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Gulf Countries Assess Damage from Record Rainfall, Compensates those Affected

Gulf countries continue to survey the damage and compensate those affected from the record rainfall. (Oman News Agency)
Gulf countries continue to survey the damage and compensate those affected from the record rainfall. (Oman News Agency)
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Gulf Countries Assess Damage from Record Rainfall, Compensates those Affected

Gulf countries continue to survey the damage and compensate those affected from the record rainfall. (Oman News Agency)
Gulf countries continue to survey the damage and compensate those affected from the record rainfall. (Oman News Agency)

The Al-Matir depression, which swept the Gulf region over the past two days, has caused human losses and massive material damage.

The Sultanate of Oman, the United Arab Emirates and Bahrain announced the end of the depression and that work was underway to reopen roads, assess the damage to infrastructure and public and private properties, and provide the necessary support to all those affected.

On Thursday, the Center for Emergency Management in Oman announced that rescue teams will continue to search for missing persons after the number of victims reached 19, most of them students.

The rainy weather condition in Oman, which was accompanied by flooding and thunderstorms, led to serious damage to public and private property.

The Regional Center for Climate Change in Saudi Arabia announced the start of a comprehensive climate study of the depression that affected the Gulf Cooperation Council (GCC) countries, its causes, and the extreme rainfall resulting from it. In a statement, the center said the study will also cover “the role of climate change” with efforts being coordinated with affected countries.

The center’s spokesman, Hussein Al-Qahtani, explained to Asharq Al-Awsat that the recent rainfall was higher than usual, which requires more research to study.

He stressed that that indicators of climate change were evident in several Saudi cities, such as Al-Namas, which witnessed hail falling in higher quantities than usual this year, in addition to other cities that saw the same situation last year, such as Taif, Buraidah, and Khamis Mushait.

He also confirmed that all climate studies presented by the National Center of Meteorology indicate that Saudi Arabia will see stronger climate phenomena in the coming years.

Last year, scientists at King Abdullah University of Science and Technology (KAUST) published a report that provided a comprehensive analysis of climate change and its consequences on the Arabian Peninsula.

The report said climate change could lead to higher temperatures and an increase in the severity and frequency of droughts, affecting agricultural and food production and leading to an increase in flash floods such as those witnessed in the region this week.

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Scientists Find Strongest Evidence Yet of Life on Alien Planet

An illustration shows a hycean world – an exoplanet with a liquid water ocean beneath a hydrogen-rich atmosphere - orbiting a red dwarf star. Based on observations by the James Webb Space Telescope, the exoplanet K2-18 b might fit in this category. This illustration was obtained by Reuters on April 16, 2025. A. Smith, N. Madhusudhan/University of Cambridge/Handout via REUTERS
An illustration shows a hycean world – an exoplanet with a liquid water ocean beneath a hydrogen-rich atmosphere - orbiting a red dwarf star. Based on observations by the James Webb Space Telescope, the exoplanet K2-18 b might fit in this category. This illustration was obtained by Reuters on April 16, 2025. A. Smith, N. Madhusudhan/University of Cambridge/Handout via REUTERS
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Scientists Find Strongest Evidence Yet of Life on Alien Planet

An illustration shows a hycean world – an exoplanet with a liquid water ocean beneath a hydrogen-rich atmosphere - orbiting a red dwarf star. Based on observations by the James Webb Space Telescope, the exoplanet K2-18 b might fit in this category. This illustration was obtained by Reuters on April 16, 2025. A. Smith, N. Madhusudhan/University of Cambridge/Handout via REUTERS
An illustration shows a hycean world – an exoplanet with a liquid water ocean beneath a hydrogen-rich atmosphere - orbiting a red dwarf star. Based on observations by the James Webb Space Telescope, the exoplanet K2-18 b might fit in this category. This illustration was obtained by Reuters on April 16, 2025. A. Smith, N. Madhusudhan/University of Cambridge/Handout via REUTERS

In a potential landmark discovery, scientists using the James Webb Space Telescope have obtained what they call the strongest signs yet of possible life beyond our solar system, detecting in an alien planet's atmosphere the chemical fingerprints of gases that on Earth are produced only by biological processes.
The two gases - dimethyl sulfide, or DMS, and dimethyl disulfide, or DMDS - involved in Webb's observations of the planet named K2-18 b are generated on Earth by living organisms, primarily microbial life such as marine phytoplankton - algae.
This suggests the planet may be teeming with microbial life, the researchers said. They stressed, however, that they are not announcing the discovery of actual living organisms but rather a possible biosignature - an indicator of a biological process - and that the findings should be viewed cautiously, with more observations needed, Reuters reported.
Nonetheless, they voiced excitement. These are the first hints of an alien world that is possibly inhabited, said astrophysicist Nikku Madhusudhan of the University of Cambridge's Institute of Astronomy, lead author of the study published in the Astrophysical Journal Letters.
"This is a transformational moment in the search for life beyond the solar system, where we have demonstrated that it is possible to detect biosignatures in potentially habitable planets with current facilities. We have entered the era of observational astrobiology," Madhusudhan said.
Madhusudhan noted that there are various efforts underway searching for signs of life in our solar system, including various claims of environments that might be conducive to life in places like Mars, Venus and various icy moons.
K2-18 b is 8.6 times as massive as Earth and has a diameter about 2.6 times as large as our planet.
It orbits in the "habitable zone" - a distance where liquid water, a key ingredient for life, can exist on a planetary surface - around a red dwarf star smaller and less luminous than our sun, located about 124 light-years from Earth in the constellation Leo. A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). One other planet also has been identified orbiting this star.

A 'HYCEAN WORLD'

About 5,800 planets beyond our solar system, called exoplanets, have been discovered since the 1990s. Scientists have hypothesized the existence of exoplanets called hycean worlds - covered by a liquid water ocean habitable by microorganisms and with a hydrogen-rich atmosphere.
Earlier observations by Webb, which was launched in 2021 and became operational in 2022, had identified methane and carbon dioxide in K2-18 b's atmosphere, the first time that carbon-based molecules were discovered in the atmosphere of an exoplanet in a star's habitable zone.
"The only scenario that currently explains all the data obtained so far from JWST (James Webb Space Telescope), including the past and present observations, is one where K2-18 b is a hycean world teeming with life," Madhusudhan said. "However, we need to be open and continue exploring other scenarios."
Madhusudhan said that with hycean worlds, if they exist, "we are talking about microbial life, possibly like what we see in the Earth's oceans." Their oceans are hypothesized to be warmer than Earth's. Asked about possible multicellular organisms or even intelligent life, Madhusudhan said, "We won't be able to answer this question at this stage. The baseline assumption is of simple microbial life."
DMS and DMDS, both from the same chemical family, have been predicted as important exoplanet biosignatures. Webb found that one or the other, or possibly both, were present in the planet's atmosphere at a 99.7% confidence level, meaning there is still a 0.3% chance of the observation being a statistical fluke.
The gases were detected at atmospheric concentrations of more than 10 parts per million by volume.
"For reference, this is thousands of times higher than their concentrations in the Earth's atmosphere, and cannot be explained without biological activity based on existing knowledge," Madhusudhan said.
Scientists not involved in the study counseled circumspection.
"The rich data from K2-18 b make it a tantalizing world," said Christopher Glein, principal scientist at the Space Science Division of the Southwest Research Institute in Texas. "These latest data are a valuable contribution to our understanding. Yet, we must be very careful to test the data as thoroughly as possible. I look forward to seeing additional, independent work on the data analysis starting as soon as next week."

TRANSIT METHOD

K2-18 b is part of the "sub-Neptune" class of planets, with a diameter greater than Earth's but less than that of Neptune, our solar system's smallest gas planet.
To ascertain the chemical composition of an exoplanet's atmosphere, astronomers analyze the light from its host star as the planet passes in front of it from the perspective of Earth, called the transit method. As the planet transits, Webb can detect a decrease in stellar brightness, and a small fraction of starlight passes through the planetary atmosphere before being detected by the telescope. This lets scientists determine the constituent gases of the planet's atmosphere.
Webb's previous observations of this planet provided a tentative hint of DMS. Its new observations used a different instrument and a different wavelength range of light.
The "Holy Grail" of exoplanet science, Madhusudhan said, is to find evidence of life on an Earth-like planet beyond our solar system. Madhusudhan said that our species for thousands of years has wondered "are we alone" in the universe, and now might be within just a few years of detecting possible alien life on a hycean world.
But Madhusudhan still urged caution.
"First we need to repeat the observations two to three times to make sure the signal we are seeing is robust and to increase the detection significance" to the level at which the odds of a statistical fluke are below roughly one in a million, Madhusudhan said.
"Second, we need more theoretical and experimental studies to make sure whether or not there is another abiotic mechanism (one not involving biological processes) to make DMS or DMDS in a planetary atmosphere like that of K2-18 b. Even though previous studies have suggested them (as) robust biosignatures even for K2-18 b, we need to remain open and pursue other possibilities," Madhusudhan said.
So the findings represent "a big if" on whether the observations are due to life, and it is in "no one's interest to claim prematurely that we have detected life," Madhusudhan said.