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This Giant Planet Survived the Death of its Star
All stars die eventually, including our Sun. Depending on the star, that can spell doom for planets. Massive stars die in cataclysmic explosions called supernovae, and their powerful blast waves can destroy any planets within range. If our Sun were massive enough to explode like this, it would mean an instantaneous end for Earth. But the Sun isn’t big enough.
Instead, the Sun’s end is more prosaic. As it runs out of fuel for fusion, it will gradually swell and cool, becoming a red giant. As it swells, it will engulf Mercury and Venus, but maybe not Earth. Astronomers aren’t certain, but Earth may survive the Sun’s swelling. If it does, it’ll face much different prospects. Earth will then orbit a white dwarf, for a time surrounded by a glorious nebula created by the Sun as it shed layers of gas. But that fate is uncertain, too.
Astronomers have found intact planets orbiting white dwarfs, showing that planets can survive the evolutionary shift of their stars. One of them is named WD 1856 b, where WD stands for white dwarf. It’s about 80 light years away, and TESS discovered it in 2019. The star it orbits is about 5.8 billion years old and half the mass of the Sun.
The planet is a giant with a radius about 10 times larger than Earth’s. It’s extremely close to its star, orbiting at about 0.02 astronomical units. It whips around the star rapidly, with an orbital period 60 times shorter than Mercury’s around the Sun.
Since its discovery, astronomers have wondered about it. To be in this orbit, the planet could have migrated inward after the star became a white dwarf. Otherwise, it would’ve been destroyed by engulfment when the star became a red giant.
This planet has led to questions about habitability. If planets can survive a star’s red giant phase, can they somehow be habitable? White dwarfs don’t generate heat by fusion, but they have remnant heat that can take trillions of years to dissipate, enough to power life on a nearby planet.
Scientists want to know how the planet survived in the first place, and new research in Nature examined its atmosphere for clues. It’s titled “Aerosols and hydrocarbons in the atmosphere of a white dwarf planet.” The lead author is Ryan MacDonald, a lecturer in extrasolar planets at the University of St. Andrews in Scotland.
“The planet is quite the oddball,” said lead author MacDonald in a press release. “It’s about the size of Jupiter, but the white dwarf it orbits is the size of Earth, so the planet is seven times larger than its star.”
Since it’s the size of Jupiter, this system could be a glimpse into the future of our Solar System. When the Sun becomes a red giant, it will engulf planets that are too close. But the fate of the more massive planets further from the Sun is unclear.
“We’re used to looking back in time when we use telescopes, but this is the first time we have been able to look forward to what might happen to the outer planets around the remnant of a Sun-like star. It’s like using a time machine to peer into the distant future of our Solar System,” added MacDonald.
“Several planet candidates have recently been identified orbiting white dwarfs, demonstrating that planets can survive the stellar post-main-sequence stage intact,” the authors write. “Little is known about the atmospheric composition of post-main-sequence planets, with the most evolved transiting planets with atmospheric detections so far orbiting subgiants.”
Some white dwarfs have debris disks made of material from the planets they destroyed when they were red giants. Astronomers think that planets can form in them, but have dismissed that possibility in this case. Image Credit: NASA/JPL-Caltech.
When a red giant star engulfs its closest planets, it can create a debris disk. Astronomers think it’s possible that explanets could form in this disk, but that’s not possible in this situation. The debris disks aren’t massive enough for a planet this massive to form.
That leaves only two explanations for WD 1856 b: it may have been engulfed by the star and somehow survived, coming out of the harrowing experience intact. Or it migrated inward without being engulfed. That inward migration didn’t have to be driven solely by the star itself. WD 1856 is actually a triple star system with two red dwarfs.
“The big question is how WD1856b ended up where it is today, and there are two theories,” said study co-author Christopher O’Connor of Northwestern’s Center for Interdisciplinary Exploration and Research in Astrophysics. “One is that the planet was swallowed by its host star as it was dying and managed to survive on the other side. The other is that the migration took place due to the gravitational effect of other objects in the system. The white dwarf is part of a triple star system, and the outer companion stars could have influenced WD1856b’s orbit.”
This work is based on observations of the planet’s atmosphere with the JWST. The researchers used the telescope to obtain transmission spectroscopy with the telescope’s NIRSpec instrument. They also determined the planet’s temperature. The results are vital clues to the planet’s history.
This is the atmospheric retrieval of the transmission spectrum of WD 1856 b from the JWST. It shows multiple CH4 absorption features and one tentative ethane feature. Image Credit: MacDonald et al. 2026 Nature.
The temperature is much higher than expected. While the expected planetary equilibrium temperature is about 160 Kelvin, the temperature as measured is between 390 and 412 K. So the planet is much hotter than it should be if it were heated only by starlight. These observations show that the planet survived the red giant phase, migrated inward and experienced heating. This can also explain the exoplanet’s tight orbit.
“On the basis of cooling models, these results indicate that WD 1856 b underwent a migration-related reheating event 3.0–5.5 Gyr into the white dwarf phase, consistent with post-main-sequence tidal evolution to the present-day 0.02-au circular orbit,” the authors write.
The JWST detected an abundance of methane in the giant planet’s atmosphere. This strongly suggests that it formed further away from the star and migrated inward. Image Credit: NASA, ESA, CSA, Joseph Olmsted (STScI)
The observations found hydrocarbons in the atmosphere, specifically methane (CH4), at about 7%. This is also evidence of the planet migrating inward after the star’s red giant phase. A 7% CH4 atmosphere is a carbon-rich atmosphere. For this much methane to be present, the planet’s H2 atmosphere had to be enriched by carbon. This strongly suggests that the planet formed beyond its system’s water and carbon monoxide ice lines, then migrated inward.
“Our findings have bearing on the long-term fate of our solar system,” O’Connor said. “In roughly five billion years, our Sun will die, and we don’t know precisely what will happen to the planets at that time. The fact that planets can survive into that final stage of the stellar life cycle really widens the range of possibilities for where and when habitable planets might exist in the universe.”
There’s much to learn about exoplanets and their fates as their stars age and leave the main sequence. While the JWST is known for examining the red-shifted light from ancient objects like the first galaxies, one of its science themes is planetary systems. It’s powerful spectrometry capabilities let it examine exoplanet atmspheres in detail, providing clues to their origins, and their fates.
“Our results provide a window into the ultimate fate of giant planets orbiting stars with masses similar to our Sun,” the authors write. “As WD 1856 b demonstrates, spectroscopy of planets orbiting white dwarfs offers a new opportunity to determine the fate of planetary systems after the death of their star,” they conclude.
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L.A. reaches deal on cost recovery for 2028 Olympics, amid warnings

A divided Los Angeles City Council finalized a deal with organizers of the 2028 Summer Olympic Games aimed at controlling the city’s costs during the global event, amid complaints that the protections don’t go far enough.
On a 10-4 vote, the council approved the Enhanced City Resources Master Agreement, which lays out the process for the city to seek reimbursement for the services it provides during the Games.
City Administrative Officer Matt Szabo said the agreement sets up additional financial safeguards, by allowing the city to tap a $270-million contingency fund set up by LA28, the privately run Olympic organizing committee, if outstanding costs remain.
Still, some on the council warned that taxpayers could wind up on the hook for $1 billion in police and other public safety costs if LA28 incurs serious losses.
“This fails to provide any safeguards for Los Angeles taxpayers and most assuredly risks the city’s fiscal stability,” Councilmember Monica Rodriguez said after voting against the agreement. Councilmembers Eunisses Hernandez, Ysabel Jurado and Nithya Raman, who is running against Mayor Karen Bass, also were opposed.
Critics of the Games have long voiced concern about the risks that surround the event.
If LA28 incurs massive financial losses, the city would cover the first $270 million. The state would absorb the next $270 million. After that, the city’s general fund, which pays for basic services, would cover any remaining shortfall.
The city’s negotiating team said L.A.’s political leaders committed the city roughly a decade ago to serve as a financial backstop for the Games, as part of the contract that made L.A. the host city.
“We are providing you today as many protections as we can, given the reality that if it is not financially successful, it does fall onto us,” Szabo said. “So there is nothing we could propose today or tomorrow or next year that would eliminate that risk.”
The council, in a flurry of votes, sidelined proposals from Councilmembers Imelda Padilla, Hernandez and Raman that were billed as a way to reduce the risk facing the city.
LA28 spokesperson Jacie Prieto Lopez, in a statement, said the newly approved agreement delivers on the committee’s commitment to “execute a safe, secure and fiscally responsible Games that benefit Los Angeles for decades to come.”
Under the terms approved by the council, LA28 would pay the city ahead of the Games for services that are ineligible for reimbursement from the federal government, such as street sweeping and deployment of traffic officers.
The terms around police protection are more complicated.
The city would first seek reimbursement from the federal government for law enforcement services, particularly in high-security zones, Szabo said. If the government fails to cover the cost of security in those areas, the city would seek all or a portion of LA28’s contingency funds to make up difference, he said.
Last year, President Trump signed the One Big Beautiful Bill Act, setting aside $1 billion for state and local governments for security, planning and other costs associated with the Games.
Some council members have voiced concerns that the federal government might not follow through on its commitment, or that only a fraction of those funds would make their way to L.A., one of several Southern California communities slated to host Olympic competitions.
In April, Rodriguez sent LA28 a letter warning the city’s public safety costs could easily blow past $1 billion if there is an emergency or major weather event.
City Controller Kenneth Mejia, in an interview, said he intends to use his office to look into LA28’s finances in the run-up to the Games. He also argued that the deal to secure the Olympics was a bad one from the beginning.
“We’re already locked into a huge financial liability. This was one of our big chances to throw in protections for the city and also provide that transparency,” said Mejia, who opposed the agreement.
If LA28 makes money on the Games, the organizing committee would be barred from distributing that surplus to any organization until it has covered its financial obligations to the city, according to the terms approved Wednesday by the council.
Szabo, appearing before the council, acknowledged that the city faces a financial risk. If LA28 does experience a financial loss, it first would tap its own $330-million contingency fund, he said.
After that, LA28 and the city would have access to a second, $270-million contingency fund set up to protect taxpayers, he said.
“Is that a likely scenario? We don’t believe so,” Szabo said. “Their reports thus far have suggested that they are meeting their targets on their sponsorships and on other revenues, and we want them to continue to hit their targets.”
Those arguments haven’t satisfied an array of activists, who urged the council to rewrite the agreement.
“LA28 has no incentive to keep the city from being forced into bankruptcy,” said Chris Tyler, spokesperson for Strategic Actions for a Just Economy, a nonprofit that advocates for low-income communities in L.A.
Under a deal reached in 2021, LA28 must reimburse the city for services that go beyond what would be provided on a normal day in key parts of the city, such as Exposition Park, the Sepulveda Basin and parts of downtown L.A.
The organizing committee is obligated to create a $270-million contingency fund that can be distributed as a surplus if the Games make money or cover any losses in the event of a shortfall.
The proposal approved Wednesday calls for the five-year-old agreement to be amended to ensure that those contingency funds can be used to cover the city’s costs in the event that other funds aren’t available.
The city and LA28 were supposed to have a draft agreement on the cost recovery process completed by October. A draft document did not surface until June.
City negotiators now head into another round of talks with LA28 on the precise level of services needed at the Convention Center, Venice Beach, Dodger Stadium and other locations. Those venue agreements must be completed in July 2027.
Under the terms approved Wednesday, the two sides must reach an accord on the cost of those additional services by October 2027.
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Trump Wants the M.M.R. Vaccine Split Into Three Separate Shots. Doctors Say It’s a Bad Idea.
President Trump is calling for immunizations for measles, mumps and rubella to be given in individual jabs in three different appointments instead of the standard combination shot.
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How to Find Lunar Ice? Moonquakes to the Rescue!
The surface of the Moon is a bleak and forbidding place that could be hiding a lot of water ice within the dusty landscape. However, most possible ice deposits don’t just stand out in an image. You need specialized mapping to find those deposits. So, scientists have devised another way to find the Moon’s frosty hidden reserves. They use seismic waves from moonquakes as locator beacons.
Geologists at the University of Maryland, Lawrence Berkeley National Laboratory, and the University of Hawai’i recently published a paper (cited below) that examines the role that seismic waves play in locating ice deposits on and in the Moon. Finding water ice is important because the users of future lunar laboratories and habitats will need a steady supply of water. In addition, ice can be used to create oxygen supplies and rocket fuels for getting around the Moon. It’s a far cheaper and more efficient source of water than bringing water and other supplies up from Earth.

A map of possible lunar water deposits around the south pole region of the Moon. Courtesy: Chandrayaan mission. Credit: ISRO.
How Did the Moon Get Water?
The origins of the lunar water caches remain something of a mystery, although the evidence points in a few directions. The most likely locations for substantial amounts of water are at the poles and other regions where some of the ice could have been delivered by comets or asteroids. There could be deposits in regions where volcanism transported water from inside the Moon to the surface, or via the solar wind or meteor showers. These bombard surface rocks, triggering chemical reactions that could release water molecules. The evidence for water is pretty substantial, based on studies of rocks brought back during the Apollo era, as well as studies made by such missions as the Chinese Chang’e 5 probe, the SOFIA project, and highly detailed images and impact modeling done by Chandrayaan scientists. It’s more likely that much of the proposed lunar water accumulated over millions or billions of years, rather than just one major delivery by a comet or asteroid impact.
Lunar water is likely some kind of briny mixture of materials from the Moon mixed with materials delivered by delivery of chondritic materials via impacts. It’s still possible that regions in the lunar interior could be warm enough to contain liquid water, although scientists need more data about the Moon’s core to prove that. Some analyses also suggest that some lunar water could date back to the time of the Moon’s formation during the impact between early Earth and a Mars-sized object. So, it’s clear that a better understanding of the nature of lunar water (as well as its locations) is in order.
These images show a very young lunar crater on the side of the moon that faces away from Earth, as viewed by NASA’s Moon Mineralogy Mapper on the Indian Space Research Organization’s Chandrayaan-1 spacecraft. On the left is an image showing brightness at shorter infrared wavelengths. On the right, the distribution of water-rich minerals (light blue) is shown around a small crater. Both water- and hydroxyl-rich materials were found to be associated with material ejected from the crater. Credits ISRO/NASA/JPL-Caltech/USGS/Brown Univ.
Future Uses of Lunar Ice
According to Nicholas Schmerr of the University of Maryland, the Artemis missions and others will rely on lunar ice deposits, no matter where they come from. “It’s crucial to identify any materials on the moon that an astronaut can make use of while they’re up there,” said Schmerr, who co-authored the team’s study. “Since they will be limited by the few resources they brought from Earth, anything they find on the moon will help them basically live off the land, especially for longer-term missions or outposts.”
Lunar ice also provides another avenue of planetary science research. Ice in the shadowed craters may well contain undisturbed deposits of ice from comets and other events from early solar system history. “The moon witnessed some of the most critical parts of the early solar system, including how water was delivered,” Schmerr said. “Studying the ice deposited there could reveal how water spread and ultimately how Earth’s oceans formed.”
Seismic Waves and Ice
Finding ice under the surface requires new thinking about how it can be located. The lunar surface is cold and dry. From studies here on Earth, scientists know that seismic waves behave differently depending on the types of material they pass through. When a quake occurs, it sends out these mechanical waves. They travel through all the materials beneath the surface, and their velocity changes depending on what they travel through at the time. The density and elasticity of materials are important factors. The velocity of a wave will tell us how deep the quake was, essentially where it occurred.
As an example, if a wave passes through an area that has a lot of ice, the waves travel two to three times faster than they would through dirt or sand. Areas with a lot of ice mixed in also see bounce back in the waves as they interact with the stiff, dense materials. If an area on the Moon has a lot of ice underground, scientists would expect to see changes in velocity of the earthquake waves as well as any possible bounce back. According to Schmerr, bounceback would also reveal other characteristics of the hidden ice. “We can use seismic waves to not just see whether ice is present but also roughly how much of it there is,” he explained.
How to Test for Lunar Ice
It’s one thing to study earthquake waves here on the home planet, but quite another to do it on the Moon. To figure out the best way to determine lunar ice deposits, the team, led by Harrison Lisabeth of Lawrence Berkeley National Laboratory, tried three approaches for detection. First, they took a volcanic rock from Arizona that is a close mimic of lunar rocks. If you crush that type of rock, it turns into an almost exact analog for lunar dust. They froze it and then X-rayed it to see how ice settled between dust grains. The second approach involved temperature models for the polar regions, where ancient ice deposits seem to exist undisturbed by sunlight. Finally, Schmerr ran computer simulations of minor moonquakes to see how they would interact with underground lunar ice. All three methods left very obvious signs of ice in the data.
Data from X-ray tomography of simulated lunar regolith showing a) the dry sample, b) a rendering of icy microstructures prepared with small amounts of water, c) grains with the ice removed, and d) ice with the grains removed. The ice acts like a cement in the pore spaces between the grains of dust. This test result showed how the ice could exist in the regolith of the Moon. Credit: Lisabeth, Schmerr, et al.
The results look very promising, and the research team was able to come up with some suggestions for further examinations of methods to find ice on the Moon. One approach is to study the microstructures of a wider array of lunar regolith analogs here on Earth. In addition, future computer models should take into account more accurate measurements of lunar topography. Finally, the team suggests that further seismic models and tests be made to determine more accurate locations and depths of ice.
?
The hunt for lunar ice is a very real one and future explorers will need that resource. The team points out that recent spectroscopic data suggests that there is between 100 and 400 mg/g of water in the lunar soil. The job now is to identify deposits that are reasonably minable for industrial use by Artemis and other missions. Planned robotic and crewed missions to the moon in the next decade will provide opportunities to apply the tools of terrestrial near-surface geophysics to locating crucial lunar resources. The next viable mission is the Chinese Chang’e-7 is set to go to the Moon in …. and will carry a seismometer capable of looking for ice deposits in its landing site near Shackleton Crater. The 2028 Artemis mission should also be able to set a Lunar Environmental Monitoring Station that can also perform seismic studies.
For More Information
Scientists Use Moonquakes to Locate Lunar Ice
The Seismic Signature of Lunar Ice
Water on the Moon? New Study Narrows Down the Most Likely Suspects
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