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Astronomers discover first green star and the reddest star ever recorded

15 October 2026 at 15:26

Despite the name, the universe’s white dwarfs can glow in a wide range of colors—even green. For the first time, astronomers have spotted a star that appears green to the human eye, and the reddest ever recorded. These outlier stars help explain how certain white dwarf stars would shine in green, pink, cyan, yellow, and purple if we actually saw them up close in space. These colorful findings are described in a study recently published in the journal RAS Techniques and Instruments.

Looking for the ‘perfect radiator’

White dwarf stars are the dense remnants left behind after stars like our sun reach the end of their lifespan. For most stars, their color gives a hint to their temperature. Cooler stars appear orange, warm stars like our sun look white. The hottest glow pale blue, similar to how a blacksmith’s iron will go from red to orange to white hot. Astronomers believed that white dwarfs followed this same rule. They even earned their name after the earliest examples were surprisingly hot and glowed in a white/pale blue. 

“Most stars, including most white dwarfs, behave like ‘perfect radiators,’ so their colour is set almost entirely by temperature. But nobody had really looked into what else might be possible for white dwarfs,” Mark Hollands, a study co-author and astronomer at the University of Warwick in England, said in a statement. “It turns out these incredibly dense stars can produce colours nobody expected, and some of them genuinely surprised me.” 

According to the team, the key to these colors is density. The atmospheres surrounding the coolest white dwarfs can reach about the same density as water (roughly 1 gram per cubic centimeter). They are also millions of times denser than the sun’s photosphere, the lowest layer of its atmosphere. Under these higher density conditions, any trace elements present (carbon, calcium, sodium, etc.) interact with the surrounding dense helium plasma. As they interact with the plasma, they can absorb light across a wider spectrum of colors than they would at lower densities. This then shifts the star’s color away from the more typical orange, white, and blue.

Unfortunately, no white dwarf sky is close enough for its color to be seen directly. Instead, the team calculated their color from data astronomers routinely collect—a star’s spectrum. The spectrum is a “fingerprint” that’s produced when starlight splits apart by wavelength, similar to how a prism splits sunlight into a rainbow. Astronomers ran these spectra through a computer model of what colors human vision can see to check what color a star’s light would appear to our eyes. 

Color-accurate simulated images of white dwarfs. Top Left panels: Sirius B is the nearest white dwarf to the Solar System, with a hot hydrogen atmosphere, resulting in a pale blue colour. WDJ1147-7449 is instead among the coolest nearby white dwarfs, giving it a featureless spectrum and an orange appearance. Top Right panels: Convective envelopes in these cool white dwarfs have dredged up carbon from their cores into their dense helium-dominated atmospheres, forming diatomic carbon molecules that lead to various pink hues. Bottom panels: Accretion of rocky debris from the white dwarf planetary systems enriches their cool helium atmospheres with elements such as calcium, magnesium, and sodium. The varying amounts/compositions of accreted material and white dwarf temperatures allow for a diverse array of colours, including green. In reality all stars would be many millions of times brighter than what can be shown on-screen. Image: Mark Hollands/University of Warwick
Color-accurate simulated images of white dwarfs. Top Left panels: Sirius B is the nearest white dwarf to the Solar System, with a hot hydrogen atmosphere, resulting in a pale blue colour. WDJ1147-7449 is instead among the coolest nearby white dwarfs, giving it a featureless spectrum and an orange appearance. Top Right panels: Convective envelopes in these cool white dwarfs have dredged up carbon from their cores into their dense helium-dominated atmospheres, forming diatomic carbon molecules that lead to various pink hues. Bottom panels: Accretion of rocky debris from the white dwarf planetary systems enriches their cool helium atmospheres with elements such as calcium, magnesium, and sodium. The varying amounts/compositions of accreted material and white dwarf temperatures allow for a diverse array of colours, including green. In reality all stars would be many millions of times brighter than what can be shown on-screen. Image: Mark Hollands/University of Warwick

The first green and the reddest red

The team applied this method to several white dwarfs across the cosmos. They found that their colors fall into distinct groups linked to what makes up a star’s atmosphere. Carbon-rich white dwarfs generally appear pink or purple. Stars enriched with debris from busted asteroids and comets, the remains of old planetary systems, tend to be more yellow. Cooler white dwarfs with atmospheres of mixed hydrogen and helium show a more cyan or pale blue tinge. This cyan-pale blue is caused by hydrogen molecules colliding with helium atoms inside their ultra-dense atmospheres.  

The most striking example is WD J1330+6435. This star is about 7,232 degrees Fahrenheit (4,000 degrees Celsius) and around 284 light-years away from Earth. Over time, it has gathered rocky material from its planetary system. All of this extra material enriched its atmosphere with calcium, lithium, and sodium. The result—a chartreuse green appearance in the team’s models. As far as the researchers are aware, no other star (living or dead) has ever been credibly reported as green.

Enriched from above: The cool white dwarf WDJ1330+6435 has accreted sodium-rich rocky material from its planetary system into its atmosphere. The immense atmospheric density causes the sodium to absorb light over broad range of yellow, orange, and red wavelengths, giving the WDJ1330+6435 a ghostly green appearance. Image: Mark A Garlick/University of Warwick.
Enriched from above: The cool white dwarf WDJ1330+6435 has accreted sodium-rich rocky material from its planetary system into its atmosphere. The immense atmospheric density causes the sodium to absorb light over broad range of yellow, orange, and red wavelengths, giving the WDJ1330+6435 a ghostly green appearance. Image: Mark A Garlick/University of Warwick.

“The traces of sodium in the atmosphere of this white dwarf absorb the orange part of the spectrum, leaving behind a ghostly green glow,” added Hollands. “Imagine standing on a planet and looking up at a green star. It feels like something out of science fiction.” 

On the opposite end of the spectrum, the team identified what could be the reddest star ever recorded—WD J1011+2845. This white dwarf is only 48 light-years away from Earth, and has a deep convection zone. This zone is full of carbon that’s been lifted up from the star’s core to its surface. The carbon molecules then distort the star’s light so much that almost all of it is squeezed into wavelengths beyond 600 nanometres. This wavelength produces an unusual deep salmon-pink glow.

Enriched from below: The cool white dwarf WDJ0902+2010 has a deep convection zone within its helium dominated outer envelope. The convection zone has reached the white dwarf core, lifting interior carbon to the surface, and forming carbon molecules. These C2 molecules strongly absorb light across the optical range, including blue, green, and yellow wavelengths, resulting in WDJ0902+2010 appearing pink to the human eye. Image: Mark A. Garlick/University of Warwick.
Enriched from below: The cool white dwarf WDJ0902+2010 has a deep convection zone within its helium dominated outer envelope. The convection zone has reached the white dwarf core, lifting interior carbon to the surface, and forming carbon molecules. These C2 molecules strongly absorb light across the optical range, including blue, green, and yellow wavelengths, resulting in WDJ0902+2010 appearing pink to the human eye. Image: Mark A. Garlick/University of Warwick.

What are the odds?

The team also studied 151 white dwarfs located within about 65 light-years (20 parsecs) from Earth. Only five of these showed unusual colors, two yellow and three pink. This suggests that about 1 in 30 of the universe’s white dwarfs shine with an unusually colored light. 

The team then measured the color temperature of the remaining 146 white dwarfs. Color temperature is commonly used to describe light bulbs using degrees Kelvin—warm white at 3,000K, cool white at 6,000 K, etc. The median color temperature of the sample was approximately 6,800K, which our eyes perceive as white. This measurement corrects a common misconception that white dwarfs are typically blue. The hotter and bluer white dwarfs are mostly brighter, so they can be seen from further away and are over-represented in surveys that only look at a star’s brightness.

“One in thirty might not sound like a huge fraction, but across the entire population of white dwarfs in the Universe, that is still a lot of oddly coloured stars out there,” added study co-author and University of Warwick astronomer Boris Gänsicke. “Yet if we take the median across a representative population of white dwarfs, we found that the average white dwarf really is white.”

The post Astronomers discover first green star and the reddest star ever recorded appeared first on Popular Science.

The criminal behind Los Angeles’ Griffith Observatory

14 October 2026 at 13:57

Griffith Observatory is one of Los Angeles’s most iconic landmarks. Part of the city’s sprawling “urban wilderness,” Griffith Park, the free public science center boasts dozens of exhibits and displays, including one of the first planetariums in the United States and the most-viewed telescope in the world. 

But there’s a dark secret behind Griffith Observatory’s founding. It might never have been built if it weren’t for the desperation of its namesake, Griffith J. Griffith, a wealthy real estate magnate who had once been a pillar of his community. In 1906, when Griffith first proposed the observatory as a gift to the city, he was hoping to salvage his reputation after the shocking crime he had committed three years earlier: the attempted murder of his wife.

Who was Griffith J. Griffith?

Born in Wales, Griffith immigrated to the United States as a teenager in 1865, initially settling in Pennsylvania. A few years later he moved to San Francisco, where he worked as a business journalist covering the West Coast mining industry. Griffith then used his expert knowledge of mining to work as a consultant for mining companies, earning himself a fortune. 

In 1882, Griffith moved to the rapidly growing city of Los Angeles and purchased 4,000 acres of the Rancho Los Feliz land grant with an eye toward development. He rented out parcels of this land for various businesses, from homes and hotels to an ostrich farm. (Although the farm eventually failed, it proved a popular tourist attraction: Some of California’s first passenger railways were built to bring sightseers to the ostriches.)

Acquaintances described Griffith as “a roly-poly pompous little fellow” and “an egomaniac.” Known for his brash personality and humor, he dressed flamboyantly, favoring a gold-handled cane and a top hat. Griffith also called himself “Colonel,” despite having never served in the military. His grandiosity led to the mocking nickname, “the Prince of Wales.”

Mugshot of white man with mustache.
Acquaintances described Griffith as “a roly-poly pompous little fellow” and “an egomaniac.” Image: Public Domain

Griffith’s doomed marriage

By the mid-1880s, Griffith was a member of Los Angeles high society. He rubbed shoulders with fellow wealthy developers whose names are still visible on city maps, such as the Bixbys, the Sepúlvedas, and the Mesmers. 

While some of these families traced their lineages back to the colonial aristocrats of Mexico or New England, the Mesmers, like Griffith, were recent European immigrants, having come to the United States from Alsace, France. Griffith soon began courting 22-year-old Christina Mesmer, nicknamed Tina, who was considered one of the city’s most eligible young ladies. 

Not only did Tina have prominent parents, she had personally inherited a major property from a childless family friend in 1885. Known as “the Briswalter tract” after the previous owner, Andre Briswalter, it was 240 acres in a prime development area just south of downtown L.A. Worth at least 35 million dollars today, the land was used by Briswalter himself for fruit orchards, but now encompasses the neighborhood of Historic South-Central.

Griffith knew that the Briswalter land would be his if he married Tina Mesmer, and made no secret of his motives. Three weeks before they were to be married, Tina informed Griffith that she had transferred partial ownership of the property to her father. It is unknown if Tina performed this transfer willingly, but Griffith wrote to her of his fear that she had become her father’s “pawn.” In the same letter, Griffith threatened to call off the wedding unless he was made sole owner.

Wishing to avoid scandal, the Mesmers relented and the wedding proceeded in 1887. However, the rocky start to the marriage was an ill omen of things to come. In public, the two presented a harmonious image of a high society couple. In private, tensions plagued their marriage, including over religion (the Mesmers were Catholic, while Griffith was Protestant).

Black and white photograph of white woman from late 1800s
In 1887, Christina ‘Tina’ Mesmer, a young Los Angeles socialite, married Griffith. Image: Public Domain

At home, Griffith was paranoid and menacing. Despite publicly supporting the Temperance movement, he was secretly an alcoholic, and his drinking worsened his behavior. Griffith’s paranoia reached a fever pitch after a narrow brush with death in 1891. 

While the Griffiths were in a carriage on their way to the grave of Tina’s recently-deceased mother, someone fired a gun at them from another carriage, grazing Griffith’s head. The attacker, who fatally shot himself before he could be apprehended, turned out to be an investor from the failed ostrich farm, who had been ruined and owed Griffith back rent.

How the idea of Griffith Park first emerged

In 1896, despite his private troubles, Griffith was at the height of his power. Ever-ambitious, he sought a way to immortalize himself. He was also flush with cash, having sold off most of the Briswalter tract acquired from Tina, but still owed a tax debt that he hoped the city would forgive. That Christmas, the Griffiths donated more than 3,000 acres of Rancho Los Feliz to the city of Los Angeles for the formation of a public park, to be called, of course, Griffith Park. 

While Griffith spoke of wanting to give back to the community and create “a place of rest and relaxation for the masses,” generosity may not have been his only motive. Critics called the huge donation a tax scheme, and pointed out that Griffith could afford to part with the land. Not only did he have Tina’s fortune, he had already rented out the most profitable parts of the Rancho Los Feliz, and what remained was no good for purposes like farming.

Griffith shoots his wife Mrs. Tina Griffith

The more his influence grew, the more unstable Griffith became. According to Tina’s later testimony at Griffith’s trial, he pulled a gun on her for the first time in May 1903, when she threatened to leave him during an argument. “He is very proud and did not want the public to know” of their marital disputes, she said. 

A few months later, the Griffiths stayed at the Hotel Arcadia in Santa Monica with their only child, 15 year-old Vandell. Tina hoped that a family vacation would calm Griffith’s nerves, but Griffith was on edge. He repeatedly asked servers in the hotel restaurant to change his food and drink, believing it had been poisoned. 

On the last night of the trip, Vandell Griffith went to the beach with the hotel owner’s son, leaving his parents alone in the hotel room. While Tina was packing, Griffith approached her with a gun in his hand. He forced her to kneel and started asking her about the death of Andre Briswalter years earlier. 

Apparently, Griffith now suspected that the Mesmers had poisoned Briswalter, and planned to poison him next. Griffith then asked Tina if she had ever been unfaithful. She assured him that she had not, and that Briswalter’s death had been natural, but he fired off a bullet at point-blank range.

Tina Mesmer Griffith survives 

Tina leapt from the window and rolled to safety, breaking her shoulder in the fall. Hotel staff soon found her and took her to a doctor. A surgeon who attended her injuries later reported that “if the bullet had struck Mrs. Griffith one-sixteenth of an inch below where it did, it would have gone through the eye socket and into the brain.” 

Tina lost her right eye, and due to the risks of infection and blood loss, doctors were not sure whether she would survive. Miraculously, she did.

Police began searching for Griffith immediately, but it was three days before they found him at a nearby bar in the midst of an alcoholic bender. The subsequent trial became a massive media scandal. Tina took the witness stand wearing a veil and black glasses to hide her injuries. 

Screenshot of vintage Los Angeles newspaper.
A sketch published in The Los Angeles Times shows how Christina ‘Tina’ Mesmer wore a veil in the courtroom to conceal her injuries. Image: Public Domain

When she entered the courtroom, “she looked at [Griffith] casually as though he were someone she had never seen,” the Los Angeles Times reported, while Griffith remained motionless, listening intently. Tina testified for an hour before fainting from exhaustion, returning later that day for a second round of questioning. Only then did the extent of the Griffiths’ private problems become public knowledge.

The outcome of the trial

Griffith’s attorneys argued that he was not in his right mind; instead, his drinking had made him delusional, a case of “alcoholic insanity.” Griffith was fined and sentenced to just two years in prison. 

Tina was granted a divorce on grounds of cruelty, one of the few legal justifications for divorce in 1903. She also received a cash settlement and full custody of Vandell, but she was unable to receive half of the estate, as she had asked for. 

The couple’s properties had long been under Griffith’s name only, including what remained of Tina’s inheritance. As one of her lawyers told the Los Angeles Times, the law prevented her from obtaining “any approximation of what really should be hers.” However, Tina was left with enough to live on, and Griffith agreed to pay for Vandell’s future education as long as he didn’t attend a Catholic university.

The aftermath

After the trial, Tina moved in with her sister. Though she stepped away from city development, she devoted herself to Catholic charities and social events. She was apparently a big fan of whist, a four-player card game. She never remarried and continued to be known as “Mrs. Griffith” until her death in 1948 at the age of 86.

When Griffith emerged from San Quentin in December 1906, he appeared to be a changed man. He gave up drinking and devoted himself to the cause of prison reform, as well as improving facilities for visitors in the park that bore his name. He also came up with an idea for a second “Christmas gift” to rehabilitate himself in the eyes of the Los Angeles public: a free science center and an outdoor theater.

However, the city was now reluctant to associate with him. As one newspaper op-ed stated, Los Angeles was “neither so poor nor so lost to [a] sense of public decency that it can afford to accept this money.”

Griffith died of liver disease in 1919 without seeing this dream become reality, but he bequeathed the funds for the Observatory and the nearby Greek Theatre to the city in his will. The project would finally move forward more than ten years after his death. 

It was Griffith and Tina’s son, Vandell Griffith, who oversaw the construction of the Observatory as president of the Los Angeles Park Board. (Vandell would later become a city police commissioner, and was described in a 1951 newspaper as “a dead honest man.”) 

When the Griffith Observatory opened in 1935, it was an instant success, part of a new wave of interactive museums that made astronomy and other sciences accessible to the public. And it all goes back to a man who destroyed his own reputation. It’s a strange chapter in the history of Los Angeles, and a reminder that the legacies people leave can be complicated.

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