performance. However, the systems need to be trained on an incredible amount of data, while humans acquire comparable skills in less time.

Water droplets under freezing conditions do not spontaneously detach from surfaces as they do at room temperature due to stronger droplet-surface interaction and lack of an energy transformation pathway. Since accumulated droplets or ice have to be removed manually or with mechanical equipment, which is costly and inefficient, preventing droplet accretion on surfaces is both scientifically intriguing and practically important. Researchers have now invented a ground-breaking self-powered mechanism of freezing droplet ejection that allows droplets to shoot themselves away, paving the way for cost-efficient and promising technological applications.

Regulars at this site will surely know of Robert Lang, physicist and origami master (art website here) whom I met a while back at the Kent Presents meetings. We became friendly and thereafter he contributed both wildlife photos and origami photos to this website (see all his posts here).

I was scheduled to meet Robert and his wife Diane today after the meetings and get a tour of their home and studio (she’s an author), thereafter then sallying forth to dinner. I hadn’t seen Robert in years, and had never met Diane, so I was looking forward to visiting their digs and to seeing some of the famous origami.

The problem was that their home and studio were in Altadena, California, near Los Angeles, so you can guess what I’m going to say next.

The home and studio are no more, taken down by wildfire. But I’ll let Robert tell the tale. His words, printed with permission, are indented below, and are supplemented with narrated videos (there are even subtitles).  This is the story of a family who lived through the fire but lost everything—except for the most important things: their lives and their animals.

Note that they actually lost two houses, as they had just bought another down the street.

Late Tuesday afternoon, we heard about the Eaton Fire, which started over in Eaton Canyon, about 2 miles to our east and several ridges over. The initial reports were that the wind was driving the fire to the east (away from us), so we were hopeful. At about 6:30 pm, though, my neighbor texted the neighborhood group that he saw a glow over the ridge to our east, and I headed up to my studio to see. By 7:30 pm I saw the fire crest that ridge and we received the “evacuate NOW” notice, so I threw as much as I could grab into my car and headed down, while my wife did the same from our home (with the dogs, tortoises, snake, and tarantula that live with us).

We spent the next few hours driving and parking to try to watch things from a distance. Surprisingly, the evacuation zone ended just to the west of our neighborhood, so after a while, I started making my way to the edge of the zone, staying out of the way of the many emergency vehicles, and presently found a spot from which I could walk to the edge of the canyon that separated me from my studio. From there, I could see the studio; I could also see that the entire multi-thousand-foot mountainside above it was in sheets of flame. The wind was blasting through the canyons, driving 50-foot plumes of flame and embers horizontally. About 1:30 am, I saw a flare-up right at the studio, and within about 10 minutes, it was engulfed. I also realized about that time that the fire would likely take down the telephone poles (and thus, potentially live wires) along my route, so I beat a hasty retreat to my car, and before long, the authorities announced that our area was now evacuation zone. We drove down the hill to Pasadena, found a quiet neighborhood out of the smoke (and, we hoped, the path of the fire), and spent a fitful rest of the night in our cars, awaiting what the morning would bring.

In the morning, my wife stayed with the animals and I drove up the hill to see what became of our house. Major roads were blocked off, but I wove through the neighborhoods, dodging still-burning homes (though the worst was past), downed wires, downed trees, and random debris, until I could get up to my neighborhood. It was a zone of total devastation: nearly all homes burned–and definitely mine. (Actually, both of ours; we had just moved down the street, so both our old house–just moved out of–and the new house–just moved into–were leveled.) I made my way up to my studio at the top of the hill, passing street after street of nothing but smoldering ruins. When I made it up, I found something incredible: the row of houses below my studio had entirely survived! I texted their owners the good news. I could see, though, that my studio had not; I parked (debris blocked my driveway), walked up, and surveyed the destruction, took a few videos and pictures for records, then high-tailed it down the hill.

Right now, the estimates are that 7000 structures were damaged or destroyed. It looks like about 2/3 of Altadena is gone. There’s a lot of snark on the internets about the rich people/celebrities/influencers in Pacific Palisades losing their houses. I haven’t seen similar snark about Altadena, which is a mixed-class, mixed-race community. There are turn-of-the-century buildings, craftsman houses, bungalows, tiny starter homes, and yes, a few mansions left over from the days when it was the summer playground of the rich. My wife grew up here; her father built their house himself in the 40s after clearing the orange groves from the parcel he bought. On the main drag downtown, the local hardware store was where you ran into your neighbors; Fox’s Restaurant had been a local landmark since 1955. All that is gone.

Ironically, I had recently returned from a business trip to Dresden, Germany, which was (famously) fire-bombed and leveled in WWII. They rebuilt. So will we. But it will be a long road to recovery.

*****************

Here a Cal Fire map of fire damage. The damaged area covers about 2/3 of Altadena. My home and studio is in the top middle of the burned civilized area, just to the left of the vertical black bar on the map.

This map is an understatement; I know some of the areas shown in gray actually burned.

Here are a few of the videos Robert posted on his YouTube site:

Panorama of the fire from the studio:

View of the mountains from the house:

Views of the destroyed house:

Views of the destroyed studio:

From Robert:

Here’s one more image for you: house-by-house fire damage. I’ve annotated where my places were. Not much left of the neighborhood.

[The key to above]: red=burned, black = OK, amber=damaged, green=“affected” (whatever that means).

Distance-wise, the studio and the houses are about a half mile apart by road, less by walking (there’s a trail up the canyon). An easy walk, except for the elevation gain (studio is about 200’ higher in elevation), so I usually drove.

Click to enlarge:  Arrows: studio is at the top, the old house at lower center, and the new house at lower right.  I’m struck by the patchy locations of the houses that survived.

As you can tell from the narration, Robert appears remarkably calm about this, as he was in his email to me about the destruction, which was headed “change of plans.”  I would be wailing with grief! But Robert and I do have one thing in common: a compulsion to document. His is with words and videos, mine involves in putting them on this site.

Best of luck, Robert and Diane, and of course we’re all sorry for your loss.

A range of brainwave-reading devices and other gadgets aim to monitor our nervous systems and intervene to improve our well-being. Do they work?

Two companies, Firefly Aerospace and ispace, are aiming to make the second and third successful private landings on the moon - and both are launching on the same Falcon 9 rocket