Friday, January 19, 2024

CLIMATE CHANGE

Climate change may reduce life expectancy by half a year, study suggests


On its own, a 1°C temperature rise might shave off about 5 months, with women and people in developing nations disproportionately affected


Peer-Reviewed Publication

PLOS



The cost of climate change may be six months off the average human lifespan, according to a study published January 18, 2024, in the open-access journal PLOS Climate by Amit Roy from Shahjalal University of Science and Technology and The New School for Social Research, U.S.

Temperature and rainfall — two telltale signals of climate change — cause myriad public health concerns, from the acute and direct (e.g., natural disasters like flooding and heat waves) to the indirect yet equally devastating (e.g., respiratory and mental illnesses). While impacts like these are observable and well documented, existing research has not established a direct link between climate change and life expectancy.

To clarify this relationship, the author evaluated average temperature, rainfall, and life expectancy data from 191 countries from 1940-2020, using GDP per capita to control for drastic differences between countries.

In addition to measuring the isolated impacts of temperature and rainfall, the author designed a first-of-its-kind composite climate change index, which combines the two variables to gauge the overarching severity of climate change.

Results indicate that in isolation, a global temperature increase of 1°C  is associated with an average human life expectancy decrease of approximately 0.44 years, or about 5 months and 1 week. A 10-point increase in the composite climate change index — which accounts for both temperature and rainfall — is expected to decrease the average life expectancy by 6 months. Women and individuals in developing nations are disproportionately affected.

Beyond the results of this study, Dr Roy is hopeful that the composite climate change index will standardize the global conversation about climate change; become a usable metric for the nonscientific public; and encourage collaboration and even friendly competition among countries to combat the impacts of climate change.

Mitigating greenhouse gas emissions and adapting to a changing environment are of particular importance, the author says.

To complement this large-scale approach, the author suggests localized future studies that consider specific severe weather events (e.g., wildfires, tsunamis, and floods), the impacts of which cannot be fully captured through analyzing temperature and rainfall alone.

Dr. Roy adds: "The global threat posed by climate change to the well-being of billions underscores the urgent need to address it as a public health crisis, as revealed by this study, emphasizing that mitigation efforts to reduce greenhouse gas emissions and proactive initiatives are essential to safeguard life expectancy and protect the health of populations worldwide."

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In your coverage please use this URL to provide access to the freely available article in PLOS Climate: https://journals.plos.org/climate/article?id=10.1371/journal.pclm.0000339

Citation: Roy A (2024) A panel data study on the effect of climate change on life expectancy. PLOS Clim 3(1): e0000339. https://doi.org/10.1371/journal.pclm.0000339

Author Countries: Bangladesh, US

Funding: The author received no specific funding for this work.

SPACE



PHOTO FREE ARTICLE

Study delivers detailed photos of galaxies’ inner structures


JWST data reveals how dust, gas assemble to form galactic disks


Peer-Reviewed Publication

OHIO STATE UNIVERSITY




COLUMBUS, Ohio – For the first time, high-resolution images captured by the James Webb Space Telescope are offering powerful insights into the complex dust patterns of nearby star-forming galaxies.  

One of the most fundamental building blocks in the universe, cosmic dust is a vital ingredient to the growth of a galaxy. When scattered, these tiny grains help plant the seeds for the creation of stars and planets alike – yet only recently, through rapid leaps in technology, have astronomers begun to shine a brighter light on their intricate physics.  

Led by scientists at The Ohio State University, an international team of astronomers used data collected by the James Webb Space Telescope’s Mid-Infrared Instrument to create stunning visuals of 19 spiral galaxies located relatively close to the Milky Way. By examining infrared light – wavelengths invisible to the naked eye – these incredibly precise images reveal how dust fertilizes the universe after being heated by both massive young stars and surrounding interstellar space radiation.  

“Using this brand new data, we’re able to see the distribution of dust emission and determine what the interstellar material in the disks of these galaxies looks like,” said Debosmita Pathak, lead author of the study and a graduate student in astronomy at Ohio State. 

The images were taken from the PHANGS-JWST Cycle 1 Treasury, a survey collaboration that uses high-powered telescopes to better understand galactic evolution. In this study, they used data collected from the first year of Webb observations to create probability distribution function (PDF) measurements that chart the galaxies’ dust emissions in the mid-infrared.  

They found that the disks of galaxies in the mid-infrared show both a normal distribution of gas (represented in the study’s PDF charts as a high peak) and a high distribution (appearing as a gentle slope). While the regions where star-forming nurseries reside look noticeably different, the shape and width of the distribution of diffuse gas in these galaxies stayed consistent.  

“Dynamically, they’ve all got very different things going on in the centers,” said Pathak. “But once you take the centers out of the picture, the disks of these galaxies look very similar to each other.” 

The study, published recently in The Astronomical Journal, suggests that because the patterns of infrared light emitted by these observed galaxies seem to be uniform, the density of the gas inside galactic disks follows a specific pattern even when shaped by very different galactic environments. “Because this dust traces out the fuel for future generations of stars,” Pathak said, “the similarity we see among galaxies hints that some aspects of star and planet formation may be universal across galaxies.” 

By illuminating another clue about the mysteries of our universe, these galactic snapshots also provide an opportunity for humans to take a look in the cosmic mirror, Pathak said.  

“It’s hard for us to get a global perspective of the Milky Way,” said Pathak. “This study tells us that if you looked at it as an outsider, you would see something similar to what we saw for a bunch of other nearby galaxies.” 

Moreover, deepening our current understanding of the structure of nearby galaxies could lead to a better grasp of astrophysics, including how various objects in the universe fit together. 

Ultimately, once more data becomes available after the next few JWST cycles, the team plans to redo much of the work with an even larger and richer sample size. 

“You can’t observe all galaxies in the universe at such high resolutions, so it helps to be able to make quantitative statements about them in general, because that allows us to extrapolate about more and more galaxies in the future,” said Pathak.  

This study was supported by the National Science Foundation, the Alexander von Humboldt Foundation, the Heising-Simons Foundation, the Natural Sciences and Engineering Research Council of Canada (NSERC), and the Simons Foundation. Other Ohio State co-authors were Adam K. Leroy, Todd A. Thompson and Laura A. Lopez.  

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Contact: Debosmita Pathak, Pathak.89@osu.edu 

Written by: Tatyana Woodall, Woodall.52@osu.edu